How did the Lucayans make use of the Rollin’s Creek South barrier island? Introduction Archaeology is the study of past human activity through examining the materials that they have left behind. The Lucayan Taíno people inhabited the Bahamas for nearly 800 years, spanning roughly from 650 CE to 1550 CE, with a population comparable to the population of the outer islands of the Bahamas today. We were interested in testing two hypotheses. One, that barrier islands were commonly settled by the Lucayans in order to take advantage of the ample resources to be found in the nearby creeks, coppice, and ocean. The other, Dr. William F. Keegan’s settlement pairing idea, that Lucayans often built settlements in pairs less than 1.5 km apart. We based our project area off of these two hypotheses after comparing possible sites with the trends in Lucayan settlements shown by Shaun Sullivan and Dr. William F. Keegan’s data. In total, Shaun Sullivan collected 15 sites on Eleuthera in 1974 for his master’s thesis, and Dr. William F. Keegan has done a lot of work within The Bahamas. When surveying our project area, we look for ecofacts (hole-punch conch, nerite shells) and artifacts. The most signiﬁcant artifact is Palmetto ware, a pottery speciﬁc to the Lucayans that we are unable to replicate. Methods The major materials used for this survey are the GPS and ﬁeld notebook that is used to document measurements. The method used in this survey was a standard phase 1 surface survey, speciﬁcally, a meandering transect, a phase 1 survey designed especially for the Bahamas. No digging or artifact collection was involved. Documentation of objects is broken down into sketching, taking a GPS waypoint, taking photographs, measuring the objects, and recording data in the ﬁeld notebook. Results • 3 main sites documented: Rollin’s Creek South site at locality 183, Rollin’s Creek Ceremonial site centered on locality 177, and Rollin’s Creek Resource site • A total of 105 pieces of Palmetto Ware was found • 3 main scatters of Palmetto Ware at Rollin’s Creek South and Rollin’s Creek Ceremonial sites • High percentages of specialty Palmetto Ware pottery found • Smooth lithic found at Rollin’s Creek Ceremonial site • Large scatter of ecofacts at Rollin’s Creek Resource site • King Helmet conch found at Rollin’s Creek Resource site Discussion Based on the ﬁndings, we located three Lucayan sites, none of which are permanent settlements because: • Findings were concentrated at speciﬁc sites and not continuously scattered (Figures 2 and 4). • Small range of pottery thicknesses indicates only one or two pots were at each site vs. a permanent settlement’s large amount of pots (Figures 9 and 10). The evidence suggests that Rollin’s Creek Ceremonial site and Rollin’s Creek South site were used for ceremonial purposes because: • Specialty pottery that was found indicates ceremonial use as it was not used in daily life. • High percentages of specialty pottery at these sites compared to Sullivan’s baseline data (Table 1). The third site, Rollin’s Creek Resource site, was likely a resource-procurement area because: • Large number of shell remains at Rollin’s Creek Resource site (ﬁgure 4) • Could have been used by permanent settlement across the creek We supported our barrier island theory because we found Lucayan sites, but found contradictory evidence for the settlement pairing theory because no permanent settlement was found. Recommendations: Our project area holds signiﬁcance in archaeological studies because it likely had ceremonial uses, while very few other documented Lucayan sites are believed to have ceremonial uses. The location of our project area brings up the question as to whether all permanent settlements had nearby satellite sites used for ceremonial and resource gathering purposes. Recommendations for future studies include completing documentation of our project area, as well as continuing to test the barrier island and settlement pairing hypotheses. Carter B


ROOT I/O data compression improvements for HEP analysis Oksana Shadura (CMS/UNL), Zhe Zhang (CMS/UNL), Brian Paul Bockelman (CMS/Morgridge Institute for Research), Philippe Canal (CMS/FNAL), Danilo Piparo (CMS/CERN) oksana.shadura@cern.ch,bbockelman@morgridge.org Introduction ZSTD - a dictionary-type algorithm (LZ77) with large search window and fast implementations of entropy coding stage, using either very fast Finite State Entropy (tANS) or Huﬀman coding. [https://github.com/facebook/zstd.git] AVAILABLE IN ROOT 6.20! ZSTD for NanoAOD (compression levels) →Better compression ratio and 2x faster decompression then ZLIB; 6x faster comparing to LZMA; ﬁle compressed with ZSTD is only 20 % bigger! NanoAOD 2019 compression ratio comparison *ZSTD-1 means ZSTD with compression level 1 →Better compression ratio then ZLIB Data ﬁle with oﬀset arrays →ZSTD has no problems with compression of data that contains the byte oﬀset of each event in the branch data (vs LZ4) CMSSW NanoAOD and MiniAOD (including LZ4) →NanoAOD - using ZSTD could be a better compromise between size of ﬁle on a disk and decompression speed for a faster analysis!; →MiniAOD - time spend in decompressing on readback is 15x less vs LZMA, while size of ﬁle with ZSTD is only 10% bigger! (thanks to David Lange for MiniAOD measurements) LHCB compression speed vs compression ratio →For the very simple ntuples with a simple structure the best choice could be LZ4: 10x time faster read speed TTree::kOnlyFlushAtCluster: faster decompression →TTrees can be forced to only create new baskets at event cluster boundaries, it simpliﬁes ﬁle layout and I/O at the cost of memory (NanoAOD 2017 size diﬀerence was 3.6 %). Recommended for simple ﬁle formats such as ntuples but not for more complex data types. tree->SetBit(TTree::kOnlyFlushAtCluster); Acknowledgements This work was supported by the National Science Foundation under Grant ACI-1450323.


Neben dem Angebot von Texten bietet RIDE durch die strukturelle und semantische Codierung der Inhalte auch vermehrt datengestützte Zugänge. Damit wird der Blick auf die Gesamtheit der Rezensionen und die rezensierten Gegenstände gefördert. Die herausgeberische Arbeit wird so vermehrt zur informationstechnologischen Gedächtnisarbeit. RIDE als DATEN RIDE als CODE RIDE als WEBSITE GitHub: https://github.com/i-d-e/ride Zenodo: https://zenodo.org/record/5081646 Das IDE zeichnet für die digitale Infrastruktur und den Publikationsworkflow von RIDE selbst verantwortlich. Die Publikationsinfrastruktur besteht aus einem Zusammenspiel von eXist-db und Wordpress. RIDE - was ist das? GitHub: https://github.com/i-d-e/ride-scripts URL: https://ride.i-d-e.de Auf der Website der Zeitschrift erhalten Leserinnen und Rezensentinnen Informationen zu den Zielen, den Methoden und Inhalten von RIDE. Jede Rezension erscheint als ein Artikel, der im HTML- Format oder als PDF gelesen werden kann. Ergänzt wird jeder Rezensions- artikel durch das “Factsheet”, das die Ergebnisse eines Fragebogens zur rezenzierten Ressource enthält. Die Sicht auf einzelne Rezensionsartikel wird ergänzt durch übergreifende Darstellungen, insbesondere Listen aller Ressourcen, Autorinnen und Diagramme mit Übersichten über die Fragebogen-Ergebnisse. Informationstechnologische Gedächtnisarbeit in der Rezensionszeitschrift RIDE Datensätze aller RIDE-Bände werden in einem GitHub- Repositorium verwaltet und im Forschungsdatenrepositorium Zenodo veröffentlicht, in welchem sie versioniert und über die Zuweisung einer DOI zitierfähig gemacht werden. RIDE (A Review Journal for Digital Editions and Resources) ist eine Open Access- Zeitschrift für Rezensionen über digitale wissenschaftliche Editionen, Text- sammlungen sowie Tools und Forschungsumgebungen für das digitale Edieren. Die Zeitschrift bietet ein Forum, in dem Expertinnen digitale Ressourcen diskutieren können, um aktuelle Praktiken einzuordnen und zu bewerten und künftige Entwicklungen mit zu gestalten. Dabei steht neben inhaltlichen Gesichtspunkten vor allem eine methodische Begutachtung der digitalen Editionen, Textsammlungen und Tools im Vordergrund. Um die Rezensentinnen zu unterstützen, werden Kriterienkataloge angeboten, die auf wichtige zu begutachtende Aspekte eingehen. ENJOY THE RIDE! RIDE erscheint seit 2014 und wird vom Institut für Dokumentologie und Editorik (IDE) herausgegeben. Bisher sind 75 Rezensionen erschienen. In RIDE nehmen Rezensionen die Form von Forschungsartikeln an, die einen Peer Review-Prozess durchlaufen. Begleitet werden die Texte durch “Factsheets”, in denen zentrale Daten zu den digitalen Ressourcen strukturiert präsentiert werden. Als Zeitschrift bietet RIDE also nicht nur Lesetexte, sondern basiert auf Daten zu den Rezensionen und den rezensierten Gegenständen. Diese werden auf der RIDE-Website in vielfältiger Form präsentiert, aber auch direkt zum Download angeboten. Verarbeitet werden die Daten durch Code, der einen wesentlichen Teil der RIDE-Workflows darstellt. Die Routinen zur Verarbeitung der Daten werden auf GitHub publiziert, darunter Skripte zur Generierung der langzeit- archivierbaren PDFs, für den Export der Metadaten über eine OAI-PMH-Schnittstelle, für die Directory of Open Access Journals (DOAJ) und für die Erstellung von Wordclouds. RIDE ist ein datengestütztes Journal. Die Rezensionen und Metadaten sind in XML/TEI kodiert, auf Basis eines TEI- Schemas in ODD (“One Document Does it all”). Außerdem wird jede Rezension als PDF archiviert. Ulrike Henny-Krahmer, Universität Rostock Frederike Neuber, Berlin Brandenburgische Akademie der Wissenschaften Martina Scholger, Universität Graz https://ride.i-d-e.de


Response of Chelidonium majus in vitro cultures and their alkaloid content under heavy metal stress Iva Doycheva1, Stefan Philipov2 1Institute of Biodiversity and Ecosystem Research, Bulgarian Academy of Sciences 2Institute of Organic Chemistry with Centre of Phytochemistry, Bulgarian Academy of Sciences Introduction Heavy metal contamination is becoming an increasing environmental problem worldwide. Heavy metals (HM) retard plant growth, yield and affect the secondary metabolism which results in fluctuations in plant metabolites, such as the alkaloids. The aim of the study was to investigate the influence of HM on the growth of in vitro cultivated plants of Chelidonium majus L. (Fig. 1) and their alkaloid content. Results and discussion Plants cultivated at the lower concentration of Cd2+ formed roots and developed normally with a gradual reduction in their growth and rooting as the concentration of the supplemented HM increased (Fig. 2). There were not any differences in the development of the plants cultivated on Cd2+according to their type of origin (Fig. 2; 3). Epinasty and browning of the leaves were observed among the plants cultivated on the medium supplemented with Pb2+. These side effects got worse as the concentration of the HM increased, and were also accompanied by a strong reduction in the rooting (Fig. 4). The plants which were obtained from seeds developed normally and did not show any of the signs of the ones which were propagated through AS (Fig. 3; 4). None of the plants cultivated on a medium supplemented with Zn2+ survived, regardless of their origin and HM concentration. A phytochemical study showed that the plants cultivated at the highest concentrations of Cd2+ and Pb2+ and also obtained through AS had the highest RAM. However, the plants cultivated at the same concentrations but obtained from seeds had lower RAM similar to that of the plants cultivated at lower concentrations of HM and propagated through AS (Fig. 5). Materials and methods The plants were cultivated on a medium B5 with double the amount of macrosalts (2B5), 0.5 g/l activated charcoal and supplemented with different concentrations of HM – Cd2+ (0.5; 1 mg/l); Pb2+ (100; 250 mg/l); Zn2+ (100; 250 mg/l). Plants were obtained in vitro from seeds or were propagated through adventitious shooting (AS). The raw alkaloid mixtures (RAM) were obtained by usual chemical procedure. For contacts: idoycheva@gmail.com Conclusions In conclusion, Ch. majus was able to cope with the influence of Cd2+ and Pb2+ in the culture medium, but not with that of Zn2+. Quantity of RAM was influenced by the HM concentration and the origin of the plants. Acknowledgements: This research was supported by the Bulgarian National Science Fund, Bulgarian Ministry of Education and Science (Project КП-06-М26/4 from 01.12.2018). Fig. 1. Chelidonium majus L. Fig. 5. RAM (%) in native plant sample and in vitro cultivated plant samples obtained through AS or seed germination. 0,92 1,54 1,51 1,39 3,56 3,78 1,94 1,01 0,81 Reference sample 2B5 - Control AS 2B5 + 0.5 mg/l Cd (AS) 2B5 + 100 mg/l Pb (AS) 2B5 + 1.0 mg/l Cd (AS) 2B5 + 250 mg/l Pb (AS) 2B5 - Control Seeds 2B5 + 1.0 mg/l Cd (S) 2B5 + 250 mg/l Pb (S) Plant material from native plants Plants material from plants propagated through adventitious shooting Plant material from plants obtained from in vitro germinated seeds BalkanBio’2021 Fig. 2. Plants propagated through AS and cultured on 2B5 supplemented with Cd2+. Fig. 4. Plants obtained through AS and cultured on 2B5 supplemented with different concentrations of Pb2+. Fig. 3. Plants obtained from seeds and cultured on 2B5 supplemented with Cd2+ or Pb2+.


Wikibase ❖open source software ❖created by WikiMedia Foundation ❖user friendly ❖rich in collaborative tools ❖using RDF ❖flexible data model ❖multilingual Reasons for WikiHum ❖Decentralisation of historical data ❖Lack of reliable and Persistent Identifiers ❖Mismatch between reference databases (VIAF, GND, Wikidata) and the needs of historians ❖Need for harmonisation of historical data Process of implementing data into WikiHum Label_pl Label_en Description_pl Description_en Królestwo Polskie (1370-1568) The Kingdom of Poland (1370-1568) terytorium Królestwa Polskiego territory of the Kingdom of Poland Tab.1 Administrative system: label and description Label_en P value The Kingdom of Poland (1370-1568) instance of administrative system The Kingdom of Poland (1370-1568) Starts at 1370-01-01 The Kingdom of Poland (1370-1568) Ends at 1568-12-31 The Kingdom of Poland (1370-1568) Aen The Crown of Poland The Kingdom of Poland (1370-1568) legal basis reformy ustrojowe XIV w. The Kingdom of Poland (1370-1568) legal basis statuty wiślicko-piotrowskie (1356-1362 r.) The Kingdom of Poland (1370-1568) subclass of secular administrative system The Kingdom of Poland (1370-1568) Wikidata ID Q1649871 The Kingdom of Poland (1370-1568) ontohgis database id https://onto.kul.pl/ontohgis/administrative_sys tem_44 Tab.2 Administrative system: statements Source: https://ontohgis.pl/ final view in WikiHUM “One Base to rule them all, one Base to ﬁnd them, One Base to bring them all, and in the Wiki bind them” Reference database for Polish historical data Content ❖Item metadata ❖DARIAH.Lab ID - Handle.net ❖External ID (e.g. Wikidata, VIAF, etc.) ❖Standards and Ontologies (CIDOC CRM, OntoHGIS, SKOS) Biographical data ❖Polish Biographical Dictionary ❖Polish National Library Authority File ❖Urzędnicy Dawnej Rzeczypospolitej. Spisy [Officials of the Old Commonwealth. Lists] ❖etc. Geographical data ❖Historical Atlas of Poland ❖Historical-Geographical Dictionary of the Polish Lands in the Middle Ages ❖Polish National Register of Boundaries ❖Polish National Register of Geographical Names Wikibase as an environment for harmonisation of data about past: the example of WikiHum Authors Adam Zapała azapala@ihpan.edu.pl Tomasz Królik tkrolik@ihpan.edu.pl The Tadeusz Manteuffel Institute of History Polish Academy of Sciences COMING SOON wikihum.lab.dariah.pl


Delivering Fine-grained Environmental Spatial Data in HPC and Cloud Converged Infrastructure PI: Michela Taufer*, Co-PI: Rodrigo Vargas↟ Project Contributors: Paula Olaya*, Camila Roa*, Jakob Luettgau*, Ricardo Llamas↟, Sophia Wen‡, I-Hsin Chung‡, Seetharami Seelam‡, Yoonho Park‡, and Jay Lofstead† *University of Tennessee, Knoxville,↟University of Delaware, ‡IBM, †Sandia National Laboratory Generating Fine-grained Environmental Spatial Data ●Environmental spatial data (i.e., terrain parameters and soil moisture) provide information about phenomena on the surface of the earth ●These data are fundamental in applications such as precision forestry and agriculture, identifying biodiversity loss, hydrology for landscape ecology, understanding vegetation changes, wildfire detection, and spotting at-risk ecosystems1 [1] Jennifer Bernstein, Karen Kemp; The Role of Spatial Science in Environmental Case Studies: A Special Collection from the University of Southern California. Case Studies in the Environment 1 January 2020; 4 (1): 1–5. Generating environmental spatial data at high-resolution is computationally expensive, hindering scientific communities’ ability to access the data Digital Elevation Model Satellite Soil Moisture Data Generation Terrain Parameters Data Transformation Training Data Testing Data ML- Training ML- Inference ML-Model Soil Moisture Predictions Analysis/ Visual Geographic statistics/ maps Terrain Parameter Generation (GEOtiled) Data Transformation ML-Prediction Soil Moisture We develop a workflow called SOMOSPIE (SOil MOisture SPatial Inference Engine) that generates fine-grained terrain parameters and soil moisture Analysis/ Visualization HPC and Cloud Convergence ●Our workflow comprises four stages: a terrain parameter generation, a data transformation, an ML-based prediction, and Analysis/Visualization ●Each of the stages leverages advanced computational techniques to transform data and generate ready-for-use environmental spatial data Our solution scales performance and enables scientific communities to access our end-to-end workflow and data on converged HPC and Cloud infrastructure Soil Moisture Maps @ <1 km Elevation models @ <1 km Terrain P. Generation Data Transformation ML Predict Analysis Visualization Satellite Soil Moisture @ 27 km Precision agriculture Environm. sciences Wildfire Detection SOMOSPIE: SOil MOisture SPatial Inference Engine Train1 Hybrid HPC-Cloud Cluster Train2 Train3 TrainN Inference Inference Inference Inference def train(): … def inference(model): … dsl.pipeline(ml-model): for i in N_years: model=train() inference(model) TektonCompiler(). compile(pipeline, “pipeline.yaml”) Inference Inference Inference Inference Inference Inference Inference Inference Inference Inference … … Predicted Soil Moisture1 Predicted Soil Moisture2 Predicted Soil Moisture3 Predicted Soil MoistureN … Open Data Hub Pipelines We use Open Data Hub Pipelines to orchestrate the execution of our workflow in cloud-native clusters (i.e., Kubernetes and OpenShift) with Cloud Object Storage The authors acknowledge the support of the National Science Foundation through the awards 1841758, 2103845, 2138811, and 1941443 Reproducibility efforts Paper Github Cloud-HPC Integration SOMOSPIE’s workflow Paper Github Trustworthiness and Reproducibility Our solution ensures trustworthiness and reproducibility in the data, software, and environment, wrapped in the scientific discovery loop ●We create a fine-grained containerized environment that automatically provides provenance information and seamlessly attaches it to the workflow components ●The containerization supports easy retrieval for reusability, reproducibility, and portability of the workflow


PHOTOVOLTAIK-INSTITUT BERLIN Mechanische Belastungsuntersuchungen Testsequenz und Probenaufbau PHOTOVOLTAIK-INSTITUT BERLIN Verschattungstoleranz UNTERSUCHUNGEN AN GESCHINDELTEN PHOTOVOLTAIK MODULEN Stefan Wendlandt PI Photovoltaik-Institut Berlin AG, Wrangelstr. 100, D-10997 Berlin, Germany, Phone: +49 (30) 814 52 64-205, mail: wendlandt@pi-berlin.com 2017.03.08-V1.0 © PI Berlin Zusammenfassung Einleitung In den letzten Jahren rückte das Design von Photovoltaikmodulen und deren Effizienzsteigerung immer mehr in den Forschungsschwerpunkt. Ein wichtiger Parameter ist dabei die Optimierung der Zellkontaktierung, da sie den Serienwiderstand und die Leistungsabgabe bei höheren Bestrahlungsstärken beeinflusst. Ein neuartiger Verbindungsansatz ist das Schindeln von Solarzellen. Geschindelte Module können hohe CTM-Werte (Cell-to-Module) erreichen. Diese Art der Verbindung ermöglicht gleichwohl mehr Möglichkeiten beim Design vom elektrischen Layout. Der Schlüssel beim Schindeln liegt jedoch in den Eigenschaften der elektrisch-leitfähigen Klebstoffe (ECA). Er muss gleichzeitig leitfähig und mechanisch flexibel sein. In dieser Arbeit haben wir die Langzeitstabilität von kommerziellen geschindelten PV-Modulen untersucht. Dafür haben wir eine spezielle Testsequenz erstellt. Unsere Ergebnisse konzentrieren sich auf die mechanische Stabilität durch Anwendung verschiedener Stresstests sowie die elektrische Leistung bei unterschiedlichen Verschattungen. Der Aufsatz endet mit einer Schwachstellenanalyse der derzeit verfügbaren geschindelten PV-Panels mit unterschiedlichen elektrischen Layouts. Wir haben verschiedene handelsübliche Schindelmodule charakterisiert und beansprucht. Dabei haben wir uns auf die mechanische Stabilität konzentriert. Wir haben einen klaren Zusammenhang zwischen der Belastung bei kurzen und langen geschindelten Zellstrings beobachtet. Während der Biegetest einen vernachlässigbaren mechanischen Einfluss auf die Module hat, hat der ML-Test einen großen Einfluss auf die Moduldesigns mit langen Zellstrings. Dort ist der Krafteinfluss aufgrund der Lage der gebrochenen Zellen deutlich sichtbar. Bei den Modulen mit den kurzen Strings ist quasi kein Einfluss sichtbar. Dies kann mit der Kraftabsorption des ECA und des Verkapselungsmaterials aufgrund seiner Elastizität und der kurzen Kantenlänge der Zellen in Richtung der Krafteinwirkung beschrieben werden. Wir möchten daher darauf hinweisen, dass der begrenzende Spannungsfaktor die Zugfestigkeit der ECA und des Verkapselungsmaterials ist. Weiterhin zeigte die Verschaltung von Brand „E“ (kurze-parallele Stränge) die beste Verschattungstoleranz und damit die höchste elektrische relative Leistungsabgabe. Dies kann durch die Zellblockaufteilung sowie die geringere Anzahl von Solarzellen pro Bypass-Dioden begründet werden. ACKNOWLEDGEMENTS: Dieses Projekt wurde mit Mitteln aus dem Horizon2020-Programm der Europäischen Union für Forschung, technologische Entwicklung und Demonstration unter der Grant Agreement Nr. 857793 (HighLite) gefördert. Abbildung 1: In unserem ersten Versuch wollten wir wissen, ob und welchen Einfluss die unterschiedlichen Verschaltungen auf die elektrische Leistung bei Verschattung haben. Dafür haben wir uns fünf unterschiedliche Verschattungsszenarien überlegt. Abbildung 2: Relative Leistungsverluste pro Verschattungsszenario darstellt über das Verhältnis verschattete Fläche zu Modulfläche gezeigt für vier der fünf Szenarien. Abbildung 5: EL-Bilder (@Isc) aller Hersteller nach den jeweiligen Tests. Auffällig ist das Modul „D“ schon initial Kontaktierungsprobleme aufzeigt. Weiterhin ist erkennbar, dass der Bending-Test keinen relevanten Schaden auf die Module ausübt. Anders hingegen beim mechanischen Belastungstest, hier sind bei den Modulen mit vertikalen Strängen („A“ und „D“), starke Zellbrüche ersichtlich. Es wird vermutet, dass die Zellen quasi zerrissen wurden, da anders als bei Brand „B“ und „C“ das ECA die Scherkräfte absorbieren kann. Mit anderen Worten


Autor: Zenaldo de Almeida Rodrigues Mestrando em Administração – Universidade Positivo Orientador: Prof. Dr. Luiz Pinheiro Linha de Pesquisa: Inovação, Estratégia e Sustentabilidade INTELIGÊNCIA ARTIFICIAL (IA) E TRABALHO: UMA ANÁLISE SOBRE OS IMPACTOS CAUSADOS PELA UTILIZAÇÃO DA INTELIGÊNCIA ARTIFICIAL NO TRABALHO DAS PESSOAS INTRODUÇÃO Nos últimos anos temos visto uma grande profusão de novas tecnologias baseadas em Inteligência Artificial (IA). Segundo Matheus (2020), nove áreas do fazer humano serão afetadas por esta nova tecnologia: Estratégia, Machine Learning (aprendizado das máquinas), Speech Voice (escrita e voz humana), Imagem Recognition (reconhecimento facial e de imagens no geral), Robotic (robótica e seus processos), Neural Networrks (redes neurais), Sentiment Analysis (análises dos sentimentos), Natural Language (estudo da linguagem natural humana), Deep Learning (aprendizado profundo e constante das máquinas). Entender os impactos que esta nova tecnologia e seus campos de atuação podem provocar na forma com que as pessoas realizam suas tarefas, passou ser um objeto de estudo significativo para a humanidade. OBJETIVOS / PERGUNTA DE PESQUISA Objetivo: Investigar a influência da inteligência artificial (IA) no trabalho e seus possíveis impactos na sociedade como um todo; RQ1: Quais as possíveis tarefas que serão afetadas pela utilização de IA e como ficará o trabalho executado por humanos? RQ2: Haverá migração de mão de obra? RQ3: Como podemos nos preparar para uma possível migração de mão de obra? REVISÃO DA LITERATURA A OCDE e a ONU, apresentam pontos comuns de preocupação com a influência da utilização da tecnologia de Inteligência Artificial. Para isso juntas desenvolveram quatro pilares de orientação aos países, com a finalidade de direcionar a utilização da IA: 1º O incentivo para pesquisa e desenvolvimento de IA , aplicadas a diferentes campos de negócios (organizações, empresas e governos); 2º A definição de princípios éticos e perspectivas regulatórias que passem pelo problema da governança de dados, parâmetros regulatórios, transparência e accountability . 3º Criar uma abordagem para a governança de tecnologias emergentes; 4º Criar uma abordagem para a transformações do trabalho, do emprego e construção de capacidades para lidar com as mudanças que já emergem com a Inteligência Artificial; Acemoglu e Restrepo (2019), apresentam que “estamos longe de uma compreensão satisfatória em como a automação em geral e a IA, impactam o mercado de trabalho e sua produtividade”. Sendo assim um objeto de estudo que nos apresenta um grande espectro de estudo a frente; Zeira (1998), nos coloca uma dicotomia de pensamentos:  O primeiro pensamento é uma visão mais APOCALÍPTICA do tema. Onde os avanços com a IA irá acabar com o trabalho humano;  O segundo reflete a visão dos economistas, que diz que os avanços tecnológicos no passado acabaram aumentando a demanda por mão de obra e salários; MÉTODO E ANÁLISE DOS DADOS Quadro 1: Metodologia CONSIDERAÇÕES FINAIS Lee (2019), em seu livro INTELIGÊNCIA ARTIFICIAL – Como os robôs estão mudando o mundo... nos traz uma perspectiva de como esta evolução da IA aconteceu. Sendo a partir de 2012 quando Geoffrey Hinton, um pesquisador da universidade de Toronto no Canadá, desenvolveu redes neurais capaz de levar máquinas a um aprendizado profundo é que a IA passou a ter uma perspectiva de utilização mais efetiva para a humanidade. Podendo a partir deste momento desempenhar tarefas hora antes destinada somente a humanos. Iansiti e Lakhani (2021), trazem uma abordagem voltada para as empresas e como a IA poderá afetar efetivamente a mão de obra nela existente, dando desta maneira um direcionamento específico para negócios, trazendo a luz perspectivas do que poderemos enfrentar em um cenário futuro; A partir do entendimento do nascimento e desenvolvimento da Inteligência Artificial, seus conceitos e aplicações. Podemos entender a dimensão dos impactos e influências da utilização desta no


Gemeinsame Infrastrukturen und Services zum Forschungsdatenmanagement in, aus und für Baden-Württemberg 1. Einleitung und Grundlage 2. Drei Fallbeispiele aus bwFDM Dr. Sophie G. Habinger1 0000-0002-5513-954X Maximilian Heber1 0000-0003-3399-7532 Dr. Philipp Kling2 0000-0003-0104-4905 1Kommunikations-, Informations-, Medienzentrum (KIM) der Universität Konstanz 2Universitätsrechenzentrum der Universität Heidelberg In Baden-Württemberg gibt es bereits eine Vielzahl an Landesdiensten und -services, die Bedarfe aus dem Forschungsdatenmanagement adressieren. Informieren, Austauschen, Vernetzen Welche FDM- Infrastrukturen gibt es in BW? Zugang zu Rechen- und Speicher- ressourcen Speicherung großer Mengen an kalten Forschungsdaten kollaboratives Arbeiten mit kleinen Datenmengen bwVisu Speicherung großer Mengen an heißen Forschungsdaten bwSFS LSDF Online Storage SDS@hd bwData Archive bwSync&Share bwFDM Helpdesks bwSupport Virtuelle Maschinen und Cloud Computing bwCloud bwUniCluster Speichern | Rechnen | Speichern und Rechnen | Kollaboration | Helpdesks/Supportservices Emilia Mikautsch1 0009-0005-1758-1790CC BY 4.0 –https://creativecommons.org/licenses/by/4.0/(Logos ausgenommen) Projektpartner der Landesinitiative: Gefördert vom: bwHelpdesk zum FDM • Rückgriff auf/Verwendung von bwSupport Portal geplant • Landesweite Helpdesk- Infrastruktur ermöglicht einfache Kollaboration der gehosteten Beratungsangebote zu den einzelnen Services ? --- --- Vernetzung Schaffung von Rahmen- bedingungen zum Austausch: • überregional: E-Science-Tage • BW-intern: AK FDM, bwFDM- Forum und Austausch mit bwHPC E-Science-Tage AK FDM bwFDM-Forum forschungsdaten.info • Technisch & administrativ: bwFDM • Inhaltlich: Redaktionsteam aus deutschsprachigem Raum forschungsdaten.info FORTH-BW fdm@DHBW


Michael Kleineberg1 , Miriam Kötter2 , Jasmin Schmitz3 , Paul Schultze-Motel4 , Katja Wermbter5 1: Distributed Network for Publishing Services, Freie Universität Berlin, Universitätsbibliothek 2: Landesinitiative openaccess.nrw / Universität Duisburg-Essen, Universitätsbibliothek 3: ZB MED - Informationszentrum Lebenswissenschaften, PUBLISSO Publikationsberatung 4: Helmholtz-Gemeinschaft / open-access.network 5: FID BAUdigital, TU Braunschweig, Universitätsbibliothek Wer wir sind • Best Practices zu: Aufbau eines Open-Access-Beratungsangebots Organisation eines Helpdesks Dokumentation der Kundenkommunikation Tools (z. B. Ticketsystem) Verteilung von Ressourcen interner und externer Kommunikation • Erstellung einer gemeinsamen Materialsammlung Mitmachen Ebenfalls auf der Agenda Sie betreiben oder planen selbst einen Open-Access-Helpdesk und möchten sich darüber austauschen? Die Fokusgruppe freut sich über neue Mitglieder! Weitere Informationen finden Sie hier: Was wir tun Liste der Helpdesks und Beratungs- angebote in den teilnehmenden Einrichtungen Sammlung der häufigsten Anfragen (z.B. zu CC-Lizenzen etc.) Kurzportraits der teilnehmenden Einrichtungen in Form von Vorträgen bei jedem Treffen Vernetzung und Kollaboration Übersicht der Helpdesks FAQ- Sammlung Vorstellung der Helpdesks Austausch über die Beratungsangebote und gegenseitige Unterstützung bei Herausforderungen Die Fokusgruppe entstand als Resultat eines Workshops des BMBF-Projekts „open-access. network“ zum Erfahrungsaustausch über den Aufbau und Betrieb von Open-Access- Helpdesks im November 2021. Die Gruppe umfasst derzeit 26 Mitglieder aus 20 verschiedenen Einrichtungen und trifft sich alle drei Monate. Für ihre Arbeit hat die Fokusgruppe zur internen Nutzung im Wiki der Fokusgruppen von open-access.network eine Übersicht von Open-Access-Helpdesks und -Beratungsange- boten angelegt. Bisher sind 21 Einträge ent- halten. In zukünftigen Treffen soll die Liste weiter ergänzt werden. Dieses Werk ist lizenziert unter einer Creative Commons Namensnennung 4.0 International Lizenz. https://open-access.network/vernetzen/digitale- fokusgruppen/fokusgruppe-open-access-helpdesks Ü b e rb lic k ü b e r d ie O A -B e ra tu n g s a n g e b o te u n d -H e lp d e s k s , d ie d e rz e it in d e r F o k u s g ru p p e o rg a n is ie rt s in d A n z a h l d e r E in trä g e U n iv e rs itä t F H P ro je k t L a n d e s v e rn e tz u n g s s te lle S o n s tig e E in ric h tu n g e n 0 2 4 6 8 1 0 1 2 1 4 1 6 Diese Veröffentlichung ist im Rahmen einer Fokusgruppe des Projekts open-access.network entstanden. Für den Inhalt sind allein die Autor*innen verantwortlich.


Follow the Lithium: The Correlation Between Li-bearing Molecules with Age, Mass, and Gravity in Brown Dwarfs Ehsan Gharib-Nezhad 1, Mark S. Marley 1, Natasha E. Batalha 1, Channon Visscher 2,3 (1) NASA Ames Research Center, Moffett Field, CA, USA (2) Dordt University, Sioux Center, IA, USA (3) Space Science Institute, Boulder, CO, USA Conclusion and Future Work The right figure is the Volume Mixing Ratios (VMR) of Li-bearing species as a function of temperature. Atomic Li and LiH are dominant species in (ultra-) hot atmospheres with Teff in ~1800-3000~K (e.g., M/L- type dwarfs). In warm atmospheres with Teff~900-1600~K (e.g., L/T-type dwarfs), LiOH, LiCl, and LiF are the most stable Li-bearing species. Historically the Li test, searching for the atomic Li line at 670 nm, has been used to distinguish early L-type brown dwarfs from stars, since Li is consumed by fusion processes for masses above 70 M_Jup (Baraffe2015, Charier1996). To better understand the presence and abundance of the different Li-bearing species in the temperature-pressure space, the Li phase diagram is represented in the left figure. In this plot, each species is shown with different colors. At each area, dashed and dotted contour lines represent 50% and 20% of that species with respect to the total protosolar lithium abundance (i.e., ~3.5x10-9) in the atmosphere. The solid black curves are the temperature-pressure (TP-) profiles of brown dwarfs from the Sonora-Bobcat cloud model created by Marley et al. (2021). The critical question is whether different Li species could serve as a tool to confirm massive ultracool objects. Li Chemistry in Brown Dwarfs Challenges with Accurate Determination of T-Y Dwarf Mass We investigate the impact of Li species on the synthetic thermal spectra of candidate T/L/M dwarfs using both cloud (Marley2021) and cloudless Sonora model (Marley2018) for Teff of 500- 2400~K and logg=5.0. The presence and the strength of their spectral features on synthetic flux spectra are assessed for different effective temperatures and surface gravities to see if they can productively be used as a high mass indicator in brown dwarfs. Ø The presence (FON) and absence (FOFF) of Li has the highest ([(FOFF) - (FON)] / FOFF) ratio, which is ~1 at the line center for Teff =2400 K, and it reduces to 0.2 for 500K. Ø LiF absorption feature is dominant at 10.5-12.5 µm. As it is predicted by thermochemical simulations, LiF mostly forms at 800-1200 K and competes with LiCl and LiOH molecules. The LiF ([(FOFF) - (FON)] / FOFF) ratio is ~10-4 for T-L type dwarfs with Teff of 900-1600 K. Ø In the range 1600K< Teff <2400K Li should be present as LiCl for masses below 70 MJup. The lack of LiCl at 14.5-18.5 µm would be an indicator of a larger mass. References and Contact Information Using LiF and LiCl to Disentangle this Age-Mass-Gravity Degeneracy Accurate calculation of the mass of ultracool dwarfs has been a serious challenge in understanding brown dwarfs. This uncertainty comes from the degeneracy in age, mass, and gravity parameters. Examples of T-L dwarfs with high uncertainty in their mass provided in the following table. Baraffe, I., Homeier, D., Allard, F., & Chabrier, G. 2015,A&A, 577, A42. Chabrier, G., Baraffe, I., & Plez, B. 1996, ApJ, 459. Marley, M. S., Saumon, D., Morley, C., et al. 2021 (Submitted) Marley, M. S., Saumon, D., Guillot, T., et al. 1996, Science,272, 1919. The traditional Li test can distinguish between low mass stars and brown dwarfs with similar spectral types. Although atomic Li still appears in model spectra down to Teff as low as 500K, this spectral region is exceedingly dark and difficult to measure. Instead, since LiF and LiCl features are located in regions where brown dwarfs are brighter, they could in principle be used as mass indicators at these lower effective temperatures. Ehsan.gharibnezhad@nasa.gov ehsangharibnezhad.github.io @ExoEhsan


References Chenu, C., Angers, D.A., Barré, P., Derrien, D., Arrouays, D., Balesdent, J., 2019. Increasing organic stocks in agricultural soils: Knowledge gaps and potential innovations. Soil and Tillage Research 188, 41-52. Elser, J., Bennett, E., 2011. Phosphorus cycle: a broken biogeochemical cycle. Nature 478, 29. Erisman, J.W., Sutton, M.A., Galloway, J., Klimont, Z., Winiwarter, W., 2008. How a century of ammonia synthesis changed the world. Nature Geoscience 1, 636. Hobley, E., Baldock, J., Hua, Q., Wilson, B., 2017. Land‐use contrasts reveal instability of subsoil organic carbon. Global change biology 23, 955-965. Hobley, E., Steffens, M., Bauke, S.L., Kögel-Knabner, I., 2018. Hotspots of soil organic carbon storage revealed by laboratory hyperspectral imaging. Scientific reports 8, 13900. Towards more efficient carbon, nitrogen and phosphorus cycling in European agricultural soils: Circular Agronomics (CA) program Yaser Ostovari1, Jan Willem Van Groenigen2, Rachel Creamer2, Julien Guigue1 ,Eleanor Hobley1, Laura Ferron2, Henk Martens2, Emily Overtuf1, Anke Neumeier1, Andreas Muskolus3, Paolo Mantovi4, Francesc Domingo Olivé5, Thomas Guggenberger6, Marek Holba7, Ingrid Kögel-Knabner1, Alix Vidal1 1TU München, Lehrstuhl für Bodenkunde, Freising, Germany, 2Wageningen University, Soil Biology Group, Wageningen, The Netherlands, 3Landwirtschaftliche Versuchsstation Berge, Berlin, Germany, 4Fondazione CRPA Studi Ricerche, Reggio Emilia, Italy, 5IRTA Mas Badia, Agricultural Experimental Station MasBadia, La Tallada d’Emporda, Spain, 6Höhere Bundeslehr- und Forschungsanstalt für Landwirtschaft Raumberg-Gumpenstein, Irdning, Austria, 7ASIO SPOL SRO, Brno, Czech Republic 1) CATALONIA, Spain (leader: IRTA) 2) BRANDENBURG, Germany (leader: IASP) 3) LUNGAU, Austria (leader: AREC) 4) EMILIA-ROMAGNA, Italy (leader: FCSR) 5) GELDERLAND, The Netherlands(leader: WUR) 6) SOUTH MORAVIA, Czech Republic (leader: ASIO) 1 2 3 4 5 6 Case Study Sites Material and methods Organic and inorganic amendments Different organic and inorganic amendments according to the case study. E.g., mineral fertilizer, pig slurry (solid or liquid fraction), manure, whey, biogas digestate, nitrogen-depleted digestate. Soil sampling for every case study Soil sampling to a depth of 1 m using a hydraulic corer. One un-disturbed half of the core for hyperspectral imaging The other half of the core for laboratory analyses. Five depths: 0-10 cm,10-20 cm, 20-40 cm, 40-80 cm and 80-100 cm. Laboratory analyses Classical bulk chemical analyses. E.g., bulk density, pH, CEC, texture, total and available C, N and P State-of the-art imaging technique: hyperspectral camera to reveal horspots of C and N storage in the soil profile (Hobley et al., 2018). A focus on hyperspectral soil analysis Introduction Mineral fertilizers: low recovery efficiency by crops. E.g., 30-50 % for nitrogen (N) and 45 % for phosphorus (P) (Tilman et al., 2002). Loss of nutrients into the environment : severe negative influence on soil (e.g. unbalanced N cycle), water (e.g., eutrophisation) and air (e.g., greenhouse gas emissions) (Elser and Bennett, 2011; Erisman et al., 2008). Less than 2% soil organic carbon (SOC) in 45% of European soils (Jones et al., 2012) and projected decline of agricultural SOC stocks of up to 24 % (Wiesmeier et al., 2016). Soil carbons stocks: not only topsoils, but also subsoils are reactive to agricultural change (Hobley et al., 2017). Impacts of organic amendments (e.g., digestate, manure) versus traditional mineral fertilizers on SOC contents and stocks are uncertain at the long-term (e.g., Chenu et al., 2019). Within the project Circular Agronomics - production of new organic fertilizers: residues (manure, digestate) treated with vacuum degasification for nitrogen depletion of residues and recovery of fertilizer. One of the objectives of Circular Agronomics Exploring medium and long-term effect of new organic fertilizers versus classical organic and mineral f


Global short wave solar radiation monitoring system GLOB Sebastian Dominik Sikora1), Anna Sjöblom Coulson1), Arthur Garreau1), Alex Klein-Paste2), Aleksey Shestov1), 1) Arctic Technology Department, UNIS The University Center in Svalbard, Svalbard, Norway 2)Department of Civil and Environmental Engineering, NTNU Norwegian University of Science and Technology, Trondheim, Norway The Arctic region presents numerous challenges for human presence, ranging from constructing on thawing permafrost to ensuring adequate food supplies. However, one of the most pressing challenges revolves around energy sources, encompassing both heat and electricity supply. Arctic settlements are typically considered off-grid systems, necessitating the development of systems of locally generated energy that are both reliable and sustainable. The goal of GLOB is to measure solar irradiation on as many as possible array planes to verify recorded values with modeled. Due to technical and costs limitations a sphere with 26 faces called rhombicuboctahedron has been pointed as most suitable for this project. The rhombicuboctahedron is a polyhedron comprised of 8 triangles and 18 squares. For this project, elements with edges measuring 10 cm for both squares and triangles have been constructed. The bottom-facing square element isn't utilized for irradiation data collection. This is because a stainless steel pipe has been employed as a support leg, passing through the bottom square and reaching the top face, which is horizontally oriented. All components required for building the rhombicuboctahedron have been meticulously designed using CAD software, and the corresponding files compatible with most 3D printers have been attached for your convenience. The elements created in CAD software used to assemble GLOB system SENSORS AND OTHER ELECTRONIC COMPONENTS Following components has been used to build complete system: 26 self-powered silicon-cell pyranometers type SP110, 1 temperature probe 107 manufactured by Campbell Sci., CR1000x logger, AM16/32B Multiplexer, CELL215 LTE modem, 7 Ah 12V battery, solar charging regulator, 20W photovoltaic module. The GLOB system view in spring (3/03/2023, https://doi.org/10.5281/zenodo.8410795) The GLOB system view in summer (30/06/2023, https://doi.org/10.5281/zenodo.8410805) The GLOB system view in autumn (5/10/2023, https://doi.org/10.5281/zenodo.8412962) Theoretical electricity (kWh) generated on 2 selected days (2/05/2023 and 6/07/2023) by a photovoltaic module with an area of 1 m2 (20% efficiency) directed in different azimuths and inclined at an angle of 0, 45, 90 or 135 degrees. Calculations based on data measured by GLOB 0 200 400 600 800 1000 00:00 04:00 08:00 12:00 16:00 20:00 GHI 00:00 04:00 08:00 12:00 16:00 20:00 S45 S90 S135 00:00 04:00 08:00 12:00 16:00 20:00 W45 W90 W135 00:00 04:00 08:00 12:00 16:00 20:00 NW45 NW90 NW135 00:00 04:00 08:00 12:00 16:00 20:00 N45 N90 N135 00:00 04:00 08:00 12:00 16:00 20:00 NE45 NE90 NE135 00:00 04:00 08:00 12:00 16:00 20:00 E45 E90 E135 00:00 04:00 08:00 12:00 16:00 20:00 SE45 SE90 SE135 00:00 04:00 08:00 12:00 16:00 20:00 SW45 SW90 SW135 AZIMUTH HORIZONTAL S S S SW SW SW W W W NW NW NW N N N NE NE NE E E E SE SE SE POA (deg) 0 45 90 135 45 90 135 45 90 135 45 90 135 45 90 135 45 90 135 45 90 135 45 90 135 02.05.2023 0,11 0,18 0,18 0,12 0,18 0,18 0,14 0,14 0,15 0,12 0,09 0,11 0,11 0,07 0,08 0,09 0,08 0,09 0,10 0,12 0,13 0,10 0,16 0,17 0,13 06.07.2023 0,17 0,19 0,15 0,06 0,18 0,15 0,09 0,18 0,15 0,08 0,16 0,15 0,11 0,15 0,15 0,09 0,16 0,15 0,12 0,18 0,15 0,08 0,18 0,16 0,09 Daily cycle of shortwave radiation (in W*m-2) received on various arrays planes, measured on May 2, 2023 by the GLOB system The GLOB system has been financed by the Svalbard Miljøvernfond: project 19/76 Scan QR code to see the full technical description of the system Sketch of the GLOB system (https://doi.org/10.5281/zenodo.8411391) Location of the GLOB system (https://toposvalbard.npolar.no/) CONTACT: Sebastian


Learning to correct for atmospheric seeing from solar observations John Armstrong and Lyndsay Fletcher University of Glasgow j.armstrong.2@research.gla.ac.uk 1. Introduction • Atmospheric seeing is ubiquitous in ground-based astronomy[1]. • We propose a post-processing correction for seeing using a machine learning algorithm known as generative adversarial network[2] (GAN). • This provides a kernel-free deblurring technique. • In models assuming some blur kernel explicitly it is hard to deal with occluded (optically thick) regions without a complex kernel estimation[9]. This is avoided in our model. Fig. 1: Discriminator[4,6] (D) Fig. 2: Generator[3,5] (G) References [1] Davies, R. and Kasper, M. (2012) Annual Reviews of Astronomy and Astrophysics, 50:350-351. [2] Goodfellow, I. et al. (2014). ArXiv e-prints. [3] Kupyn, O. et al. (2017). ArXiv e-prints. [4] Isola, P. et al. (2017). Proceedings – 30th IEEE Conference on Computer Vision and Pattern Recognition. [5] Lecun, Y. et al. (1998). Proceedings of the IEEE, 86(11):2278-2324. [6] Li, C. and Wand, M. (2016). Lecture Notes in Computer Science, 9907 LNCS:702-716. [7] Tsuneta, S. et al. (2008). Solar Physics, 249(2):167-196. [8] He, K. et al. (2015). ArXiv e-prints. [9] Nah, S. et al. (2016). ArXiv e-prints. Overview • We employ a post-processing machine learning algorithm to correct for atmospheric seeing. • The model is trained on data from SOT on Hinode which is imprinted with an artificial blur. • The model is then applied to data from CRISP with promising results. 2. Discriminator and Generator • There are two parts to a GAN: discriminator (D) and generator (G). • The goal of the generator is to fool the discriminator into thinking the data that it has created is real. • The discriminator wants to classify whether or not data is real. • The two play a game against each other and train simultaneously. D divides the generated and true images into 64, 128, 256, 512 segments, respectively (different colours represent the number of segments produced). D classifies each segment as real or fake. G learns the difference between the sharp and blurred image[8]. G adds what it has learnt to the blurry image for comparison with the sharp image. G reassembles the segments. 3. Blur Model Blur image via randomly offsetting the image w.r.t. itself twice and averaging. Fig. 3: SOT[7] image pre- and post-blurred 4. CRISP Ca II 8542ÅCorrection 5. Conclusion • Reconstructs lines well from CRISP data. • This shows that the image deblurring works perceptually and preserves spectral integrity. • This implies that the method can be used to correct for atmospheric seeing. Fig. 4: Correcting a CRISP observation of the 2014-09-06 flare. Blurry Sharp Corrected


Managing the Scientific Software Ecosystem with Spack Todd Gamblin*, Gregory Becker*, Kiel Friedt*, Alicia Klinvex†, Gregory L. Lee*, Matthew LeGendre*, Peter Scheibel*, Barry Smith‡, James Willenbring† *Lawrence Livermore National Laboratory †Sandia National Laboratories ‡Argonne National Laboratory Combinatorial software complexity Large scientific codes can be extremely complex ARES tcl tk scipy python cmake hpdf opclient boost zlib numpy bzip2 LAPACK gsl HDF5 gperftools papi GA bdivxml sgeos_xml Scallop rng perﬂib memusage timers Silo SAMRAI HYPRE matprop overlink qd LEOS MSlib Laser CRETIN tdf Cheetah DSD Teton Nuclear ASCLaser MPI ncurses sqlite readline openssl BLAS Physics Utility Math External Types of Packages Developers build 4 versions of ARES 36 different ways. Linux BG/Q Cray XE6 MVAPICH MVAPICH2 OpenMPI BG/Q MPI Cray MPI GCC C P L D C P L D Intel 14 C P L D Intel 15 C P L D D PGI D C P L D C L D Clang C P L D C L D XL C P L D Dependency graph for one configuration of ARES, an LLNL multi-physics code. (L)ite (D)evelopment spack/opt/ linux-x86_64/ gcc-4.7.2/ mpileaks-1.1-0f54bf34cadk/ intel-14.1/ hdf5-1.8.15-lkf14aq3nqiz/ bgq/ xl-12.1/ hdf5-1-8.16-fqb3a15abrwx/ ... mpileaks mpi callpath dyninst libdwarf libelf Hash Spack can install arbitrarily many configurations of each package https://spack.io github/LLNL/spack @spackpm Spack has a rapidly growing open source community Spec syntax lets users build on demand –Build scientific software from source for best performance & portability across exotic platforms –Automate deployment for app developers, facility staff, and users –Provide integration testing harness for large software stacks. –No more manual builds: spack install <package> Done. –Build a community; leverage build automation work across facilities & teams Spack is a flexible, build-from-source package manager for scientific software that supports multiple versions, compilers, and configurations. Overview and Goals $ spack install mpileaks unconstrained $ spack install mpileaks@3.3 @ custom version $ spack install mpileaks@3.3 %gcc@4.7.3 % custom compiler $ spack install mpileaks@3.3 %gcc@4.7.3 +threads +/- build option $ spack install mpileaks@3.3 cppflags=‘-O3’ setting compiler flags $ spack install mpileaks@3.3 os=CNL10 target=haswell setting target for cross-compile $ spack install mpileaks@3.3 ^mpich@3.2 %gcc@4.9.3 ^ constraints on dependencies `spack fiind` shows what is installed. $ spack find ==> 103 installed packages. -- linux-x86_64 / gcc@4.4.7 -------------------------------- ImageMagick@6.8.9-10 glib@2.42.1 libtiff@4.0.3 pango@1.36.8 qt@4.8.6 SAMRAI@3.9.1 graphlib@2.0.0 libtool@2.4.2 parmetis@4.0.3 qt@5.4.0 adept-utils@1.0 gtkplus@2.24.25 libxcb@1.11 pixman@0.32.6 ravel@1.0.0 atk@2.14.0 harfbuzz@0.9.37 libxml2@2.9.2 py-dateutil@2.4.0 readline@6.3 boost@1.55.0 hdf5@1.8.13 llvm@3.0 py-ipython@2.3.1 scotch@6.0.3 callpath@1.0.2 jpeg@9a mpich@3.0.4 py-numpy@1.9.1 stat@2.1.0 dyninst@8.1.2 libdwarf@20130729 ncurses@5.9 py-pytz@2014.10 xz@5.2.0 -- linux-x86_64 / gcc@4.8.2 -------------------------------- adept-utils@1.0.1 boost@1.55.0 cmake@5.6-special libdwarf@20130729 mpich@3.0.4 adept-utils@1.0.1 cmake@5.6 dyninst@8.1.2 libelf@0.8.13 openmpi@1.8.2 -- linux-x86_64 / intel@14.0.2 ----------------------------- hwloc@1.9 mpich@3.0.4 starpu@1.1.4 -- linux-x86_64 / intel@15.0.0 ----------------------------- adept-utils@1.0.1 boost@1.55.0 libdwarf@20130729 libelf@0.8.13 mpich@3.0.4 -- linux-x86_64 / intel@15.0.1 ----------------------------- adept-utils@1.0.1 callpath@1.0.2 libdwarf@20130729 mpich@3.0.4 boost@1.55.0 hwloc@1.9 libelf@0.8.13 starpu@1.1.4 $ spack find callpath ==> 2 installed packages. -- linux-x86_64 / clang@3.4 ———————— -- linux-x86_64 / gcc@4.9.2 ------------- callpath@1.0.2 callpath@1.0.2 $ spack find -dl callpath ==> 2 installed packages. -- linux-x86_64 / clang@3.4 ----------- -- linux-x86_64 / gcc@4.9.2 --------- -- xv2clz2 callpath@1.0.2 udltshs callpath@1.0.2 ckjazss ^adept-utils@1.0


MEASUREMENT OF THE UNDERGROUND ARGON RADIOPURITY FOR DARK MATTER DIRECT SEARCHES Ludovico Luzzi (CIEMAT) on behalf of DarkSide Collaboration • C.E. Aalseth et al. 2020 JINST 15 P02024 (Feb. 2020) LOW RADIOACTIVITY UAr FOR DARKSIDE-20K DARKSIDE-20K EXPERIMENT AND UNDERGROUND ARGON DS-20k aims to <0.1 background events except coherent neutrino scatters after all TPC & veto event selection criteria in ROI (20-200 keVnr) within 20.2 t fiducial volume during 10 y run. Liquid argon is used as active medium because of its scintillation and ionization characteristics. DarkSide-20k (DS-20k) is a two- phase liquid argon detector, under construction at LNGS. DArT is a small low-background detector designed to measure the 𝟑𝟗𝐀𝐫 depletion factor of different UAr batches (URANIA + ARIA): OFHC Cu cylinder, 1 l active volume, PMMA support structure with TPB coating, Readout two PDMs (1 cm² SiPMs) from DS-20k (DArTeyes). Located at LSC (1400 m.w.e.) will be installed inside ArDM single-phase: • 13 PMTs will see ~1 tonne AAr buffer used as shield and veto • New Pb-shield attached to existing Polyethilene shield • Substitution of AAr bath by pressurized LN2 @ 85 K. No veto • Installation in an ad-hoc Pb-castle flushed with Rn-free air (undergorund only) DArT IN ArDM: PRESENT AND FUTURE DArT: FROM CIEMAT TO LSC Why Argon? Underground argon (UAr), depleted of 𝟑𝟗𝐀𝐫 Future Ar-based experiments (DarkSide-20k, Argo) will use UAr. Main limitation Intrinsic activity of 𝟑𝟗𝐀𝐫in atmospheric argon (via spallation of cosmic rays on 𝟒𝟎𝐀𝐫): • beta decay with Qβ = 565 keV • t1/2 = 269 y • ~1 Bq/kg • Procurement of 50 tonnes of UAr from the Kinder- Morgan facility in Cortez (Colorado, USA) • Extraction of 330 kg/day, with 99.9% purity • UAr transported to Sardinia for final chemical purification at Aria The Aria and Urania projects are two fundamental steps in order to provide tonnes of detector-grade UAr. • Big cryogenic distillation column in Seruci, Sardinia • Final chemical purification of the UAr • Can process O(1 tonne/day) with 10³ reduction of all chemical impurities • Ultimate goal is to isotopically separate 𝟑𝟗𝐀𝐫from 𝟒𝟎𝐀𝐫 (at the rate of 10 kg/day in Seruci II) Urania Aria 350 m Seruci-I Seruci-II Specific setup for tests in surface (CIEMAT) and undeground (LSC): With all that it is clearly seen the 39Ar on top of the background, assuming a featureless línear background and considering a threshold of 33 keV it is possible to measure 1.0 cps. No uncertainty is quoted here because an understanding of the systematics is still ongoing. Bibliography Two events from the present setup of DArT are showed. From the difference between α decay (top) and β decay (bottom) Pulse Shape Discrimination (PSD) is performed and electron recoil events can be isolated. Comparing everything from surface to underground with lead shield, a reduction of the background is observed. Once adding the lead shield (black) the background is significantly reduced and the 39Ar β spectrum for low • arXiv:1707.08145v1 [physics.ins-det] 25 Jul 2017 PRELIMINARY For tests only AAr is used. The triplet lifetime is very long (1230 ns) because of the slower SiPM response: 𝐟𝟔𝟒𝟎is defined so the signal is integrated in the first 640 ns to define the fast component of the pulse energies is visible.


2 3 4 If I look at myself in the CP mirror I just see myself! All measurements are in agreement with the SM prediction within 68% CL. A CP odd state is excluded at 99.7% CL (3.0 σ) ● Exclusion for CP-odd hypothesis:  Observed (exp.) significance = 3.0σ (2.6σ)  ϕCP distribution in bins of NN score Investigated τ decay channels The τh are identified with the DeepTau NN-based ID2 Decay modes identified with MVA-algorithm3 τ + τ − The cross-section of the H→ττ process has a sinusoidal shape d σ d ϕCP ∝const −cos(ϕCP−2α H τ τ) The Higgs through the looking glass. Measurement of the CP quantum number of the Higgs boson in H→ττ decays Andrea Cardini (DESY) on behalf of the CMS collaboration CP-violation in the Higgs couplings is investigated in: ● HVV couplings ●Yukawa coupling: ●Production via ttH and ggH ●Decays into τ leptons The Standard Model predicts that I have spin-parity 0+ But do I? Better check with a CP mirror We invert spatial coordinates and swap particles with anti-particles 1 2 Multicategory classification used to identify the Higgs decays from genuine ττ and lep./jet→τh backgrounds: ●BDT for fully hadronic channels ●Neural Network for semileptonic Signal parametrized as function of αHττ: weighted combination of CP even odd and maximum mixing cases ~ 90% of background estimated with data-driven methods ●Tau embedding for genuine ττ processes ●FF method for j→τh fakes NN MACHINE LEARNING BDT Likelihood profiled1 with respect to: 1. CP mixing angle 2. Yukawa couplings 3. CP mixing angle + inclusive Higgs production signal strength 4. Higgs production signal strengths (ggH + VBF) 5. CP mixing angle for Run 2, Run 3 and HL-LHC 5 3 Each decay plane is defined by two vectors4: a momentum and a reference vector CP even αΗττ= 0° CP mix αΗττ= 45° CP odd αΗττ= 90° Machine learning techniques can help in identifying me At the LHC I am surrounded by processes that can produce similar signatures to my decays to τ leptons CP mixing angle Acoplanarity angle a1(1260) ρ(770) The spin correlation is preserved for decays to leptons and via mesonic resonances pion momentum impact parameter (IP) polarimeter vector (h) References. 1. CMS-HIG-20-006: “Analysis of the CP structure of the Yukawa coupling between the Higgs boson and τ leptons in proton-proton collisions at √s= 13 TeV” 2. CMS-DP-2019-033: “Performance of the DeepTau algorithm for the discrimination of taus against jets, electron, and muons” 3. CMS-DP-2020-041: “Identification of hadronic tau decay channels using multivariate analysis (MVA decay mode)” 4. Andrea Cardini: “Measurement of the CP properties of the Higgs boson in its decays to τ leptons with the CMS experiment” 2 4 1 3 4 6 CP mixing angle measured with simultaneous fit for signal and background models over full Run 2 Fit performed with ●NN/BDT score for ML background categories ●Acoplanarity angle distributions in bins of NN/BDT score for higgs category → split by decay mode To be continued in Run 3 Uncertainty statistically dominated 1 5 7 d σ d ϕCP


> Programm Heeremannscher Hof · Hofsaal im Erdgeschoss Königsstraße 47 48143 Münster > Wozu berechtigt Not? Workshop der Kolleg-Forschergruppe 8. April 2014 > Veranstaltungsort Sebastian Laukötter und Reinold Schmücker Kolleg-Forschergruppe „Normenbegründung in Medizinethik und Biopolitik“ Die Zahl der Teilnehmer ist begrenzt. Wir bitten daher um Anmeldung unter: normenbegruendung@wwu.de www.normenbegruendung-in-der-bioethik.de > Organisation Bildnachweis: Stefan Klatt. 9:30 Begrüßung 9:45 – 10:35 Wozu berechtigt Not? Zur Notwendigkeit und Möglichkeit einer Ethik für Notsituationen Reinold Schmücker (Münster) 10:35 – 11:25 Moralisch retten Guntolf Herzberg (Berlin) 11:55 – 12:45 Notsituationen als Herausforderung an die Moralphilosophie. Grundsätzliche Überlegungen über Möglichkeiten und Grenzen der Ethik Héctor Wittwer (Berlin) 15:00 – 15:50 Not und die Grenzen der Moral Simon Derpmann (Münster) 15:50 – 16:40 ‚Handeln aus Not‘. Moralphilosophische Implikationen eines durchaus gewöhnlichen Sprachspiels Anke Thyen (Ludwigsburg) 17:10 – 18:00 Wozu verpﬂ ichtet Not? Überlegungen zum Status globaler Hilfspﬂ ichten Sebastian Laukötter (Münster)


Abstract Experimental Experimental H. S. Medeiros1, R. S. Pessoa1, 2, J. C. Sagás1, M. A. Fraga1,3, *, L. V. Santos1,2, H. S. Maciel1,2, M. Massi1 and A. S. da Silva Sobrinho1 References References Results Results Acknowledgments Acknowledgments Conclusions Conclusions 1Plasma and Processes Laboratory, Technological Institute of Aeronautics, 12228-900, S. J. dos Campos, SP, Brazil 2IP&D, University of Vale do Paraíba, 12244-000, S. J. dos Campos, SP, Brazil 3Institute for Advanced Studies, IEAv-DCTA, 12228-001, S. J. dos Campos, Brazil SixCy thin films deposited at low temperature by dual DC magnetron sputtering: Effect of power supplied to Si and C cathode targets on film physicochemical properties A DC dual magnetron sputtering system with graphite (C) and silicon (Si) targets was used to grow stoichiometric and non-stoichiometric silicon carbide (SixCy) thin films at low temperature. Two independently DC power sources were used to enable the total discharge power be shared, under certain proportions, between the Si and C magnetron cathodes. The motivation was to control the sputtering rate of each target so as to vary the stoichiometric ratio x/y of the deposited films. The species content, thickness and chemical bonds of as-deposited SixCy films were studied by Rutherford backscattering spectroscopy (RBS), profilometry, Fourier transform infrared absorption (FTIR) and Raman spectroscopy respectively. Overall, the present work reveals a new reliable plasma sputtering technique for low temperature growth of amorphous SixCy thin films with the capability of tuning the degree of formation of a-SiC, a-Si and a-C bonds in the film bulk. 0 1000 2000 3000 4000 5000 Si Si-O-Si and/or Si-O-C Si-C 45% 50% 40% 30% 0% Transmissمo (a.u) Numero de onda (cm -1) 20% 100 200 300 400 Channel 0 1 2 3 4 5 6 Yield (#/uC/keV/msr)1/2 0.5 1.0 1.5 2.0 Energy (MeV) Si C N O mafraga@ita.br Carbon Target Silicon Target Shutter Substrate holder Vacuum System Gas Line Deposition Chamber DC Power Source Gas Injection System (b) Figure 1. Photograph of the magnetron co-sputtering deposition system. 4.a) FTIR RBS 4.b) Profilometry 60% C target %Si=39,81 %C=38,89 0 1000 2000 3000 4000 5000 Si Si-C Si-O-Si and/or Si-O-C 100% 80% 70% 60% 55% 50% Transmissمo (a.u) Numero de onda (cm -1) (a) 0 10 20 30 40 50 60 70 80 90 100 0,1 1 10 C/Si % de potência no alvo de carbono teorico experimental 63% stoichiometry (a) 0 20 40 60 80 100 0 100 200 300 400 500 600 700 Vc Ic Vsi Isi (b) Corrente no alvo, IX (mA) Tensمo da discarga, Vdc (V) % de potência no alvo de carbono 0 100 200 300 400 500 600 700 Electrical Raman 400 600 800 1000 1200 1400 1600 1800 2000 0 20 40 60 80 100 120 140 160 70% C target Raman shift (cm -1) Intensidade (a.u.) (d) 400 600 800 1000 1200 1400 1600 1800 2000 0 50 100 150 200 250 300 350 400 80% C target Raman shift (cm -1) Intensidade(a.u.) (e) 400 600 800 1000 1200 1400 1600 1800 2000 0 10 20 30 40 Intensidade (a.u.) Raman shift (cm -1) 20% C target (a) SiC (TO) SiC (LO) 400 600 800 1000 1200 1400 1600 1800 2000 0 10 20 30 40 50 60 70 80 60% C target Raman shift (cm -1) Intensidade (a.u.) (c) SiC (TO) SiC (LO) 400 600 800 1000 1200 1400 1600 1800 2000 10 15 20 25 30 35 40 (b) Raman shift (cm -1) 45% C target Intensidade (a.u.) SiC (TO) SiC (LO) i. Fig. 1 and Fig. 2 show photographs and the scheme of the magnetron co-sputtering deposition arrangement used. ii. The magnetrons are disposed in parallel and angled at approximately 20º from the central axis (see Fig. 2). iii. The targets of the magnetron are made of carbon and silicon, both of high purity (99.99%). iv. As sputtering gas was used argon. The pressure was maintained fixed at 5.0 mTorr and the Ar flow rate at 10 sccm. v. The films were deposited varying the fraction of applied power in each magnetron target for a total value of 200 W. vi. RBS, FTIR, Raman and profilometry techniques were utilized to investigate film composition, chemical bonding and deposition rate, respectively. Figure


This project has received funding from the European Union's Horizon 2020 research and innovation programme under grant agreement No 952439. STELLAR : a EU twinning project on LOFAR data analysis and knowledge transfer Abstract: The Scientiﬁc and Technological Excellence by Leveraging LOFAR Advancements in Radio Astronomy (STELLAR) is a project of mutual collaboration and know-how transfer in the ﬁeld of radio astronomy, solar physics and space weather using the LOFAR instrument and data. Two institutions from Bulgaria, beneﬁt from technical and scientiﬁc know-how exchange from world-leading RA institutions - ASTRON (the Netherlands) and DIAS (Ireland) via series of training hands-on sessions, workshops, seminars and project-focused schools for both students and senior staff. The poster presents the activities so far and future plans. All results, links to videos and outreach activities are hosted at a dedicated web-site. The STELLAR project is funded by the European Union's Horizon 2020 research and innovation programme under grant agreement No 952439. It is coordinated by the Institute of Astronomy, Bulgarian Academy of Sciences. A. Antonova(1) , К. Kozarev(1), A. Avramova-Boncheva(1), R. Miteva(1), M. Dechev(1), P. Zucca(2), E. Carley(3), S. Maloney(3), P. Petkov(4) Afﬁliations: (1) Institute of Astronomy and National Astronomical Observatory, Bulgarian Academy of Sciences, Bulgaria; (2) ASTRON, the Netherlands; (3) DIAS, Ireland; (4) Technical University of Soﬁa, Bulgaria General Information: • Call: H2020- WIDESPREAD-2018-2020, Twinning topic • EU Grant: 899 877 EUR • Duration: 36 months • Start Date: 01 September, 2020 Highlights Period 1: Online courses freely available at https://stellar-h2020.eu/ : ASTRON Training I on RF Technology and RF Development I; Space Weather Training I - Introduction to Space Weather at DIAS; ASTRON Training I on RF Technology and RF Development; ASTRON Training II on Phased Array Digital Signal Processing. Online seminars also freely available at https://stellar-h2020.eu/ Other activities: LOFAR Data School Staff Visits to ASTRON (LOFAR Operations and Science, Data reduction) Staff Visit I and II to DIAS (Space Weather Data Analysis) STELLAR Consortium Members: • IANAO (https://astro.bas.bg/) • TUS (http://www.tu-sofia.bg/) • ASTRON (https://www.astron.nl/) • DIAS (https://www.dias.ie/) Visit to ASTRON RF school at TUS, Soﬁa Visit to the LOFAR core stations Visit to Westerbork Visit to the LOFAR-IE station Visit to the LOFAR-IE station Synergistic Activity: the LOFAR-BG Project (https://lofar.bg/) • The consortium at present: IANAO, TU, SU, SHU • Included in the Bulgarian National Roadmap for Science Infrastructures (Ministry of Education and Science of Bulgaria) • Received funding for building and maintaining LOFAR station • Site selected (close to the Rozhen Observatory), RF checked and approved STELLAR objectives: •To transfer scientific and technical knowledge and capacity in radio astronomy from the highly experienced staff in ASTRON and DIAS to IANAO and TUS staff by means of versatile training activities; •To expand the research potential of the local solar and space weather scientists through a combi- nation of target training activities and research discussions and collaborations using LOFAR observa- tions; •To provide an opportunity for IANAO and TUS scientific and engineering personnel to build the necessary expertise and technical capabilities required for the building and operation of a Bulgarian LOFAR station


SET CoP Aims: To provide an opportunity to share, reflect on, evaluate and develop the team’s practice To provide a platform for the showcasing and discussion of good practice To provide a showcase for new and innovative teaching and learning development practices To foster collaborative practices amongst the members of the Student Engagement Team Advantages: “Having a regular opportunity to get together means we can adapt things fairly quickly and suggest changes if needed” “Provides a safe space for discussing practice and a valuable informal meet-up” “I could be open and honest about arising issues / concerns with systems / expectations etc.” “The team could provide reassurance and support which was invaluable” “Supports a culture of collaboration, trust and respect” “The SET CoP is friendly and supportive” “It’s reassuring to be able to bring questions or ideas to the group and know that they will be listened to and discussed” “Useful conversations - I like that the atmosphere is generally informal” Challenges: “Not everyone is always present, the time and date doesn’t always suit all - particularly for part-time members of the team” “One member of the team had to travel a long distance to attend, which was not ideal” “Trying to convene CoP meetings over the summer when people were taking holidays. Due to the small size of our team, it proved difficult to get enough people to make it viable during this period” “The SET CoP is a forum for discussion about the provision of academic writing and information literacy support.” Contribution to the provision of student Academic Writing support: Highlighting current issues during 1:1s Sharing/applying training attended Discussing student/tutor feedback Disseminating exemplars and discussing how we support students with those assignments What next? As ASAs we believe SET CoP brings many advantages to our day-to-day role, but how do we know for sure a CoP has an impact on the quality of student academic support? Can we measure this? And if so, how? This is perhaps something to consider at future SET CoP meetings. Contact Us... Claire Olson olsonc@edgehill.ac.uk Andrew Tomkins tomkinsa@edgehill.ac.uk Scan the QR code: Tell us what you think. Have you ever been part of a CoP? We would love to hear about any of your experiences, or provide feedback on this poster. The establishment of a Community of Practice (CoP) to improve student academic support Further reading Cox, A., 2005. What are communities of practice? A comparative review of four seminal works. Journal of Information Science [online]. 31 (6), pp. 527-540. Available from: https://doi.org/10.1177/0165551505057016. Gómez, R.L. and Suárex, A.M., 2021. Extending impact beyond the community: Protocol for a scoping review of evidence of the impact of communities of practice on teaching and learning in higher education. International Journal of Educational Research Open [online]. 2, 100048. Available from: https://doi.org/10.1016/j.ijedro.2021.100048. Lesser, E.L. and Storck, J., 2001. Communities of practice and organizational performance. IBM Systems Journal [online]. 40 (4), pp. 831-841. Available from: https://doi.org/10.1147/sj.404.0831. Wenger, E., 1998. Communities of practice: Learning, meaning and identity. Cambridge: Cambridge University Press. Wenger, E., 2011. Communities of practice: a brief introduction. In: STEP Leadership Workshop, 20 October 2011, Eugene, OR [online]. Eugene: University of Oregon. Available from: https://scholarsbank.uoregon.edu/xmlui/handle/1794/11736 [Accessed 24 March 2022]. UniSkills Edge Hill University - Student Engagement Team Student Engagement Team Community of Practice:  The Student Engagement Team Community of Practice (SET CoP) was formed in April 2019  The SET CoP currently consists of seven Academic Skills Advisors (ASAs), who meet every six weeks  The meetings are minuted and report to the Student Engagement Team meeting  There is a rolling chair  Most meetings take place off ca


What Can Joint Survey Processing (JSP) do for Time-Domain Studies? Ranga Ram Chary (Caltech/IPAC) for the JSP Team rchary@caltech.edu; Feb 2022 Abstract Joint Survey Processing (JSP) is the pixel level combination of ground- and space-based datasets such as Euclid (2023+), Rubin (2023+) and Roman (2027+). It is particularly important for mitigating source confusion which affects 50% of the sources in deep seeing-limited datasets such as those that will be taken by Rubin/LSST. By using location and morphology priors on static sources derived from space-datasets such as Euclid and Roman, and estimating accurate time- and location-dependent point spread functions for the ground- based data, one can model the scene in individual frames forward. The residuals after subtracting the modeled scene from the data, reveal transient events down to the shot noise limit of the individual images or in time- integrated coadds, even in crowded fields. This significantly improves the detectability of transient events, both in number and in faintness. JSP is therefore highly relevant for 1. detection of microlensing events, 2. moving objects like nearby stars and asteroids, 3. supernovae, and 4. tidal disruption events close to the high surface brightness centers of galaxies. In addition, by providing accurate multi-band photometry on galaxies one can derive accurate photometric redshifts and galaxy physical parameters which can be used to select host galaxies and transient electromagnetic counterparts for multi-messenger studies such as those where the positional error circles can be large (e.g. LIGO gravitational wave events, ultra high-energy cosmic rays or fast radio bursts). Figure 1: Map of the entire sky (from J-C. Cuillandre) in celestial coordinates showing the Euclid coverage (15000 sq-deg in yellow), and the Rubin coverage (20000 sq-deg) as the colored rectangles. There are also 3 deep fields totaling 40 sq-deg – two in the South and one in the North. Opportunities for time domain science come from the 7500 sq- deg overlap area which will have deep multi-wavelength optical and NIR data with sub- arcsecond resolution, and the 30 sq-deg high latitude deep fields in the South. In 2027+, the Roman microlensing survey towards the Galactic bulge, a potential Roman Galactic Plane survey and 15 sq-deg SN survey will also provide new opportunities to search for variable events. Figure 2: 5-year sensitivity of the Rubin/LSST ugrizy survey (blue) in comparison with the Euclid deep field sensitivities (green). Potentially the LSST deep drilling fields will be another 2.5 mags deeper than that shown while the Euclid wide field will be 2 mags shallower. The Euclid deep fields will have about 20 visits while the LSST area will have about ~100 visits. Figure 3: The blended fraction of sources in seeing-limited data (Rubin) as a function of apparent magnitude, in extragalactic fields. In the deep fields, more than half the sources are blended with other nearby sources. Combined with variable Rubin seeing, measuring variability in these faint sources is challenging. Forward modeling the scene using the high resolution space data (from Euclid or Roman), enables the detection of transients down to the shot noise limit of the surveys. Figure 4: An illustration of joint survey processing on Hubble/ACS and Subaru/HSC data from Faisst et al. (2022). By using priors on the position and morphologies of sources derived from the high resolution ACS data and fitting for these known sources in the HSC/Subaru data, faint transients which are on top of host galaxies (e.g. SNe or nuclear AGN) can be detected. This method also can help reveal moving objects like stars or asteroids if the time baseline is large enough. Summary The detection of variable sources at the sensitivity limit of upcoming, confusion-limited ground-based surveys requires forward modeling of the scene by using priors from the high resolution space-platform data. This requires joint pixel level pr


OBSERVATIONAL PROPERTIES OF PUFFY ACCRETION DISC ABSTRACT We have performed a general rela/vis/c radia/ve magnetohydrodynamics (GRRMHD) simula/ons of a stable accre/on disc around a stellar-mass black hole (BH) with sub-Eddington mass accre/on rates. The numerical solu/ons revealed an elevated ver/cal structure - above a dense geometrically thin core of dimensionless thickness ℎ!/𝑟∼0.1, resembling a classic thin accre/on disc, a puﬀed-up, op/cally and geometrically thick layer of lower density and ℎ"/𝑟∼ 1.0 is formed. We refer to this solu/on as the Puﬀy disc. We discuss the observa/onal proper/es of a puﬀy discs, in par/cular the geometrical obscura/on at higher observing inclina/ons of the inner area by the puﬀed-up region, and collima/on of radia/on along the accre/on disc spin axis. These eﬀects may explain the apparent super-Eddington luminosity of some ultraluminous X-ray binaries. We also present synthe/c spectra of puﬀy discs, and show that they are qualita/vely similar to Comptonized thin disc spectra. We demonstrate that the exis/ng XSPEC spectral models provide good ﬁts to synthe/c spectra of puﬀy discs but cannot correctly recover the input luminosity, nor the black hole spin. We suggest that puﬀy discs may correspond to X-ray binary systems in the intermediate spectral state with luminosi/es above 0.3 of the Eddington luminosity. Debora Lančová1, Maciek Wielgus2,5, Odele Straub3, Włodek Kluźniak4, Ramesh Narayan5, David Abarca4, Gabriel Török1 and Marek Abramowicz1,4 KORAL CODE The simula*ons were performed using GRRMHD code KORAL (Sądowski et al. 2013a, 2014a), a ﬁnite-diﬀerence Godunov type code solving coevolu*on of gas, radia*on and magne*c ﬁeld in an arbitrary metric. Coupling of gas and radia*on is solved semi-implicitly using M1 closure scheme. We obtain in total 30 mil. corehours on Polish supercomputer Prometheus, part of the PLgrid infrastructure. This computa*onal resources enables us to run a number of simula*ons with diﬀerent ini*al condi*ons to obtain three simula*ons with diﬀerent mass accre*on rates. 1Ins*tute of Physics, Silesian University in Opava, Czech Republic 2Max-Planck-Ins*tut für Radioastronomie, Germany 3ORIGINS Excellence Cluster, Germany 4Nicolaus Copernicus Astronomical Centre, Polish Academy of Sciences, Poland 5Black Hole Ini*a*ve at Harvard University, USA We are studying a mildly sub-Eddington accre*on onto a non-rota*ng stellar mass BH with a mildly sub- Eddintgon accre*on rate. The classical models of accre*on discs repor*ng a thermal and viscous instability in this regime, however, our solu*on is stable thanks to the strong ver*cal net ﬂux of magne*c ﬁeld. The magne*c pressure inside the disc is at the same order as the radia*on pressure, both strongly dominates over the gas pressure. This also cause the accre*on disk to be “puﬀy” - with geometrically thin dense core (1) and geometrically and op*cally thick turbulent puﬀy region (2). Although the core resembles a standard thin disc, the op*cally thick puﬀy region and the posi*on of the photosphere has a strong inﬂuence on the observa*onal proper*es and thus the disc observa*onal appearance is very diﬀerent from a standard models. On the ﬁgure, the thick white line denotes the posi*on of the photosphere, while the dashed line is the density scale-height. The color contours are showing the gas temperature. 2 1 OBSERVATIONAL APPEARANCE Radia*on from the disk is beamed to the direc*on of the axis and obscured for viewing angles close to the equatorial plane, in contrast with the standard thin disc model. The inner parts of the disc and the central BH is completely hidden from observers with high inclina*on. At the same *me for low inclina*on observer the disc radiates all the way to the BH horizon, leaving no trace of the innermost stable circular orbit. Three columns on the le` are showing the picture of a puﬀy disk for three diﬀerent mass-accre*on rate compared to the 0.6 ̇𝑀#$$ standard thin disc image in the right column, with i


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


Dependence of IR-Bright AGN Activity on Halo Mass and Redshift in the SPT Cluster Surveys Benjamin Floyd B 1 Mark Brodwin 1 Rebecca E. A. Canning 2 The SPT Collaboration 1University of Missouri–Kansas City 2University of Portsmouth Motivation We know that environment plays a role in galaxy evolution (e.g., Dressler, 1980, 1984), but how exactly? What are the predominant environmental-dependent mechanisms that are behind the rapid mass assembly (Mancone et al., 2010), en- hanced star formation (Brodwin et al., 2013) and increased AGN activity (Martini et al., 2013) that has been observed in galaxy clusters at high-redshift (z ≳1.4). Independently both Brodwin et al. (2013) and Ehlert et al. (2015) arrived at sim- ilar conclusions that galaxy–galaxy merging within the clusters may be the mechanisms driving galaxy evolution in galaxy clusters early in their history. In sufficiently gas-rich galaxy–galaxy merging, the gas will be dynamically disrupted triggering both enhanced star-formation activity and allows for gas to funnel into the galactic nucleus and accrete onto the central supermassive black hole creating an AGN. Similar to Ehlert et al. (2015), we aim to model the AGN incidence in galaxy clusters as tracers of galaxy evolution of the cluster members. SPT Cluster Sample Our cluster sample derives from two galaxy cluster surveys carried out by the 10-meter South Pole Telescope (SPT; Carlstrom et al., 2011) the 2500 deg2 SPT-SZ survey (Bleem et al., 2015) and the deep, 100 deg2 SPTpol 100d survey (Huang et al., 2020). Combined we have a cluster sample of over 300 clusters with a median redshift of z ∼0.69 and median cluster mass of M500 ∼3.73 × 1014M⊙. By using the SPT cluster surveys we are able to span a wide range of redshifts (see Fig 1.) and as the SPT detects clusters using the Sunyaev–Zel’dovich Effect (SZE) we have an effectively uniform-selected mass sample. Figure 1. Mass and redshift distribution of the SPT cluster surveys. IR-Bright AGN Selection Our AGN are selected using Spitzer/IRAC imaging in 3.6 µm and 4.5 µm wavelengths. We find a color selection of [3.6 µm]− [4.5 µm] ≥0.7 to be optimal in selecting AGN that would have been otherwise selected by a IRAC color-color selection (e.g., Stern et al., 2005) as shown in Figure 2. Furthermore, to account for Eddington bias in the form of photometric uncertainty we employ a fuzzy membership selection to our data in order to create the final sample as seen in Figure 3. Using our selection criteria, we select ∼2200 AGN candidates. 0.0 0.2 0.4 0.6 0.8 1.0 1.2 1.4 1.6 Photometric Redshift 0.0 0.2 0.4 0.6 0.8 1.0 1.2 1.4 [3.6] - [4.5] (Vega) Stern Wedge AGN Non-Active Galaxies 0.0 1.0 2.0 3.0 4.0 5.0 6.0 7.0 8.0 9.0 Lookback Time (Gyr) 101 103 N Figure 2. IRAC colors of all objects in the Spitzer Deep Wide-Field Survey (SDWFS; Ashby, Stern, et al., 2009) detected in 4.5 µm with SNR ≥5. Red points are objects that satisfy the AGN selection criterion as described in Stern et al. (2005). Blue hexbins are SDWFS objects that do not fall within the Stern wedge criterion. Our IRAC color selection is shown as the solid black line. 0.25 0.00 0.25 0.50 0.75 1.00 1.25 1.50 [3.6 m] - [4.5 m] (Vega) Original: = 0.89, = 0.15 Corrected: = 0.72, = 0.12 Degree of Membership = 0.56 SDWFS Number Counts Figure 3. Example of applying our Eddington bias correction and computing degrees of membership into our AGN sample. The original color and color error of the object is assumed to form a Normal distribution as given by the dashed curve which is then convolved with the deeper SDWFS number count distribution to account for Eddington bias. The object’s degree of membership into our sample is given by the integral of the corrected color (solid curve) above our cut off. Preliminary Trends Preliminary analysis on the our data sample and has found some initial interesting trends such as indications of an inverse trend of AGN richness with cluster mass at a fixed redshift as can be seen in Figure 4.


Grant applicants Open science is a priority for Kim, she only has a short publication list. She uses pre-registrations and shares her pre-prints, peer-review. She works together in an electronic notebook and afterwards shares the metadata, datasets and protocols in trusted repositories. Publishing in journals with a high impact factor is a priority for John, he already has a lot of high impact factor publications. He finds data management an administrative task and only shares data when requested by the journal. He doesn’t even share his metadata. Mia has a lot of high impact factor publications. She developed an app that citizens can download to help collect data for her research project. She decided to share nothing of the research (not even the metadata) because of sensitive personal data. Koen collaborates with industry and contributed to many patents, due to related IP issues he has a short publication list and does not share many datasets. He does have an open attitude towards open science. Once he can share, he will. Afterall he wants to contribute to society & researchers. MIA KOEN KIM JOHN Rewards_A2.indd 1 02/05/2023 21:34


Fast Dynamic Load Balancing Tools for Extreme Scale Systems Parallel unstructured applications running on the latest petascale systems require partitions optimizing specific balance metrics. Methods combining the most powerful graph based and geometric methods with ParMA diffusive methods directly operating on an unstructured mesh are discussed. The SSE is focused on extending ParMA to support applications with relational structures that can be expressed with a graph structure. More Information: http://www.scorec.rpi.edu/parma Contact: Cameron Smith smithc11@rpi.edu and Mark Shephard shephard@rpi.edu Cameron W. Smith, Gerrett Diamond, and Mark S. Shephard Rensselaer Polytechnic Institute, USA ParMA: Partitioning using Mesh Adjacencies Guide partitioning decisions with mesh adjacency information • Mesh and partition model adjacencies represent application data more completely then standard (hyper)graph-partitioning models. • All mesh entities can be considered; (hyper)graph uses a subset of the adjacency information. • Complete mesh - O(1) time adjacency queries. Advantages • Avoid graph construction and directly account for multiple entity types important for the solve process • Easy to use with diffusive procedures – compliments other partition methods via incremental refinements Diffusive Approach • Iteratively migrate small sets of elements to (1) reduce the peak imbalance and (2) reduce the number of entities on the part boundaries. Diffusive Iteration Stages • Weight computation – compute weights and exchange with peers • Targeting – determined how much weight each peer can accept • Element selection – select elements for migration • Migration – move elements to peers Complete mesh adjacency structure. . Dynamic Partitioning of Unstructured Meshes Tools for re-partitioning an unstructured mesh due to changing work loads or communication patterns are required to: • Balance work, reduce communications, output distribution, execute in parallel quickly, use little memory, and provide API Common Methods • Graph, hypergraph, geometric diffusive, and local Examples will demonstrate that specific combinations are needed to reach really large part counts (> 500K). 1 - “Controlling Unstructured Mesh Partitions for Massively Parallel Simulations”, Min Zhou, et al., 2010 Geometric recursive inertial bisection Dual graph partition Mesh Example of partitioning methods. Global partitioning [1]. Local partitioning [1]. *** • *** *** • **** Partitioning to One Million Parts Multiple tools needed to maintain partition quality at scale [2] • Local and global topological and geometric methods via Zoltan and Zoltan2 integration ParMA quickly reduces large imbalances and improves part shape • 1.6B element mesh from 128K to 1M parts then running ParMA. 128K partition has less than 7% imbalance for all entity orders. • Global RIB – 103 seconds ParMA – 20 seconds 209% vtx imb reduced to 6%, perfect elm imb increased to 4%, and 5.5% reduction in avg vtx per part suspension upright Mira parameters: a = 10% b = 70% g = 64k *If memory is limited additional methods are available. • 12.9B element mesh from 128K (< 7% imb) to 1M parts then ParMA. • Local ParMETIS – 60 seconds. ParMA – 36 seconds 35% vtx imb reduced to 5%, 11% elm imb reduced to 5%, and 0.6% reduction in avg vtx Extending Application Support Goal • Support applications operating on graph-like structures. Three demonstrations: • Finite element unstructured mesh-based analysis • Hierarchic multi-scale for soft tissue modeling • Scale-free graphs for discrete event simulations Approach • Define N-graph abstraction to directly represent both graph and mesh relational structures: • defined as 𝐺" 𝑉, 𝐸&, 𝐸', … , 𝐸")' where: 𝑉: atomic units 𝑢+ of the domain Ω which uniquely exist on one part s.t. Ω = ∪∀+ 𝑢+, and 𝐸+: relations 𝑒+(𝑢, 𝑣) of type 𝑖between vertices 𝑢 and 𝑣where 𝑢, 𝑣 ∈𝑉and 𝑢 ≠𝑣. • Optionally, vertices and edges may be assigned associated weights 𝑤. • Implement EnGPar - N-Graph based v


Evaluating TDP-43 Targets in Amyotrophic Lateral Sclerosis Using Drosophila and Patient Spinal Cords Alexander Blythe1, Erik Lehmkuhl1, Suvitha Loganathan1, Eric Alsop4, Dianne Barrameda1, Bhavani B. Siddegowda1, Archi Joardar1, Kendall Jensen4, Daniela C. Zarnescu1,2,3 1Department of Molecular and Cellular Biology, 2Department of Neuroscience, 3Department of Neurology, 4Translational Genomics Research Institute Introduction and Background DLP DLP HRP w1118 D42>TDP-43WT D42>TDP-43G298S Figure 3. Images of dissected larval neuromuscular junctions (NMJ) treated with immunofluorescent staining. Horseradish peroxidase (HRP) is used as a control to emphasize changes in DLP levels. An additional diagram showing the different nervous tissue types in developing Drosophila larvae is shown. Sample Type Spinal Region TDP-43 Pathology Disease Mutation Control Thoracic No NA Control Lumbar No NA Control Cervical No NA Disease Thoracic Unknown C9orf72 Disease Lumbar Yes TDP-43 Disease Cervical Yes C9orf72 Disease Lumbar Yes OPTN, SETX Disease Lumbar Yes DCTN1 Disease Lumbar Yes NEK1 Figure 2. Larval turning times were used to assay locomotor function in 3rd instar larvae. DLP overexpression (OE) resulted in a rescue of locomotor function while DLP knockdown (RNAi) exacerbated TDP-43-induced locomotor dysfunction. N=33- 40. Asterisks (*) indicate p-values less than 0.05. Significance tests were performed using the Mann U Whitney Test. Effect of DLP mRNA Levels on Larval Motor Function DLP Visualized at the Larval Neuromuscular Junction DLP Levels in VNCs and NMJs During TDP-43 Proteinopathy DLP Levels in VNCs and NMJs During TDP-43 Proteinopathy Figure 5. Quantification of DLP levels in the ventral nerve cords (VNCs) of 3rd instar larvae. Western blots were run on homogenized VNCs from control larvae and larvae expressing TDP-43WT and TDP- 43G298S in the motor neurons. 10 VNCs were used in each sample. DLP intensity was normalized to Ponceau stain. Figure 4. Quantification of DLP levels in 4 terminal boutons at the NMJ of 3rd instar larvae relative to bouton size. N=3. Comparison of w1118 to D42>TDP-43G298S yields a p-value of 0.044. Asterisks (*) denote p-values less than 0.05. DLP Human Ortholog (GPC4) Levels in Spinal Tissue In 97% of ALS cases and about 45% of frontotemporal dementia cases, insoluble cytoplasmic aggregates containing highly phosphorylated TDP-43 have been identified as pathological hallmarks1. Considering these complexes and their noted neurotoxicity, a current hypothesis for TDP-43’s potential role in modifying neurodegenerative phenotypes during ALS is the ribostasis hypothesis, which posits that TDP-43 binds to and sequesters mRNAs into cytoplasmic insoluble complexes in motor neurons. These aggregates result in translational repression of affected mRNAs and severely dysregulate protein homeostasis, leading to motor neuron stress and eventually death2. Figure 1. Ribostasis hypothesis: Cytoplasmic TDP-43-induced sequestration of mRNAs into insoluble complexes results in translational repression of affected mRNAs, thereby lowering protein levels and disrupting proteostasis in motor neurons. A Drosophila model of ALS has been developed by overexpressing either wild- type or mutant TDP-43 in motor neurons, using a motor neuron-specific D42 driver with different versions of the TDP-43 bound to UAS promoters. These models have demonstrated ALS phenotypes including cytoplasmic TDP-43 aggregates, reduced lifespan, sleep fragmentation, and locomotor dysfunction3. Following tagged ribosome affinity purifications (TRAP) and RNA immunoprecipitations (RIP), potential mRNA candidates with both low ribosome association and co-precipitation with TDP-43 have been identified4. One such candidate is dally-like protein (DLP), a glypican present in the extracellular matrix of developing motor neurons. By determining if changed DLP levels exacerbate or rescue ALS phenotypes in developing larvae and observing if DLP protein levels are alter


The way to Open Science: the case of Spanish researchers Candela Ollé¶, Alexandre López-Borrull¶, Remedios Melero2, Juan-José Boté-Vericad3, Ernest Abadal3 1 Faculty of Information and Communication Sciences at Universitat Oberta de Catalunya, Barcelona 2 Institute of Agrochemistry and Food Technology. Consejo Superior de Investigaciones Científicas (CSIC), València. 3 Departament de Biblioteconomia, Documentació i Comunicació Audiovisual & Centre de Recerca en Informació, Comunicació i Cultura. Universitat de Barcelona, Barcelona. Introduction and methodology The poster describes the results of the online survey on open science carried out on researchers affiliated with universities and Spanish research centres and focused on open access to scientific publications, the publication process, the management of research data and the review of open articles. The main objective was to identify the perception and habits of researchers with regard to practices closely linked to open science and the scientific value added is that offers an in-depth picture of researchers as one of the main actors to whom this transformation and implementation of open science will fall. It focuses on the different aspects of OS: open access, open data, publication process and open review in order to identify habits and perceptions. This is to make possible an implementation of the OS movement. The survey was carried out among researchers who had published in the years 2020-2021, according to data obtained from WoS. It was emailed to a total of 8,188 researchers and obtained a total of 666 responses, of which 554 were complete, the rest being forms with some questions unanswered. The overall conclusions are as follows: - The meaning of open science and its implementation are emerging topics that still require promotion, training and even persuasion to be carried out. - APCs present an economic barrier to those groups that do not have funding available for paying for them, although they are not the main criterion when selecting a journal. - Although Open Peer Review may seem innovative and emerging, many researchers have published or reviewed in journals that offer the opportunity for open review. - Tenure and evaluation policies do seem to have a clear effect on the behaviour of researchers with regard to open science. - Resolving the issue of evaluation in research may clearly condition the habitual uses of researchers when selecting a journal as well as the payment of APCs. - Researchers state that they share research data more for reasons of persuasion than out of an obligation to carry it out. - Researchers do not seem to question the objectives of open science, although they do question the pathways or difficulties that may arise from day to day. - Open access to publications and open research data are two realities that are increasingly consolidated in the scientific community. - Researchers seem aware that we are undergoing change, where academic evaluation or policies relating to open science, its implementation and shifting habits among researchers may change. In this sense, more and better support is needed on the part of institutions and teacher support services. References Abadal, Ernest; Abad-García, Francisca; Anglada, Lluís; Boté-Vericad, Juan-José; Esteve, Asunción; González-Teruel, Aurora; Labastida, Ignasi; López-Borrull, Alexandre; Ollé, Candela; Melero, Remedios; Rodríguez-Gairín, Josep Manel; Santos-Hermosa, Gema (2023a). Ciencia abierta en España 2023: informe de situación y análisis de la percepción. Barcelona-València: Grupo Ciencia Abierta. http://hdl.handle.net/2445/200020 Abadal, Ernest; Anglada, Lluís; Labastida, Ignasi; Melero, Remedios; Ollé-Castellà, Candela (2023b). Recomendaciones a la administración pública para facilitar la implantación del modelo de ciencia abierta en España. http://hdl.handle.net/2445/198759 Ollé C, López-Borrull A, Melero R, Boté-Vericad J-J, Rodríguez-Gairín J-M, Abadal E (2023) Habits and percepti


Universität Tübingen · Philosophische Fakultät Seminar für Sprachwissenschaft Keplerstr. 2 · 72074 Tübingen Telefon +49 7071 29-77352 · https://talar.sfb833.uni-tuebingen.de Datenübernahme durch TALAR, das Tübinger Archive of Language Resources Vorhandene Daten in TALAR • Gepflegte Referenzdaten o Tübinger Baumbank-Collection o GermaNet • Gehostete Daten o Daten des SFB 833/SFB 441 o Daten des GRK 1808 • Daten externer Partner o SFB 638 o Index Thomisticus Treebank o ... • Community Daten o Universal Dependency Treebanks (UD) Zertifizierung des Repositoriums Seminar für Sprachwissenschaft Philosophische Fakultät Tübingen Archive of Language Resources (TALAR) Spezialisierung • Baumbanken/Treebanks • Wortnetze • Word-Embeddings Modalität • geschrieben • gesprochen Akzeptierte Datenformate • GermaNet XML-Format • CoNLL-U • Word-Embeddings • Weitere Formate nach Absprache Ansprechperson(en) • Thorsten Trippel • Claus Zinn Suchmöglichkeiten in den gepflegten Daten Zertifikat erteilt am 01. Juni 2023 Aktuell: turnusgemäße Erneuerung Daten Einbringen Initiale Datenübermittlung • Übermittlung nach BagIT-Standard • Werkzeugunterstützung: Bagman Voraussetzung: • Unterstützte Datentypen o Qualitätsgesichert o Auswahlprozess • Datenüberlassungsvertrag o Muster siehe https://uni-tuebingen.de/de/134320 • Offene Lizenz: CC-BY 4.0 oder höher • Metadaten nach ISO 24622 • Unterstützte Profile § CourseProfile § ExperimentProfile § LexicalResourceProfile § ResourceBundle Findable • Auffindbar mit persistentem Identifikator (PID) • Handle / DOI • Nachweis über Forschungsdatensuchmaschinen • z. B. VLO • Auffindbarkeit über Standardsuchmaschinen Accessible • Downloadmöglichkeit freier Daten • Zugang zu vorhandenen zugangsbeschränkten Daten • Metadaten frei zugänglich über technische Protokolle Interoperable • Je nach Datentyp • Nutzbar in den vorhandenen Auswertungswerkzeugen • Metadaten: standardkonform und maschinell interpretierbar Reusable • Nutzbar unter den Bedingungen der Lizenzen in eigener Software • Verwendung in anderen Projektkontexten • Klare Rechte an den Daten • Vertrauenswürdige Aufbewahrung F A I R Scott Martens (2013). TüNDRA: A Web Application for Treebank Search and Visualization. In: Proceedings of The Twelfth Workshop on Treebanks and Linguistic Theories (TLT12), Sofia, pp. 133—144. Hinrichs, Marie and Lawrence, Richard and Hinrichs, Erhard (2020): Exploring and Visualizing Wordnet Data with GermaNet Rover. In Proceedings of the CLARIN Annual Conference 2020, pp. 32-36. C. Zinn: Bagman - A Tool that Supports Researchers Archiving Their Data. Selected papers from the CLARIN Annual Conference 2021 (Virtual Event), Linköping University Electronic Press, vol. 189, pages 181-189, 2022. § SpeechCorpusProfile § TextCorpusProfile § ToolProfile § WebLichtWebService