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2017EGUGA..1915045L | The knowledge of sea level height is important for many different sectors as navigation transport building infrastructures tourism or maritime sports between others. Tides are mainly composed of an astronomical part and a meteorological one. Sometimes their joined action is the responsible of extreme behaviors in the s... | 2017-04-01T00:00:00Z | ['2017EGUGA..1915045L'] | null | More than 70 years of continuous sea level records on the Santander Bay. | 2,017 | 0 | 0.18 | ['PUB_PDF'] | 0 | null |
2018cosp...42E3546S | AcousticGravity Waves AGW generated by tsunamis propagating in the open ocean perturb the ionosphere and generate Traveling Ionospheric Disturbances TID. Recent investigations show that continuous monitoring of tsunamigenic TIDs can be used as a tsunami early warning system provided such TIDs are properly characterized... | 2018-07-01T00:00:00Z | ['2018cosp...42E3546S'] | null | Influence of source geometry in determining the characteristics of tsunamiinduced TIDs | 2,018 | 0 | 0.1 | null | 0 | null |
2017CoBAO..64..116H | In 2014 a new monitoring project started at the observational base Saravand of the Byurakan astrophysical observatory. This project initiated for revealing natural and artificial objects at the nearEarth space. This is a kind of continuation of earlier observational projects implemented at the observatory prior the col... | 2017-12-01T00:00:00Z | ['10.52526/25792776-2017.1-116', '2017CoBAO..64..116H'] | ['Near-Earth space', 'artificial satellites', 'cosmic junk', 'monitoring'] | New observational project for revealing natural and anthropogenic threats at the nearEarth space | 2,017 | 0 | 0.12 | ['PUB_HTML', 'PUB_PDF'] | 0 | null |
2017CoBAO..64..102M | We present the Byurakan Astrophysical Observatory BAO Plate Archive Project that is aimed at digitization extraction and analysis of archival data and building an electronic database and interactive sky map. BAO Plate Archive consists of 37500 photographic plates and films obtained with 2.6m telescope 1m and 0.5m Schmi... | 2017-12-01T00:00:00Z | ['10.52526/25792776-2017.1-102', '2017CoBAO..64..102M'] | ['photographic plates', 'plate archives', 'digitization', 'astrometry', 'photometry', 'spectroscopy', 'databases', 'virtual observatories'] | BAO Plate Archive Project | 2,017 | 0 | 0.17 | ['PUB_HTML', 'PUB_PDF'] | 1 | null |
2017EGUGA..1916905B | Source Apportionment SA is the identification of ambient air pollution sources and the quantification of their contribution to pollution levels. This task can be accomplished using different approaches chemical transport models and receptor models. Receptor models are derived from measurements and therefore are conside... | 2017-04-01T00:00:00Z | ['2017EGUGA..1916905B'] | null | Preliminary Results of the first European Source Apportionment intercomparison for Receptor and Chemical Transport Models | 2,017 | 0 | 0.12 | ['PUB_PDF'] | 0 | null |
2013M&PSA..76.5342M | Cluster chondrite clasts with distinct chondrule populations occur in the same UOC breccia. This indicates repeated chondrule forming events or the creation of different chondrule populations during a single event by sizesorting. | 2013-09-01T00:00:00Z | ['2013M&PSA..76.5342M'] | null | Distinct Chondrule Populations in Different UOC Cluster Chondrite Clasts | 2,013 | 0 | 0 | ['PUB_PDF'] | 0 | null |
2017Ciel...79..546M | Gographie de Pluton Qui nous observe Pulsar binaire record Rayons cosmiques nergtiques Ondes gravitationnelles U Antliae 40 Eridani BC Lastrode 2006 VW139288P Fron cosmique Tempte de neige sur Mars Oxyde de titane sur Wasp19b La matire organique des comtes Chondrites carbones | 2017-11-01T00:00:00Z | ['2017Ciel...79..546M'] | null | Lastronomie dans le monde | 2,017 | 0 | 0 | null | 0 | null |
2017Ciel...79..542N | Cadran situ rue du Vlodrome 102 Retinne | 2017-11-01T00:00:00Z | ['2017Ciel...79..542N'] | null | Cadrans solaires de Wallonie | 2,017 | 0 | 0 | null | 0 | null |
2018cosp...42E3160S | Nonthermal particle distributions are ubiquitous in the solarwind and near Earth space plasma their presence having frequently been confirmed by interplanetary missions. Such distributions represent suprathermal deviations from the Maxwellian equilibrium and are expected to exist in any lowdensity plasma in the Univers... | 2018-07-01T00:00:00Z | ['2018cosp...42E3160S'] | null | Effect of density gradient on nonlinear structures in a dusty plasma | 2,018 | 0 | 0 | null | 0 | null |
2014yCat..22100001C | During the first 10 months of science operations more than 2000 solartype stars were selected by the Kepler Asteroseismic Science Consortium KASC to be observed as part of an asteroseismic survey of the Sunlike population in the Kepler field of view. Solarlike oscillations were detected by Kepler in more than 500 stars... | 2014-01-01T00:00:00Z | ['2014yCat..22100001C', '10.26093/cds/vizier.22100001'] | ['Abundances: [Fe/H]', 'Effective temperatures', 'Stars: masses', 'Stars: ages'] | VizieR Online Data Catalog Asteroseismic study of solartype stars Chaplin 2014 | 2,014 | 0 | 0.26 | ['PUB_HTML'] | 0 | null |
2017AdSpR..59.2407M | Uranus together with Neptune in our Solar System belongs to a class of planets called ice giants which have never been explored using a dedicated mission. A mission to explore the ice giants is one of the highest priority missions of NASA. In this paper we present a new and unique multiprobe multiplanet spacecraft to e... | 2017-05-01T00:00:00Z | ['10.1016/j.asr.2017.02.012', '2017AdSpR..59.2407M'] | ['Ice giants', 'Mission design', 'Outer planets', 'Saturn', 'Uranus'] | Oceanus A multispacecraft flagship mission concept to explore Saturn and Uranus | 2,017 | 0 | 0.31 | ['PUB_HTML'] | 6 | null |
2014AGUFMSH21C4129P | Extreme Space Weather events are large solar flares or geomagnetic storms which can cost billions of dollars to recover from. We have few examples of such events the Carrington Event the solar superstorm is one of the few that had superlatives in three categories size of solar flare drop in Dst and amplitude of aa. Kep... | 2014-12-01T00:00:00Z | ['2014AGUFMSH21C4129P'] | ['7524 Magnetic fields', 'SOLAR PHYSICS', 'ASTROPHYSICS', 'AND ASTRONOMY', '7536 Solar activity cycle', 'SOLAR PHYSICS', 'ASTROPHYSICS', 'AND ASTRONOMY', '7594 Instruments and techniques', 'SOLAR PHYSICS', 'ASTROPHYSICS', 'AND ASTRONOMY', '7938 Impacts on humans', 'SPACE WEATHER'] | Pushing the Envelope of Extreme Space Weather | 2,014 | 0 | 0.1 | null | 0 | null |
2023yCat..19210122M | Both rho CrB and 88 Leo have synoptic Sindex time series from the Mount Wilson Observatory MWO HK Project ranging from near the beginning of the program in 1966 to its termination in 2003 see Figure 1. The MWO Sindex measures the ratio of emission from 1 cores of the CaII H and K lines to the sum of two nearby 20 pseud... | 2023-02-01T00:00:00Z | ['10.26093/cds/vizier.19210122', '2023yCat..19210122M'] | ['Asteroseismology', 'Stars: G-type', 'Stars: diameters', 'Stars: masses', 'Stars: ages', 'Optical', 'X-ray sources'] | VizieR Online Data Catalog Chromospheric activity of rho CrB and 88 Leo Metcalfe 2021 | 2,023 | 0 | 0.25 | ['PUB_HTML'] | 0 | null |
2018cosp...42E3277S | Millimetron observatory under development at the Lebedev Physical Institute includes a spacebased 10meter telescope operating at millimeter and infrared wavelengths from 0.02 to 17 mm millimetron.ru. In the singledish mode it can detect exoplanets in the lowest spectral band. We provide the list of exoplanets that woul... | 2018-07-01T00:00:00Z | ['2018cosp...42E3277S'] | null | Exoplanetary candidates to observations with Millimetron | 2,018 | 0 | 0.06 | null | 0 | null |
2014yCat..35720034G | We used data collected by the NASA planethunter mission Kepler. P 2 data files. | 2014-10-01T00:00:00Z | ['10.26093/cds/vizier.35720034', '2014yCat..35720034G', '2014yCat..35729034G'] | ['Stars: G-type', 'Stars: variable'] | VizieR Online Data Catalog Pulsating solarlike stars in Kepler Garcia 2014 | 2,014 | 0 | 0.19 | ['PUB_HTML'] | 0 | null |
2018cosp...42E3823Z | Double neutron star DNS merger events are promising candidates of short Gammaray Burst sGRB progenitors as well as highfrequecy gravitational wave GW emitters. On August 17 2017 such a coinciding event was detected by both the LIGOVirgo gravitational wave detector network as GW170817 and GammaRay Monitor on board NASAs... | 2018-07-01T00:00:00Z | ['2018cosp...42E3823Z'] | null | A peculiar lowluminosity short gammaray burst from a double neutron star merger progenitor | 2,018 | 0 | 0.19 | null | 0 | null |
2017CBET.4367....3W | The available astrometry spanning Feb. 1028 the following preliminary parabolic orbital elements by G. V. Williams and an ephemeris appear on MPEC 2017E06. T 2017 Apr. 29.5264 TT Peri. 341.1099 Node 186.5945 2000.0 q 4.967364 AU Incl. 125.6559 | 2017-03-01T00:00:00Z | ['2017CBET.4367....3W'] | null | Comet C2017 D3 Atlas | 2,017 | 0 | 0 | ['PUB_HTML'] | 0 | null |
2017EGUGA..1916366H | The Ganymede Laser Altimeter GALA is one of the instruments selected for ESAs Jupiter Icy Moons Explorer JUICE. A fundamental goal of any exploratory space mission is to characterize and measure the shape topography and rotation of the target bodies. A state of the art tool for this task is laser altimetry because it c... | 2017-04-01T00:00:00Z | ['2017EGUGA..1916366H'] | null | Status of the Ganymede Laser Altimeter GALA for ESAs Jupiter Icy Moons Explorer JUICE | 2,017 | 0 | 0.06 | ['PUB_PDF'] | 0 | null |
2017EGUGA..1915803N | The central European lake district extends within the Bohemian forest and Bavarian forest Mountains. It includes 8 glacial lakes extending in altitudes from 935 to 1087 m a.s.l. All of them have been oligotrophic and forests of the lake catchments are dominated by Norway spruce Picea abies. Plen lake PL catchment is at... | 2017-04-01T00:00:00Z | ['2017EGUGA..1915803N'] | null | Mercury in the central European lake district case study Plen lake | 2,017 | 0 | 0.17 | ['PUB_PDF'] | 0 | null |
2017Ge&Ae..57..190P | The 22year variation in the frequency of aurora occurrence is found through an analysis of data of the Russian network of meteorological stations from 18371909. This variation is obtained in a form of asymmetry between even and odd solar cycles. We found that the nature of the 22year variation depends on the latitude o... | 2017-03-01T00:00:00Z | ['10.1134/S0016793217020116', '2017Ge&Ae..57..190P'] | null | 22year cycle in the frequency of aurora occurrence in XIX century Latitudinal effects | 2,017 | 0 | 0.1 | ['PUB_HTML'] | 1 | null |
2024SPIE13096E..28K | GHOST is a newly operational optical fiberfed highresolution spectrograph at the Gemini South 8.1m telescope. It currently offers the choice of two resolution modes captured by one or two input IFUs with a FOV of 1.2 and a spectral resolving power of 56000 and 76000 for the unbinned CCDs. At the highresolution mode one... | 2024-07-01T00:00:00Z | ['2024SPIE13096E..28K', '10.1117/12.3021130'] | null | Roadmap of GHOSTGeminis precision radial velocity mode | 2,024 | 0 | 0.16 | ['PUB_HTML'] | 1 | null |
2013ICRC...33.3447B | TeV gammaray emission has been recently observed from the direction of open clusters containing many massive stars and dense concentrations of matter. We consider the high energy processes occurring within the massive binary systems and also within their environment by assuming that nuclei from the stellar winds are ac... | 2013-01-01T00:00:00Z | ['2013ICRC...33.3447B'] | ['binaries: general — radiation mechanisms: non-thermal — gamma-rays: theory'] | Gammarays and Neutrinos Produced Around Massive Binary Systems by Nuclei Accelerated Within the Binaries | 2,013 | 0 | 0.1 | ['ADS_PDF', 'ADS_SCAN'] | 0 | null |
2017IJMPA..3250148W | The 21dimensional KleinGordon oscillator under a magnetic field in the presence of a minimal length in the noncommutative NC space is analyzed via the momentum space representation. Energy eigenvalue of the system is obtained by employing the Jacobi polynomials. In further steps the special cases are discussed and the ... | 2017-09-01T00:00:00Z | ['2017IJMPA..3250148W', '10.1142/S0217751X17501482'] | ['Klein–Gordon oscillator', 'noncommutative space', 'minimal length', '03.65.Pm', '04.20.Jb', 'Relativistic wave equations', 'Exact solutions'] | 21dimensional KleinGordon oscillator under a magnetic field in the presence of a minimal length in the noncommutative space | 2,017 | 0 | 0.22 | ['PUB_HTML', 'PUB_PDF'] | 8 | null |
2024SPIE13102E..26M | Atmospheric interference noise and attenuation are a few limitations that arise when observing emissions of submillimeter wavelengths using groundbased telescopes. Ongoing research conducted on highaltitude balloons allow a new direction in observing these distributed emissions and eliminates all possible atmospheric i... | 2024-08-01T00:00:00Z | ['10.1117/12.3018025', '2024SPIE13102E..26M'] | null | A customizable fivestage intermediate frequency lownoise amplifier and readout chain for the Astrophysics Stratospheric Telescope for Highspectral Resolution Observations at Submillimeterwavelengths ASTHROS | 2,024 | 0 | 0.21 | ['PUB_HTML'] | 0 | null |
2024SPIE13097E..0VT | With the commissioning of the refurbished adaptive secondary mirror ASM for the 6.5meter MMT Observatory under way special consideration had to be made to properly calibrate the mirror response functions to generate an interaction matrix IM. The commissioning of the ASM is part of the MMT Adaptive optics exo Planet cha... | 2024-08-01T00:00:00Z | ['10.1117/12.3020489', '2024SPIE13097E..0VT'] | null | ESCAPE efficient synthesis of calibrations for adaptive optics through pseudosynthetic and empirical methods | 2,024 | 0 | 0.16 | ['PUB_HTML'] | 0 | null |
2017EGUGA..1915532J | The monthly global gravity field solutions derived using the measurements from the GRACE Gravity Recovery and Climate Experiment satellites have been continuously improved by the processing centers. One of the improvements in the processing method is a more detailed calibration of the onboard accelerometers in the GRAC... | 2017-04-01T00:00:00Z | ['2017EGUGA..1915532J'] | null | Effect of the improved accelerometer calibration method on AIUBs GRACE monthly gravity field solution | 2,017 | 0 | 0.06 | ['PUB_PDF'] | 0 | null |
2017EGUGA..1915411K | Installed onboard the German research aircraft HALO the integratedpath differentialabsorption IPDA lidar CHARMF measures weighted vertical columns of the greenhouse gases CO2 and CH4 below the aircraft and along its flight track aiming at high accuracy and precision. CHARMF was designed and built as an airborne demonst... | 2017-04-01T00:00:00Z | ['2017EGUGA..1915411K'] | null | Test Flight Results of the New Airborne CH4 and CO2 Lidar CHARMF | 2,017 | 0 | 0.18 | ['PUB_PDF'] | 0 | null |
2017EGUGA..1915513D | Little is known about compositional and structural diversity of super Earths. SuperEarths are distinct from miniNeptunes in terms of the origin of their atmospheres i.e. which are outgassed from the interior. Modeling the outgassing rates that arise from interior dynamics is key in order to inform the interpretation of... | 2017-04-01T00:00:00Z | ['2017EGUGA..1915513D'] | null | Outgassing of stagnantlid planets | 2,017 | 0 | 0.1 | ['PUB_PDF'] | 0 | null |
2024PhRvC.109b5803R | We have previously shown R. Rizaldy A. R. Alfarasyi A. Sulaksono and T. Sumaryada Phys. Rev. C 100 055804 2019 10.1103PhysRevC.100.055804 that Fermisurface distortion can affect nuclear matter and neutron star NS properties within the relativistic meanfield formalism. However our previous results had the caveat that th... | 2024-02-01T00:00:00Z | ['10.1103/PhysRevC.109.025803', '2024PhRvC.109b5803R'] | null | Impact of Fermisurface distortion in a relativistic meanfield model on the moment of inertia and tidal deformability of neutron stars | 2,024 | 0 | 0.06 | ['PUB_HTML'] | 1 | null |
2017EGUGA..1916160H | Soil moisture is one of the terrestrial essential climate variables that has critical role in the water energy and carbon cycles. There are different ways available for the retrieval of this essential variable e.g. remote sensing hydrological models insitu measurements and etc.. However the time series of these retriev... | 2017-04-01T00:00:00Z | ['2017EGUGA..1916160H'] | null | Investigation of the impact of the nonlinear relations among soil moisture products over data fusion process | 2,017 | 0 | 0.06 | ['PUB_PDF'] | 0 | null |
2017EGUGA..1917148O | Spectral images of Mars recorded by OMEGA Observatoire pour la Minralogie lEau les Glaces et lActivit on Mars Express can be used to deduce the mean effective radius reff and optical depth i of water ice particles in clouds. Using new data sets for a priori surface temperature vertical profiles of atmospheric temperatu... | 2017-04-01T00:00:00Z | ['2017EGUGA..1917148O'] | null | Water ice cloud property retrievals at Mars with OMEGASpatial distribution and column mass | 2,017 | 0 | 0.06 | ['PUB_PDF'] | 0 | null |
2017EGUGA..1915618J | Shock waves are ubiquitous in the universe and act to slow down and heat supersonic flows. In collisionless space plasmas shocks are able to accelerate particles to very high energy through various processes. Many processes relating to shock nonstationarity and plasma dynamics are subgyroscale and have therefore previo... | 2017-04-01T00:00:00Z | ['2017EGUGA..1915618J'] | null | Shock nonstationarity observed by MMS | 2,017 | 0 | 0 | ['PUB_PDF'] | 0 | null |
2017EGUGA..1916029A | The Max Planck Institute for Biogeochemistry MPIBGC has been operating a FourierTransform Spectrometer FTS on Ascension Island 8 S 14 W as part of the Total Carbon Column Observation Network TCCON. Since 2012 this instrument has been observing columnaveraged dryair mole fractions commonly referred to as Xgas of greenho... | 2017-04-01T00:00:00Z | ['2017EGUGA..1916029A'] | null | Biomass burning signals over the South Atlantic Ocean before and during the El Nio event of 201516 | 2,017 | 0 | 0.12 | ['PUB_PDF'] | 0 | null |
2017EGUGA..1914639Z | The FERMILAT gammaray experiment observed a surprisingly large number of solar events with gammaray emission above photon energies of 100 MeV. The emission is likely due to piondecay photons. This implies that the acceleration of protons in the solar corona to energies above 300 MeV is much more frequent than previousl... | 2017-04-01T00:00:00Z | ['2017EGUGA..1914639Z'] | null | HESPERIA studies on the nature of highenergy solar gammaray events | 2,017 | 0 | 0.06 | ['PUB_PDF'] | 0 | null |
2017EGUGA..1916489F | Motherofpearl clouds appear irregularly in the winter stratosphere at high northern latitudes about 2030 km above the surface of the Earth. The size range of the cloud particles is near that of visible light which explains their extraordinary beautiful colours. We argue that the Norwegian painter Edvard Munch could wel... | 2017-04-01T00:00:00Z | ['2017EGUGA..1916489F'] | null | Screaming Clouds | 2,017 | 0 | 0.34 | ['PUB_PDF'] | 0 | null |
2017EGUGA..1917145J | The Mercury Orbiter Radioscience Experiment MORE is one of the instruments on board the BepiColombo Mercury Planetary Orbiter MPO designed to estimate the Mercurys gravity field and rotational state and to perform a wide set of tests of relativistic gravity. The experiments exploits a highly stable multifrequency radio... | 2017-04-01T00:00:00Z | ['2017EGUGA..1917145J'] | null | Contribution of BepiColombos MORE radio science experiment to the determination of Mercurys interior structure | 2,017 | 0 | 0.12 | ['PUB_PDF'] | 0 | null |
2017EGUGA..1916026L | The COSIMA TOFSIMS spectrometer aboard Rosetta has collected nearly 40000 particles in orbit around 67PChuryumovGerasimenko from August 2014 to September 2016. These particles have been identified using the COSISCOPE optical microscope which imaged the 10 mm x 10 mm targets before and after exposure to the cometary env... | 2017-04-01T00:00:00Z | ['2017EGUGA..1916026L'] | null | Optical properties of particles collected by COSIMA around 67PChuryumov Gerasimenko | 2,017 | 0 | 0.06 | ['PUB_PDF'] | 0 | null |
2017EGUGA..1915162L | WAVEPAL is based on a general theory that we have developed for the frequency and wavelet analysis of irregularly sampled time series. It is based on the LombScargle periodogram that we extend to algebraic operators accommodating for the presence of a polynomial trend in the model for the data in addition to the period... | 2017-04-01T00:00:00Z | ['2017EGUGA..1915162L'] | null | WAVEPAL A Software for Frequency and Wavelet Analysis of Irregularly Sampled Time Series | 2,017 | 0 | 0.28 | ['PUB_PDF'] | 0 | null |
2024PhRvC.109b5805T | We explore the influence of symmetry energy and the cut potential on the properties of pure nucleonic and hyperonrich neutron stars employing the relativistic meanfield RMF model with the S271 parameter set. The effects of symmetry energy are modulated by the SUBvSUB coupling while the cut potential is governed by th... | 2024-02-01T00:00:00Z | ['2024PhRvC.109b5805T', '10.1103/PhysRevC.109.025805'] | null | Influence of the symmetry energy and cut potential on the properties of pure nucleonic and hyperonrich neutron star matter | 2,024 | 0 | 0.14 | ['PUB_HTML'] | 0 | null |
2017EGUGA..1916702G | Alberto GarcaRigo 1 David RomaDollase 2 Manuel HernndezPajares 1 Zishen Li 3 Michael Terkildsen 4 German Olivares 4 Reza GhoddousiFard 5 Denise Dettmering 6 Eren Erdogan 6 Haris Haralambous 7 Yannick Bniguel 8 Jens Berdermann 9 Martin Kriegel 9 Anna KrypiakGregorczyk 10 Tamara Gulyaeva 11 Attila Komjathy 12 Panagiotis ... | 2017-04-01T00:00:00Z | ['2017EGUGA..1916702G'] | null | St. Patricks Day 2015 geomagnetic storm analysis based on Real Time Ionosphere Monitoring | 2,017 | 0 | 0.16 | ['PUB_PDF'] | 0 | null |
2017CBET.4434....2W | The available astrometry the following elliptical orbital elements by G. V. Williams from 87 observations spanning Sept. 1129 and an ephemeris appear on MPEC 2017.S213. Epoch 2017 July 26.0 TT T 2017 July 28.0582 TT Peri. 99.9742 e 0.312971 Node 252.3863 2000.0 q 2.178983 AU Incl. 11.8532 a 3.171603 AU n 0.174... | 2017-09-01T00:00:00Z | ['2017CBET.4434....2W'] | null | Comet P2017 S5 Atlas | 2,017 | 0 | 0.06 | ['PUB_HTML'] | 0 | null |
2024Mirro...7...33C | The NOIRLab component of the U.S. Extremely Large Telescope Program USELTP is steadily advancing towards its Conceptual Design Review by the U.S. National Science Foundation NSF in December 2024. Here we highlight recent progress in the technical development and community engagement aspects of the program. | 2024-06-01T00:00:00Z | ['2024Mirro...7...33C'] | null | USELTP Moving Forward | 2,024 | 0 | 0.21 | ['PUB_PDF'] | 0 | null |
2024JATIS..10c9002P | The goal of deformable mirrors DMs is to correct aberrated optical wavefronts in spaceborne electrooptical EO payloads. It is used as part of an activeadaptive optics system. A continuoussurface metalbased DM is highly reliable and less complex to assemble has better stability of the active surface is less expensive an... | 2024-07-01T00:00:00Z | ['10.1117/1.JATIS.10.3.039002', '2024JATIS..10c9002P'] | ['mirror', 'correction accuracy', 'spherical aberration', 'qualification model', 'piezoelectric actuator', 'wavefront', 'optomechanical', 'root mean square'] | Design and qualification of an aluminum deformable mirror for spaceborne electrooptical payloads | 2,024 | 0 | 0.14 | ['PUB_HTML'] | 0 | null |
2014SPIE.9148E..51S | An adaptive optics system running at 1500 Hz was integrated using commercially available components. The deformable mirror was made by Alpao and has 277 actuators on a 15mm pitch. The wavefront sensor is based on the OCAM2 EMCCD Electronmultiplying chargecoupled device camera from First Light Imaging and a 2020 lenslet... | 2014-07-01T00:00:00Z | ['10.1117/12.2056395', '2014SPIE.9148E..51S'] | null | 1500Hz adaptive optics system using commercially available components | 2,014 | 0 | 0.1 | ['PUB_HTML'] | 0 | null |
2016xnnd.confE..67T | Powerful winds driven by active galactic nuclei AGN are often invoked to play a fundamental role in the evolution of both supermassive black holes SMBHs and their host galaxies quenching star formation and explaining the tight SMBHgalaxy relations. A strong support of this quasar mode feedback came from the recent Xray... | 2016-06-01T00:00:00Z | ['2016xnnd.confE..67T'] | null | Can supermassive black holes influence the evolution of their host galaxies | 2,016 | 0 | 0.19 | ['PUB_PDF'] | 0 | null |
2016shin.confE.127Y | Modern observations are revealing the Suns largescale magnetic field to have a complex nonpotential structure. Moreover it is now widely believed that the loss of equilibrium of twisted magnetic flux ropes is responsible for many if not all coronal mass ejections. But predicting where these flux ropes will form and in ... | 2016-07-01T00:00:00Z | ['2016shin.confE.127Y'] | null | The Global Distribution of Magnetic Helicity in the Suns Corona | 2,016 | 0 | 0 | null | 0 | null |
2016sofi.prop...38V | Magnetic fields permeate the Galactic ISM and have a significant influence on the formation of molecular clouds and stars. Farinfrared polarization from thermal dust grains aligned with the fields provides the strongest method for mapping the magnetic field strength and orientation. However the exact method of grain al... | 2016-01-01T00:00:00Z | ['2016sofi.prop...38V'] | ['SOFIA 05_0038'] | Characterizing the FIR polarization spectrum in Galactic Clouds | 2,016 | 0 | 0.2 | null | 0 | null |
2016sofi.prop...36C | We propose higher angular resolution HAWC Dband and deeper polarimetric observations twice the integration time than the tabulated ROC plan for the dense core of the nearby 140 pc dark cloud L1544. We will use these data to test ambipolar diffusion models of this prestellar core and to critically compare HAWC polarimet... | 2016-01-01T00:00:00Z | ['2016sofi.prop...36C'] | ['SOFIA 05_0036'] | The Magnetic Fields of the Dense and Diffuse Cores in L1544 | 2,016 | 0 | 0.1 | null | 0 | null |
2016cxo..prop.4896K | We will use the LETG to characterize the EUVemitting boundary layer BL and disk wind of two dwarf novae in outburst. These data will allow us to test stateoftheart BL models determine the outflow geometry and kinematics and characterize the aperiodic EUV variability. However the program is also a pathfinder for the Gre... | 2016-09-01T00:00:00Z | ['2016cxo..prop.4896K'] | null | EUV Emission from Accreting White Dwarfs in Outburst A Pathfinder for the Great Observatories Accretion Legacy Survey | 2,016 | 0 | 0 | null | 0 | null |
2016cosp...41E1776S | Signatures of the seismic activity in the ionospheric F2 region have been studied by analyzing the measurement of electron and ion temperatures during the occurrence of earthquake. The ionospheric electron and ion temperatures data recorded by the RPA payload aboard the Indian SROSSC2 satellite during the period from J... | 2016-07-01T00:00:00Z | ['2016cosp...41E1776S'] | null | Ionospheric Response Due to Seismic Activity | 2,016 | 0 | 0.06 | null | 0 | null |
2016cosp...41E1778S | The Stratospheric Sudden Warming SSW is one of the most spectacular phenomena in the atmosphere and has impacts on the Earths lower middle and upper atmospheres. Lidar is one of the best instrument to study Earths middle atmospheric thermal structure with very temporal and vertical resolution. A Nd YAG laser based Rayl... | 2016-07-01T00:00:00Z | ['2016cosp...41E1778S'] | null | Analysis of Stratospheric Sudden Warming SSW over Tropical and Subtropical Regions of India using Rayleigh Lidar and Satellite measurements | 2,016 | 0 | 0 | null | 0 | null |
2016cxo..prop.4994H | Chandra Xray surveys have revolutionized our view of the growth of black holes across cosmic time. Recently fundamental questions have emerged about the connection of AGN to their host large scale structures that clearly demand a wide deep survey over a large area comparable to the recent extensive Chandra surveys in s... | 2016-09-01T00:00:00Z | ['2016cxo..prop.4994H'] | null | The Chandra Deep WideField Survey Completing the new generation of Chandra extragalactic surveys | 2,016 | 0 | 0.12 | null | 0 | null |
2016csss.confE..57B | The 32 Ori moving group was discovered almost a decade ago and despite the fact that it represents thefirst northern young 20 Myr stellar aggregate within 100 pc of the Sun a comprehensive characterisationof the stellar content of the group has yet to be performed. We hereby present the first largescalespectroscopic s... | 2016-06-01T00:00:00Z | ['10.5281/zenodo.56486', '2016csss.confE..57B'] | ['stars: kinematics', 'stars: pre-main-sequence', 'open clusters and associations: individual: 32 Ori', 'techniques: spectroscopy', 'Zenodo community cs19'] | A Stellar Census Of The 32 Ori Moving Group | 2,016 | 0 | 0.17 | ['PUB_HTML'] | 0 | null |
2016cosp...41E2166Z | BeiDou Navigation Satellite System BDS does not have the ability of global navigation and positioning currently. The whole tracking observation of satellite orbit and the geometry of reference station are not perfect. These situations influence the accuracy of satellite orbit determination. Based on the theory and meth... | 2016-07-01T00:00:00Z | ['2016cosp...41E2166Z'] | null | Contribution Analysis of BDSGPS Combined Orbit Determination | 2,016 | 0 | 0 | null | 0 | null |
2016cxo..prop.4989P | Cas A is one of only a handful of young supernova remnants to exhibit time variations in thermal and nonthermal emission and is the only remnant to show evidence for an evolving young central neutron star. Here we propose to continue our multicycle monitoring program with three 50 ksec observations of Cas A spaced by a... | 2016-09-01T00:00:00Z | ['2016cxo..prop.4989P'] | null | Continued Multicycle Monitoring of the Young Galactic Supernova Remnant Cassiopeia A | 2,016 | 0 | 0.06 | null | 0 | null |
2016cosp...41E2164Z | Ionizing radiation and microgravity were considered to be the most important stress factors of space environmental the respective study of the biological effects of the radiation and microgravity carried out earlier but the interaction of the effects of radiation with microgravity started later and due to difference of... | 2016-07-01T00:00:00Z | ['2016cosp...41E2164Z'] | null | Simulated microgravity influenced the expression of DNA damage repair genes | 2,016 | 0 | 0.12 | null | 0 | null |
2016cosp...41E1867S | The DArk Matter Explorer DAMPE is a satellite based experiment aiming for dark matter search and many other topics astronomy interested. The Plastic Scintillator Detector PSD gives DAMPE the ability to measure charge of the crossing particles and separate gamma from electrons which are necessary for achieving the goals... | 2016-07-01T00:00:00Z | ['2016cosp...41E1867S'] | null | The Plastic Scintillator Detector of the DAMPE space experiment | 2,016 | 0 | 0.1 | null | 0 | null |
2016cosp...41E2066W | The CassiniHuygens mission is entering its final phase. The landing of Huygens on Titan and flybys performed by the Cassini probe during the last ten years revolutionized our knowledge about that moon revealing a complex fluviolacustrine environment. Despite significant differences in composition temperature and gravit... | 2016-07-01T00:00:00Z | ['2016cosp...41E2066W'] | null | Morphology of river deltas on Titan and Earth | 2,016 | 0 | 0.12 | null | 0 | null |
2016cosp...41E2064W | We use observations from the MESSENGER spacecraft in orbit around Mercury to investigate interplanetary coronal mass ejections ICMEs near 0.3 AU. MESSENGER is the first spacecraft since Helios 1 and 2 in the 1980s to make in situ measurements of the interplanetary medium at heliocentric distances lt 0.5 AU. Because ext... | 2016-07-01T00:00:00Z | ['2016cosp...41E2064W'] | null | Interplanetary coronal mass ejections at Mercury Database and effects on the magnetosphere | 2,016 | 0 | 0.1 | null | 0 | null |
2016shin.confE.119M | Magnetic topology is a powerful tool for describing the structure of magnetic fields during three dimensional reconnection. The bifurcation of magnetic null points is one of the most important ways by which magnetic topology can evolve. However most studies on null point bifurcation take an analytical approach that neg... | 2016-07-01T00:00:00Z | ['2016shin.confE.119M'] | null | Null Point Bifurcations During 3D Magnetic Reconnection | 2,016 | 0 | 0.18 | null | 0 | null |
2016cosp...41E1866S | Ionizing radiation IR is a known mutagen responsible for causing DNA strand breaks in all living organisms. Strand breaks thus created can be repaired by different mechanisms including homologous recombination HR one of the key mechanisms maintaining genome stability. Here we used previously generated Arabidopsis thali... | 2016-07-01T00:00:00Z | ['2016cosp...41E1866S'] | null | The study on spaceflight induced DNA damage in Arabidopsis thaliana and the protective effect of hydrogen | 2,016 | 0 | 0.06 | null | 0 | null |
2016cosp...41E1865S | We address the problem of determining the limiting energetic ring current ion spectrum resulting from electromagnetic ion cyclotron EMICwaveioninteractions. We solve the problem in a relativistic regimeincorporating a cold background multiion plasma component and without assuming a predetermined form for the particle e... | 2016-07-01T00:00:00Z | ['2016cosp...41E1865S'] | null | Energetic ring current ion spectra shaped by EMIC wave scattering loss | 2,016 | 0 | 0 | null | 0 | null |
2016gac..conf..317R | Solution of the small value of the cosmological constant problem is presented based on multidimensional gravity. | 2016-01-01T00:00:00Z | ['2016gac..conf..317R', '10.1142/9789814759816_0068'] | null | Spacetime foam and the cosmological constant problem | 2,016 | 0 | 0 | ['PUB_HTML', 'PUB_PDF'] | 0 | null |
2016diga.confE...3R | I review some of the mechanisms coupling disk dynamics to the scale of star cluster formation. In particular I show how the complex structure of the bar both triggers the formation of massive cluster and regulates the formation of star in the innermost regions. I also discuss the effect of stellar feedback in affecting... | 2016-10-01T00:00:00Z | ['10.5281/zenodo.163104', '2016diga.confE...3R'] | ['Discs in galaxies', 'Zenodo community discs2016'] | Star Formation Regulated By Disk Dynamics | 2,016 | 0 | 0.1 | ['PUB_HTML'] | 0 | null |
2016xmm..prop..158B | Central Compact Objects CCOs are a handful of faint and young Xrayemitting neutron stars at the center of bright supernova remnantsusually lacking detection at any other wavelength. So far only eightsources are classified as CCOs. Three of them are known to be neutronstars with periods in the range 0.10.4 s and dipolar... | 2016-10-01T00:00:00Z | ['2016xmm..prop..158B'] | null | Unveiling the Central Compact Object nature of CXOU J181852.0150213 | 2,016 | 0 | 0.06 | null | 0 | null |
2016yCat..51520075O | Our survey instrument nicknamed AggieCam consists of an Apogee Alta F16M camera with a 40964096pixel Kodak KAD16083 CCD that is thermoelectrically cooled down to T45C relative to ambient. Testing of the CCD showed a dark current of 0.2eSUPSUPpixs at temperatures of 25C relative to ambient. The optics include a Mamiya p... | 2016-09-01T00:00:00Z | ['2016yCat..51520075O', '10.26093/cds/vizier.51520075'] | ['Associations: stellar', 'Clusters: open', 'Stars: variable', 'Binaries: eclipsing', 'Stars: pre-main sequence', 'Stars: nearby', 'Stars: double and multiple', 'Planets'] | VizieR Online Data Catalog Photometric survey of IC 2391 eta Cha and USco Oelkers 2016 | 2,016 | 0 | 0.14 | ['PUB_HTML'] | 0 | null |
2016xnnd.confE..82C | High energy studies of astrophysical dust complement observations of dusty interstellar gas at other wavelengths. With high resolution Xray spectroscopy dust scattering significantly enhances the total extinction optical depth and alters the shape of photoelectric absorption edges. This effect is modulated by the dust ... | 2016-06-01T00:00:00Z | ['2016xnnd.confE..56C', '2016xnnd.confE..82C'] | null | The effects of dust scattering on highresolution Xray absorption edge structure | 2,016 | 0 | 0.2 | ['PUB_PDF'] | 0 | null |
2016yCat..17830004W | Our sample consists of bright host stars with multiplanet transiting systems from Kepler. Out of 5779 Kepler Objects of Interest httpexoplanetarchive.ipac.caltech.edu we selected all the systems with a Kepler magnitude KSUBPSUB brighter than 13.5mag and with at least two planet candidates. The sample includes 343 plane... | 2016-05-01T00:00:00Z | ['2016yCat..17830004W', '10.26093/cds/vizier.17830004'] | ['Stars: double and multiple', 'Planets', 'Stars: masses', 'Effective temperatures', 'Abundances: [Fe/H]', 'Stars: diameters'] | VizieR Online Data Catalog Properties of Kepler multiplanet candidate systems Wang 2014 | 2,016 | 0 | 0.1 | ['PUB_HTML'] | 0 | null |
2016xmm..prop...89S | Fermi has detected over 200 gammaray pulsars of varying types in 8 yearsof operations but the socalled soft lt 100 MeV gammaray pulsarsremain relatively elusive. Typically singlepeaked younger and moreenergetic than GeV pulsars such pulsars were particularly hard to detectwith Fermi prior to the release of Pass 8. Incr... | 2016-10-01T00:00:00Z | ['2016xmm..prop...89S'] | null | Searching for soft gammaray pulsars in unassociated Fermi LAT sources with | 2,016 | 0 | 0.12 | null | 0 | null |
2016wfc..rept....8B | The Wide Field Camera 3 WFC3 UVIS detector possesses an intrinsic signal during exposures even in the absence of light known as dark current. A daily monitor program is employed every HST cycle to characterize and measure this current as well as to create calibration files which serve to subtract the dark current from ... | 2016-04-01T00:00:00Z | ['2016wfc..rept....8B'] | ['Hubble Space Telescope', 'HST', 'Space Telescope Science Institute', 'STScI', 'WFC3', 'UVIS', 'calibration'] | WFC3UVIS Dark Calibration Monitoring Results and Improvements to Dark Reference Files | 2,016 | 0 | 0.21 | ['PUB_PDF'] | 0 | null |
2016xmm..prop...80T | During outbursts black hole BH transients enter into different spectralstates depending on the mass accretion rate as well as at least one otherphysical parameter. Although we do not know which second parameter ismost important candidates include jet power disk viscosity which maybe related to magnetic field generation... | 2016-10-01T00:00:00Z | ['2016xmm..prop...80T'] | null | The Black Hole Transient 4U 163047 in the LowSoft State | 2,016 | 0 | 0.1 | null | 0 | null |
2016wfc..rept....4M | An improved set of flat fields was delivered to the HST archive on February 23 2016 as part of the UVIS 2.0 photometric calibration. This new methodology treats the two UVIS chips as separate detectors when computing the flats and zeropoints. The most significant difference in the new flats is that each chip is now nor... | 2016-03-01T00:00:00Z | ['2016wfc..rept....4M'] | ['Hubble Space Telescope', 'HST', 'Space Telescope Science Institute', 'STScI', 'WFC3', 'UVIS', 'flat fields', 'photometry', 'repeatability'] | UVIS 2.0 ChipDependent Flats | 2,016 | 0 | 0.06 | ['PUB_PDF'] | 0 | null |
2016xmm..prop...81A | The discovery of bright ringlike Xray emission at the heart of thelarge supernova remnant SNR HB3 has invoked many possible explanationsfor this unique morphology including a second SNR a presupernovacircumstellar shell or an unusual density distribution. Howeverprevious observations of this remnant have either suffere... | 2016-10-01T00:00:00Z | ['2016xmm..prop...81A'] | null | A ring around the heart of supernova remnant HB3 | 2,016 | 0 | 0.17 | null | 0 | null |
2016yCat..18149006R | We measure the equivalent widths of Ly and the C III doublet in the restframe UV spectra of 11 gravitationally lensed galaxies at 1.6ltzlt3.1. Spectra were obtained using the MagE spectrograph on the Clay Magellan II telescope as part of a large study of the restframe ultraviolet spectral properties of bright lensed ga... | 2016-03-01T00:00:00Z | ['10.26093/cds/vizier.18149006', '2016yCat..18149006R'] | ['Galaxies: nearby', 'Equivalent widths', 'Gravitational lensing'] | VizieR Online Data Catalog CIII emission in near amp far starforming galaxies Rigby 2015 | 2,016 | 0 | 0.14 | ['PUB_HTML'] | 0 | null |
2016yCat..35930007H | Column density NSUBHSUB and extinction ASUBVSUB values are sample of YSO sources in the ONC. Nearinfrared colours based on the VISION Meingast et al. 2016AampA...587A.153M catalogue were employed to calculate extinction values using the NICER algorithm Lombardi et al. 2001AampA...377.1023L and assuming RSUBVSUB3.1. Col... | 2016-07-01T00:00:00Z | ['10.26093/cds/vizier.35930007', '2016yCat..35930007H'] | ['Extinction', 'Infrared sources', 'X-ray sources', 'YSOs'] | VizieR Online Data Catalog NH and AV Towards YSOs in the ONC Hasenberger 2016 | 2,016 | 0 | 0.16 | ['PUB_HTML'] | 0 | null |
2016yCat..51500200H | Cz 30 was observed using the WisconsinIndianaYaleNOAO WIYN 0.9m telescope with the S2KB imager a 20482048 pixel CCD with a pixel scale of 0.6pixel providing a total field of view of 20.520.5. Observations were taken on 2012 February 17 in B V and I filters with a typical seeing of about 1.5 and the CCD centered near th... | 2016-06-01T00:00:00Z | ['2016yCat..51500200H', '10.26093/cds/vizier.51500200'] | ['Clusters: open', 'Photometry: UBVRI', 'Equivalent widths', 'Radial velocities', 'Effective temperatures', 'Abundances: [Fe/H]'] | VizieR Online Data Catalog Photometry and spectroscopy of stars in Cz 30 Hayes 2015 | 2,016 | 0 | 0 | ['PUB_HTML'] | 0 | null |
2016yCat.2042....0H | A narrowband spectrometer compensated for seeing and transparency variations has been constructed and used to measure the strength of the calcium Kline 3933.68 in 146 Atype stars. The observations were made in the spring of 1966 with the No.4 16inch 40cm telescope at Kitt Peak National Observatory. P 1 data file. | 2016-11-01T00:00:00Z | ['2016yCat.2042....0H'] | ['Photometry: K-line', 'Stars: A-type'] | VizieR Online Data Catalog KLine Photometry of A Stars Henry 1969 | 2,016 | 0 | 0 | null | 0 | null |
2016yCat..17820045D | All the spectroscopy and imaging observations reported here were obtained with the ShangriLa telescope SLT IAU site code O44 at the Lijiang Station of the Yunnan Observatory of the Chinese Academy of Sciences. The SLT started its operation in 2008. This is a 2.4m altazimuth mounted RitcheyChretien telescope. The rms po... | 2016-03-01T00:00:00Z | ['2016yCat..17820045D', '10.26093/cds/vizier.17820045'] | ['Active gal. nuclei', 'Galaxies: Seyfert', 'Accretion', 'Spectroscopy'] | VizieR Online Data Catalog SEAMBHs. I. Mrk 142 Mrk 335 and IRAS F123973333 Du 2014 | 2,016 | 0 | 0.25 | ['PUB_HTML'] | 0 | null |
2016xnnd.confE..21H | The Cherenkov Telescope Array CTA is a nextgeneration observatory for very high energy VHE gammaray astronomy. With one array of imaging atmospheric Cherenkov telescopes each in the northern and southern hemispheres CTA will provide fullsky coverage enhance flux sensitivity by one order of magnitude compared to current... | 2016-06-01T00:00:00Z | ['2016xnnd.confE..21H'] | null | Synergies with CTA and VHE Astrophysics | 2,016 | 0 | 0 | ['PUB_PDF'] | 0 | null |
2016yCat..51500191R | Nearinfrared images of the CygnusX DR15 region were obtained with the OMEGA 2000 camera at the 3.5m telescope of the Calar Alto Observatory atop Sierra de los Filabres in Almeria Spain during the nights of 2010 February 2nd and March 3rd. The data set consists of 900s coadded exposures in the J H and K bands 1.209 1.64... | 2016-06-01T00:00:00Z | ['10.26093/cds/vizier.51500191', '2016yCat..51500191R'] | ['YSOs', 'Photometry: infrared'] | VizieR Online Data Catalog Infrared photometry of YSOs in CygnusX DR15 RiveraGalvez 2015 | 2,016 | 0 | 0.1 | ['PUB_HTML'] | 0 | null |
2016yCat..74514346S | FLAMES observations towards four open clusters in the LMC and SMC were retrieved from the ESO archive and are used to study the IHVCs towards these galaxies and their variation on small scales. P 1 data file. | 2016-06-01T00:00:00Z | ['2016yCat..74514346S'] | ['Magellanic Clouds', 'Clusters: open'] | VizieR Online Data Catalog Earlytype stars in SMC and LMC Smoker 2015 | 2,016 | 0 | 0.06 | null | 0 | null |
2016yCat..74512750X | Our sample was collected directly from the sample of Nemmen et al. 2012 Cat. JotherSci338.1445 but some blazars in Nemmen et al. 2012 Cat. JotherSci338.1445 were not clean Fermi blazars 2LAC Ackermann et al. 2011 Cat. JApJ743171. We removed the nonclean blazars. P 1 data file. | 2016-01-01T00:00:00Z | ['2016yCat..74512750X'] | ['BL Lac objects', 'QSOs', 'Gamma rays'] | VizieR Online Data Catalog Blazar sequence Xiong 2015 | 2,016 | 0 | 0.1 | null | 0 | null |
2016wfc..rept....3D | We analyze 6 years of standard star observations acquired with the WFC3UVIS imager between 2009 and 2015. Observations of the three white dwarf standard stars GD 153 GD 71 and G191B2B were obtained at multiple dither positions near the center of the array and in all fourcorner subarrays. Departing from previous practic... | 2016-11-01T00:00:00Z | ['2016wfc..rept....3D'] | ['Hubble Space Telescope', 'HST', 'Space Telescope Science Institute', 'STScI', 'WFC3', 'UVIS', 'photometry', 'inverse sensitivity', 'two-chip'] | UVIS 2.0 Chipdependent Inverse Sensitivity Values | 2,016 | 0 | 0.17 | ['PUB_PDF'] | 3 | null |
2016yCat..17810124C | A goal of this work is to find selfconsistent and accurate ways to predict the properties of stellar lightcurve variability and to use this variability to calibrate against other methods of determining their fundamental parameters. Thus it may be possible to develop the analysis of granular flicker measurements in a wa... | 2016-01-01T00:00:00Z | ['10.26093/cds/vizier.17810124', '2016yCat..17810124C'] | ['Stars: double and multiple', 'Stars: masses', 'Effective temperatures'] | VizieR Online Data Catalog Granulation model for 508 KIC stars Cranmer 2014 | 2,016 | 0 | 0.06 | ['PUB_HTML'] | 0 | null |
2016yCat..35890110A | The data analysed in this publication comprise two distinct types of observations. The first is of SN II optical spectroscopy obtained during their photospheric phases i.e. from discovery to at most 100 days post explosion. These data are used to extract absorption line pEW measurements. The second data set is emission... | 2016-07-01T00:00:00Z | ['2016yCat..35890110A', '10.26093/cds/vizier.35890110'] | ['H II regions', 'Supernovae'] | VizieR Online Data Catalog SN II in host HII regions Anderson 2016 | 2,016 | 0 | 0.18 | ['PUB_HTML'] | 0 | null |
2016xnnd.confE..18E | Galaxy clusters are located at the crossroads of intergalactic filaments and are still forming through the continuous merging and accretion of smaller structures from the surrounding cosmic web. Deep widefield Xray studies of the outskirts of the most massive clusters bring us valuable insight into the processes leadin... | 2016-06-01T00:00:00Z | ['2016xnnd.confE..18E'] | null | Cluster outskirts and the missing baryons | 2,016 | 0 | 0.14 | ['PUB_PDF'] | 0 | null |
2016yCat..35890078B | Individual time averaged spectra of HSUB2SUBSUP16SUP HSUB2SUBSUP18SUPO110101 lines observed with the Odin satellite as used for Fig. 1 map plus a partial map not shown in the paper Fig. 2 time evolution analysis and averages shown in Fig. 3. By default these are the averages of the two combinations of autocorrelatorrec... | 2016-03-01T00:00:00Z | ['10.26093/cds/vizier.35890078', '2016yCat..35890078B'] | ['Comets', 'Radio lines', 'Spectra: millimetric/submm'] | VizieR Online Data Catalog C2012 F6 Lemmon and C2013 R1 spectra Lovejoy Biver 2016 | 2,016 | 0 | 0.12 | ['PUB_HTML'] | 0 | null |
2015AGUFMSH53A2479J | In this study we analyze the abundances of suprathermal heavy ions in 75 Corotating Interaction Region CIR events between January 1st 1995 and December 31st 2008. We correlate the heavy ion abundances in these CIRs with those measured in the solar wind and suprathermal populations upstream of these events. Our analysis... | 2015-12-01T00:00:00Z | ['2015AGUFMSH53A2479J'] | ['2102 Corotating streams', 'INTERPLANETARY PHYSICS', '2126 Heliosphere/interstellar medium interactions', 'INTERPLANETARY PHYSICS', '7513 Coronal mass ejections', 'SOLAR PHYSICS', 'ASTROPHYSICS', 'AND ASTRONOMY', '7954 Magnetic storms', 'SPACE WEATHER'] | Abundance and Source Population of Suprathermal Heavy Ions in Corotating Interaction Regions | 2,015 | 0 | 0.06 | null | 0 | null |
2017GReGr..49...41K | It is shown that continuous causal isomorphisms on twodimensional Minkowski spacetime can be characterized by the invariance of wave equations. | 2017-03-01T00:00:00Z | ['2017GReGr..49...41K', '10.1007/s10714-017-2206-y'] | ['Causal isomorphism', 'Causal relation', 'Wave equation', "Zeeman's theorem"] | On continuous causal isomorphisms on twodimensional Minkowski spacetimes | 2,017 | 0 | 0.14 | ['PUB_HTML'] | 2 | null |
2017Ge&Ae..57..251B | An algorithm for retrieving the AL index dynamics from the parameters of solarwind plasma and the interplanetary magnetic field IMF has been developed. Along with other geoeffective parameters of the solar wind an integral parameter in the form of the cumulative sum NVSUP2SUP is used to determine the process of substor... | 2017-05-01T00:00:00Z | ['10.1134/S0016793217030021', '2017Ge&Ae..57..251B'] | null | Effect of solar dynamics parameters on the formation of substorm activity | 2,017 | 0 | 0.22 | ['PUB_HTML'] | 10 | null |
2017GCN.21929....1H | Our collaboration GROWTH JAGWAR CaltechNRAO TTUNRAO has continued to monitor the evolution of the radio counterpart to GW170817SSS17a discovered on September 23 2017 with the Jansky VLA Mooley et al. LVC GCN 21814 and Corsi et al. LVC GCN 21815 with ongoing observations at frequencies of 1.4 GHz 3 GHz and 6 GHz. Respon... | 2017-09-01T00:00:00Z | ['2017GCN.21929....1H'] | null | LIGOVIRGO G298048 Latest 3 GHz Detection of Radio Counterpart to SSS17a | 2,017 | 0 | 0.1 | ['PUB_HTML'] | 0 | null |
2017GCN.22122....1L | We have reanalysed offline noisesubtracted data for the LIGO Hanford Observatory H and the LIGO Livingston Observatory L around the time of the binary black hole merger event G288732 GW170608 GCNs 21221 and 21239 taking into account our most uptodate understanding of both calibration and waveform modelling uncertainti... | 2017-11-01T00:00:00Z | ['2017GCN.22122....1L'] | null | LIGOVirgo G288732GW170608 updated localization from parameter estimation | 2,017 | 0 | 0.06 | ['PUB_HTML'] | 0 | null |
2017LPI....48.2103K | This work utilizes MNF technique to map the spectral variability and delineate various basaltic units. CSFD technique was used to determine the age of units. | 2017-03-01T00:00:00Z | ['2017LPI....48.2103K'] | null | Volcanic and Compositional History of Mare Nectaris Using Chandrayaan1 Moon Mineralogy MapperM3 Data | 2,017 | 0 | 0.1 | ['PUB_PDF'] | 0 | null |
2017LPI....48.2205B | Participants in NASA Goddards Planetary Science Winter School design a flight instrument under consideration for proposal. We present results and future plans. | 2017-03-01T00:00:00Z | ['2017LPI....48.2205B'] | null | Training Early Career Scientists in Flight Instrument Design Through Experiential Learning NASA Goddards Planetary Science Winter School | 2,017 | 0 | 0 | ['PUB_PDF'] | 0 | null |
2017LPI....48.1528M | We created a model to investigate the role of orbital variability on postNoachian martian climate and surface conditions. | 2017-03-01T00:00:00Z | ['2017LPI....48.1528M'] | null | The Role of Obliquity in PostNoachian Martian Surface Conditions | 2,017 | 0 | 0.14 | ['PUB_PDF'] | 0 | null |
2017LPI....48.3002F | An introduction of imaging method of Lunar Regolith Penetrating Radar LRPR which will be carried by the CE5 lander. | 2017-03-01T00:00:00Z | ['2017LPI....48.3002F'] | null | An Imaging Method of Change5 Lunar Regolith Penetrating Radar | 2,017 | 0 | 0.12 | ['PUB_PDF'] | 0 | null |
2017LPI....48.2304S | We perform coregistration of topographic data sets from orbital observations of the Moon to measure its rotational dynamics. | 2017-03-01T00:00:00Z | ['2017LPI....48.2304S'] | null | Measurements of Moons Rotation by CoRegistration of Laser Altimeter Profiles and Stereo Terrain Models | 2,017 | 0 | 0 | ['PUB_PDF'] | 0 | null |
2017LPI....48.1904S | Fly me to the Moon Dark surfaces I shall find But colours I seek. | 2017-03-01T00:00:00Z | ['2017LPI....48.1904S'] | null | Wavelengths Selection for LEDIlluminated Multispectral Imaging on PROSPECT for Luna27 | 2,017 | 0 | 0 | ['PUB_PDF'] | 0 | null |
2017LPI....48.2799T | We expose the CM2 chondrite Murchison to a simulated micrometeorite impact event. Results include spectral data and nanoscale chemical and structural analyses. | 2017-03-01T00:00:00Z | ['2017LPI....48.2799T'] | null | Analyzing the Chemical and Spectral Effects of Pulsed Laser Irradiation to Simulate Space Weathering of a Carbonaceous Chondrite | 2,017 | 0 | 0 | ['PUB_PDF'] | 0 | null |
2017LPI....48.2302J | Isotopes and volatile element estimates for a dry Moon are consistent with the recently proposed highenergy highangularmomentum giant impact model. | 2017-03-01T00:00:00Z | ['2017LPI....48.2302J'] | null | Testing Models of Lunar Origin K Isotopes Radiogenic Isotopes and Volatile Elements | 2,017 | 0 | 0.06 | ['PUB_PDF'] | 0 | null |
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