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2020ApJ...896..118C | Plasmaspheric hiss is known to be a major contributor to the dynamic losses of Earths radiation belt electrons. While previous computation attempts of hissdriven electron losses are limited to the cold plasma approximation in this study we find that hot plasma effects will modify the hiss dispersion relation and result... | 2020-06-01T00:00:00Z | ['Van Allen radiation belts', 'Planetary magnetospheres', 'Space plasmas', '1758', '997', '1544'] | Hot Plasma Effects on the Pitchangle Scattering Rates of Radiation Belt Electrons Due to Plasmaspheric Hiss | 2,020 | 0 | 0.26 | 12 | https://ui.adsabs.harvard.edu/link_gateway/2020ApJ...896..118C/EPRINT_PDF | ['1758', '997', '1544'] | ['Van Allen radiation belts', 'Planetary magnetospheres', 'Space plasmas'] | ['Van Allen radiation belts', 'Planetary magnetospheres', 'Space plasmas'] |
2020ApJ...888...69B | An analytic model of the timedependent electric and magnetic fields of an astrophysical jet is presented. These fields satisfy the timedependent Faradays law and describe a jet with increasing length. The electric field contains both electrostatic and inductive parts. The electrostatic part corresponds to the rate of i... | 2020-01-01T00:00:00Z | ['Accretion', 'jets', 'magnetohydrodynamics', 'stellar jets', 'stellar accretion disks', 'young stellar objects', 'Collimation', '14', '870', '1964', '1607', '1579', '1834', '268'] | Analytic Model for the Timedependent Electromagnetic Field of an Astrophysical Jet | 2,020 | 0 | 0.19 | 3 | https://ui.adsabs.harvard.edu/link_gateway/2020ApJ...888...69B/EPRINT_PDF | ['14', '870', '1964', '1607', '1579', '1834', '268'] | ['Accretion', 'Jets', 'Magnetohydrodynamics', 'Stellar jets', 'Stellar accretion disks', 'Young stellar objects', 'Collimation'] | ['Accretion', 'Jets', 'Magnetohydrodynamics', 'Stellar jets', 'Stellar accretion disks', 'Young stellar objects', 'Collimation'] |
2022pds..data...54M | Mesick PDART 2019 Mars Odyssey Improved DND Products | 2022-01-01T00:00:00Z | ['2001', '2019', 'PDS', 'PDS4', 'derived', 'dnd', 'grs', 'improved', 'mars', 'mesick', 'n', 'odyssey', 'pdart', 'product', 'science'] | Mesick PDART 2019 Mars Odyssey Improved DND Products Bundle | 2,022 | 0 | 0.06 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2022pds..data...54M/EPRINT_PDF | ['2001', '2019'] | ['Solar dynamo', 'Reverberation mapping'] | ['Solar dynamo', 'Reverberation mapping'] |
2022RNAAS...6..224M | The analysis of high resolution spectra of the HgMn star HD 35548A recorded by the SWP camera on board the International Ultraviolet Explorer reveals no variations of the farultraviolet flux of this star over about 21 hr in 1981. The resonance lines of Ga II and Ga III characteristic of classical HgMn stars are salient... | 2022-10-01T00:00:00Z | ['Chemically peculiar stars', 'Mercury-manganese stars', '226', '1025'] | The Behavior of HgMn Stars in the Far UVPaper 17 HD 35548A | 2,022 | 0 | 0 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2022RNAAS...6..224M/EPRINT_PDF | ['226', '1025'] | ['Chemically peculiar stars', 'Mercury-manganese stars'] | ['Chemically peculiar stars', 'Mercury-manganese stars'] |
2020ApJ...900...49P | We derive an equation of state EOS for magnetized chargeneutral nuclear matter relevant for a neutron star NS. The calculations are performed within an effective chiral model based on the generalization of the model with nonlinear selfinteractions of the mesons along with the crosscoupling term. This model is extend... | 2020-09-01T00:00:00Z | ['Neutron stars', '1108'] | An Equation of State for Magnetized Neutron Star Matter and Tidal Deformation in Neutron Star Mergers | 2,020 | 0 | 0.31 | 8 | https://ui.adsabs.harvard.edu/link_gateway/2020ApJ...900...49P/EPRINT_PDF | ['1108'] | ['Neutron stars'] | ['Neutron stars'] |
2024RNAAS...8..241S | Both Christian Huygens and William Derham expressed ideas that are prescient to the concept of a circumstellar habitable zone liquid water is a precondition for life there is a region within the solar system within which liquid surface water can exist upon planets the stars are suns around which planetary systems shoul... | 2024-09-01T00:00:00Z | ['Habitable zone', 'Exoplanets', '696', '498'] | Christian Huygens and William Derham and 18th Century Precursors to the Habitable Zone | 2,024 | 0 | 0 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2024RNAAS...8..241S/EPRINT_PDF | ['696', '498'] | ['Habitable zone', 'Exoplanets'] | ['Habitable zone', 'Exoplanets'] |
2021pds..data..174N | PDS4 Data Providers Handbook DPH version 1.16.0 2021 | 2021-01-01T00:00:00Z | ['1.16.0', '2021', 'PDS', 'PDS4', 'data', 'dph', 'handbook', 'pds4', "provider's", 'version'] | PDS4 Planetary Science Data Providers Handbook DPH Version 1.16.0 | 2,021 | 0 | 0 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2021pds..data..174N/EPRINT_PDF | ['2021'] | ['Exoplanet atmospheric composition '] | ['Exoplanet atmospheric composition '] |
2021pds..data..176N | PDS4 Concepts version 1.16.0 2021 | 2021-01-01T00:00:00Z | ['1.16.0', '2021', 'PDS', 'PDS4', 'concept', 'pds4', 'version'] | PDS4 Planetary Science Concepts Version 1.16.0 | 2,021 | 0 | 0 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2021pds..data..176N/EPRINT_PDF | ['2021'] | ['Exoplanet atmospheric composition '] | ['Exoplanet atmospheric composition '] |
2022PASP..134k5002L | Since the idea of bionic Lobster eye micropore optics was put forward the possibility of focusing hard Xrays by this new lightweight Xray optics has been proposed. Limited by the technological conditions of the aspect ratio 500 low surface roughness 1 nm and the difficulty of applying metal coatings inside such narrow ... | 2022-11-01T00:00:00Z | ['X-ray transient sources', 'X-ray telescopes', 'X-ray astronomy', 'X-ray surveys', 'X-ray identification', '1852', '1825', '1810', '1824', '1817'] | Fabrication and Performance of Lobster Eye XRay Micro Pore Optics with the Ultrahigh Aspect Ratio | 2,022 | 0 | 0.31 | 5 | https://ui.adsabs.harvard.edu/link_gateway/2022PASP..134k5002L/EPRINT_PDF | ['1852', '1825', '1810', '1824', '1817'] | ['X-ray transient sources', 'X-ray telescopes', 'X-ray astronomy', 'X-ray surveys', 'X-ray identification'] | ['X-ray transient sources', 'X-ray telescopes', 'X-ray astronomy', 'X-ray surveys', 'X-ray identification'] |
2022ApJ...941...29L | Theoretical absorption oscillator strengths and wavelengths for rotational transitions of the C SUP2SUPv 0X SUP2SUPv bands with v 06 of nitric oxide are reported. The Molecular Quantum Defect Orbital method has been used in the calculations and the known interaction between the C SUP2SUPv 0 Rydberg and the B SUP2SUP... | 2022-12-01T00:00:00Z | ['Molecular spectroscopy', 'Line intensities', 'Line positions', '2095', '2084', '2085'] | Transition Energies and Line Oscillator Strengths of the C SUP2SUP0X SUP2SUP06 Absorption Bands of Nitric Oxide. A Theoretical Study | 2,022 | 0 | 0.2 | 3 | https://ui.adsabs.harvard.edu/link_gateway/2022ApJ...941...29L/EPRINT_PDF | ['2095', '2084', '2085'] | ['Molecular spectroscopy', 'Line intensities', 'Line positions'] | ['Molecular spectroscopy', 'Line intensities', 'Line positions'] |
2022pds..data...25D | Localization position and orientation information for the Mars 2020 Perseverence Rover | 2022-01-01T00:00:00Z | ['2020', 'PDS', 'PDS4', 'derived', 'information', 'localization', 'mars', 'mission', 'orientation', 'perseverence', 'position', 'rover', 'science'] | Mars 2020 Rover PLACES Bundle | 2,022 | 0 | 0.06 | 1 | https://ui.adsabs.harvard.edu/link_gateway/2022pds..data...25D/EPRINT_PDF | ['2020'] | ['Exoplanet atmospheric variability'] | ['Exoplanet atmospheric variability'] |
2021pds..data..149H | This bundle contains crustal magnetic field maps and equivalent source dipole arrays for Mercury based on the MESSENGER magnetic field data. This work was funded by a 2016 NASA ROSES DDAP proposal. Grant number NNH16ZDA001NDDAP. | 2021-01-01T00:00:00Z | ['2016', 'PDS', 'PDS4', 'array', 'based', 'bundle', 'contains', 'crustal', 'data', 'ddap', 'derived', 'dipole', 'equivalent', 'field', 'funded', 'grant', 'mag', 'magnetic', 'magnetometer', 'map', 'mercury', 'messenger', 'nasa', 'nnh16zda001n-ddap', 'number', 'proposal', 'rose', 'science', 'source', 'work'] | MESSENGER MAG Crustal Field Map | 2,021 | 0 | 0 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2021pds..data..149H/EPRINT_PDF | ['2016'] | ['Quenched galaxies'] | ['Quenched galaxies'] |
2022RNAAS...6...69M | The analysis of high resolution SWP spectra obtained through the large aperture with the International Ultraviolet Explorer reveals that the farultraviolet flux of Oct did not vary. In particular the flux remained stable in a series of seven spectra taken consecutively over 3 hr and 24 minutes. This time interval is m... | 2022-04-01T00:00:00Z | ['Pulsating variable stars', '1307'] | The Absence of Far UV Variability in the IUE Spectra of Oct HD 215573 | 2,022 | 0 | 0.06 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2022RNAAS...6...69M/EPRINT_PDF | ['1307'] | ['Pulsating variable stars'] | ['Pulsating variable stars'] |
2023ApJ...958..159C | In 1972 early August a series of interplanetary shocks were observed in the heliosphere from 0.8 to 2.2 au. These shocks were attributed to a series of brilliant flares and plasma clouds since at that time coronal mass ejections CMEs and their interplanetary counterparts ICMEs were unknown to the scientific community. ... | 2023-12-01T00:00:00Z | ['Solar activity', 'Interplanetary shocks', 'Solar flares', 'Solar coronal mass ejections', '1475', '829', '1496', '310'] | Interplanetary Signatures during the 1972 Early August Solar Storms | 2,023 | 0 | 0.35 | 1 | https://ui.adsabs.harvard.edu/link_gateway/2023ApJ...958..159C/EPRINT_PDF | ['1475', '829', '1496', '310'] | ['Solar activity', 'Interplanetary shocks', 'Solar flares', 'Solar coronal mass ejections'] | ['Solar activity', 'Interplanetary shocks', 'Solar flares', 'Solar coronal mass ejections'] |
2020ApJ...899...43C | Observations show that particle velocity distributions in space plasmas generally exhibit a nonMaxwellian highenergy tail that can be well fitted with kappa distributions. To better understand the correlation between realistic particle velocity distributions and plasma wave excitation we investigate the linear cyclotro... | 2020-08-01T00:00:00Z | ['Van Allen radiation belt', 'Planetary magnetosphere', 'Space plasmas', '1758', '997', '1544'] | Effects of Superthermal Plasmas on the Linear Growth of Multiband EMIC Waves | 2,020 | 0 | 0.23 | 8 | https://ui.adsabs.harvard.edu/link_gateway/2020ApJ...899...43C/EPRINT_PDF | ['1758', '997', '1544'] | ['Van Allen radiation belts', 'Planetary magnetospheres', 'Space plasmas'] | ['Van Allen radiation belts', 'Planetary magnetospheres', 'Space plasmas'] |
2020ApJ...888...10T | Electron excitation collision strengths and transition probabilities Avalues for the ironpeak element Cr II lines are of high importance for the stellar and nebular abundance studies. Collision and radiative parameters are presented for all possible inelastic transitions between the Cr II 512 finestructure levels cove... | 2020-01-01T00:00:00Z | ['Atomic spectroscopy', 'Laboratory astrophysics', '2099', '2004'] | Collision and Radiative Parameters for Cr II Lines Observed in Stellar and Nebular Spectra | 2,020 | 0 | 0.22 | 7 | https://ui.adsabs.harvard.edu/link_gateway/2020ApJ...888...10T/EPRINT_PDF | ['2099', '2004'] | ['Atomic spectroscopy', 'Laboratory astrophysics'] | ['Atomic spectroscopy', 'Laboratory astrophysics'] |
2020ApJ...892...10J | Energetic ions in Mercurys magnetosphere are very dynamic similar to those in the magnetosphere of Earth. In this study we present two energetic proton observations by MErcury Surface Space ENvironment GEochemistry and Ranging near the cusp region of Mercury. For one case we have observed a large flux of energetic prot... | 2020-03-01T00:00:00Z | ['Plasma physics', 'Mercury (planet)', 'Planetary magnetospheres', 'Space plasmas', '2089', '1024', '997', '1544'] | Energetic Ion Dynamics Near the Cusp Region of Mercury | 2,020 | 0 | 0.18 | 4 | https://ui.adsabs.harvard.edu/link_gateway/2020ApJ...892...10J/EPRINT_PDF | ['2089', '1024', '997', '1544'] | ['Plasma physics', 'Mercury (planet)', 'Planetary magnetospheres', 'Space plasmas'] | ['Plasma physics', 'Mercury (planet)', 'Planetary magnetospheres', 'Space plasmas'] |
2020ApJ...891..100S | Pyroxenes Ca Mg Fe MnSUB2SUBSiSUB2SUBOSUB6SUB belong to the most abundant rock forming minerals that make up the surface of rocky planets and moons. Therefore sputtering of pyroxenes by solar wind ions has to be considered as a very important process for modifying the surface of planetary bodies. This is increased due ... | 2020-03-01T00:00:00Z | ['Solar wind', 'Exosphere', 'The Moon', 'Lunar composition', 'Mercury (planet)', 'Laboratory astrophysics', '1534', '499', '1692', '948', '1024', '2004'] | Dynamic Potential Sputtering of Lunar Analog Material by Solar Wind Ions | 2,020 | 0 | 0.34 | 24 | https://ui.adsabs.harvard.edu/link_gateway/2020ApJ...891..100S/EPRINT_PDF | ['1534', '499', '1692', '948', '1024', '2004'] | ['Solar wind', 'Exosphere', 'The Moon', 'Lunar composition', 'Mercury (planet)', 'Laboratory astrophysics'] | ['Solar wind', 'Exosphere', 'The Moon', 'Lunar composition', 'Mercury (planet)', 'Laboratory astrophysics'] |
2021pds..data..144R | This collection contains electron browse data from the Plasma experiment PLS on Voyager 1 from the Saturn encounter. The data includes 96 second averages of the electron 105950 eV density and temperature measurements. | 2021-01-01T00:00:00Z | ['1', '10-5950', '96', 'PDS', 'PDS4', 'average', 'browse', 'collection', 'contains', 'data', 'density', 'electron', 'encounter', 'ev', 'experiment', 'includes', 'measurement', 'plasma', 'pls', 'saturn', 'science', 'second', 'temperature', 'titan', 'voyager'] | Voyager 1 Plasma Science Experiment PLS Saturn Derived Electron Browse 96 Second Data Collection | 2,021 | 0 | 0.06 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2021pds..data..144R/EPRINT_PDF | ['1', '96'] | ['Unknown', 'Particle astrophysics'] | ['Unknown', 'Particle astrophysics'] |
2020ApJ...893...83T | Recent numerical simulations of rotating stellar convection have suggested the possible existence of retrograde slow equator fast poles or socalled antisolar differential rotation states in slowly rotating stars possessing a large Rossby number. We aim to understand whether such rotational states exist from the onset o... | 2020-04-01T00:00:00Z | ['Stellar convective zones', 'Stellar interiors', 'Astrophysical fluid dynamics', 'Internal waves', 'Stellar rotation', '301', '1606', '101', '819', '1629'] | Assessment of Critical Convection and Associated Rotation States in Models of Sunlike Stars Including a Stable Layer | 2,020 | 0 | 0.25 | 5 | https://ui.adsabs.harvard.edu/link_gateway/2020ApJ...893...83T/EPRINT_PDF | ['301', '1606', '101', '819', '1629'] | ['Stellar convective zones', 'Stellar interiors', 'Astrophysical fluid dynamics', 'Internal waves', 'Stellar rotation'] | ['Stellar convective zones', 'Stellar interiors', 'Astrophysical fluid dynamics', 'Internal waves', 'Stellar rotation'] |
2020ApJ...894...41R | It has been suggested by Weinberg et al. that an instability due to the nonlinear coupling of a neutron stars tide to its p and gmodes could affect the gravitationalwave phase evolution of a neutron star binary. Weinberg suggests that this instability can turn on as the gravitational waves pass through the sensitive ba... | 2020-05-01T00:00:00Z | ['Neutron stars', 'Close binary stars', 'Gravitational waves', 'Compact binary stars', '1108', '254', '678', '283'] | Constraints on Nonlinear Tides due to pg Mode Coupling from the Neutron Star Merger GW170817 | 2,020 | 0 | 0.23 | 6 | https://ui.adsabs.harvard.edu/link_gateway/2020ApJ...894...41R/EPRINT_PDF | ['1108', '254', '678', '283'] | ['Neutron stars', 'Close binary stars', 'Gravitational waves', 'Compact binary stars'] | ['Neutron stars', 'Close binary stars', 'Gravitational waves', 'Compact binary stars'] |
2023RNAAS...7..113S | Photometric H observations of the young open cluster King 16 have been used to search for emissionline stars. Seven cluster members with enhanced H emission are identified of which five are new discoveries. Three of these newly found objects have a nearinfrared excess which suggests they may be Herbig AeBe stars. H emi... | 2023-06-01T00:00:00Z | ['Be stars', 'Herbig Ae/Be stars', 'Open star clusters', '142', '723', '1160'] | A Photometric H Survey of the Open Cluster King 16 | 2,023 | 0 | 0.31 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2023RNAAS...7..113S/EPRINT_PDF | ['142', '723', '1160'] | ['Be stars', 'Herbig Ae/Be stars', 'Open star clusters'] | ['Be stars', 'Herbig Ae/Be stars', 'Open star clusters'] |
2021pds..data..153V | This collection contains Voyager 2 Jupiter CRS derived pulse height ion one hour averaged data | 2021-01-01T00:00:00Z | ['2', 'PDS', 'PDS4', 'averaged', 'collection', 'contains', 'cosmic', 'cr', 'data', 'derived', 'ganymede', 'height', 'hour', 'ion', 'jupiter', 'one', 'pulse', 'ray', 'subsystem', 'voyager'] | Voyager 2 Jupiter CRS Derived Pulse Height Ion Averaged Data Collection | 2,021 | 0 | 0 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2021pds..data..153V/EPRINT_PDF | ['2'] | ['53 Persei stars'] | ['53 Persei stars'] |
2021pds..data..152V | This collection contains Voyager 2 Jupiter CRS 15 minute averaged ion data. | 2021-01-01T00:00:00Z | ['15', '2', 'PDS', 'PDS4', 'averaged', 'collection', 'contains', 'cosmic', 'cr', 'data', 'ganymede', 'ion', 'jupiter', 'minute', 'ray', 'subsystem', 'voyager'] | Voyager 2 Jupiter CRS Derived Ion Averaged Data Collection | 2,021 | 0 | 0 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2021pds..data..152V/EPRINT_PDF | ['15', '2'] | ['Achondrites', '53 Persei stars'] | ['Achondrites', '53 Persei stars'] |
2021pds..data..141R | This collection contains electron fit data from the Plasma experiment PLS on Voyager 1 from the Saturn encounter. The data includes 96 second res. density and temperature measurements for various types of electrons 105950 eV. | 2021-01-01T00:00:00Z | ['1', '10-5950', '96', 'PDS', 'PDS4', 'collection', 'contains', 'data', 'density', 'electron', 'encounter', 'ev', 'experiment', 'fit', 'includes', 'measurement', 'plasma', 'pls', 're', 'saturn', 'science', 'second', 'temperature', 'titan', 'type', 'various', 'voyager'] | Voyager 1 Plasma Science Experiment PLS Saturn Derived Electron Parameters 96 Second Data Collection | 2,021 | 0 | 0 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2021pds..data..141R/EPRINT_PDF | ['1', '96'] | ['Unknown', 'Particle astrophysics'] | ['Unknown', 'Particle astrophysics'] |
2021pds..data..139R | This collection contains ion browse data from the Plasma experiment PLS on Voyager 1 from the Saturn encounter. The data includes 96 second density temperature and velocity components for proton and heavy ions. | 2021-01-01T00:00:00Z | ['1', '96', 'PDS', 'PDS4', 'browse', 'collection', 'component', 'contains', 'data', 'density', 'encounter', 'experiment', 'heavy', 'includes', 'ion', 'plasma', 'pls', 'proton', 'saturn', 'science', 'second', 'temperature', 'titan', 'velocity', 'voyager'] | Voyager 1 Plasma Science Experiment PLS Saturn Derived Ion Fits Browse 96 Second Data Collection | 2,021 | 0 | 0 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2021pds..data..139R/EPRINT_PDF | ['1', '96'] | ['Unknown', 'Particle astrophysics'] | ['Unknown', 'Particle astrophysics'] |
2021pds..data..137R | This collection contains Voyager 1 Plasma PLS ion data from the Saturns magnetosheath. The data includes 96 second data of the ion mass charge density velocity and thermal speed for the first and second ion species. | 2021-01-01T00:00:00Z | ['1', '96', 'PDS', 'PDS4', 'charge', 'collection', 'contains', 'data', 'density', 'experiment', 'first', 'includes', 'ion', 'magnetosheath', 'mass', 'plasma', 'pls', 'saturn', "saturn's", 'science', 'second', 'specie', 'speed', 'thermal', 'titan', 'velocity', 'voyager'] | Voyager 1 Plasma Science Experiment PLS Saturn Derived Ion Magnetosheath 96 Second Data Collection | 2,021 | 0 | 0 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2021pds..data..137R/EPRINT_PDF | ['1', '96'] | ['Unknown', 'Particle astrophysics'] | ['Unknown', 'Particle astrophysics'] |
2021pds..data..138N | This collection contains Voyager 1 Saturn encounter ephemeris data in Kronographic L1 coordinates covering the period 19801110 to 19801118. The data was generated by the Voyager MAG team from Voyager SEDR. Due to inaccuracies in Voyager SEDR as well as changes in the values of some key parameters e.g. Saturnian radius ... | 2021-01-01T00:00:00Z | ['1', '1980-11-10', '1980-11-18', 'PDS', 'PDS4', 'also', 'bundle', 'change', 'collection', 'contains', 'coordinate', 'covering', 'data', 'due', 'e.g', 'encounter', 'ephemeris', 'generated', 'improved', 'inaccuracy', 'included', 'key', 'kronographic', 'l1', 'mag', 'parameter', 'period', 'radius', 'saturn', 'saturnian', ... | Voyager 1 Saturn POS Ephemeris Kronographic L1 Coords Browse SEDR Data Collection | 2,021 | 0 | 0 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2021pds..data..138N/EPRINT_PDF | ['1'] | ['Unknown'] | ['Unknown'] |
2018GeoRL..45.3615K | Here we demonstrate that changes of the North Atlantic subtropical high and its regional rainfall pattern during midHolocene precessional changes and idealized 4xCOSUB2SUB increase can both be understood as a remote response to increased land heating near North Africa. Despite different sources and patterns of radiativ... | 2018-04-01T00:00:00Z | ['3305', '3373', '3344', '3337', '3322'] | Remote Drying in the North Atlantic as a Common Response to Precessional Changes and COSUB2SUB Increase Over Land | 2,018 | 0 | 0.22 | 11 | https://ui.adsabs.harvard.edu/link_gateway/2018GeoRL..45.3615K/EPRINT_PDF | ['3305', '3373', '3344', '3337', '3322'] | ['Unknown', 'Unknown', 'Unknown', 'Unknown', 'Unknown'] | ['Unknown', 'Unknown', 'Unknown', 'Unknown', 'Unknown'] |
2019ApJ...885...25B | The relativistic mean field RMF model is considered as one of the best methods to study the nuclear system that has a high degree of isospin asymmetry and baryon density. In the present contribution we take 25 wellknown parameter sets of the RMF model to discuss the parametric dependence of the neutron and hyperon star... | 2019-11-01T00:00:00Z | ['Neutron stars', 'Compact objects', 'Nuclear astrophysics', 'Neutron star cores', '1108', '288', '1129', '1107'] | Effects of meson on the EOS Maximum Masses and Radii of Hyperon Stars | 2,019 | 0 | 0.26 | 16 | https://ui.adsabs.harvard.edu/link_gateway/2019ApJ...885...25B/EPRINT_PDF | ['1108', '288', '1129', '1107'] | ['Neutron stars', 'Compact objects', 'Nuclear astrophysics', 'Neutron star cores'] | ['Neutron stars', 'Compact objects', 'Nuclear astrophysics', 'Neutron star cores'] |
2021ApJ...909..132N | Faraday cups can measure velocity distribution functions of space plasmas and are frequent instruments on heliophysics missions. A new version of a Faraday cup instrument is in development for the Luna 26 mission and will be used for fast monitoring of the solar wind plasma parameters. The prototype of this instrument ... | 2021-03-01T00:00:00Z | ['Interplanetary dust', 'Interstellar dust', 'Solid matter physics', '821', '836', '2090'] | Detection of Dust Particles Using Faraday Cup Instruments | 2,021 | 0 | 0.25 | 3 | https://ui.adsabs.harvard.edu/link_gateway/2021ApJ...909..132N/EPRINT_PDF | ['821', '836', '2090'] | ['Interplanetary dust', 'Interstellar dust', 'Solid matter physics'] | ['Interplanetary dust', 'Interstellar dust', 'Solid matter physics'] |
2020PSJ.....1...76C | Acetylene and benzene are two common molecules formed in Titans atmosphere and are likely components of the lake evaporites. It is known that these two molecules can form a cocrystal a molecule with a structure that is unique from that of the component molecules. Thus we sought to study this cocrystal using an experime... | 2020-12-01T00:00:00Z | ['Molecular spectroscopy', 'Experimental techniques', 'Surface ices', '2095', '2078', '2117'] | Experimental Investigation of the AcetyleneBenzene Cocrystal on Titan | 2,020 | 0 | 0.23 | 7 | https://ui.adsabs.harvard.edu/link_gateway/2020PSJ.....1...76C/EPRINT_PDF | ['2095', '2078', '2117'] | ['Molecular spectroscopy', 'Experimental techniques', 'Surface ices'] | ['Molecular spectroscopy', 'Experimental techniques', 'Surface ices'] |
2020pds..data..138M | Raw data products for the Mars 2020 Perseverance Rover Hazard Cameras. | 2020-01-01T00:00:00Z | ['2020', 'PDS', 'PDS4', 'calibrated', 'camera', 'data', 'derived', 'engineering', 'hazard', 'instrument', 'mars', 'mission', 'partially', 'perseverance', 'processed', 'product', 'raw', 'rover', 'science', 'suite'] | Mars 2020 Hazard Cameras Bundle raw products | 2,020 | 0 | 0.1 | 2 | https://ui.adsabs.harvard.edu/link_gateway/2020pds..data..138M/EPRINT_PDF | ['2020'] | ['Exoplanet atmospheric variability'] | ['Exoplanet atmospheric variability'] |
2022ApJ...925..102G | We present analytic integral solutions for the secondorder induced gravitational waves GWs. After presenting all the possible secondorder source terms we calculate explicitly the solutions for the GWs induced by the linear scalar and tensor perturbations during matter and radiationdominated epochs. | 2022-01-01T00:00:00Z | ['343', '902', '678'] | Analytic Integral Solutions for Induced Gravitational Waves | 2,022 | 0 | 0.27 | 16 | https://ui.adsabs.harvard.edu/link_gateway/2022ApJ...925..102G/EPRINT_PDF | ['343', '902', '678'] | ['Cosmology', 'Large-scale structure of the universe', 'Gravitational waves'] | ['Cosmology', 'Large-scale structure of the universe', 'Gravitational waves'] |
2023RNAAS...7..207M | Analysis of coadded high resolution spectra of the chemically peculiar star HD 53929 recorded by the SWP and LWR cameras on board the International Ultraviolet Explorer yields estimates of the abundances of silicon and manganese respectively 1.5 and 6 times the solar abundances in the atmosphere of this star. The synth... | 2023-10-01T00:00:00Z | ['Chemically peculiar stars', 'Manganese stars', '226', '1004'] | New Abundance Determinations for the B9 Mn Star HD 53929 | 2,023 | 0 | 0.27 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2023RNAAS...7..207M/EPRINT_PDF | ['226', '1004'] | ['Chemically peculiar stars', 'Manganese stars'] | ['Chemically peculiar stars', 'Manganese stars'] |
2020ApJ...898...92C | The abundance of methyl formate MF HCOOCHSUB3SUB in starforming regions of the interstellar medium ISM suggests the presence of protonated MF HSUPSUPMF. However no spectroscopic data exist for isolated HSUPSUPMF. Here we address the vibrational properties of HSUPSUPMF and its HSUPSUPMFLSUBn2SUB clusters L ArNSUB2SUB b... | 2020-07-01T00:00:00Z | ['Astrochemistry', 'Laboratory astrophysics', 'Interstellar medium', 'Molecular spectroscopy', 'Chemical abundances', 'Electron impact ionization', 'Molecule destruction', '75', '2004', '847', '2095', '224', '2059', '2075'] | Vibrational Spectroscopy of a Potential Interstellar Ion Protonated Methyl Formate | 2,020 | 0 | 0.18 | 1 | https://ui.adsabs.harvard.edu/link_gateway/2020ApJ...898...92C/EPRINT_PDF | ['75', '2004', '847', '2095', '224', '2059', '2075'] | ['Astrochemistry', 'Laboratory astrophysics', 'Interstellar medium', 'Molecular spectroscopy', 'Chemical abundances', 'Electron impact ionization', 'Unknown'] | ['Astrochemistry', 'Laboratory astrophysics', 'Interstellar medium', 'Molecular spectroscopy', 'Chemical abundances', 'Electron impact ionization', 'Unknown'] |
2021pds..data..183P | PRIMASSL at the Small Bodies Node SBN of the NASA Planetary Data System PDS is a spectral library that contains the results of the PRIMitive Asteroids Spectroscopic Survey PRIMASS. As of June 2021 this library gathers spectra of about 642 asteroids from 10 families and two groups of asteroids that had been sparsely stu... | 2021-01-01T00:00:00Z | ['Asteroids', '72'] | PRIMASSL Spectra Bundle V1.0 | 2,021 | 0 | 0 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2021pds..data..183P/EPRINT_PDF | ['72'] | ['Asteroids'] | ['Asteroids'] |
2021pds..data..178R | This collection contains ancillary data describing configuration of the Voyager 1 PLS Faraday detector cups. | 2021-01-01T00:00:00Z | ['1', 'PDS', 'PDS4', 'experiment', 'plasma', 'saturn', 'science', 'titan', 'voyager'] | Voyager 1 Plasma Science Experiment PLS Saturn Faraday Cup Data Collection | 2,021 | 0 | 0 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2021pds..data..178R/EPRINT_PDF | ['1'] | ['Unknown'] | ['Unknown'] |
2021pds..data..172N | PDS4 Standards Reference version 1.16.0 2021 | 2021-01-01T00:00:00Z | ['1.16.0', '2021', 'PDS', 'PDS4', 'pds4', 'reference', 'standard', 'version'] | PDS4 Planetary Science Standards Reference Version 1.16.0 | 2,021 | 0 | 0 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2021pds..data..172N/EPRINT_PDF | ['2021'] | ['Exoplanet atmospheric composition '] | ['Exoplanet atmospheric composition '] |
2019ApJ...885..122Z | Our recent investigations indicate that interplanetary magnetic clouds MCs have a hightwist core and a weaktwist outer shell. Utilizing the velocitymodified uniformtwist forcefree flux rope model we further investigate the relationship between the twist profile of magnetic field lines and the distribution of the plasma... | 2019-11-01T00:00:00Z | ['Interplanetary magnetic fields', '824'] | The Relationship of Magnetic Twist and Plasma Motion in a Magnetic Cloud | 2,019 | 0 | 0.18 | 1 | https://ui.adsabs.harvard.edu/link_gateway/2019ApJ...885..122Z/EPRINT_PDF | ['824'] | ['Interplanetary magnetic fields'] | ['Interplanetary magnetic fields'] |
2021pds..data..166B | Terrain mesh data products for the Mars 2020 Perseverance Rover Mast Camera Zoom Camera created by the operations team. | 2021-01-01T00:00:00Z | ['2020', 'PDS', 'PDS4', 'calibrated', 'camera', 'created', 'data', 'derived', 'instrument', 'mars', 'mast', 'mastcam-zoom', 'mesh', 'mission', 'operation', 'partially', 'perseverance', 'processed', 'product', 'raw', 'rover', 'science', 'suite', 'team', 'terrain', 'zoom'] | Mars 2020 Mast Camera Zoom Bundle from Operations Team terrain mesh products | 2,021 | 0 | 0 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2021pds..data..166B/EPRINT_PDF | ['2020'] | ['Exoplanet atmospheric variability'] | ['Exoplanet atmospheric variability'] |
2021RNAAS...5..239M | Evidence is presented that lanthanides are present and overabundant in the atmosphere of the sharplined A1 V star HR 4138. This interesting object needs to be reclassified as a Chemically Peculiar star. | 2021-10-01T00:00:00Z | ['Chemical abundances', 'Chemically peculiar stars', '224', '226'] | The Occurrence of Lanthanides in the Atmosphere of the A1 V Star HR 4138 | 2,021 | 0 | 0.14 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2021RNAAS...5..239M/EPRINT_PDF | ['224', '226'] | ['Chemical abundances', 'Chemically peculiar stars'] | ['Chemical abundances', 'Chemically peculiar stars'] |
2020ApJ...897L..39N | The solar wind nonradial velocity components observed beyond the Alfvn point are usually attributed to waves the interaction of different streams or other transient phenomena. However Earthorbiting spacecraft as well as monitors at L1 indicate systematic deviations of the wind velocity from the radial direction. Since ... | 2020-07-01T00:00:00Z | ['Heliosphere', 'Solar wind', 'Fast solar wind', '711', '1534', '1872'] | Nonradial Solar Wind Propagation through the Heliosphere | 2,020 | 0 | 0.3 | 10 | https://ui.adsabs.harvard.edu/link_gateway/2020ApJ...897L..39N/EPRINT_PDF | ['711', '1534', '1872'] | ['Heliosphere', 'Solar wind', 'Fast solar wind'] | ['Heliosphere', 'Solar wind', 'Fast solar wind'] |
2022pds..data..114T | This version of the Photopolarimeter Radiometer PPR for GO bundle was created by the PDS Atmospheres node in 2022 | 2022-01-01T00:00:00Z | ['2022', 'PDS', 'PDS4', 'amalthea', 'atmosphere', 'bundle', 'callisto', 'created', 'europa', 'galileo', 'ganymede', 'gll', 'go', 'io', 'jupiter', 'node', 'orbiter', 'pct', 'pds', 'photopolarimeter', 'ppr', 'radiometer', 'rct', 'version'] | Galileo Orbiter Photopolarimeter Radiometer PPR for GO Bundle | 2,022 | 0 | 0.1 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2022pds..data..114T/EPRINT_PDF | ['2022'] | ['Exoplanet surface composition'] | ['Exoplanet surface composition'] |
2021pds..data...85H | This bundle contains the MESSENGER Energetic Particle and Plasma Spectrometer EPPS calibrated observations also known as DDRs. The system encompasses 2 instrument subsystems the Energetic Particle Spectrometer EPS and the Fast Imaging Plasma Spectrometer FIPS. This data set contains FIPS instrument data. FIPS covers t... | 2021-01-01T00:00:00Z | ['13', '2', '46', 'PDS', 'PDS4', 'also', 'bundle', 'calibrated', 'contains', 'cover', 'data', 'ddr', 'ddrs', 'earth', 'encompasses', 'energetic', 'energy/charge', 'epps', 'eps', 'ev/q', 'fast', 'fips', 'https://doi.org/10.17189/1519743', 'imaging', 'instrument', 'kev/q', 'known', 'le', 'mercury', 'mess-e/v/h/sw-epps-3-... | Messenger Epps Fips DDR Bundle | 2,021 | 0 | 0.1 | 1 | https://ui.adsabs.harvard.edu/link_gateway/2021pds..data...85H/EPRINT_PDF | ['13', '2', '46'] | ['Unknown', '53 Persei stars', 'Antapex'] | ['Unknown', '53 Persei stars', 'Antapex'] |
2021pds..data...78H | This bundle contains MESSENGER Energetic Particle and Plasma Spectrometer EPPS advanced data products also known as DDRDAPs. This bundle contains data from the Energetic Particle Spectrometer EPS subsystem. EPS covers the energy range of 25 to gt 500 keV for electrons and 10 keVnucleon to 3 MeV total energy for ions. T... | 2021-01-01T00:00:00Z | ['10', '25', '3', '500', 'PDS', 'PDS4', 'advanced', 'also', 'bundle', 'contains', 'cover', 'data', 'ddr/daps', 'earth', 'electron', 'energetic', 'energy', 'epps', 'eps', 'https://doi.org/10.17189/1519741', 'ion', 'kev', 'kev/nucleon', 'known', 'mercury', 'mess-e/v/h/sw-epps-3-eps-ddr-v1.0', 'messenger', 'mev', 'particl... | Messenger Epps EPS DDR Bundle | 2,021 | 0 | 0 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2021pds..data...78H/EPRINT_PDF | ['10', '25', '3', '500'] | ['Absolute magnitude', 'All-sky cameras', 'A dwarf stars', 'Exozodiacal dust'] | ['Absolute magnitude', 'All-sky cameras', 'A dwarf stars', 'Exozodiacal dust'] |
2021pds..data...69R | This bundle contains MESSENGER Energetic Particle and Plasma Spectrometer EPPS calibrated observations also known as CDRs. This bundle contains Fast Imaging Plasma Spectrometer FIPS instrument data. FIPS covers the energycharge range of less than 50 eVq to 20 keVq. These data were previously released as a PDS3 data set... | 2021-01-01T00:00:00Z | ['20', '50', 'PDS', 'PDS4', 'also', 'bundle', 'calibrated', 'cdrs', 'contains', 'cover', 'data', 'earth', 'energetic', 'energy/charge', 'epps', 'ev/q', 'fast', 'fips', 'https://doi.org/10.17189/1519742', 'imaging', 'instrument', 'kev/q', 'known', 'le', 'mercury', 'mess-e/v/h/sw-epps-3-fips-cdr-v1.0', 'messenger', 'obse... | MESSENGER EPPS Calibrated FIPS Data Bundle | 2,021 | 0 | 0.1 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2021pds..data...69R/EPRINT_PDF | ['20', '50'] | ['Ae stars', 'Ap stars'] | ['Ae stars', 'Ap stars'] |
2022RNAAS...6...90O | We use a nearest neighbor algorithm combined with the machine learning clustering function DensityBased Spatial Clustering of Applications with Noise to analyze a subset of quasars from the Sloan Digital Sky Survey. Our analysis shows evidence of clustering up to z 2 with evidence of an increase in clustering at lower... | 2022-05-01T00:00:00Z | ['Quasars', 'Clustering', '1319', '1908'] | The Study of Quasar Clustering at Low Redshifts | 2,022 | 0 | 0.27 | 1 | https://ui.adsabs.harvard.edu/link_gateway/2022RNAAS...6...90O/EPRINT_PDF | ['1319', '1908'] | ['Quasars', 'Clustering'] | ['Quasars', 'Clustering'] |
2021pds..data..145R | This collection contains ion fit data from the Plasma experiment PLS on Voyager 1 in Saturns magnetosphere. The data includes 96 second ion mass charge number of ion species density thermal speed velocity for the first and second ion species. | 2021-01-01T00:00:00Z | ['1', '96', 'PDS', 'PDS4', 'charge', 'collection', 'contains', 'data', 'density', 'experiment', 'first', 'fit', 'includes', 'ion', 'magnetosphere', 'mass', 'number', 'plasma', 'pls', 'saturn', "saturn's", 'science', 'second', 'specie', 'speed', 'thermal', 'titan', 'velocity', 'voyager'] | Voyager 1 Plasma Science Experiment PLS Saturn Derived Ion Fits 96 Second Data Collection | 2,021 | 0 | 0.06 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2021pds..data..145R/EPRINT_PDF | ['1', '96'] | ['Unknown', 'Particle astrophysics'] | ['Unknown', 'Particle astrophysics'] |
2023RNAAS...7...66W | Our knowledge about the multiplicity of intermediate mass A and Btype stars is still incomplete in particular for high 3 multiplicity systems. Here we report the discovery of a new companion to the nearby roAp star HIP 47145 HR 3831 with a K band flux ratio of 4 based on a VLTIGRAVITY interferometric observation. This... | 2023-04-01T00:00:00Z | ['Multiple stars', 'Ap stars', 'Optical interferometry', '1081', '50', '1168'] | Discovery of a 0.64 M SUBSUB 13.4 au Companion to the roAp Star HIP 47145 HR 3831 IM Vel | 2,023 | 0 | 0.36 | 1 | https://ui.adsabs.harvard.edu/link_gateway/2023RNAAS...7...66W/EPRINT_PDF | ['1081', '50', '1168'] | ['Multiple stars', 'Ap stars', 'Optical interferometry'] | ['Multiple stars', 'Ap stars', 'Optical interferometry'] |
2023RNAAS...7..208V | We discuss the discovery of a significant meteoric event over Don Benito Spain described in two news reports from the regional newspaper Extremadura. These reports detail intense light loud noises and shattered windows in Don Benito during 1926 December. Despite limited information this research note aims to share the ... | 2023-10-01T00:00:00Z | ['Bolides', '172'] | A Possible Superbolide Over Don Benito Spain in 1926 December 27 | 2,023 | 0 | 0.23 | 1 | https://ui.adsabs.harvard.edu/link_gateway/2023RNAAS...7..208V/EPRINT_PDF | ['172'] | ['Bolides'] | ['Bolides'] |
2023RNAAS...7...84D | In this study we used archival supernova data from a publicly available database to look for a blue excess in the early light curves of SN Ia. This blue excess represents a simple proposed method to differentiate between single and doubledegenerate formation scenarios. Our search found 2 candidates out of 40 SN Ia and ... | 2023-05-01T00:00:00Z | ['Type Ia supernovae', 'White dwarf stars', 'Degenerate matter', 'Optical astronomy', 'Light curves', 'Astronomy databases', '1728', '1799', '367', '1776', '918', '83'] | Looking for the Blue Bump in the Early Light Curve of SN Ia using an Open Supernovae Catalog | 2,023 | 0 | 0.31 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2023RNAAS...7...84D/EPRINT_PDF | ['1728', '1799', '367', '1776', '918', '83'] | ['Type Ia supernovae', 'White dwarf stars', 'Degenerate matter', 'Optical astronomy', 'Light curves', 'Astronomy databases'] | ['Type Ia supernovae', 'White dwarf stars', 'Degenerate matter', 'Optical astronomy', 'Light curves', 'Astronomy databases'] |
2021PSJ.....2...28C | The Mars Reconnaissance Orbiters Shallow Radar SHARAD emits radar signals and records their reflections from layer boundaries within the Martian north polar ice cap. Previous studies have suggested that the ice cap is composed of thin dustrich layers between thicker layers of nearly pure water ice. The prevailing hypot... | 2021-02-01T00:00:00Z | ['Planetary science', '1255'] | Lower Bounds on the Thickness and Dust Content of Layers within the North Polar Layered Deposits of Mars from Radar Forward Modeling | 2,021 | 0 | 0.26 | 15 | https://ui.adsabs.harvard.edu/link_gateway/2021PSJ.....2...28C/EPRINT_PDF | ['1255'] | ['Planetary science'] | ['Planetary science'] |
2021RNAAS...5...59M | Evidence is reported for the first time for the presence of the Hg II line in a Narval I profile of Maia the fourth brightest member of the Pleiades open cluster. The Hg II line in Maia absorbs about 2 of the local continuum and can be reproduced with an overabundance of mercury of about 4000 times the solar mercury ab... | 2021-03-01T00:00:00Z | ['Chemically peculiar stars', 'Mercury-manganese stars', '226', '1025'] | Detection of the Hg II Line at 3983.93 in One Optical Spectrum of Maia | 2,021 | 0 | 0.19 | 1 | https://ui.adsabs.harvard.edu/link_gateway/2021RNAAS...5...59M/EPRINT_PDF | ['226', '1025'] | ['Chemically peculiar stars', 'Mercury-manganese stars'] | ['Chemically peculiar stars', 'Mercury-manganese stars'] |
2021RNAAS...5...37M | The farUV spectral energy distribution of Dor recorded by IUE is compared to that of the constant and normal star Dra which has similar fundamental parameters. Dor has much less flux than Dra shortwards of 1800 due to the accumulation of very strong absorption lines of Si II in particular autoionization lines arou... | 2021-02-01T00:00:00Z | ['Bp stars', '178'] | The Large Farultraviolet Flux Deficiency of Doradus B8 IIIp Si | 2,021 | 0 | 0.1 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2021RNAAS...5...37M/EPRINT_PDF | ['178'] | ['Bp stars'] | ['Bp stars'] |
2021RNAAS...5...81M | Evidence is presented that the far ultraviolet flux of Maia recorded by the International Ultraviolet Explorer is variable over a timescale of a few hours. In contrast the radial velocity of the Si II doublet near 1530 does not vary on short timescales. | 2021-04-01T00:00:00Z | ['Chemically peculiar stars', '226'] | The Rapid Farultraviolet Variability of Maia Recorded by IUE | 2,021 | 0 | 0.21 | 3 | https://ui.adsabs.harvard.edu/link_gateway/2021RNAAS...5...81M/EPRINT_PDF | ['226'] | ['Chemically peculiar stars'] | ['Chemically peculiar stars'] |
2020ApJ...901..167M | The stability of the pickup ions in the outer heliosheath is a vital factor in the generation of the energetic neutral atom ENA ribbon observed by the Interstellar Boundary EXplorer according to the secondary ENA mechanism. Most previous studies of the pickup ion stability assumed simple idealized velocity distribution... | 2020-10-01T00:00:00Z | ['Heliosphere', 'Heliosheath', 'Heliopause', 'Pickup ions', '711', '710', '707', '1239'] | Mirror Instability Driven by Pickup Ions in the Outer Heliosheath | 2,020 | 0 | 0.27 | 12 | https://ui.adsabs.harvard.edu/link_gateway/2020ApJ...901..167M/EPRINT_PDF | ['711', '710', '707', '1239'] | ['Heliosphere', 'Heliosheath', 'Heliopause', 'Pickup ions'] | ['Heliosphere', 'Heliosheath', 'Heliopause', 'Pickup ions'] |
2020ApJ...893...55Z | We carried out a statistical study on the effects of strong geomagnetic activity on the mesopause over the auroral region from 2002 to 2018. When the auroral electrojet index increased significantly the energetic electron precipitation from the Medium Energy Proton and Electron Detector was enhanced by several multiple... | 2020-04-01T00:00:00Z | ['Earth atmosphere', 'Mesopause', 'Mesosphere', 'Aeronomy', '437', '1029', '1030', '22'] | Response of the Highlatitude Upper Mesosphere to Energetic Electron Precipitation | 2,020 | 0 | 0.18 | 3 | https://ui.adsabs.harvard.edu/link_gateway/2020ApJ...893...55Z/EPRINT_PDF | ['437', '1029', '1030', '22'] | ['Earth atmosphere', 'Mesopause', 'Mesosphere', 'Aeronomy'] | ['Earth atmosphere', 'Mesopause', 'Mesosphere', 'Aeronomy'] |
2022pds..data...39P | This bundle contains raw radio data that can be used to determine the position and velocity of the MESSENGER spacecraft during flybys of Venus and Mercury and during orbital operations around Mercury. The bundle also contains measurements of occultation times and calibrations for the effects of Earths ionosphere and tr... | 2022-01-01T00:00:00Z | ['14', '15', '24', '25', '26', '34', '35', '43', '45', '54', '55', '63', '65', 'PDS', 'PDS4', 'activity', 'also', 'antenna', 'archive', 'around', 'bundle', 'calibration', 'change', 'condition', 'contains', 'correction', 'data', 'deep', 'determine', 'ds', 'dsn', 'earth', "earth's", 'effect', 'environment', 'ephemeris', ... | MESSENGER RSS Raw Data Bundle | 2,022 | 0 | 0 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2022pds..data...39P/EPRINT_PDF | ['14', '15', '24', '25', '26', '34', '35', '43', '45', '54', '55', '63', '65'] | ['Accretion', 'Achondrites', 'Algol variable stars', 'All-sky cameras', 'Almanacs', 'Amateur astronomers', 'Amateur astronomy', 'Annular eclipses', 'Ansae', 'Apex', 'Aphelion', 'Apsides', 'Argument of perigee'] | ['Accretion', 'Achondrites', 'Algol variable stars', 'All-sky cameras', 'Almanacs', 'Amateur astronomers', 'Amateur astronomy', 'Annular eclipses', 'Ansae', 'Apex', 'Aphelion', 'Apsides', 'Argument of perigee'] |
2022pds..data...97G | This collection contains the documents associated with the Galileo Heavy Ion Counter Derived Ion Fluxes October 89 Solar Event Calibrated Bundle. | 2022-01-01T00:00:00Z | ['89', 'PDS', 'PDS4', 'associated', 'bundle', 'calibrated', 'collection', 'contains', 'counter', 'derived', 'document', 'event', 'flux', 'galileo', 'heavy', 'ion', 'october', 'orbiter', 'solar', 'system'] | Galileo HIC Derived Ion Fluxes October 89 Solar Event Document Collection | 2,022 | 0 | 0 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2022pds..data...97G/EPRINT_PDF | ['89'] | ['Astronomical radiation sources'] | ['Astronomical radiation sources'] |
2022pds..data..117N | This document collection contains all the standards documentation for the NASA PDS Version 3 Standards including all known versions of the PDS3 Standards Reference SR Data Dictionary DD Data Providers Handbook DPH and Design Document. | 2022-01-01T00:00:00Z | ['3', 'PDS', 'PDS4', 'collection', 'contains', 'data', 'dd', 'design', 'dictionary', 'document', 'documentation', 'dph', 'handbook', 'including', 'known', 'nasa', 'pds', 'pds3', "provider's", 'reference', 'sr', 'standard', 'version'] | PDS3 Standards Collection | 2,022 | 0 | 0.06 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2022pds..data..117N/EPRINT_PDF | ['3'] | ['A dwarf stars'] | ['A dwarf stars'] |
2022pds..data..123N | PDS4 Standards Reference version 1.18.0 2022 | 2022-01-01T00:00:00Z | ['1.18.0', '2022', 'PDS', 'PDS4', 'pds4', 'reference', 'standard', 'version'] | PDS4 Planetary Science Standards Reference Version 1.18.0 | 2,022 | 0 | 0 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2022pds..data..123N/EPRINT_PDF | ['2022'] | ['Exoplanet surface composition'] | ['Exoplanet surface composition'] |
2022pds..data..129G | 2020 PDART NEAR MSI updated deblurr algorithm. | 2022-01-01T00:00:00Z | ['433', 'PDS', 'PDS4', 'asteroid', 'earth', 'eros', 'imager', 'multi-spectral', 'near', 'raw', 'rendezvous', 'science'] | NEAR MSI Deblurred Images | 2,022 | 0 | 0.06 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2022pds..data..129G/EPRINT_PDF | ['433'] | ['Early astronomical instruments'] | ['Early astronomical instruments'] |
2022pds..data..128N | PDS4 Concepts version 1.18.0 2022 | 2022-01-01T00:00:00Z | ['1.18.0', '2022', 'PDS', 'PDS4', 'concept', 'pds4', 'version'] | PDS4 Planetary Science Concepts Version 1.18.0 | 2,022 | 0 | 0 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2022pds..data..128N/EPRINT_PDF | ['2022'] | ['Exoplanet surface composition'] | ['Exoplanet surface composition'] |
2022pds..data..127N | PDS4 Concepts version 1.19.0 2022 | 2022-01-01T00:00:00Z | ['1.19.0', '2022', 'PDS', 'PDS4', 'concept', 'pds4', 'version'] | PDS4 Planetary Science Concepts Version 1.19.0 | 2,022 | 0 | 0 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2022pds..data..127N/EPRINT_PDF | ['2022'] | ['Exoplanet surface composition'] | ['Exoplanet surface composition'] |
2022pds..data..126N | PDS4 Data Providers Handbook DPH version 1.18.0 2022 | 2022-01-01T00:00:00Z | ['1.18.0', '2022', 'PDS', 'PDS4', 'data', 'dph', 'handbook', 'pds4', "provider's", 'version'] | PDS4 Planetary Science Data Providers Handbook DPH Version 1.18.0 | 2,022 | 0 | 0 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2022pds..data..126N/EPRINT_PDF | ['2022'] | ['Exoplanet surface composition'] | ['Exoplanet surface composition'] |
2023ApJ...955...14G | Recent spacecraft observations have shown that magnetic reconnection occurs commonly in turbulent environments at shocks. At quasiperpendicular shocks magnetic field lines are bent by the backstreaming reflected ions which form a current sheet in the foot region and then electronscale reconnection occurs when the curre... | 2023-09-01T00:00:00Z | ['Space plasmas', 'Plasma physics', 'Solar magnetic reconnection', 'Planetary bow shocks', '1544', '2089', '1504', '1246'] | Properties of Electronscale Magnetic Reconnection at a Quasiperpendicular Shock | 2,023 | 0 | 0.25 | 3 | https://ui.adsabs.harvard.edu/link_gateway/2023ApJ...955...14G/EPRINT_PDF | ['1544', '2089', '1504', '1246'] | ['Space plasmas', 'Plasma physics', 'Solar magnetic reconnection', 'Planetary bow shocks'] | ['Space plasmas', 'Plasma physics', 'Solar magnetic reconnection', 'Planetary bow shocks'] |
2021PSJ.....2..180N | While it has long been known that Titans haze and atmosphere are dynamic on seasonal timescales recent results have revealed that they also exhibit significant subseasonal variations. Here we report on observations of Titan acquired over an eightmonth period between 2014 April and 2015 March with the Spectrograph for I... | 2021-10-01T00:00:00Z | ['Ground-based astronomy', 'Atmospheric variability', 'Saturnian satellites', '686', '2119', '1427'] | Tracking Shortterm Variations in the Haze Distribution of Titans Atmosphere with SINFONI VLT | 2,021 | 0 | 0.27 | 1 | https://ui.adsabs.harvard.edu/link_gateway/2021PSJ.....2..180N/EPRINT_PDF | ['686', '2119', '1427'] | ['Ground-based astronomy', 'Atmospheric variability', 'Saturnian satellites'] | ['Ground-based astronomy', 'Atmospheric variability', 'Saturnian satellites'] |
2024ApJ...963...64Y | Space plasmas are turbulent and maintain different types of critical points or flow nulls. Electron vortex as one type of flow null structure is crucial in the energy cascade in turbulent plasmas. However due to the limited time resolution of the spacecraft observations one can never analyze the threedimensional proper... | 2024-03-01T00:00:00Z | ['Plasma physics', 'Space plasmas', 'Plasma astrophysics', '2089', '1544', '1261'] | Reconstruction of Electron Vortex in Space Plasmas | 2,024 | 0 | 0.3 | 1 | https://ui.adsabs.harvard.edu/link_gateway/2024ApJ...963...64Y/EPRINT_PDF | ['2089', '1544', '1261'] | ['Plasma physics', 'Space plasmas', 'Plasma astrophysics'] | ['Plasma physics', 'Space plasmas', 'Plasma astrophysics'] |
2024PSJ.....5...27P | We analyze the polarization observations of the DidymosDimorphos system before and after the impact by the NASA Double Asteroid Redirection Test spacecraft on Dimorphos. We fit empirical polarization phase curve models and statistically confirm the discovery by Gray et al. about the degree of linear polarization of the... | 2024-01-01T00:00:00Z | ['Asteroid surfaces', 'Near-Earth objects', 'Polarimetry', '2209', '1092', '1278'] | Modeling Linear Polarization of the DidymosDimorphos System before and after the DART Impact | 2,024 | 0 | 0.42 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2024PSJ.....5...27P/EPRINT_PDF | ['2209', '1092', '1278'] | ['Asteroid surfaces', 'Near-Earth objects', 'Polarimetry'] | ['Asteroid surfaces', 'Near-Earth objects', 'Polarimetry'] |
2022pds..data...55H | An Examination of Soil Crusts on the Floor of Jezero crater Mars | 2022-01-01T00:00:00Z | ['2020', 'PDS', 'PDS4', 'crater', 'crust', 'derived', 'examination', 'floor', 'jezero', 'mars', 'pixl', 'science', 'soil', 'spectrometer'] | An Examination of Soil Crusts on the Floor of Jezero crater Mars | 2,022 | 0 | 0.06 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2022pds..data...55H/EPRINT_PDF | ['2020'] | ['Exoplanet atmospheric variability'] | ['Exoplanet atmospheric variability'] |
2022pds..data...50K | This bundle contains the Voyager 2 Plasma Wave Spectrometer spectrum analyzer data from the entire mission in calibrated CDF files | 2022-01-01T00:00:00Z | ['2', 'PDS', 'PDS4', 'analyzer', 'bundle', 'calibrated', 'cdf', 'contains', 'data', 'entire', 'file', 'jupiter', 'mission', 'neptune', 'plasma', 'saturn', 'science', 'solar', 'spectrometer', 'spectrum', 'system', 'uranus', 'voyager', 'wave'] | Voyager 2 PWS Low Rate Spectrum Analyzer Data Bundle | 2,022 | 0 | 0 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2022pds..data...50K/EPRINT_PDF | ['2'] | ['53 Persei stars'] | ['53 Persei stars'] |
2022pds..data...51K | This bundle contains Voyager 1 Plasma Wave Spectrometer PWS raw waveform data and documentation for all available telemetry frames from SCET 19780821T054136.299Z through 20220205T081807.031Z. | 2022-01-01T00:00:00Z | ['1', '1978-08-21t05:41:36.299z', '2022-02-05t08:18:07.031z', 'PDS', 'PDS4', 'available', 'bundle', 'contains', 'data', 'documentation', 'frame', 'interstellar', 'jupiter', 'medium', 'partially', 'particle', 'plasma', 'processed', 'pws', 'raw', 'saturn', 'scet', 'science', 'solar', 'spectrometer', 'telemetry', 'voyager... | Voyager 1 Plasma Wave Science Uncalibrated Waveforms Entire Mission Bundle | 2,022 | 0 | 0 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2022pds..data...51K/EPRINT_PDF | ['1'] | ['Unknown'] | ['Unknown'] |
2022pds..data...47S | Data from the Ultraviolet Spectrometer instruments on the Mariner 6 and Mariner 7 spacecrafts. | 2022-01-01T00:00:00Z | ['6', '69', '7', 'PDS', 'PDS4', 'data', 'instrument', 'mariner', 'mars', 'spacecraft', 'spectrometer', 'ultraviolet'] | Mariner 6 and 7 Ultraviolet Spectrometer Bundle | 2,022 | 0 | 0 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2022pds..data...47S/EPRINT_PDF | ['6', '69', '7'] | ['A subdwarf stars', 'Ascending node', 'A subgiant stars'] | ['A subdwarf stars', 'Ascending node', 'A subgiant stars'] |
2022pds..data...43K | These are reprocessed measurements by the Engergetic Particle Detector EPD instrument onboard the Galileo spacecraft that orbited Jupiter and measured intensities of ion and electron radiation in the keV and MeV energy range. This set is version 31 of reprocessing and version 1.0 of PDS delivery. The TOFxE and DeltaExE... | 2022-01-01T00:00:00Z | ['1.0', '1.000000e+38', '31', 'PDS', 'PDS4', 'ambient', 'cannot', 'channelized', 'column', 'comma', 'continuously', 'counted', 'data', 'delivery', 'deltaexe', 'deposited', 'detector', 'different', 'downlinked', 'electron', 'energetic', 'energy', 'energy_kev', 'engergetic', 'entry', 'epd', 'epd/cms/tofxe', 'event', 'eve... | Galileo EPD Calibrated Corrected TimeofFlight Event Data Collection | 2,022 | 0 | 0 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2022pds..data...43K/EPRINT_PDF | ['31'] | ['AM Canum Venaticorum stars'] | ['AM Canum Venaticorum stars'] |
2022pds..data...15N | This collection contains Voyager 2 Jupiter encounter magnetometer data given in Heliographic coordinates and averaged from the 60 ms instrument sample rate to a 1.92 second resampled rate. All magnetic field observations are measured in nanoTesla. All of the magnetic field data are calibrated. | 2022-01-01T00:00:00Z | ['1.92', '2', '60', 'PDS', 'PDS4', 'averaged', 'calibrated', 'collection', 'contains', 'coordinate', 'data', 'encounter', 'field', 'fluxgate', 'ganymede', 'given', 'heliographic', 'instrument', 'jupiter', 'm', 'magnetic', 'magnetometer', 'measured', 'nanotesla', 'observation', 'rate', 'resampled', 'sample', 'second', '... | Voyager 2 Magnetometer Jupiter Resampled Heliographic RTN Coords 1.92 Second Data Collection | 2,022 | 0 | 0 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2022pds..data...15N/EPRINT_PDF | ['2', '60'] | ['53 Persei stars', 'Apparent position'] | ['53 Persei stars', 'Apparent position'] |
2022pds..data...11R | This bundle contains Venus Express cleaned highresolution 128 Hz magnetic field data acquired by the fluxgate magnetometer gradiometer onboard the Venus Express spacecraft. The data are expressed in Venus Solar Orbital VSO coordinates and RadialEastNorth coordinates. This work was funded by a 2017 NASA ROSES SSW propos... | 2022-01-01T00:00:00Z | ['128', '2017', 'PDS', 'PDS4', 'acquired', 'bundle', 'cleaned', 'contains', 'coordinate', 'data', 'express', 'expressed', 'field', 'fluxgate', 'funded', 'gradiometer', 'grant', 'high-resolution', 'hz', 'magnetic', 'magnetometer', 'nasa', 'nnh17zda001n-ssw', 'number', 'onboard', 'orbital', 'proposal', 'radial-east-north... | Venus Express Cleaned HighResolution 128 Hz Magnetic Field Data Bundle | 2,022 | 0 | 0.06 | 1 | https://ui.adsabs.harvard.edu/link_gateway/2022pds..data...11R/EPRINT_PDF | ['128', '2017'] | ['B stars', 'AGN host galaxies'] | ['B stars', 'AGN host galaxies'] |
2022pds..data...16N | This collection contains Voyager 2 Jupiter encounter magnetometer data given in Heliographic coordinates and averaged from the 60 ms instrument sample rate to a 9.6 second resampled rate. All magnetic field observations are measured in nanoTesla. All of the magnetic field data are calibrated. | 2022-01-01T00:00:00Z | ['2', '60', '9.6', 'PDS', 'PDS4', 'averaged', 'calibrated', 'collection', 'contains', 'coordinate', 'data', 'encounter', 'field', 'fluxgate', 'ganymede', 'given', 'heliographic', 'instrument', 'jupiter', 'm', 'magnetic', 'magnetometer', 'measured', 'nanotesla', 'observation', 'rate', 'resampled', 'sample', 'second', 't... | Voyager 2 Magnetometer Jupiter Resampled Heliographic RTN Coords 9.60 Second Data Collection | 2,022 | 0 | 0 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2022pds..data...16N/EPRINT_PDF | ['2', '60'] | ['53 Persei stars', 'Apparent position'] | ['53 Persei stars', 'Apparent position'] |
2022pds..data...31L | This bundle contains the results from the simulation study presented in Lapenta G. Schriver D. Walker R. J. Berchem J. Echterling N. F. El Alaoui M. Travnicek P. Do we need to consider electrons kinetic effects to properly model a planetary magnetosphere the case of Mercury JGR 2022. httpsdoi.org The data includes full... | 2022-01-01T00:00:00Z | ['2017', '2022', '80nssc19k0789', '80nssc19k0841', '80nssc19k0846', '80nssc21k0053', 'PDS', 'PDS4', 'advanced', 'alaoui', 'along', 'ames', 'berchem', 'bundle', 'case', 'center', 'code', 'computer', 'computing', 'conserving', 'consider', 'contains', 'data', 'derived', 'division', 'doi:10.1016/j.jcp.2017.01.002', 'echter... | Do we need to consider electrons kinetic effects to properly model a planetary magnetosphere the case of Mercury simulation data bundle | 2,022 | 0 | 0 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2022pds..data...31L/EPRINT_PDF | ['2017', '2022'] | ['AGN host galaxies', 'Exoplanet surface composition'] | ['AGN host galaxies', 'Exoplanet surface composition'] |
2023ApJ...953....8S | The expandingbox model of the solar wind has been adopted in the literature within the context of magnetohydrodynamics hybrid and full particleincell simulations to investigate the dynamic evolution of the solar wind. The present paper extends such a method to the framework of selfconsistent quasilinear kinetic theory.... | 2023-08-01T00:00:00Z | ['Solar wind', '1534'] | Expandingbox Quasilinear Model of the Solar Wind | 2,023 | 0 | 0.34 | 5 | https://ui.adsabs.harvard.edu/link_gateway/2023ApJ...953....8S/EPRINT_PDF | ['1534'] | ['Solar wind'] | ['Solar wind'] |
2022ApJS..261...18G | The Interstellar Boundary Explorer IBEX is a NASA satellite in Earth orbit dedicated to observing both interstellar neutral atoms entering the heliosphere and energetic neutral atoms ENAs from the interstellar boundaries from roughly 10 eV to 6 keV. This work presents the averaged maps energy spectra and temporal varia... | 2022-08-01T00:00:00Z | ['Heliosphere', 'Heliosheath', '711', '710'] | One Solar Cycle of Heliosphere Observations with the Interstellar Boundary Explorer Energetic Neutral Hydrogen Atoms Observed with IBEXLo from 10 eV to 2 keV | 2,022 | 0 | 0.34 | 5 | https://ui.adsabs.harvard.edu/link_gateway/2022ApJS..261...18G/EPRINT_PDF | ['711', '710'] | ['Heliosphere', 'Heliosheath'] | ['Heliosphere', 'Heliosheath'] |
2022pds..data..115S | This version of the Ultraviolet Spectrometer UVS for GO bundle was created by the PDS Atmospheres node in 2022 | 2022-01-01T00:00:00Z | ['2022', 'PDS', 'PDS4', 'atmosphere', 'bundle', 'callisto', 'created', 'europa', 'galileo', 'ganymede', 'go', 'io', 'jupiter', 'node', 'orbiter', 'pds', 'plasma', 'spectrometer', 'star', 'torus', 'ultraviolet', 'uv', 'version'] | Galileo Orbiter Ultraviolet Spectrometer UVS for GO Bundle | 2,022 | 0 | 0.1 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2022pds..data..115S/EPRINT_PDF | ['2022'] | ['Exoplanet surface composition'] | ['Exoplanet surface composition'] |
2024RNAAS...8...97B | This paper employs machine learning to estimate stellar temperatures using photometric data focusing on the GAIA ESA Archive Data Release 3 data set. The study underscores the effectiveness of neural networks in deciphering intricate relationships within the data. Notably the addition of metallicity improves model accu... | 2024-04-01T00:00:00Z | ['Photometric systems', 'Photometry', 'Stellar effective temperatures', 'Neural networks', 'Outlier detection', '1233', '1234', '1597', '1933', '1934'] | Enhancing Stellar Temperature Estimation through Machine Learning and Multifaceted Data Exploration | 2,024 | 0 | 0.22 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2024RNAAS...8...97B/EPRINT_PDF | ['1233', '1234', '1597', '1933', '1934'] | ['Photometric systems', 'Photometry', 'Stellar effective temperatures', 'Neural networks', 'Outlier detection'] | ['Photometric systems', 'Photometry', 'Stellar effective temperatures', 'Neural networks', 'Outlier detection'] |
2020AJ....160...48C | The subject of the present paper is the analysis of the orbital solutions for eight binaries WDS 024020436 HDS 347 WDS 025525950 MLR 520 WDS 031196131 HDS 407 WDS 045707350 YSC 145 WDS 052024105 HDS 701 WDS 064670822 HDS 940AB WDS 082591623 HDS 1199 and WDS 225505132 HU 785. Seven orbits are determined for the ... | 2020-07-01T00:00:00Z | ['Fundamental parameters of stars', 'Visual binary stars', '555', '1777'] | Orbits for Eight Binaries | 2,020 | 0 | 0.31 | 6 | https://ui.adsabs.harvard.edu/link_gateway/2020AJ....160...48C/EPRINT_PDF | ['555', '1777'] | ['Fundamental parameters of stars', 'Visual binary stars'] | ['Fundamental parameters of stars', 'Visual binary stars'] |
2020ApJ...895....8C | The deexcitation ray lines in solar flares result from energetic ions e.g. protons particles interacting with the ambient nuclei in the solar atmosphere. The centroid and width of lines contain a wealth of information on the directionality composition and spectra of energetic ions as well as properties of the interacti... | 2020-05-01T00:00:00Z | ['The Sun', 'Solar flares', 'Solar gamma-ray emission', 'Solar energetic particles', '1693', '1496', '1497', '1491'] | A Spectroscopic Method Based on the Shapes of Nuclear Deexcitation Ray Lines in Solar Flares | 2,020 | 0 | 0.28 | 3 | https://ui.adsabs.harvard.edu/link_gateway/2020ApJ...895....8C/EPRINT_PDF | ['1693', '1496', '1497', '1491'] | ['The Sun', 'Solar flares', 'Solar gamma-ray emission', 'Solar energetic particles'] | ['The Sun', 'Solar flares', 'Solar gamma-ray emission', 'Solar energetic particles'] |
2019ApJ...882L..17M | Lunar indigenous Xe isotopic abundances provide crucial information on relationships not only between gas reservoirs in the solar protoplanetary disk but also regarding planetary fractionation processes and possible space weather effects due to an active young Sun. The indigenous lunar Xe isotopic composition is not ye... | 2019-09-01T00:00:00Z | ['Lunar origin', 'Solar abundances', 'Planetary atmospheres', 'Isotopic abundances', '966', '1474', '1244', '867'] | Lunar Xenon and the Origin of the Indigenous Component | 2,019 | 0 | 0.17 | 2 | https://ui.adsabs.harvard.edu/link_gateway/2019ApJ...882L..17M/EPRINT_PDF | ['966', '1474', '1244', '867'] | ['Lunar origin', 'Solar abundances', 'Planetary atmospheres', 'Isotopic abundances'] | ['Lunar origin', 'Solar abundances', 'Planetary atmospheres', 'Isotopic abundances'] |
2021RNAAS...5...54M | The abundances of several elements in the atmosphere of the HgMn star 14 Sge HR 7664 are derived from the analysis of highresolution spectra obtained recently with the spectropolarimeter NeoNarval. A large phosphorus overabundance about 60 times the solar abundance is found. This study is the beginning of a systematic ... | 2021-03-01T00:00:00Z | ['Chemically peculiar stars', '226'] | The Abundance of Phosphorus in the HgMn Star 14 Sge | 2,021 | 0 | 0.26 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2021RNAAS...5...54M/EPRINT_PDF | ['226'] | ['Chemically peculiar stars'] | ['Chemically peculiar stars'] |
2022RNAAS...6..267M | The analysis of two spectra of the Mn Hg star HD 29589 recorded by the SWP camera on board the International Ultraviolet Explorer does not reveal variations of the farultraviolet flux over a thirteen years time interval. The TESS lightcurve of HD 29589 shows a complex pattern of oscillations with variable amplitudes an... | 2022-12-01T00:00:00Z | ['Chemically peculiar stars', 'Mercury-manganese stars', '226', '1025'] | The Behavior of HgMn Stars in the Far UVPaper 21 HD 29589 | 2,022 | 0 | 0.12 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2022RNAAS...6..267M/EPRINT_PDF | ['226', '1025'] | ['Chemically peculiar stars', 'Mercury-manganese stars'] | ['Chemically peculiar stars', 'Mercury-manganese stars'] |
2022RNAAS...6..238M | The analysis of the coadded high resolution SWP spectrum of the Hg star HD 209459 recorded by the International Ultraviolet Explorer reveals the presence of two resonance lines of Hg II at 1649.92 and 1942.28 . The line synthesis of the least blended resonance line at 1942.28 yields a mercury abundance of about 1000 t... | 2022-11-01T00:00:00Z | ['Chemically peculiar stars', 'Mercury-manganese stars', '226', '1025'] | The Mercury Lines in the Mean Far Ultraviolet Spectrum of HD 209459 | 2,022 | 0 | 0.18 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2022RNAAS...6..238M/EPRINT_PDF | ['226', '1025'] | ['Chemically peculiar stars', 'Mercury-manganese stars'] | ['Chemically peculiar stars', 'Mercury-manganese stars'] |
2020ApJ...901...20L | Recently an electronscale coherent structure known as a magnetic hole MH was observed in the Earths magnetosheath. It has been found that the MH is characterized by decreasing magnetic field strength and increasing parameters such as electron density temperature and temperature anisotropy. Observations suggest that ele... | 2020-09-01T00:00:00Z | ['Magnetic fields', 'Space plasmas', 'Plasma jets', '994', '1544', '1263'] | In Situ Evidence of a Magnetic Hole Downstream of the Magnetic Reconnection in the Magnetopause Reconnection | 2,020 | 0 | 0.23 | 2 | https://ui.adsabs.harvard.edu/link_gateway/2020ApJ...901...20L/EPRINT_PDF | ['994', '1544', '1263'] | ['Magnetic fields', 'Space plasmas', 'Plasma jets'] | ['Magnetic fields', 'Space plasmas', 'Plasma jets'] |
2023RNAAS...7...11M | The analysis of five spectra of the Hg Mn spectroscopic binary star HD 77350 recorded by the SWP camera on board the International Ultraviolet Explorer reveals one instance of variation of the farultraviolet flux of this star shortwards of 1800 . The analysis of the coadded SWP spectrum built from the high resolution S... | 2023-01-01T00:00:00Z | ['Chemically peculiar stars', 'Mercury-manganese stars', '226', '1025'] | The Behavior of HgMn Stars in the Far UVPaper 25 HD 77350 | 2,023 | 0 | 0.18 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2023RNAAS...7...11M/EPRINT_PDF | ['226', '1025'] | ['Chemically peculiar stars', 'Mercury-manganese stars'] | ['Chemically peculiar stars', 'Mercury-manganese stars'] |
2023RNAAS...7...49M | The analysis of seventeen spectra of the Bp Heweak star HD 125823 recorded by the SWP camera on board the International Ultraviolet Explorer reveals no variations of the farultraviolet spectral energy distribution of this star over a time interval of three years. However line variations are present in the range 1400 up... | 2023-03-01T00:00:00Z | ['Chemically peculiar stars', 'Helium-weak stars', '226', '717'] | The Behavior of Bp Heweak Stars in the Far UVPaper 2 HD 125823 | 2,023 | 0 | 0.2 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2023RNAAS...7...49M/EPRINT_PDF | ['226', '717'] | ['Chemically peculiar stars', 'Helium-weak stars'] | ['Chemically peculiar stars', 'Helium-weak stars'] |
2020ApJ...888L..16C | Both magnetic reconnection and turbulence can play crucial roles in space plasmas. The current layers developing during magnetic reconnection can collapse into various smallscale coherent structures such as current filaments. These current filaments can significantly modulate the kineticscale turbulence. However the qu... | 2020-01-01T00:00:00Z | ['Interplanetary turbulence', 'Space plasmas', 'Plasma jets', '830', '1544', '1263'] | Relationship between Current Filaments and Turbulence During a Turbulent Reconnection | 2,020 | 0 | 0.27 | 5 | https://ui.adsabs.harvard.edu/link_gateway/2020ApJ...888L..16C/EPRINT_PDF | ['830', '1544', '1263'] | ['Interplanetary turbulence', 'Space plasmas', 'Plasma jets'] | ['Interplanetary turbulence', 'Space plasmas', 'Plasma jets'] |
2020ApJ...888...25M | The first laboratory evidence of a radiative shock RS decelerating during its free expansion phase in an optically thick medium is presented. A shock is generated in a multilayer solid target under the irradiation of a highpower laser at the GEKKO XII laser facility. The rear surface of the target is connected to a gas... | 2020-01-01T00:00:00Z | ['Laboratory astrophysics', 'Experimental techniques', 'Shocks', '2004', '2078', '2086'] | Laboratory Observation of Radiative Shock Deceleration and Application to SN 1987A | 2,020 | 0 | 0.26 | 4 | https://ui.adsabs.harvard.edu/link_gateway/2020ApJ...888...25M/EPRINT_PDF | ['2004', '2078', '2086'] | ['Laboratory astrophysics', 'Experimental techniques', 'Shocks'] | ['Laboratory astrophysics', 'Experimental techniques', 'Shocks'] |
2020ApJ...897...75G | A newly calculated ab initio potential energy surface is used to compute collisiondriven statechanging cross sections and rate coefficients over a range from 5 to 100 K for CNSUPSUPSUP1SUP the smallest anion detected in the interstellar medium interacting with He an abundant species in this environment. We compare our ... | 2020-07-01T00:00:00Z | ['Diffuse molecular clouds', 'Molecular clouds', 'Molecular physics', 'Collision processes', 'Radiative processes', 'De-excitation rates', 'Excitation rates', '2058', '2065', '1072', '2055', '381', '2066', '2067'] | Rotationally Inelastic Collisions of CNSUPSUP with He Computing Cross Sections and Rates in the Interstellar Medium | 2,020 | 0 | 0.24 | 11 | https://ui.adsabs.harvard.edu/link_gateway/2020ApJ...897...75G/EPRINT_PDF | ['2058', '2065', '1072', '2055', '381', '2066', '2067'] | ['Molecular physics', 'Collision physics', 'Molecular clouds', 'Radiative processes', 'Diffuse molecular clouds', 'De-excitation rates', 'Excitation rates'] | ['Molecular physics', 'Collision physics', 'Molecular clouds', 'Radiative processes', 'Diffuse molecular clouds', 'De-excitation rates', 'Excitation rates'] |
2020ApJ...896..103B | The migrations of solid objects throughout the solar system are thought to have played key roles in disk evolution and planet formation. However our understanding of these migrations is limited by a lack of quantitative constraints on their timings and distances recovered from laboratory measurements of meteorites. The... | 2020-06-01T00:00:00Z | ['Meteorites', 'Magnetic fields', 'Primordial magnetic fields', 'Asteroid belt', 'Kuiper belt', 'Protoplanetary disks', 'Chondrules', 'Chondrites', '1038', '994', '1294', '70', '893', '1300', '229', '228'] | Constraints on the Distances and Timescales of Solid Migration in the Early Solar System from Meteorite Magnetism | 2,020 | 0 | 0.34 | 25 | https://ui.adsabs.harvard.edu/link_gateway/2020ApJ...896..103B/EPRINT_PDF | ['1038', '994', '1294', '70', '893', '1300', '229', '228'] | ['Meteorites', 'Magnetic fields', 'Primordial magnetic fields', 'Asteroid belt', 'Kuiper belt', 'Protoplanetary disks', 'Chondrules', 'Chondrites'] | ['Meteorites', 'Magnetic fields', 'Primordial magnetic fields', 'Asteroid belt', 'Kuiper belt', 'Protoplanetary disks', 'Chondrules', 'Chondrites'] |
2022RNAAS...6...19J | In this work I estimate the number of close stellar encounters on a specific crosssectional area that may contain a planetary disk in a crowded star formation cluster. The approximation employs Monte Carlo runs to estimate the most likely value of the number of encounters as a function of stellar densities from 1.6 10... | 2022-01-01T00:00:00Z | ['363', '490', '1184', '1300', '1596'] | Estimation of the Number of Stellar Encounters on a Crosssectional Area containing a Planetary Disk in Birth Clusters of Stars | 2,022 | 0 | 0.23 | 2 | https://ui.adsabs.harvard.edu/link_gateway/2022RNAAS...6...19J/EPRINT_PDF | ['363', '490', '1184', '1300', '1596'] | ['Debris disks', 'Exoplanet dynamics', 'Orbits', 'Protoplanetary disks', 'Stellar dynamics'] | ['Debris disks', 'Exoplanet dynamics', 'Orbits', 'Protoplanetary disks', 'Stellar dynamics'] |
2020RNAAS...4...93G | We analyze the environmental features and growth history of highredshift halos from cosmological simulation data to determine the conditions that lead to Population III star formation. We use supportvector classification SVC to determine the separation in featurespace between Population III halos and halos that form no... | 2020-06-01T00:00:00Z | ['Population III stars', 'Galaxy formation', '1285', '595'] | Halo Environment for Population III Star Formation | 2,020 | 0 | 0.25 | 0 | https://ui.adsabs.harvard.edu/link_gateway/2020RNAAS...4...93G/EPRINT_PDF | ['1285', '595'] | ['Population III stars', 'Galaxy formation'] | ['Population III stars', 'Galaxy formation'] |
2020ApJ...888...39L | The synthesis of chlorinebearing species in CO ice was studied by the irradiation of CHSUB3SUBClCO ice at 10 K with vacuumultraviolet VUV light and energetic electrons. In contrast to the photochemical behavior of CHSUB3SUBFCO ice photolysis of CHSUB3SUBClCO ice with Ly or broadband VUV light afforded various products.... | 2020-01-01T00:00:00Z | ['Astrochemistry', 'Molecular spectroscopy', 'Line positions', 'Molecule formation', 'Galaxy chemical evolution', 'Chemical abundances', '75', '2095', '2085', '2076', '580', '224'] | Formation of Halogenbearing Species. II. Irradiation of Chloromethane in Carbon Monoxide Ice with VUV Light and Electrons | 2,020 | 0 | 0.14 | 1 | https://ui.adsabs.harvard.edu/link_gateway/2020ApJ...888...39L/EPRINT_PDF | ['75', '2095', '2085', '2076', '580', '224'] | ['Astrochemistry', 'Molecular spectroscopy', 'Line positions', 'Unknown', 'Galaxy chemical evolution', 'Chemical abundances'] | ['Astrochemistry', 'Molecular spectroscopy', 'Line positions', 'Unknown', 'Galaxy chemical evolution', 'Chemical abundances'] |
2020ApJ...889...40S | The deuteriumhydrogen DH ratio of primordial water partitioned into a planetary interior seems to be different on Earth and Mars. Water from volcanic rocks originating from Earths deep mantle has a low DH ratio with high SUP3SUPHeSUP4SUPHe ratios implying that it was inherited partially from the solar nebula. In contra... | 2020-01-01T00:00:00Z | ['Mars', 'Planet formation', 'Earth (planet)', 'Planetary atmospheres', 'Planetary science', '1007', '1241', '439', '1244', '1255'] | DH Ratio in the Interiors of Rocky Protoplanets Accreting in the Solar Nebula | 2,020 | 0 | 0.25 | 5 | https://ui.adsabs.harvard.edu/link_gateway/2020ApJ...889...40S/EPRINT_PDF | ['1007', '1241', '439', '1244', '1255'] | ['Mars', 'Planet formation', 'Earth (planet)', 'Planetary atmospheres', 'Planetary science'] | ['Mars', 'Planet formation', 'Earth (planet)', 'Planetary atmospheres', 'Planetary science'] |
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