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The Second APOKASC Catalog: The Empirical Approach
DOI: 10.3847/1538-4365/aaebfd Bibcode: 2018ApJS..239...32P

Chaplin, William J.; Cunha, Katia; Smith, Verne V. +33 more

We present a catalog of stellar properties for a large sample of 6676 evolved stars with Apache Point Observatory Galactic Evolution Experiment spectroscopic parameters and Kepler asteroseismic data analyzed using five independent techniques. Our data include evolutionary state, surface gravity, mean density, mass, radius, age, and the spectroscop…

2018 The Astrophysical Journal Supplement Series
Gaia 257
Gaia DR2 proper motions of dwarf galaxies within 420 kpc. Orbits, Milky Way mass, tidal influences, planar alignments, and group infall
DOI: 10.1051/0004-6361/201833343 Bibcode: 2018A&A...619A.103F

Fritz, T. K.; Battaglia, G.; Brook, C. +5 more

A proper understanding of the Milky Way (MW) dwarf galaxies in a cosmological context requires knowledge of their 3D velocities and orbits. However, proper motion (PM) measurements have generally been of limited accuracy and are available only for more massive dwarfs. We therefore present a new study of the kinematics of the MW dwarf galaxies. We …

2018 Astronomy and Astrophysics
Gaia 255
Discovery of pulsations from NGC 300 ULX1 and its fast period evolution
DOI: 10.1093/mnrasl/sly030 Bibcode: 2018MNRAS.476L..45C

Haberl, F.; Vasilopoulos, G.; Maitra, C. +1 more

The supernova impostor SN 2010da located in the nearby galaxy NGC 300, later identified as a likely supergiant B[e] high-mass X-ray binary, was simultaneously observed by NuSTAR and XMM-Newton between 2016 December 16 and 20, over a total time span of ∼310 ks. We report the discovery of a strong periodic modulation in the X-ray flux with a pulse p…

2018 Monthly Notices of the Royal Astronomical Society
XMM-Newton 250
The optical afterglow of the short gamma-ray burst associated with GW170817
DOI: 10.1038/s41550-018-0511-3 Bibcode: 2018NatAs...2..751L

Im, M.; Pian, E.; Palazzi, E. +33 more

The binary neutron star merger GW170817 was the first multi-messenger event observed in both gravitational and electromagnetic waves1,2. The electromagnetic signal began approximately two seconds post-merger with a weak, short burst of gamma rays3, which was followed over the next hours and days by the ultraviolet, optical an…

2018 Nature Astronomy
eHST 248
Dark Energy Survey Year 1 Results: The Photometric Data Set for Cosmology
DOI: 10.3847/1538-4365/aab4f5 Bibcode: 2018ApJS..235...33D

Benoit-Lévy, A.; Bechtol, K.; Smith, M. +87 more

We describe the creation, content, and validation of the Dark Energy Survey (DES) internal year-one cosmology data set, Y1A1 GOLD, in support of upcoming cosmological analyses. The Y1A1 GOLD data set is assembled from multiple epochs of DES imaging and consists of calibrated photometric zero-points, object catalogs, and ancillary data products—e.g…

2018 The Astrophysical Journal Supplement Series
Gaia eHST 247
Solar wind stream interaction regions throughout the heliosphere
DOI: 10.1007/s41116-017-0011-z Bibcode: 2018LRSP...15....1R

Richardson, Ian G.

This paper focuses on the interactions between the fast solar wind from coronal holes and the intervening slower solar wind, leading to the creation of stream interaction regions that corotate with the Sun and may persist for many solar rotations. Stream interaction regions have been observed near 1 AU, in the inner heliosphere (at

2018 Living Reviews in Solar Physics
Ulysses 242
Elucidating ΛCDM: Impact of Baryon Acoustic Oscillation Measurements on the Hubble Constant Discrepancy
DOI: 10.3847/1538-4357/aaa1ed Bibcode: 2018ApJ...853..119A

Halpern, M.; Weiland, J. L.; Hinshaw, G. +3 more

We examine the impact of baryon acoustic oscillation (BAO) scale measurements on the discrepancy between the value of the Hubble constant (H 0) inferred from the local distance ladder and that from Planck cosmic microwave background (CMB) data. While the BAO data alone cannot constrain H 0, we show that combining the latest B…

2018 The Astrophysical Journal
Planck 240
Planetary Spectrum Generator: An accurate online radiative transfer suite for atmospheres, comets, small bodies and exoplanets
DOI: 10.1016/j.jqsrt.2018.05.023 Bibcode: 2018JQSRT.217...86V

Villanueva, G. L.; Smith, M. D.; Faggi, S. +2 more

We have developed an online radiative-transfer suite (https://psg.gsfc.nasa.gov) applicable to a broad range of planetary objects (e.g., planets, moons, comets, asteroids, TNOs, KBOs, exoplanets). The Planetary Spectrum Generator (PSG) can synthesize planetary spectra (atmospheres and surfaces) for a broad range of wavelengths (UV/Vis/near-IR/IR/f…

2018 Journal of Quantitative Spectroscopy and Radiative Transfer
ExoMars-16 237
H- Opacity and Water Dissociation in the Dayside Atmosphere of the Very Hot Gas Giant WASP-18b
DOI: 10.3847/2041-8213/aab272 Bibcode: 2018ApJ...855L..30A

Fortney, Jonathan J.; Stevenson, Kevin B.; Désert, Jean-Michel +7 more

We present one of the most precise emission spectra of an exoplanet observed so far. We combine five secondary eclipses of the hot Jupiter WASP-18b (T day ∼ 2900 K) that we secured between 1.1 and 1.7 µm with the Wide Field Camera 3 instrument on board the Hubble Space Telescope. Our extracted spectrum (S/N = 50, R ∼ 40) does not …

2018 The Astrophysical Journal
eHST 236
Macromolecular organic compound s from the depths of Enceladus
DOI: 10.1038/s41586-018-0246-4 Bibcode: 2018Natur.558..564P

Postberg, Frank; Trieloff, Mario; Schmidt, Jürgen +18 more

Saturn's moon Enceladus harbours a global water ocean, which lies under an ice crust and above a rocky core. Through warm cracks in the crust a cryo-volcanic plume ejects ice grains and vapour into space that contain materials originating from the ocean. Hydrothermal activity is suspected to occur deep inside the porous core, powered by tidal diss…

2018 Nature
Cassini 234