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LSST: From Science Drivers to Reference Design and Anticipated Data Products
DOI: 10.3847/1538-4357/ab042c Bibcode: 2019ApJ...873..111I

Aubourg, Éric; Strauss, Michael A.; Anderson, Scott F. +324 more

We describe here the most ambitious survey currently planned in the optical, the Large Synoptic Survey Telescope (LSST). The LSST design is driven by four main science themes: probing dark energy and dark matter, taking an inventory of the solar system, exploring the transient optical sky, and mapping the Milky Way. LSST will be a large, wide-fiel…

2019 The Astrophysical Journal
Gaia 3899
Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics beyond ΛCDM
DOI: 10.3847/1538-4357/ab1422 Bibcode: 2019ApJ...876...85R

Casertano, Stefano; Riess, Adam G.; Yuan, Wenlong +2 more

We present an improved determination of the Hubble constant from Hubble Space Telescope (HST) observations of 70 long-period Cepheids in the Large Magellanic Cloud (LMC). These were obtained with the same WFC3 photometric system used to measure extragalactic Cepheids in the hosts of SNe Ia. Gyroscopic control of HST was employed to reduce overhead…

2019 The Astrophysical Journal
Gaia eHST 1873
A 3D Dust Map Based on Gaia, Pan-STARRS 1, and 2MASS
DOI: 10.3847/1538-4357/ab5362 Bibcode: 2019ApJ...887...93G

Speagle, Joshua S.; Zucker, Catherine; Finkbeiner, Douglas +2 more

We present a new three-dimensional map of dust reddening, based on Gaia parallaxes and stellar photometry from Pan-STARRS 1 and 2MASS. This map covers the sky north of a decl. of -30°, out to a distance of a few kiloparsecs. This new map contains three major improvements over our previous work. First, the inclusion of Gaia parallaxes dramatically …

2019 The Astrophysical Journal
Gaia 1031
The Carnegie-Chicago Hubble Program. VIII. An Independent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch
DOI: 10.3847/1538-4357/ab2f73 Bibcode: 2019ApJ...882...34F

Madore, Barry F.; Freedman, Wendy L.; Beaton, Rachael L. +10 more

We present a new and independent determination of the local value of the Hubble constant based on a calibration of the tip of the red giant branch (TRGB) applied to Type Ia supernovae (SNe Ia). We find a value of H 0 = 69.8 ± 0.8 (±1.1% stat) ± 1.7 (±2.4% sys) km s-1 Mpc-1. The TRGB method is both precise and accur…

2019 The Astrophysical Journal
Gaia eHST 748
The Optical to Mid-infrared Extinction Law Based on the APOGEE, Gaia DR2, Pan-STARRS1, SDSS, APASS, 2MASS, and WISE Surveys
DOI: 10.3847/1538-4357/ab1c61 Bibcode: 2019ApJ...877..116W

Wang, Shu; Chen, Xiaodian

A precise interstellar dust extinction law is critically important to interpret observations. There are two indicators of extinction: the color excess ratio (CER) and the relative extinction. Compared to the CER, the wavelength-dependent relative extinction is more challenging to be determined. In this work, we combine spectroscopic, astrometric, …

2019 The Astrophysical Journal
Gaia 379
The Circular Velocity Curve of the Milky Way from 5 to 25 kpc
DOI: 10.3847/1538-4357/aaf648 Bibcode: 2019ApJ...871..120E

Hogg, David W.; Rix, Hans-Walter; Ness, Melissa K. +1 more

We measure the circular velocity curve v c(R) of the Milky Way with the highest precision to date across Galactocentric distances of 5 ≤ R ≤ 25 kpc. Our analysis draws on the six-dimensional phase-space coordinates of ≳23,000 luminous red giant stars, for which we previously determined precise parallaxes using a data-driven model that c…

2019 The Astrophysical Journal
Gaia 355
Kinematics in Young Star Clusters and Associations with Gaia DR2
DOI: 10.3847/1538-4357/aaef8c Bibcode: 2019ApJ...870...32K

Sills, Alison; Feigelson, Eric D.; Hillenbrand, Lynne A. +2 more

The Gaia mission has opened a new window into the internal kinematics of young star clusters at the sub-km s-1 level, with implications for our understanding of how star clusters form and evolve. We use a sample of 28 clusters and associations with ages from ∼1-5 Myr, where lists of members are available from previous X-ray, optical, an…

2019 The Astrophysical Journal
Gaia eHST 296
How to Constrain Your M Dwarf. II. The Mass-Luminosity-Metallicity Relation from 0.075 to 0.70 Solar Masses
DOI: 10.3847/1538-4357/aaf3bc Bibcode: 2019ApJ...871...63M

Gaidos, Eric; Rizzuto, Aaron C.; Kraus, Adam L. +11 more

The mass-luminosity relation for late-type stars has long been a critical tool for estimating stellar masses. However, there is growing need for both a higher-precision relation and a better understanding of systematic effects (e.g., metallicity). Here we present an empirical relationship between {M}{KS} and M * sp…

2019 The Astrophysical Journal
Gaia eHST 291
Water Vapor and Clouds on the Habitable-zone Sub-Neptune Exoplanet K2-18b
DOI: 10.3847/2041-8213/ab59dc Bibcode: 2019ApJ...887L..14B

Fortney, Jonathan J.; Knutson, Heather A.; Howard, Andrew W. +13 more

Results from the Kepler mission indicate that the occurrence rate of small planets (<3 R ) in the habitable zone of nearby low-mass stars may be as high as 80%. Despite this abundance, probing the conditions and atmospheric properties on any habitable-zone planet is extremely difficult and has remained elusive to date. Here, we repo…

2019 The Astrophysical Journal
Gaia eHST 262
A Large Catalog of Accurate Distances to Local Molecular Clouds: The Gaia DR2 Edition
DOI: 10.3847/1538-4357/ab2388 Bibcode: 2019ApJ...879..125Z

Alves, João; Speagle, Joshua S.; Zucker, Catherine +4 more

We present a uniform catalog of accurate distances to local molecular clouds informed by the Gaia DR2 data release. Our methodology builds on that of Schlafly et al. First, we infer the distance and extinction to stars along sightlines toward the clouds using optical and near-infrared photometry. When available, we incorporate knowledge of the ste…

2019 The Astrophysical Journal
Gaia 230