Search Publications

The Complete Light-curve Sample of Spectroscopically Confirmed SNe Ia from Pan-STARRS1 and Cosmological Constraints from the Combined Pantheon Sample
DOI: 10.3847/1538-4357/aab9bb Bibcode: 2018ApJ...859..101S

Berger, E.; Kirshner, R. P.; Rest, A. +37 more

We present optical light curves, redshifts, and classifications for 365 spectroscopically confirmed Type Ia supernovae (SNe Ia) discovered by the Pan-STARRS1 (PS1) Medium Deep Survey. We detail improvements to the PS1 SN photometry, astrometry, and calibration that reduce the systematic uncertainties in the PS1 SN Ia distances. We combine the subs…

2018 The Astrophysical Journal
Planck eHST 2313
Milky Way Cepheid Standards for Measuring Cosmic Distances and Application to Gaia DR2: Implications for the Hubble Constant
DOI: 10.3847/1538-4357/aac82e Bibcode: 2018ApJ...861..126R

Casertano, Stefano; Filippenko, Alexei V.; Riess, Adam G. +9 more

We present Hubble Space Telescope (HST) photometry of a selected sample of 50 long-period, low-extinction Milky Way Cepheids measured on the same WFC3 F555W-, F814W-, and F160W-band photometric system as extragalactic Cepheids in Type Ia supernova host galaxies. These bright Cepheids were observed with the WFC3 spatial scanning mode in the optical…

2018 The Astrophysical Journal
Gaia eHST 601
First data release of the Hyper Suprime-Cam Subaru Strategic Program
DOI: 10.1093/pasj/psx081 Bibcode: 2018PASJ...70S...8A

Ono, Yoshiaki; Ouchi, Masami; Momose, Rieko +107 more

The Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP) is a three-layered imaging survey aimed at addressing some of the most important outstanding questions in astronomy today, including the nature of dark matter and dark energy. The survey has been awarded 300 nights of observing time at the Subaru Telescope, and it started in 2014 March. This…

2018 Publications of the Astronomical Society of Japan
eHST 588
Gaia Data Release 2. Catalogue validation
DOI: 10.1051/0004-6361/201833234 Bibcode: 2018A&A...616A..17A

Jordi, C.; Luri, X.; Cantat-Gaudin, T. +35 more

Context. The second Gaia data release (DR2) contains very precise astrometric and photometric properties for more than one billion sources, astrophysical parameters for dozens of millions, radial velocities for millions, variability information for half a million stars from selected variability classes, and orbits for thousands of solar system obj…

2018 Astronomy and Astrophysics
Gaia eHST 552
A catalogue of masses, structural parameters, and velocity dispersion profiles of 112 Milky Way globular clusters
DOI: 10.1093/mnras/sty1057 Bibcode: 2018MNRAS.478.1520B

Hilker, M.; Baumgardt, H.

We have determined masses, stellar mass functions, and structural parameters of 112 Milky Way globular clusters by fitting a large set of N-body simulations to their velocity dispersion and surface density profiles. The velocity dispersion profiles were calculated based on a combination of more than 15000 high-precision radial velocities which we …

2018 Monthly Notices of the Royal Astronomical Society
eHST 452
New Parallaxes of Galactic Cepheids from Spatially Scanning the Hubble Space Telescope: Implications for the Hubble Constant
DOI: 10.3847/1538-4357/aaadb7 Bibcode: 2018ApJ...855..136R

Casertano, Stefano; Anderson, Jay; Filippenko, Alexei V. +8 more

We present new measurements of the parallax of seven long-period (≥10 days) Milky Way (MW) Cepheid variables (SS CMa, XY Car, VY Car, VX Per, WZ Sgr, X Pup, and S Vul) using one-dimensional astrometric measurements from spatial scanning of Wide-Field Camera 3 on the Hubble Space Telescope (HST). The observations were obtained at ∼6 month intervals…

2018 The Astrophysical Journal
Gaia INTEGRAL eHST 449
The Dearth of z ∼ 10 Galaxies in All HST Legacy Fields—The Rapid Evolution of the Galaxy Population in the First 500 Myr
DOI: 10.3847/1538-4357/aab03f Bibcode: 2018ApJ...855..105O

Oesch, P. A.; Bouwens, R. J.; Illingworth, G. D. +2 more

We present an analysis of all prime HST legacy fields spanning >800 arcmin2 in the search for z ∼ 10 galaxy candidates and the study of their UV luminosity function (LF). In particular, we present new z ∼ 10 candidates selected from the full Hubble Frontier Field (HFF) data set. Despite the addition of these new fields, we find a low…

2018 The Astrophysical Journal
eHST 369
A galaxy lacking dark matter
DOI: 10.1038/nature25767 Bibcode: 2018Natur.555..629V

Mowla, Lamiya; van Dokkum, Pieter; Romanowsky, Aaron J. +9 more

Studies of galaxy surveys in the context of the cold dark matter paradigm have shown that the mass of the dark matter halo and the total stellar mass are coupled through a function that varies smoothly with mass. Their average ratio Mhalo/Mstars has a minimum of about 30 for galaxies with stellar masses near that of the Milky…

2018 Nature
eHST 343
ALMA Survey of Lupus Protoplanetary Disks. II. Gas Disk Radii
DOI: 10.3847/1538-4357/aab890 Bibcode: 2018ApJ...859...21A

Guidi, G.; Testi, L.; Hogerheijde, M. +10 more

We present Atacama Large Millimeter/Sub-Millimeter Array (ALMA) Band 6 observations of a complete sample of protoplanetary disks in the young (∼1-3 Myr) Lupus star-forming region, covering the 1.33 mm continuum and the 12CO, 13CO, and C18O J = 2-1 lines. The spatial resolution is ∼0.″25 with a medium 3σ continuum s…

2018 The Astrophysical Journal
eHST 342
The Binary Neutron Star Event LIGO/Virgo GW170817 160 Days after Merger: Synchrotron Emission across the Electromagnetic Spectrum
DOI: 10.3847/2041-8213/aab2ad Bibcode: 2018ApJ...856L..18M

Berger, E.; Chornock, R.; Fong, W. +17 more

We report deep Chandra X-ray Observatory (CXO), Hubble Space Telescope (HST), and Karl J. Jansky Very Large Array (VLA) observations of the binary neutron star event GW170817 at t < 160 days after merger. These observations show that GW170817 has been steadily brightening with time and might have now reached its peak, and constrain the emission…

2018 The Astrophysical Journal
eHST 334