Search Publications

Close Binary Companions to APOGEE DR16 Stars: 20,000 Binary-star Systems Across the Color-Magnitude Diagram
DOI: 10.3847/1538-4357/ab8acc Bibcode: 2020ApJ...895....2P

Green, Paul J.; Hogg, David W.; Majewski, Steven R. +21 more

Many problems in contemporary astrophysics—from understanding the formation of black holes to untangling the chemical evolution of galaxies—rely on knowledge about binary stars. This, in turn, depends on the discovery and characterization of binary companions for large numbers of different kinds of stars in different chemical and dynamical environ…

2020 The Astrophysical Journal
Gaia 107
The Sloan Digital Sky Survey Reverberation Mapping Project: Estimating Masses of Black Holes in Quasars with Single-epoch Spectroscopy
DOI: 10.3847/1538-4357/abbc1c Bibcode: 2020ApJ...903..112D

Brandt, W. N.; Shen, Yue; Peterson, Bradley M. +19 more

It is well known that reverberation mapping of active galactic nuclei (AGNs) reveals a relationship between AGN luminosity and the size of the broad-line region, and that use of this relationship, combined with the Doppler width of the broad emission line, enables an estimate of the mass of the black hole at the center of the active nucleus based …

2020 The Astrophysical Journal
eHST 106
The MOSDEF Survey: The Variation of the Dust Attenuation Curve with Metallicity
DOI: 10.3847/1538-4357/aba35e Bibcode: 2020ApJ...899..117S

Siana, Brian; Azadi, Mojegan; Shivaei, Irene +14 more

We derive a UV-optical stellar dust attenuation curve of galaxies at z = 1.4-2.6 as a function of gas-phase metallicity. We use a sample of 218 star-forming galaxies, excluding those with very young or heavily obscured star formation, from the MOSFIRE Deep Evolution Field survey with Hα, Hβ, and [N II]λ 6585 spectroscopic measurements. We constrai…

2020 The Astrophysical Journal
eHST 104
A Mildly Relativistic Outflow from the Energetic, Fast-rising Blue Optical Transient CSS161010 in a Dwarf Galaxy
DOI: 10.3847/2041-8213/ab8cc7 Bibcode: 2020ApJ...895L..23C

Lundqvist, P.; Reichart, D. E.; Kochanek, C. S. +35 more

We present X-ray and radio observations of the Fast Blue Optical Transient CRTS-CSS161010 J045834-081803 (CSS161010 hereafter) at t = 69-531 days. CSS161010 shows luminous X-ray (LX ∼ 5 × 1039 erg s-1) and radio (Lν ∼ 1029 erg s-1 Hz-1) emission. The radio emission peaked…

2020 The Astrophysical Journal
INTEGRAL 101
The Zwicky Transient Facility Census of the Local Universe. I. Systematic Search for Calcium-rich Gap Transients Reveals Three Related Spectroscopic Subclasses
DOI: 10.3847/1538-4357/abb45c Bibcode: 2020ApJ...905...58D

Kulkarni, S. R.; Rusholme, Ben; Kaplan, David L. +49 more

Using the Zwicky Transient Facility alert stream, we are conducting a large spectroscopic campaign to construct a complete, volume-limited sample of transients brighter than 20 mag, and coincident within 100″ of galaxies in the Census of the Local Universe catalog. We describe the experiment design and spectroscopic completeness from the first 16 …

2020 The Astrophysical Journal
Gaia 100
The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: CO Excitation and Atomic Carbon in Star-forming Galaxies at z = 1-3
DOI: 10.3847/1538-4357/abb82f Bibcode: 2020ApJ...902..109B

Carilli, Chris; Inami, Hanae; Boogaard, Leindert A. +16 more

We investigate the CO excitation and interstellar medium (ISM) conditions in a cold gas mass-selected sample of 22 star-forming galaxies at z = 0.46-3.60, observed as part of the ALMA Spectroscopic Survey in the Hubble Ultra Deep Field (ASPECS). Combined with Very Large Array follow-up observations, we detect a total of 34 CO $J\to J-1$ transition…

2020 The Astrophysical Journal
eHST 100
Quenching as a Contest between Galaxy Halos and Their Central Black Holes
DOI: 10.3847/1538-4357/ab9633 Bibcode: 2020ApJ...897..102C

Barro, Guillermo; Bell, Eric F.; Ferguson, Henry C. +27 more

Existing models of galaxy formation have not yet explained striking correlations between structure and star formation activity in galaxies, notably the sloped and moving boundaries that divide star-forming from quenched galaxies in key structural diagrams. This paper uses these and other relations to "reverse engineer" the quenching process for ce…

2020 The Astrophysical Journal
eHST 97
The Next Generation Virgo Cluster Survey (NGVS). XXX. Ultra-diffuse Galaxies and Their Globular Cluster Systems
DOI: 10.3847/1538-4357/aba433 Bibcode: 2020ApJ...899...69L

Liu, Chengze; Cuillandre, Jean-Charles; Gwyn, S. D. J. +14 more

We present a study of ultra-diffuse galaxies (UDGs) in the Virgo Cluster based on deep imaging from the Next Generation Virgo Cluster Survey. Applying a new definition for the UDG class based on galaxy scaling relations, we define samples of 44 and 26 UDGs using expansive and restrictive selection criteria, respectively. Our UDG sample includes ob…

2020 The Astrophysical Journal
eHST 96
Cosmicflows-4: The Calibration of Optical and Infrared Tully-Fisher Relations
DOI: 10.3847/1538-4357/ab901c Bibcode: 2020ApJ...896....3K

Seibert, Mark; Anand, Gagandeep S.; Tully, R. Brent +5 more

This study is a part of the Cosmicflows-4 project with the aim of measuring the distances of more than ∼10,000 spiral galaxies in the local universe up to ∼15,000 $\mathrm{km}\,{{\rm{s}}}^{-1}$ . New H I line width information has come primarily from the Arecibo Legacy Fast ALFA Survey. Photometry of our sample galaxies has been carried out in opt…

2020 The Astrophysical Journal
eHST 95
The Evolution of Dust Disk Sizes from a Homogeneous Analysis of 1-10 Myr old Stars
DOI: 10.3847/1538-4357/ab70ba Bibcode: 2020ApJ...895..126H

Pascucci, Ilaria; Testi, Leonardo; Pinilla, Paola +4 more

We utilize ALMA archival data to estimate the dust disk size of 152 protoplanetary disks in Lupus (1-3 Myr), Chamaeleon I (2-3 Myr), and Upper-Sco (5-11 Myr). We combine our sample with 47 disks from Tau/Aur and Oph whose dust disk radii were estimated, as here, through fitting radial profile models to visibility data. We use these 199 homogeneous…

2020 The Astrophysical Journal
Gaia 95