Search Publications

The Extremely Luminous Quasar Survey in the Sloan Digital Sky Survey Footprint. III. The South Galactic Cap Sample and the Quasar Luminosity Function at Cosmic Noon
DOI: 10.3847/1538-4357/aaf86c Bibcode: 2019ApJ...871..258S

Fan, Xiaohui; McGreer, Ian D.; Huang, Yun-Hsin +11 more

We have designed the Extremely Luminous Quasar Survey (ELQS) to provide a highly complete census of unobscured UV-bright quasars during the cosmic noon, z = 2.8-5.0. Here we report the discovery of 70 new quasars in the ELQS South Galactic Cap (ELQS-S) quasar sample, doubling the number of known extremely luminous quasars in 4237.3 deg2

2019 The Astrophysical Journal
XMM-Newton 39
TESS Asteroseismology of the Known Red-giant Host Stars HD 212771 and HD 203949
DOI: 10.3847/1538-4357/ab44a8 Bibcode: 2019ApJ...885...31C

Stock, Stephan; Reffert, Sabine; Chaplin, William J. +45 more

The Transiting Exoplanet Survey Satellite (TESS) is performing a near all-sky survey for planets that transit bright stars. In addition, its excellent photometric precision enables asteroseismology of solar-type and red-giant stars, which exhibit convection-driven, solar-like oscillations. Simulations predict that TESS will detect solar-like oscil…

2019 The Astrophysical Journal
Gaia 39
Record-breaking Coronal Magnetic Field in Solar Active Region 12673
DOI: 10.3847/2041-8213/ab3042 Bibcode: 2019ApJ...880L..29A

Fleishman, Gregory D.; Anfinogentov, Sergey A.; Stupishin, Alexey G. +1 more

The strongest magnetic fields on the Sun are routinely detected at dark sunspots. The magnitude of the field is typically about 3000 G, with only a few exceptions that reported the magnetic field in excess of 5000 G. Given that the magnetic field decreases with height in the solar atmosphere, no coronal magnetic field above ∼2000 G has ever been r…

2019 The Astrophysical Journal
Hinode 39
SDSS-IV eBOSS Spectroscopy of X-Ray and WISE AGNs in Stripe 82X: Overview of the Demographics of X-Ray- and Mid-infrared-selected Active Galactic Nuclei
DOI: 10.3847/1538-4357/ab108b Bibcode: 2019ApJ...876...50L

Ananna, Tonima Tasnim; Salvato, Mara; Vivek, M. +5 more

We report the results of a Sloan Digital Sky Survey IV eBOSS program to target X-ray sources and mid-infrared-selected Wide-field Infrared Survey Explorer (WISE) active galactic nucleus (AGN) candidates in a 36.8 deg2 region of Stripe 82. About half this survey (15.6 deg2) covers the largest contiguous portion of the Stripe 8…

2019 The Astrophysical Journal
XMM-Newton 39
The Elusive Majority of Young Moving Groups. I. Young Binaries and Lithium-rich Stars in the Solar Neighborhood
DOI: 10.3847/1538-4357/ab1018 Bibcode: 2019ApJ...877...60B

Baranec, Christoph; Law, Nicholas M.; Riddle, Reed +8 more

Young stars in the solar neighborhood serve as nearby probes of stellar evolution and represent promising targets to directly image self-luminous giant planets. We have carried out an all-sky search for late-type (≈K7-M5) stars within 100 pc selected primarily on the basis of activity indicators from the Galaxy Evolution Explorer and ROSAT. Approx…

2019 The Astrophysical Journal
Gaia 39
Infrared Contributions of X-Ray Selected Active Galactic Nuclei in Dusty Star-forming Galaxies
DOI: 10.3847/1538-4357/aaf73b Bibcode: 2019ApJ...871...87B

Azadi, Mojegan; Cooray, Asantha; Ma, Jingzhe +3 more

We investigate the infrared (IR) contribution from supermassive black hole activity versus host galaxy emission in the mid- to far-IR spectrum for a large sample of X-ray bright active galactic nuclei (AGN) residing in dusty, star-forming host galaxies. We select 703 AGN with {L}{{X}}={10}42{--}{10}46 erg s-1<…

2019 The Astrophysical Journal
Herschel 38
Detection of a 50° long Trailing Tidal Tail for the Globular Cluster M5
DOI: 10.3847/1538-4357/ab441d Bibcode: 2019ApJ...884..174G

Grillmair, Carl J.

Using photometry and proper motions from Gaia Data Release 2, we detect a 50° long stream of about 70 stars extending westward from the halo globular cluster M5. Based on the similarities in distance, proper motions, inferred color-magnitude distribution, and trajectory, we identify this stream as the trailing tidal tail of M5. While the surface d…

2019 The Astrophysical Journal
Gaia 38
Episodically Active Asteroid 6478 Gault
DOI: 10.3847/2041-8213/ab1be8 Bibcode: 2019ApJ...876L..19J

Kotulla, Ralf; Jewitt, David; Rajagopal, Jayadev +4 more

We present imaging and spectroscopic observations of 6478 Gault, a ∼6 km diameter inner main-belt asteroid currently exhibiting strong, comet-like characteristics. Three distinct tails indicate that ultra-slow dust (ejection speed 0.15 ± 0.05 m s-1) was emitted from Gault in separate episodes beginning UT 2018 October 28 ± 5 (Tail A), U…

2019 The Astrophysical Journal
eHST 38
Discovery of a New Stellar Subpopulation Residing in the (Inner) Stellar Halo of the Milky Way
DOI: 10.3847/2041-8213/ab5286 Bibcode: 2019ApJ...886L...8F

Beers, Timothy C.; Placco, Vinicius M.; Robin, Annie C. +8 more

We report the discovery of a unique collection of metal-poor giant stars that exhibit anomalously high levels of 28Si, clearly above typical Galactic levels. Our sample spans a narrow range of metallicities, peaking at -1.07 ± 0.06, and exhibits abundance ratios of [Si, Al/Fe] that are as extreme as those observed in Galactic globular c…

2019 The Astrophysical Journal
Gaia 38
Short-duration Stellar Flares in GALEX Data
DOI: 10.3847/1538-4357/ab3df8 Bibcode: 2019ApJ...883...88B

Brasseur, C. E.; Osten, Rachel A.; Fleming, Scott W.

We report on a population of short-duration near-ultraviolet (NUV) flares in stars observed by the Kepler and Galaxy Evolution Explorer (GALEX) missions. We analyzed the NUV light curves of 34,276 stars observed from 2009 to 2013 by both the GALEX (NUV) and Kepler (optical) space missions with the eventual goal of investigating multiwavelength fla…

2019 The Astrophysical Journal
Gaia 38