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The Search for Binary Supermassive Black Holes among Quasars with Offset Broad Lines Using the Very Long Baseline Array
DOI: 10.3847/1538-4357/abfa9a Bibcode: 2021ApJ...914...37B

Eracleous, Michael; Lazio, T. Joseph W.; Breiding, Peter +4 more

In several previous studies, quasars exhibiting broad emission lines with ≳1000 km s-1 velocity offsets with respect to the host galaxy rest frame have been discovered. One leading hypothesis for the origin of these velocity-offset broad lines is the dynamics of a binary supermassive black hole (SMBH). We present high-resolution radio i…

2021 The Astrophysical Journal
Gaia 14
X-Ray Spectroscopy of the Highly Magnetized Pulsar PSR J1846-0258, Its Wind Nebula, and Hosting Supernova Remnant Kes 75
DOI: 10.3847/1538-4357/abd32b Bibcode: 2021ApJ...908..212G

Gotthelf, E. V.; Safi-Harb, S.; Straal, S. M. +1 more

We present broadband X-ray spectroscopy of the energetic components that make up the supernova remnant (SNR) Kesteven 75 using concurrent 2017 August 17-20 XMM-Newton and NuSTAR observations, during which the pulsar PSR J1846-0258 is found to be in the quiescent state. The young remnant hosts a bright pulsar wind nebula powered by the highly energ…

2021 The Astrophysical Journal
XMM-Newton 14
Lyman Continuum Emission Escaping from Luminous Green Pea Galaxies at z = 0.5
DOI: 10.3847/1538-4357/abd84e Bibcode: 2021ApJ...909...92M

Malkan, Matthew A.; Malkan, Brian K.

Compact starburst galaxies are thought to include many or most of the galaxies from which substantial Lyman continuum emission can escape into the intergalactic medium. Li & Malkan used Sloan Digital Sky Survey photometry to find a population of such starburst galaxies at z ∼ 0.5. They were discovered by their extremely strong [O III] λλ4959+5…

2021 The Astrophysical Journal
eHST 14
Measuring the Average Molecular Gas Content of Star-forming Galaxies at z = 3-4
DOI: 10.3847/1538-4357/ac01d7 Bibcode: 2021ApJ...916...12B

Carilli, Chris; Feltre, Anna; Bacon, Roland +15 more

We study the molecular gas content of 24 star-forming galaxies at z = 3-4, with a median stellar mass of 109.1 M, from the MUSE Hubble Ultra Deep Field (HUDF) Survey. Selected by their Lyα λ1216 emission and HF160W-band magnitude, the galaxies show an average $\langle {\mathrm{EW}}_{\mathrm{Ly}\alpha }^{0}\rangle …

2021 The Astrophysical Journal
eHST 14
GRB 191016A: A Long Gamma-Ray Burst Detected by TESS
DOI: 10.3847/1538-4357/abe6a2 Bibcode: 2021ApJ...911...43S

Barclay, Thomas; Daylan, Tansu; Fausnaugh, Michael +8 more

The Transiting Exoplanet Survey Satellite (TESS) exoplanet-hunting mission detected the rising and decaying optical afterglow of GRB 191016A, a long gamma-ray burst (GRB) detected by Swift-BAT but without prompt XRT or UVOT follow-up due to proximity to the Moon. The afterglow has a late peak at least 1000 s after the BAT trigger, with a brightest…

2021 The Astrophysical Journal
Gaia 14
The HST See Change Program. I. Survey Design, Pipeline, and Supernova Discoveries
DOI: 10.3847/1538-4357/abed4d Bibcode: 2021ApJ...912...87H

Richard, Johan; Muzzin, Adam; Hoekstra, Henk +53 more

The See Change survey was designed to make z > 1 cosmological measurements by efficiently discovering high-redshift Type Ia supernovae (SNe Ia) and improving cluster mass measurements through weak lensing. This survey observed twelve galaxy clusters with the Hubble Space Telescope (HST) spanning the redshift range z = 1.13-1.75, discovering 57 …

2021 The Astrophysical Journal
eHST 14
SN 2018agk: A Prototypical Type Ia Supernova with a Smooth Power-law Rise in Kepler (K2)
DOI: 10.3847/1538-4357/ac2c84 Bibcode: 2021ApJ...923..167W

Pál, András; Barclay, Thomas; Kilpatrick, Charles D. +73 more

We present the 30 minutes cadence Kepler/K2 light curve of the Type Ia supernova (SN Ia) SN 2018agk, covering approximately one week before explosion, the full rise phase, and the decline until 40 days after peak. We additionally present ground-based observations in multiple bands within the same time range, including the 1 day cadence DECam obser…

2021 The Astrophysical Journal
eHST 14
A Broadband X-Ray View of the Precessing Accretion Disk and Pre-eclipse Dip in the Pulsar Her X-1 with NuSTAR and XMM-Newton
DOI: 10.3847/1538-4357/abe122 Bibcode: 2021ApJ...909..186B

Pottschmidt, Katja; Staubert, Rüdiger; Wilms, Jörn +5 more

We present a broadband X-ray timing study of the variations in pulse behavior with the superorbital cycle in the low-mass X-ray binary Her X-1. This source shows a 35 day superorbital modulation in X-ray flux that is likely caused by occultation by a warped, precessing accretion disk. Our data set consists of four joint XMM-Newton and NuSTAR obser…

2021 The Astrophysical Journal
XMM-Newton 14
KCWI Observations of the Extended Nebulae in Mrk 273
DOI: 10.3847/1538-4357/abf4da Bibcode: 2021ApJ...914...17L

Leung, Gene C. K.; Coil, Alison L.; Perrotta, Serena +1 more

Ultraluminous infrared galaxies (ULIRGs) represent a critical stage in the merger-driven evolution of galaxies when active galactic nucleus (AGN) activity is common and AGN feedback is expected. We present high-sensitivity and large field-of-view integral field spectroscopy of the ULIRG Mrk 273 using new data from the Keck Cosmic Web Imager (KWCI)…

2021 The Astrophysical Journal
eHST 14
HAWC+/SOFIA Polarimetry in L1688: Relative Orientation of Magnetic Field and Elongated Cloud Structure
DOI: 10.3847/1538-4357/ac0cf2 Bibcode: 2021ApJ...918...39L

Kwon, Woojin; Fissel, Laura M.; Li, Di +14 more

We present a study of the relative orientation between the magnetic field and elongated cloud structures for the ρ Oph A and ρ Oph E regions in L1688 in the Ophiuchus molecular cloud. Combining inferred magnetic field orientation from HAWC+ 154 µm observations of polarized thermal emission with column density maps created using Herschel subm…

2021 The Astrophysical Journal
Herschel 14