activity
20052025
most citedThe Baryon Oscillation Spectroscopic Survey of SDSS-III

2.1k citations · 16.4k across the 135 of their papers we have counts for

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Showing 2020Show all

6 papers · 1 filter

astro-ph.HE2020★ 72 cited

Rapid Variability of Sgr A* across the Electromagnetic Spectrum

G. Witzel, G. Martinez, S. P. Willner +17

Sagittarius A* (Sgr A*) is the variable radio, near-infrared (NIR), and X-ray source associated with accretion onto the Galactic center black hole. We have analyzed a comprehensive…

astro-ph.HE2020★ 59 cited

General relativistic MHD simulations of non-thermal flaring in Sagittarius A*

Koushik Chatterjee, Sera Markoff, Joseph Neilsen +10

Sagittarius A* exhibits regular variability in its multiwavelength emission, including daily X-ray flares and roughly continuous near-infrared (NIR) flickering. The origin of this…

astro-ph.GA2020★ 17 cited

AzTEC Survey of the Central Molecular Zone: Data Reduction, Analysis, and Preliminary Results

Yuping Tang, Q. Daniel Wang, Grant W. Wilson +14

We present a large-scale survey of the central molecular zone (CMZ) of our Galaxy, as well as a monitoring program of Sgr A*, with the AzTEC/Large Millimeter Telescope (LMT) in the…

astro-ph.HE2020★ 13 cited

The X-ray outburst of the Galactic Center magnetar over six years of Chandra observations

N. Rea, F. Coti Zelati, D. Vigano' +16

The magnetar SGR J1745-2900 discovered at parsecs distance from the Milky Way central black hole, Sagittarius A*, represents the closest pulsar to a supermassive black hole ever de…

astro-ph.HE2020★ 48 cited

A Deep CFHT Optical Search for a Counterpart to the Possible Neutron Star -- Black Hole Merger GW190814

Nicholas Vieira, John J. Ruan, Daryl Haggard +10

We present a wide-field optical imaging search for electromagnetic counterparts to the likely neutron star - black hole (NS-BH) merger GW190814/S190814bv. This compact binary merge…

astro-ph.HE2020★ 12 cited

The Chandra High Resolution X-ray Spectrum of Quiescent Emission from Sgr A*

L. Corrales, F. K. Baganoff, Q. D. Wang +7

In quiescence, Sgr A* is surprisingly dim, shining 100,000 times less than expected for its environment. This problem has motivated a host of theoretical models to explain radiativ…