output
20022026
most citedGW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

9.8k citations

Showing 2012 · astro-ph.COShow all

10 papers · 2 filters

astro-ph.CO2012★ 28 cited

Intragroup and Galaxy-Linked Diffuse X-ray Emission in Hickson Compact Groups

Tyler D. Desjardins, Sarah C. Gallagher, Panayiotis Tzanavaris +9

Isolated compact groups of galaxies (CGs) present a range of dynamical states, group velocity dispersions, and galaxy morphologies with which to study galaxy evolution, particularl…

astro-ph.CO2012★ 273 cited

The Imprint of The Extragalactic Background Light in the Gamma-Ray Spectra of Blazars

LAT Collaboration

The light emitted by stars and accreting compact objects through the history of the Universe is encoded in the intensity of the extragalactic background light (EBL). Knowledge of t…

astro-ph.CO2012★ 41 cited

The high-redshift (z>3) AGN population in the 4 Ms Chandra Deep Field South

F. Vito, C. Vignali, R. Gilli +10

We present results from a spectral analysis of a sample of high-redshift (z>3) X-ray selected AGN in the 4 Ms Chandra Deep Field South (CDF-S), the deepest X-ray survey to date. Th…

astro-ph.CO2012★ 161 cited

Submillimeter Follow-up of WISE-Selected Hyperluminous Galaxies

Jingwen Wu, Chao-Wei Tsai, Jack Sayers +20

We have used the Caltech Submillimeter Observatory (CSO) to follow-up a sample of WISE-selected, hyperluminous galaxies, so called W1W2-dropout galaxies. This is a rare (~ 1000 all…

astro-ph.CO2012★ 205 cited

The First Hyper-Luminous Infrared Galaxy Discovered by WISE

Peter R. M. Eisenhardt, Jingwen Wu, Chao-Wei Tsai +21

We report the discovery by the Wide-field Infrared Survey Explorer of the z = 2.452 source WISE J181417.29+341224.9, the first hyperluminous source found in the WISE survey. WISE 1…

astro-ph.CO2012★ 108 cited

A 200-s Quasi-Periodicity Following the Tidal Disruption of a Star by a Dormant Black Hole

R. C. Reis, J. M. Miller, M. T. Reynolds +4

Supermassive black holes (SMBHs; $M\gtrsim10^5\msun$) are known to exist at the centre of most galaxies with sufficient stellar mass. In the local Universe, it is possible to infer…