activity
20152019
most citedA kilonova as the electromagnetic counterpart to a gravitational-wave source

888 citations · 2k across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.GA201934 cited

Optically variable active galactic nuclei in the 3 yr VST survey of the COSMOS field

D. De Cicco, M. Paolillo, S. Falocco +16

The analysis of the variability of active galactic nuclei (AGNs) at different wavelengths and the study of possible correlations among different spectral windows are nowadays a maj…

astro-ph.HE201812 cited

The long-term optical evolution of the black hole candidate MAXI J1659-152

Jesus M. Corral-Santana, Manuel A. P. Torres, Tariq Shahbaz +13

We present 5 years of optical and infrared data of the black hole candidate MAXI J1659-152 covering its 2010 outburst, decay and quiescence. Combining optical data taken during the…

astro-ph.GA2017

Luminous and obscured quasars and their host galaxies

Agnese Del Moro, David M. Alexander, Franz E. Bauer +4

The most heavily-obscured, luminous quasars might represent a specific phase of the evolution of actively accreting supermassive black holes and their host galaxies, possibly relat…

astro-ph.HE201756 cited

ALMA and GMRT constraints on the off-axis gamma-ray burst 170817A from the binary neutron star merger GW170817

Sam Kim, Steve Schulze, Lekshmi Resmi +31

Binary neutron-star mergers (BNSMs) are among the most readily detectable gravitational-wave (GW) sources with LIGO. They are also thought to produce short -ray bursts (SGRBs),…

astro-ph.HE2017888 cited

A kilonova as the electromagnetic counterpart to a gravitational-wave source

S. J. Smartt, T. -W. Chen, A. Jerkstrand +118

Gravitational waves were discovered with the detection of binary black hole mergers and they should also be detectable from lower mass neutron star mergers. These are predicted to…

astro-ph.GA201736 cited

Deepest view of AGN X-ray variability with the 7 Ms Chandra Deep Field-South survey

X. C. Zheng, Y. Q. Xue, W. N. Brandt +13

We systematically analyze X-ray variability of active galactic nuclei (AGNs) in the 7~Ms \textit{Chandra} Deep Field-South survey. On the longest timescale ( years), we…