activity
20102026
most citedThe Early Data Release of the Dark Energy Spectroscopic Instrument

343 citations · 3.7k across the 123 of their papers we have counts for

collaborators
Showing 2018Show all

7 papers · 1 filter

astro-ph.GA2018

Searching for intermediate-mass black holes in NGC3310

Megan Argo, Joseph Coppola, Mar Mezcua +2

Intermediate-mass black holes are theoretically predicted but observationally elusive, and evidence for them is often indirect. The nearby face-on spiral galaxy NGC3310 has hosted…

astro-ph.GA2018★ 193 cited

Titans of the Early Universe: The Prato Statement on the Origin of the First Supermassive Black Holes

Tyrone E. Woods, Bhaskar Agarwal, Volker Bromm +30

In recent years, the discovery of massive quasars at z~7 has provided a striking challenge to our understanding of the origin and growth of supermassive black holes in the early Un…

astro-ph.GA2018★ 2 cited

Intra-night optical variability of AGN in the COSMOS field with the KMTNet

Joonho Kim, Marios Karouzos, Myungshin Im +5

Active Galactic Nucleus (AGN) variability can be used to study the physics of the region in the vicinity of the central black hole. In this paper, we investigated intra-night optic…

astro-ph.GA2018★ 43 cited

Glimmering in the dark: modeling the low-mass end of the relation and of the quasar luminosity function

Fabio Pacucci, Abraham Loeb, Mar Mezcua +1

The relation establishes a connection between central black holes (BHs) and their host spheroids. Supported by observations at $M_{\bullet} \gtrsim 10^5 \, M_{\od…

astro-ph.GA2018★ 37 cited

The extended radio jet of an off-nuclear low-mass AGN in NGC 5252

M. Mezcua, M. Kim, L. C. Ho +1

CXO J133815.6+043255 is an ultraluminous X-ray source (ULX) with ultraviolet, optical, and radio counterparts located 10 kpc away from the nucleus of the galaxy NGC 5252. Optical s…

astro-ph.GA2018★ 64 cited

Exploring the limits of AGN feedback: black holes and the star formation histories of low-mass galaxies

Ignacio Martin-Navarro, Mar Mezcua

Energy feedback, either from active galactic nuclei (AGN) or from supernovae, is required to understand galaxy formation within a -Cold Dark Matter cosmology. We study a sample…