output
19942026
most citedComprehensive nucleosynthesis analysis for ejecta of compact binary mergers

610 citations

researchers with a paper here

Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.

collaborating institutions
Showing 2012 · astro-ph.COShow all

17 papers · 2 filters

astro-ph.CO2012★ 56 cited

Mosaiced wide-field VLBI observations of the Lockman Hole/XMM

Enno Middelberg, Adam Deller, Ray Norris +6

Active Galactic Nuclei (AGN) play a decisive role in galaxy evolution, particularly so when operating in a radiatively inefficient mode, where they launch powerful jets that reshap…

astro-ph.CO2012★ 101 cited

Radio Continuum Surveys with Square Kilometre Array Pathfinders

Ray P. Norris, J. Afonso, D. Bacon +48

In the lead-up to the Square Kilometre Array (SKA) project, several next-generation radio telescopes and upgrades are already being built around the world. These include APERTIF (T…

astro-ph.CO2012★ 76 cited

Occupation of X-ray selected galaxy groups by X-ray AGN

V. Allevato, A. Finoguenov, G. Hasinger +12

We present the first direct measurement of the mean Halo Occupation Distribution (HOD) of X-ray selected AGN in the COSMOS field at z < 1, based on the association of 41 XMM and 17…

astro-ph.CO2012★ 84 cited

Spectral Energy Distributions of Type 1 AGN in the COSMOS Survey I - The XMM-COSMOS Sample

M. Elvis, H. Hao, F. Civano +39

The "Cosmic Evolution Survey" (COSMOS) enables the study of the Spectral Energy Distributions (SEDs) of Active Galactic Nuclei (AGN) because of the deep coverage and rich sampling…

astro-ph.CO2012★ 59 cited

The nature of the unresolved extragalactic soft CXB

N. Cappelluti, P. Ranalli, M. Roncarelli +11

In this paper we investigate the power spectrum of the unresolved 0.5-2 keV CXB with deep Chandra 4 Ms observations in the CDFS. We measured a signal which, on scales >30", is sign…

astro-ph.CO2012★ 62 cited

Deep observations of CO line emission from star-forming galaxies in a cluster candidate at z=1.5

M. Aravena, C. L. Carilli, M. Salvato +20

We report results from a deep Jansky Very Large Array (JVLA) search for CO 1-0 line emission from galaxies in a candidate galaxy cluster at z~1.55 in the COSMOS field. We target 4…

astro-ph.CO2012★ 38 cited

Constraints on the faint end of the quasar luminosity function at z~5 in the COSMOS field

H. Ikeda, T. Nagao, K. Matsuoka +12

We present the result of our low-luminosity quasar survey in the redshift range of 4.5 < z < 5.5 in the COSMOS field. Using the COSMOS photometric catalog, we selected 15 quasar ca…

astro-ph.CO2012★ 417 cited

Bolometric luminosities and Eddington ratios of X-ray selected Active Galactic Nuclei in the XMM-COSMOS survey

E. Lusso, A. Comastri, B. D. Simmons +25

Bolometric luminosities and Eddington ratios of both X-ray selected broad-line (Type-1) and narrow-line (Type-2) AGN from the XMM-Newton survey in the COSMOS field are presented. T…

astro-ph.CO2012★ 59 cited

Chandra High resolution Observations of CID-42, a candidate recoiling SMBH

F. Civano, M. Elvis, G. Lanzuisi +15

We present Chandra High Resolution Camera observations of CID-42, a candidate recoiling supermassive black hole (SMBH) at z=0.359 in the COSMOS survey. CID-42 shows two optical com…

astro-ph.CO2012★ 299 cited

The Mean Star Formation Rate of X-ray selected Active Galaxies and its Evolution from z=2.5: Results from PEP-Herschel

D. J. Rosario, P. Santini, D. Lutz +37

(Abridged) We study relationships between the SFR and the nuclear properties of X-ray selected AGNs out to z=2.5, using far-IR data in three extragalactic deep fields as part of th…

astro-ph.CO2012★ 220 cited

HerMES: deep number counts at 250, 350, and 500 microns in the COSMOS and GOODS-N fields and the build-up of the cosmic infrared background

M. Béthermin, E. Le Floc'h, O. Ilbert +58

ABRIGED Herschel/SPIRE has provided confusion limited maps of deep fields at 250, 350, and 500um, as part of the HerMES survey. Due to confusion, only a small fraction of the Cosmi…

astro-ph.CO2012★ 149 cited

A tidal disruption-like X-ray flare from the quiescent galaxy SDSS J120136.02+300305.5

R. D. Saxton, A. M. Read, P. Esquej +4

SDSS J120136.02+300305.5 was detected in an XMM-Newton slew from June 2010 with a flux 56 times higher than an upper limit from ROSAT, corresponding to Lx~3x10^44 ergs/s. It has th…

astro-ph.CO2012★ 113 cited

Recoiling black holes: electromagnetic signatures, candidates, and astrophysical implications

S. Komossa

Supermassive black holes (SMBHs) may not always reside right at the centers of their host galaxies. This is a prediction of numerical relativity simulations, which imply that the n…

astro-ph.CO2012★ 287 cited

A Herschel view of the far-infrared properties of submillimetre galaxies

B. Magnelli, D. Lutz, P. Santini +48

We study a sample of 61 submillimetre galaxies (SMGs) selected from ground-based surveys, with known spectroscopic redshifts and observed with Herschel as part of the PACS Evolutio…

astro-ph.CO2012★ 18 cited

First simultaneous optical/near-infrared imaging of an X-ray selected, high-redshift cluster of galaxies with GROND: the galaxy population of XMMU J0338.7+0030 at z=1.1

D. Pierini, R. Suhada, R. Fassbender +28

The XMM-Newton Distant Cluster Project is a serendipitous survey for clusters of galaxies at redshifts z>=0.8 based on deep archival XMM-Newton observations. ... Low-significance c…

astro-ph.CO2012★ 221 cited

Enhanced star formation rates in AGN hosts with respect to inactive galaxies from PEP-Herschel observations

P. Santini, D. J. Rosario, L. Shao +35

We compare the average star formation (SF) activity in X-ray selected AGN hosts with mass-matched control inactive galaxies,including star forming and quiescent sources, at 0.5<z<2…

astro-ph.CO2012★ 37 cited

Clustering of X-Ray-Selected AGN

Nico Cappelluti, Viola Allevato, Alexis Finoguenov

The study of the angular and spatial structure of the X-ray sky has been under investigation since the times of the Einstein X-ray Observatory. This topic has fascinated more than…