activity
20132026
most citedThe COSMOS2015 Catalog: Exploring the 1<z<6 Universe with half a million galaxies

1.2k citations · 6.8k across the 184 of their papers we have counts for

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Showing 2017Show all

19 papers · 1 filter

astro-ph.GA2017★ 67 cited

Infrared Selection of Obscured Active Galactic Nuclei in the COSMOS Field

Yu-Yen Chang, Emeric Le Floc'h, Stéphanie Juneau +13

We present a study of the connection between black hole accretion, star formation, and galaxy morphology at z<=2.5. We focus on active galactic nuclei (AGNs) selected by their mid-…

astro-ph.GA2017★ 72 cited

AGN Populations in Large Volume X-ray Surveys: Photometric Redshifts and Population Types found in the Stripe 82X Survey

Tonima Tasnim Ananna, Mara Salvato, Stephanie LaMassa +16

Multi-wavelength surveys covering large sky volumes are necessary to obtain an accurate census of rare objects such as high luminosity and/or high redshift active galactic nuclei (…

astro-ph.GA2017★ 48 cited

Near Infrared Variability of obscured and unobscured X-ray selected AGN in the COSMOS field

P. Sánchez, P. Lira, R. Cartier +9

We present our statistical study of near infrared (NIR) variability of X-ray selected Active Galactic Nuclei (AGN) in the COSMOS field, using UltraVISTA data. This is the largest s…

astro-ph.HE2017★ 25 cited

The NuSTAR Extragalactic Survey: Average broad-band X-ray spectral properties of the NuSTAR detected AGN

A. Del Moro, D. M. Alexander, J. A. Aird +18

We present a study of the average X-ray spectral properties of the sources detected by the NuSTAR extragalactic survey, comprising observations of the E-CDFS, EGS and COSMOS fields…

astro-ph.GA2017★ 13 cited

Chandra and NuSTAR follow-up observations of Swift-BAT selected AGN

Stefano Marchesi, Luke Tremblay, Marco Ajello +5

Based on current models of the Cosmic X-ray Background (CXB), heavily obscured Active Galactic Nuclei (AGN) are expected to make up ~10% of the peak emission of the CXB and ~20% of…

astro-ph.GA2017★ 86 cited

An ALMA survey of submillimeter galaxies in the COSMOS field: Multiwavelength counterparts and redshift distribution

Drew Brisbin, Oskari Miettinen, Manuel Aravena +28

We carried out targeted ALMA observations of 129 fields in the COSMOS region at 1.25 mm, detecting 152 galaxies at S/N5 with an average continuum RMS of 150 Jy. These fiel…

astro-ph.GA2017★ 20 cited

The Hunt for Red Quasars: Luminous Obscured Black Hole Growth Unveiled in the Stripe 82 X-ray Survey

Stephanie M. LaMassa, Eilat Glikman, Marcella Brusa +18

We present results of a ground-based near-infrared campaign with Palomar TripleSpec, Keck NIRSPEC, and Gemini GNIRS to target two samples of reddened active galactic nucleus (AGN)…

astro-ph.HE2017★ 54 cited

The NuSTAR Serendipitous Survey: Hunting for The Most Extreme Obscured AGN at >10 keV

G. B. Lansbury, D. M. Alexander, J. Aird +27

We identify sources with extremely hard X-ray spectra (i.e., with photon indices of Gamma<0.6 in the 13 sq. deg. NuSTAR serendipitous survey, to search for the most highly obscured…

astro-ph.HE2017★ 5 cited

Inferring Compton-thick AGN candidates at z>2 with Chandra using the >8 keV restframe spectral curvature

L. Baronchelli, M. Koss, K. Schawinski +10

To fully understand cosmic black hole growth we need to constrain the population of heavily obscured active galactic nuclei (AGN) at the peak of cosmic black hole growth (1-…

astro-ph.GA2017★ 139 cited

The VLA-COSMOS 3~GHz Large Project: Cosmic evolution of radio AGN and implications for radio-mode feedback since z~5

V. Smolcic, M. Novak, I. Delvecchio +8

Based on a sample of over 1,800 radio AGN at redshifts out to z~5, which have typical stellar masses within ~3x(10^{10}-10^{11}) Msol, and 3 GHz radio data in the COSMOS field, we…

astro-ph.GA2017★ 40 cited

Type 2 AGN host galaxies in the Chandra-COSMOS Legacy Survey: No Evidence of AGN-driven Quenching

Hyewon Suh, Francesca Civano, Guenther Hasinger +16

We investigate the star formation properties of a large sample of ~2300 X-ray-selected Type 2 Active Galactic Nuclei (AGNs) host galaxies out to z~3 in the Chandra COSMOS Legacy Su…

astro-ph.GA2017★ 197 cited

The VLA-COSMOS 3 GHz Large Project: Multiwavelength counterparts and the composition of the faint radio population

V. Smolcic, I. Delvecchio, G. Zamorani +18

(abridged) We study the composition of the faint radio population selected from the VLA-COSMOS 3GHz Large Project. The survey covers a 2.6sq.deg. area with a mean rms of ~2.3uJy/b,…

astro-ph.GA2017★ 169 cited

The VLA-COSMOS 3 GHz Large Project: The cosmic star formation history since z~5

M. Novak, V. Smolcic, J. Delhaize +19

We make use of the deep Karl G. Jansky Very Large Array (VLA) COSMOS radio observations at 3 GHz to infer radio luminosity functions of star-forming galaxies up to redshifts of z~5…

astro-ph.GA2017★ 180 cited

The VLA-COSMOS 3~GHz Large Project: AGN and host-galaxy properties out to z6

I. Delvecchio, V. Smolcic, G. Zamorani +29

We explore the multiwavelength properties of AGN host galaxies for different classes of radio-selected AGN out to z6 via a multiwavelength analysis of about 7700 radio so…

astro-ph.GA2017★ 203 cited

VLA-COSMOS 3GHz Large Project: The infrared-radio correlation of star-forming galaxies and AGN to

J. Delhaize, V. Smolcic, I. Delvecchio +22

We examine the behaviour of the infrared-radio correlation (IRRC) over the range using new, highly sensitive 3GHz observations with the Karl G. Jansky Very Large Array (VLA…

astro-ph.GA2017★ 32 cited

An ALMA survey of submillimetre galaxies in the COSMOS field: The extent of the radio-emitting region revealed by 3 GHz imaging with the Very Large Array

Oskari Miettinen, Mladen Novak, Vernesa Smolčić +32

We determine the radio size distribution of a large sample of 152 SMGs in COSMOS that were detected with ALMA at 1.3 mm. For this purpose, we used the observations taken by the VLA…

astro-ph.GA2017★ 96 cited

AGN vs. host galaxy properties in the COSMOS field

G. Lanzuisi, I. Delvecchio, S. Berta +13

The coeval AGN and galaxy evolution and the observed local relations between SMBHs and galaxy properties suggest some connection or feedback between SMBH growth and galaxy build-up…

astro-ph.HE2017★ 104 cited

The Chandra COSMOS legacy survey: Energy Spectrum of the Cosmic X-ray Background and constraints on undetected populations

Nico Cappelluti, Yanxia Li, Angelo Ricarte +15

Using {\em Chandra} observations in the 2.15 deg COSMOS legacy field, we present one of the most accurate measurements of the Cosmic X-ray Background (CXB) spectrum to date i…

astro-ph.HE2017★ 23 cited

X-ray spectral properties of seven heavily obscured Seyfert 2 galaxies

Stefano Marchesi, Marco Ajello, Andrea Comastri +3

We present the combined Chandra and Swift-BAT spectral analysis of seven Seyfert 2 galaxies selected from the Swift-BAT 100-month catalog. We selected nearby (z<=0.03) sources lack…