activity
19992023
most citedMass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function

2k citations · 25k across the 225 of their papers we have counts for

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131 papers · 1 filter

astro-ph.GA2023★ 1 cited

A rest-frame near-IR study of clumps in galaxies at 1 < z < 2 using JWST/NIRCam: connection to galaxy bulges

Boris S. Kalita, John D. Silverman, Emanuele Daddi +4

A key question in galaxy evolution has been the importance of the apparent `clumpiness' of high redshift galaxies. Until now, this property has been primarily investigated in rest-…

astro-ph.GA2023★ 10 cited

COSMOS-Web: Intrinsically Luminous z10 Galaxy Candidates Test Early Stellar Mass Assembly

Caitlin M. Casey, Hollis B. Akins, Marko Shuntov +39

We report the discovery of 15 exceptionally luminous candidate galaxies discovered in the first 0.28 deg of JWST/NIRCam imaging from the COSMOS-Web Sur…

astro-ph.GA2023★ 55 cited

IllustrisTNG in the HSC-SSP: image data release and the major role of mini mergers as drivers of asymmetry and star formation

Connor Bottrell, Hassen M. Yesuf, Gergö Popping +13

At fixed galaxy stellar mass, there is a clear observational connection between structural asymmetry and offset from the star forming main sequence, SFMS. Herein, we use the TNG…

astro-ph.GA2023

Uncovering a Massive z~7.7 Galaxy Hosting a Heavily Obscured Radio-Loud QSO Candidate in COSMOS-Web

Erini Lambrides, Marco Chiaberge, Arianna Long +47

In this letter, we report the discovery of the highest redshift, heavily obscured, radio-loud AGN candidate selected using JWST NIRCam/MIRI, mid-IR, sub-mm, and radio imaging in th…

astro-ph.GA2023★ 8 cited

Unveiling the distant Universe: Characterizing Galaxies in the first epoch of COSMOS-Web

Maximilien Franco, Hollis B. Akins, Caitlin M. Casey +47

We report the identification of 15 galaxy candidates at using the initial COSMOS-Web JWST observations over 77 arcmin through four NIRCam filters (F115W, F150W, F277W,…

astro-ph.GA2023★ 9 cited

Resolving galactic-scale obscuration of X-ray AGN at with COSMOS-Web

John D. Silverman, Vincenzo Mainieri, Xuheng Ding +25

A large fraction of the accreting supermassive black hole population is shrouded by copious amounts of gas and dust, particularly in the distant () Universe. While much…

astro-ph.GA2023

HYPERION. Interacting companion and outflow in the most luminous quasar

R. Tripodi, J. Scholtz, R. Maiolino +11

We present ALMA deep observations of the [CII] 158 m emission line and the continuum at 253 GHz and 99 GHz towards SDSS J0100+2802 at , the most luminous quasi-stel…

astro-ph.GA2023★ 64 cited

Quasar Luminosity Function at z = 7

Yoshiki Matsuoka, Masafusa Onoue, Kazushi Iwasawa +41

We present the quasar luminosity function (LF) at , measured with 35 spectroscopically confirmed quasars at . The sample of 22 quasars from the Subaru High-…

astro-ph.GA2023

Morphological asymmetries of quasar host galaxies with Subaru Hyper Suprime-Cam

Shenli Tang, John D. Silverman, Hassen M. Yesuf +7

How does the host galaxy morphology influence a central quasar or vice versa? We address this question by measuring the asymmetries of 2424 SDSS quasar hosts at using b…

astro-ph.GA2023★ 26 cited

JWST and ALMA imaging of dust-obscured, massive substructures in a typical star-forming disk galaxy

Wiphu Rujopakarn, Christina C. Williams, Emanuele Daddi +8

We present an identification of dust-attenuated star-forming galactic-disk substructures in a typical star-forming galaxy (SFG), UDF2, at . To date, substructures contai…

astro-ph.GA2023

The eROSITA Final Equatorial-Depth Survey (eFEDS): Host-galaxy Demographics of X-ray AGNs with Subaru Hyper Suprime-Cam

Junyao Li, John D. Silverman, Andrea Merloni +12

We investigate the physical properties, such as star-forming activity, disk vs. bulge nature, galaxy size, and obscuration of 3796 X-ray selected AGNs at in the eFEDS f…

astro-ph.GA2023★ 29 cited

The cosmic web of X-ray active galactic nuclei seen through the eROSITA Final Equatorial Depth Survey (eFEDS)

Johan Comparat, Wentao Luo, Andrea Merloni +17

Which galaxies in the general population turn into active galactic nuclei (AGNs) is a keystone of galaxy formation and evolution. Thanks to SRG/eROSITA's contiguous 140 square degr…

astro-ph.GA2022★ 127 cited

Detection of stellar light from quasar host galaxies at redshifts above 6

Xuheng Ding, Masafusa Onoue, John D. Silverman +41

The detection of starlight from the host galaxies of quasars during the reionization epoch () has been elusive, even with deep HST observations. The current highest redshift q…

astro-ph.GA2022★ 13 cited

COSMOS-Web: An Overview of the JWST Cosmic Origins Survey

Caitlin M. Casey, Jeyhan S. Kartaltepe, Nicole E. Drakos +82

We present the survey design, implementation, and outlook for COSMOS-Web, a 255 hour treasury program conducted by the James Webb Space Telescope in its first cycle of observations…

astro-ph.GA2022★ 50 cited

Opening the era of quasar host studies at high redshift with JWST

Xuheng Ding, John D. Silverman, Masafusa Onoue

We measure the host galaxy properties of five quasars with selected from SDSS and AEGIS, which fall within the JWST/HST CEERS survey area. A PSF library is constr…

astro-ph.GA2022★ 2 cited

A machine learning approach to assessing the presence of substructure in quasar host galaxies using the Hyper Suprime-Cam Subaru Strategic Program

Chris Nagele, John D. Silverman, Tilman Hartwig +4

The conditions under which galactic nuclear regions become active are largely unknown, although it has been hypothesized that secular processes related to galaxy morphology could p…

astro-ph.GA2022★ 41 cited

The hidden side of cosmic star formation at z > 3: Bridging optically-dark and Lyman break galaxies with GOODS-ALMA

Mengyuan Xiao, David Elbaz, Carlos Gómez-Guijarro +37

Our current understanding of the cosmic star formation history at z>3 is primarily based on UV-selected galaxies (i.e., LBGs). Recent studies of H-dropouts have revealed that we ma…

astro-ph.GA2022★ 24 cited

The Prime Focus Spectrograph Galaxy Evolution Survey

Jenny Greene, Rachel Bezanson, Masami Ouchi +2

We present the Prime Focus Spectrograph (PFS) Galaxy Evolution pillar of the 360-night PFS Subaru Strategic Program. This 130-night program will capitalize on the wide wavelength c…

astro-ph.GA2022★ 6 cited

ALPINE: A Large Survey to Understand Teenage Galaxies

A. L. Faisst, L. Yan, M. Béthermin +13

A multiwavelength study of galaxies is important to understand their formation and evolution. Only in the recent past, thanks to the Atacama Large (Sub) Millimeter Array (ALMA), we…

astro-ph.GA2022★ 11 cited

Concordance between observations and simulations in the evolution of the mass relation between supermassive black holes and their host galaxies

Xuheng Ding, John D. Silverman, Tommaso Treu +7

We carry out a comparative analysis of the relation between the mass of supermassive black holes (BHs) and the stellar mass of their host galaxies at using well-matched…

astro-ph.GA2022★ 4 cited

Inferences on relations between distant supermassive black holes and their hosts complemented by the galaxy fundamental plane

John Silverman, Junyao Li, Xuheng Ding

The realization of fundamental relations between supermassive black holes and their host galaxies would have profound implications in astrophysics. To add further context to studie…

astro-ph.GA2022★ 22 cited

On the Connection between Supermassive Black Hole and Galaxy Growth in the Reionization Epoch

Junyao Li, John D. Silverman, Takuma Izumi +6

The correlation between the mass of supermassive black holes (SMBHs; ) and their host galaxies () in the reionization epoch provides valuab…

astro-ph.GA2022★ 19 cited

The ALPINE-ALMA [CII] Survey: the population of [CII]-undetected galaxies and their role in the -SFR relation

Michael Romano, L. Morselli, P. Cassata +22

The [CII] 158m emission line represents so far one of the most profitable tools for the investigation of the high-redshift galaxies in the early Universe. Being one of the brig…

astro-ph.GA2022★ 15 cited

The ALPINE-ALMA [CII] Survey: Investigation of 10 Galaxies at with [OII] and [CII] Line Emission ISM Properties and [OII]SFR Relation

Brittany N. Vanderhoof, A. L. Faisst, L. Shen +23

We present main-sequence ALPINE galaxies (log() = 9.2-11.1 and ) at with optical [OII] measurements from Ke…