activity
19952025
most citedThe reversal of the star formation-density relation in the distant universe

1.6k citations · 2k across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.HE2025★ 3 cited

The Advanced X-ray Imaging Satellite (AXIS) Community Science Book

Michael Koss, Nafisa Aftab, Steven W. Allen +395

The AXIS Community Science Book represents the collective effort of 592 scientists worldwide to define the transformative science enabled by the Advanced X-ray Imaging Satellite (A…

astro-ph.GA2025

Radio Follow-Up Observations of a Weak-Line Quasar Exhibiting Remarkable X-ray Variability

Ayushi Chhipa, M. Vivek, Nayana A. J. +6

SDSSJ1539+3954 (), a radio-quiet weak-line quasar (WLQ), exhibited exceptional X-ray variability in 20192020, with its X-ray flux increasing by over 20 times fro…

astro-ph.GA2025★ 1 cited

Intervening nuclear obscuration changing the X-ray look of the QSO CFHQS J164121+375520

Fabio Vito, William Nielsen Brandt, Andrea Comastri +16

X-ray observations of the optically selected QSO CFHQS J164121+375520 (hereafter J1641) revealed that its flux dropped by a factor from 2018, when it was a bri…

astro-ph.HE2024

The Remarkable X-ray Spectra and Variability of the Ultraluminous Weak-Line Quasar SDSS J1521+5202

Shouyi Wang, W. Niel Brandt, Bin Luo +4

We present a focused X-ray and multiwavelength study of the ultraluminous weak-line quasar (WLQ) SDSS J1521+5202, one of the few X-ray weak WLQs that is amenable to basic X-ray spe…

astro-ph.GA2024★ 17 cited

Fast SMBH growth in the SPT2349--56 protocluster at

Fabio Vito, William N. Brandt, Andrea Comastri +7

Protoclusters at are gas-rich regions characterized by high star-formation activity. The same physical properties that enhance star formation in protoclusters are also though…

astro-ph.CO2024★ 3 cited

The XMM-SERVS X-ray eXtended Galaxy Cluster (XVXGC) catalog

Weiwei Xu, Linhua Jiang, Ran Li +4

To explain the well-known tension between cosmological parameter constraints obtained from the primary CMB and those drawn from galaxy cluster samples, we propose a possible explan…