activity
20082026
most citedAn upper limit on the contribution of accreting white dwarfs to the type Ia supernova rate

197 citations · 1.7k across the 73 of their papers we have counts for

collaborators
Showing 2023Show all

14 papers · 1 filter

astro-ph.GA2023★ 1 cited

Unraveling the Mysteries of Galaxy Clusters: Recurrent Inference Deconvolution of X-ray Spectra

Carter Rhea, Julie Hlavacek-Larrondo, Ralph Kraft +3

In the realm of X-ray spectral analysis, the true nature of spectra has remained elusive, as observed spectra have long been the outcome of convolution between instrumental respons…

astro-ph.IM2023★ 2 cited

LEM All-Sky Survey: Soft X-ray Sky at Microcalorimeter Resolution

Ildar Khabibullin, Massimiliano Galeazzi, Akos Bogdan +23

The Line Emission Mapper (LEM) is an X-ray Probe with with spectral resolution ~2 eV FWHM from 0.2 to 2.5 keV and effective area >2,500 cm at 1 keV, covering a 33 arcmin diamet…

astro-ph.HE2023

Mapping the Intracluster Medium in the Era of High-resolution X-ray Spectroscopy

Congyao Zhang, Irina Zhuravleva, Maxim Markevitch +24

High-resolution spectroscopy in soft X-rays will open a new window to map multiphase gas in galaxy clusters and probe physics of the intracluster medium (ICM), including chemical e…

astro-ph.HE2023

Probing extreme black-hole outflows on short timescales via high spectral-resolution X-ray imagers

Ciro Pinto, James F. Steiner, Arash Bodaghee +7

We investigate outflows and the physics of super-Eddington versus sub-Eddington regimes in black hole systems. Our focus is on prospective science using next-generation high-resolu…

astro-ph.IM2023★ 2 cited

Revolutionary Solar System Science Enabled by the Line Emission Mapper X-ray Probe

William R. Dunn, Dimitra Koutroumpa, Jennifer A. Carter +27

The Line Emission Mapper's (LEM's) exquisite spectral resolution and effective area will open new research domains in Astrophysics, Planetary Science and Heliophysics. LEM will pro…

astro-ph.GA2023★ 7 cited

UNCOVER: The growth of the first massive black holes from JWST/NIRSpec -- spectroscopic redshift confirmation of an X-ray luminous AGN at z=10.1

Andy D. Goulding, Jenny E. Greene, David J. Setton +27

The James Webb Space Telescope is now detecting early black holes (BHs) as they transition from "seeds" to supermassive BHs. Recently Bogdan et al. (2023) reported the detection of…

astro-ph.GA2023★ 29 cited

X-ray metal line emission from the hot circumgalactic medium: probing the effects of supermassive black hole feedback

Nhut Truong, Annalisa Pillepich, Dylan Nelson +15

We derive predictions from state-of-the-art cosmological galaxy simulations for the spatial distribution of the hot circumgalactic medium (CGM, ) through its…

astro-ph.CO2023★ 11 cited

Painting baryons onto N-body simulations of galaxy clusters with image-to-image deep learning

Urmila Chadayammuri, Michelle Ntampaka, John ZuHone +2

Galaxy cluster mass functions are a function of cosmology, but mass is not a direct observable, and systematic errors abound in all its observable proxies. Mass-free inference can…

astro-ph.GA2023★ 5 cited

A high black hole to host mass ratio in a lensed AGN in the early Universe

Lukas J. Furtak, Ivo Labbé, Adi Zitrin +34

Early JWST observations have uncovered a new population of red sources that might represent a previously overlooked phase of supermassive black hole growth (Kocevski et al. 2023; M…

astro-ph.HE2023★ 4 cited

First Detection of an Over-Massive Black Hole Galaxy UHZ1: Evidence for Heavy Black Hole Seed Formation from Direct Collapse

Priyamvada Natarajan, Fabio Pacucci, Angelo Ricarte +3

The recent Chandra-JWST discovery of a quasar in the z = 10.1 galaxy UHZ1 reveals that accreting supermassive black holes (SMBHs) were already in place 470 million years after the…

astro-ph.GA2023

Properties of the Line-of-Sight Velocity Field in the Hot and X-ray Emitting Circumgalactic Medium of Nearby Simulated Disk Galaxies

J. A. ZuHone, G. Schellenberger, A. Ogorzalek +16

The hot, X-ray-emitting phase of the circumgalactic medium of massive galaxies is believed to be the reservoir of baryons from which gas flows onto the central galaxy and into whic…

astro-ph.GA2023★ 19 cited

Resonant scattering of the OVII X-ray emission line in the circumgalactic medium of TNG50 galaxies

Dylan Nelson, Chris Byrohl, Anna Ogorzalek +15

We study the impact of resonantly scattered X-ray line emission on the observability of the hot circumgalactic medium (CGM) of galaxies. We apply a Monte Carlo radiative transfer p…

astro-ph.GA2023★ 9 cited

Circumgalactic Medium on the Largest Scales: Detecting X-ray Absorption Lines with Large-Area Microcalorimeters

Akos Bogdan, Ildar Khabibullin, Orsolya Kovacs +22

The circumgalactic medium (CGM) plays a crucial role in galaxy evolution as it fuels star formation, retains metals ejected from the galaxies, and hosts gas flows in and out of gal…

astro-ph.GA2023★ 20 cited

Evidence for heavy seed origin of early supermassive black holes from a z~10 X-ray quasar

Akos Bogdan, Andy Goulding, Priyamvada Natarajan +9

Observations of quasars reveal that many supermassive black holes (BHs) were in place less than 700 million years after the Big Bang. However, the origin of the first BHs remains a…