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20032026
most citedThe Chandra Deep Field-South Survey: 4 Ms Source Catalogs

581 citations · 9.2k across the 114 of their papers we have counts for

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47 papers · 1 filter

astro-ph.GA2026

Constructing X-ray Spectral Models of Galaxies: Varying Contributions from X-ray Binary Populations with Host Galaxy Properties

Emerson Gehr, Bret D. Lehmer, Antara R. Basu-Zych +7

Recent work has shown that the emission from X-ray binary (XRB) populations in galaxies varies with stellar mass (), star formation rate (SFR), and metallicity (). Such…

astro-ph.GA2025

Deep X-ray observation of NGC 3221: everything everywhere all at once

Sanskriti Das, Smita Mathur, Bret D. Lehmer +3

We present a comprehensive analysis of 475 ks (438 ks unpublished & 37 ks archival) XMM-Newton/EPIC-pn observation of a nearby, highly inclined, star-forming, luminous infrared gal…

astro-ph.GA2025

XMM-Newton Conclusively Identifies an Active Galactic Nucleus in a Green Pea Galaxy

Peter G. Boorman, Jiří Svoboda, Daniel Stern +23

Green Pea galaxies are a class of compact, low-mass, low-metallicity star-forming galaxies in the relatively local universe. They are believed to be analogues of high-redshift gala…

astro-ph.GA2025★ 3 cited

Emission Line Diagnostics for IMBHs in Dwarf Galaxies: Accounting for BH Seeding and ULX Excitation

Chris T. Richardson, Jordan Wels, Kristen Garofali +13

Dwarf AGN serve as the ideal systems for identifying intermediate mass black holes (IMBHs) down to the most elusive regimes (). However, the ubiquitousl…

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.GA2023

Modeling the High-Energy Ionizing Output from Simple Stellar and X-ray Binary Populations

Kristen Garofali, Antara R. Basu-Zych, Benjamin D. Johnson +9

We present a methodology for modeling the joint ionizing impact due to a "simple X-ray population" (SXP) and its corresponding simple stellar population (SSP), where "simple" refer…