activity
20052024
most citedThe Evolution of Normal Galaxy X-ray Emission Through Cosmic History: Constraints from the 6 Ms Chandra Deep Field-South

230 citations · 1.1k across the 27 of their papers we have counts for

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20 papers · 1 filter

astro-ph.GA2024

An Empirical Framework Characterizing the Metallicity and Star-Formation History Dependence of X-ray Binary Population Formation and Emission in Galaxies

Bret D. Lehmer, Erik B. Monson, Rafael T. Eufrasio +12

We present a new empirical framework modeling the metallicity and star-formation history (SFH) dependence of X-ray luminous ( ergs s) point-source population lu…

astro-ph.GA2023★ 16 cited

Revisiting the Properties of X-ray AGN in the SSA22 Protocluster: Normal SMBH and Host-Galaxy Growth for AGN in a Overdensity

Erik B. Monson, Keith Doore, Rafael T. Eufrasio +6

We analyze the physical properties of 8 X-ray selected active galactic nuclei (AGN) and one candidate protoquasar system (ADF22A1) in the SSA22 protocluster by fitting t…

astro-ph.GA2023★ 10 cited

Lightning: An X-ray to Submillimeter Galaxy SED-Fitting Code With Physically-Motivated Stellar, Dust, and AGN Models

Keith Doore, Erik B. Monson, Rafael T. Eufrasio +3

We present an updated version of Lightning, a galaxy spectral energy distribution (SED) fitting code that can model X-ray to submillimeter observations. The models in Lightning inc…

astro-ph.GA2022★ 4 cited

The Impact of Inclination-dependent Attenuation on Ultraviolet Star Formation Rate Tracers

Keith Doore, Rafael T. Eufrasio, Bret D. Lehmer +3

We examine and quantify how hybrid (e.g., UV+IR) star formation rate (SFR) estimators and the - relation depend on inclination for disk-dominated galaxies using spe…

astro-ph.GA2022★ 29 cited

Elevated Hot Gas and High-Mass X-ray Binary Emission in Low Metallicity Galaxies: Implications for Nebular Ionization and Intergalactic Medium Heating in the Early Universe

Bret D. Lehmer, Rafael T. Eufrasio, Antara Basu-Zych +4

High-energy emission associated with star formation has been proposed as a significant source of interstellar medium (ISM) ionization in low-metallicity starbursts and an important…

astro-ph.GA2021★ 13 cited

On the Impact of Inclination-Dependent Attenuation on Derived Star Formation Histories: Results from Disk Galaxies in the Great Observatories Origins Deep Survey Fields

Keith Doore, Rafael T. Eufrasio, Bret D. Lehmer +4

We develop and implement an inclination-dependent attenuation prescription for spectral energy distribution (SED) fitting and study its impact on derived star-formation histories.…

astro-ph.GA2021★ 21 cited

On the Nature of AGN and Star Formation Enhancement in the SSA22 Protocluster: The HST WFC3 IR View

Erik B. Monson, Bret D. Lehmer, Keith Doore +9

We examine possible environmental sources of the enhanced star formation and active galactic nucleus (AGN) activity in the SSA22 protocluster using Hubble WFC3 F160W ($\…

astro-ph.GA2021★ 12 cited

Local Analogs to High-Redshift Galaxies: I. Characterization of Dust Emission and Star Formation History

Skarleth M Motiño Flores, Tommy Wiklind, Rafael T. Eufrasio

Star-forming dwarf galaxies have properties similar to those expected in high-redshift galaxies. Hence, these local galaxies may provide insights into the evolution of the first ga…

astro-ph.GA2020★ 90 cited

The Metallicity Dependence of the High-Mass X-ray Binary Luminosity Function

Bret D. Lehmer, Rafael T. Eufrasio, Antara Basu-Zych +7

We present detailed constraints on the metallicity dependence of the high mass X-ray binary (HMXB) X-ray luminosity function (XLF). We analyze ~5 Ms of Chandra data for 55 actively…

astro-ph.GA2020★ 16 cited

Evidence in favour of density wave theory through star formation history maps and spatially resolved stellar clusters

Shameer Abdeen, Daniel Kennefick, Julia Kennefick +7

Stationary Density Wave Theory predicts the existence of an age gradient across the spiral arms with a phase crossing at the co-rotation radius. Using star formation history (SFH)…

astro-ph.GA2020★ 34 cited

X-ray Binary Luminosity Function Scaling Relations in Elliptical Galaxies: Evidence for Globular Cluster Seeding of Low-Mass X-ray Binaries in Galactic Fields

Bret D. Lehmer, Andrew P. Ferrell, Keith Doore +10

We investigate X-ray binary (XRB) luminosity function (XLF) scaling relations for Chandra detected populations of low-mass XRBs (LMXBs) within the footprints of 24 early-type galax…

astro-ph.GA2020★ 4 cited

The Environment of Lyman Break Analogues (ELBA) survey: Star-forming galaxies in small groups

L. Santana-Silva, T. S. Gonçalves, A. Basu-Zych +7

The Environment of Lyman Break Analogues (ELBA) survey is an imaging survey of 33 of the southern sky. The survey was observed in {\it u}, {\it g}, {\it r}, and {\it i} b…

astro-ph.GA2019★ 24 cited

Investigating the Origins of Spiral Structure in Disk Galaxies through a Multiwavelength Study

Ryan Miller, Daniel Kennefick, Julia Kennefick +5

The density-wave theory of spiral structure proposes that star formation occurs in or near a spiral-shaped region of higher density that rotates rigidly within the galactic disk at…

astro-ph.GA2019★ 125 cited

X-ray Binary Luminosity Function Scaling Relations for Local Galaxies Based on Subgalactic Modeling

Bret D. Lehmer, Rafael T. Eufrasio, Panayiotis Tzanavaris +7

We present new Chandra constraints on the X-ray luminosity functions (XLFs) of X-ray binary (XRB) populations, and their scaling relations, for a sample of 38 nearby galaxies (D =…

astro-ph.GA2017★ 35 cited

On the Spatially Resolved Star-Formation History in M51 II: X-ray Binary Population Evolution

B. D. Lehmer, R. T Eufrasio, L. Markwardt +7

We present a new technique for empirically calibrating how the X-ray luminosity function (XLF) of X-ray binary (XRB) populations evolves following a star-formation event. We first…

astro-ph.GA2017★ 36 cited

On the Spatially Resolved Star Formation History in M51 I: Hybrid UV+IR Star Formation Laws and IR Emission from Dust Heated by Old Stars

R. T. Eufrasio, B. D. Lehmer, A. Zezas +10

We present Lightning, a new spectral energy distribution (SED) fitting procedure, capable of quickly and reliably recovering star formation history (SFH) and extinction parameters.…

astro-ph.GA2017★ 14 cited

Further constraints on variations in the IMF from LMXB populations

Mark B. Peacock, Stephen E. Zepf, Arunav Kundu +6

We present constraints on variations in the initial mass function (IMF) of nine local early-type galaxies based on their low mass X-ray binary (LMXB) populations. Comprised of accr…

astro-ph.GA2016★ 230 cited

The Evolution of Normal Galaxy X-ray Emission Through Cosmic History: Constraints from the 6 Ms Chandra Deep Field-South

B. D. Lehmer, A. R. Basu-Zych, S. Mineo +17

We present measurements of the evolution of normal-galaxy X-ray emission from 0-7 using local galaxies and galaxy samples in the 6 Ms Chandra Deep Field-South (CDF-S) s…

astro-ph.GA2015

A Multiwavelength Study of Tadpole Galaxies in the Hubble Ultra Deep Field

Amber N. Straughn, Elysse N. Voyer, Rafael T. Eufrasio +6

Multiwavelength data are essential in order to provide a complete picture of galaxy evolution and to inform studies of galaxies' morphological properties across cosmic time. Here w…

astro-ph.GA2014★ 16 cited

Star Formation Histories Across the Interacting Galaxy NGC 6872, the Largest-Known Spiral

Rafael T. Eufrasio, Eli Dwek, Richard G. Arendt +5

NGC 6872, hereafter the Condor, is a large spiral galaxy that is interacting with its closest companion, the S0 galaxy IC 4970. The extent of the Condor provides an opportunity for…