activity
20112026
most citedInterpreting the Ionization Sequence in AGN Emission-Line Spectra

56 citations · 246 across the 13 of their papers we have counts for

collaborators

15 papers

astro-ph.GA2026

A Comprehensive AGN Inventory for the Dwarf-Dominated RESOLVE and ECO Surveys: Mass-Dependent AGN Types and Occupation Fractions

Mugdha S. Polimera, Sheila J. Kannappan, Chris T. Richardson +7

We catalog Active Galactic Nuclei (AGN) in the volume- and mass-limited RESOLVE and ECO surveys using (i) the BPT plot with standard and alternate demarcations, (ii) the BPT plot a…

astro-ph.GA2026

The Goldilocks Molecule: H Emission Lines Can Identify Elusive Dwarf AGN

Morgan Micharski, Chris Richardson

We propose using H emission lines as a novel diagnostic to identify dwarf AGN by running photoionization models incorporating active intermediate-mass black holes and using a…

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…

astro-ph.GA2023★ 2 cited

Modeling the molecular gas content and CO-to-H2 conversion factors in low-metallicity star-forming dwarf galaxies

L. Ramambason, V. Lebouteiller, S. C. Madden +8

Low-metallicity dwarf galaxies often show no or little CO emission, despite the intense star formation observed in local samples. Both simulations and resolved observations indicat…

astro-ph.GA2022★ 35 cited

Inferring the HII region escape fraction of ionizing photons from infrared emission lines in metal-poor star-forming dwarf galaxies

L. Ramambason, V. Lebouteiller, A. Bik +8

(abridged) Quantifying the ISM porosity to ionizing photons in nearby galaxies may improve our understanding of the mechanisms leading to Lyman Continuum photons leakage from galax…

astro-ph.GA2022★ 34 cited

RESOLVE and ECO: Finding Low-Metallicity Dwarf AGN Candidates Using Optimized Emission-Line Diagnostics

Mugdha S. Polimera, Sheila J. Kannappan, Chris T. Richardson +6

Existing star-forming vs. active galactic nucleus (AGN) classification schemes using optical emission-line diagnostics mostly fail for low-metallicity and/or highly star-forming ga…

astro-ph.GA2022★ 22 cited

Optical and JWST Mid-IR Emission Line Diagnostics for Simultaneous IMBH and Stellar Excitation in z~0 Dwarf Galaxies

C. T. Richardson, C. Simpson, M. S. Polimera +4

Current observational facilities have yet to conclusively detect intermediate mass black holes (IMBHs) that fill in the evolutionary gap between early unive…

astro-ph.GA2019★ 4 cited

Addressing the [O III]/H\b{eta} Offset of Dwarf Galaxies in the RESOLVE Survey

Chris T. Richardson, Mugdha S. Polimera, Sheila J. Kannappan +2

Metal poor dwarf galaxies in the local universe, such as those found in the RESOLVE galaxy survey, often produce high [O III]/H\b{eta} ratios close to the star forming demarcation…

astro-ph.GA2017★ 1 cited

An Atlas of Star-Forming Galaxy Equivalent Widths

Helen Meskhidze, Chris T. Richardson

We present an atlas of starburst galaxy emission lines spanning 10 orders of magnitude in ionizing flux and 7 orders of magnitude in hydrogen number density. Coupling SEDs from Sta…

astro-ph.GA2016★ 22 cited

Interpreting the Ionization Sequence in Star-Forming Galaxy Emission-Line Spectra

Chris T. Richardson, James T. Allen, Jack A. Baldwin +4

High ionization star forming (SF) galaxies are easily identified with strong emission line techniques such as the BPT diagram, and form an obvious ionization sequence on such diagr…

astro-ph.CO2013★ 56 cited

Interpreting the Ionization Sequence in AGN Emission-Line Spectra

Chris T. Richardson, James T. Allen, Jack A. Baldwin +2

We investigate the physical cause of the great range in the ionization level seen in the spectra of narrow lined active galactic nuclei (AGN). Mean field independent component anal…

astro-ph.GA2013★ 4 cited

Detecting the rapidly expanding outer shell of the Crab Nebula: where to look

Xiang Wang, G. J. Ferland, J. A. Baldwin +2

We present a range of steady-state photoionization simulations, corresponding to different assumed shell geometries and compositions, of the unseen postulated rapidly expanding out…

astro-ph.CO2013★ 29 cited

Classification and analysis of emission-line galaxies using mean field independent component analysis

James T. Allen, Paul C. Hewett, Chris T. Richardson +2

We present an analysis of the optical spectra of narrow emission-line galaxies, based on mean field independent component analysis (MFICA). Samples of galaxies were drawn from the…

astro-ph.GA2013★ 19 cited

The Nature of the H2-Emitting Gas in the Crab Nebula

C. T. Richardson, J. A. Baldwin, G. J. Ferland +4

Understanding how molecules and dust might have formed within a rapidly expanding young supernova remnant is important because of the obvious application to vigorous supernova acti…

astro-ph.GA2011★ 18 cited

H2 Temperatures in the Crab Nebula

E. D. Loh, J. A. Baldwin, G. J. Ferland +4

We used K-band spectra to measure the H2 excitation temperatures in six molecular knots associated with the filaments in the Crab Nebula. The temperatures are quite high - in the r…