activity
20162026
most citedHubble Space Telescope Observations of Extended [O III] λ5007 Emission in Nearby QSO2s: New Constraints On AGN / Host Galaxy Interaction

107 citations · 759 across the 35 of their papers we have counts for

collaborators

35 papers

astro-ph.GA2026

On the Tully-Fisher Relation for Active Galaxies -- I: Evidence of Larger Scatter

Justin H. Robinson, Mitchell Revalski, Misty C. Bentz +12

We present an investigation of the Tully-Fisher (TF) relation solely for galaxies hosting an active galactic nucleus (AGN). Using 22 galaxies with primary, z-independent distances,…

astro-ph.GA2026★ 1 cited

An Analysis of AGN Feedback in the Compact Galaxy Group Stephan's Quintet

Maura Kathleen Shea, D. Michael Crenshaw, Travis C. Fischer +7

Compact galaxy groups are ideal laboratories for studying the effects of interactions between AGN and multiple nearby galaxies. Recent JWST observations of the nearby compact group…

astro-ph.GA2025

Footprints in the Wind: Probing X-ray Outflows in NGC 7469 using Near-Infrared Emission Lines

Léa M. Feuillet, Steve Kraemer, Anna Trindade Falcão +7

AGN winds play an important role in the co-evolution of supermassive black holes and their host galaxies, yet their driving mechanisms and impact on star formation remain subjects…

astro-ph.GA2025

Hot, Photoionized X-ray Gas in Two Luminous Type 2 Quasars: Chandra-HST Evidence for a Wind-Driven Sequence

Anna Trindade Falcão, S. Kraemer, L. Feuillet +17

We present new Chandra/ACIS-S imaging spectroscopy of two luminous type 2 quasars, FIRST J120041.4+314745 (=0.116) and 2MASX J13003807+5454367 (=0.088), and compare their X-r…

astro-ph.GA2025

Spatially Resolved, Multiphase Mass Outflows of the Seyfert 1 Galaxy NGC 3227

Julia Falcone, D. Michael Crenshaw, Mitchell Revalski +6

We present spatially resolved mass outflow rates of the ionized and molecular gas in the narrow line region of the Seyfert 1 galaxy NGC 3227. Using long-slit spectroscopy and [O II…

astro-ph.GA2025★ 1 cited

The Shape of AGN-Driven Winds in the Seyfert Galaxy NGC 3516

Jacob Tutterow, Nicholas Ferree, D. Michael Crenshaw +7

Active galactic nuclei (AGN) are known to drive ionized gas into their host galaxies, which may affect the evolution of both the central supermassive black holes and their hosts. I…

astro-ph.GA2025

Quantifying Feedback from Narrow Line Region Outflows in Nearby Active Galaxies. V. The Expanded Sample

Mitchell Revalski, D. Michael Crenshaw, Garrett E. Polack +8

We present spatially-resolved measurements of the ionized gas masses and mass outflow rates for six low-redshift ( 0.02) active galaxies. In this study, we expand our sampl…

astro-ph.GA2024

Hubble Space Telescope Observations of Nearby Type 1 Quasars. I. Characterisation of the Extended [O III] 5007Å Emission

Anna Trindade Falcão, S. B. Kraemer, T. C. Fischer +13

We use the Hubble Space Telescope to analyse the extended [O III] 5007A emission in seven bright radio-quiet type 1 quasars (QSO1s), focusing on the morphology and physical conditi…

astro-ph.GA2024

Determining the Extents, Geometries, and Kinematics of Narrow-Line Region Outflows in Nearby Seyfert Galaxies

Garrett E. Polack, Mitchell Revalski, D. Michael Crenshaw +5

Outflowing gas from supermassive black holes in the centers of active galaxies has been postulated as a major contributor to galactic evolution. To explore the interaction between…

astro-ph.GA2024

An Analysis of AGN-Driven Outflows in the Seyfert 1 Galaxy NGC 3227

Julia Falcone, D. Michael Crenshaw, Travis C. Fischer +8

We have characterized the ionized, neutral, and warm molecular gas kinematics in the Seyfert 1 galaxy NGC 3227 using observations from the Hubble Space Telescope Space Telescope Im…

astro-ph.GA2023★ 59 cited

Complex AGN feedback in the Teacup galaxy. A powerful ionised galactic outflow, jet-ISM interaction, and evidence for AGN-triggered star formation in a giant bubble

G. Venturi, E. Treister, C. Finlez +10

The ~0.1 type-2 QSO J1430+1339 (the 'Teacup') is a complex galaxy showing a loop of ionised gas ~10 kpc in diameter, co-spatial radio bubbles, a compact (~1 kpc) jet, and outflo…

astro-ph.GA2023

The MUSE Ultra Deep Field (MUDF). IV. A pair of X-ray weak quasars at the heart of two extended Lyα nebulae

Elisabeta Lusso, Emanuele Nardini, Michele Fumagalli +10

We present the results obtained from follow-up observations of the MUSE Ultra Deep Field (MUDF) at X-ray energies with XMM-Newton. The MUDF is centred on a unique field with two br…

astro-ph.GA2023★ 34 cited

Metal line emission from galaxy haloes at z~1

Rajeshwari Dutta, Matteo Fossati, Michele Fumagalli +12

We present a study of the metal-enriched halo gas, traced using MgII and [OII] emission lines, in two large, blind galaxy surveys - the MUSE (Multi Unit Spectroscopic Explorer) Ana…

astro-ph.GA2023★ 19 cited

The MUSE Ultra Deep Field (MUDF). III. Hubble Space Telescope WFC3 Grism Spectroscopy and Imaging

Mitchell Revalski, Marc Rafelski, Michele Fumagalli +18

We present extremely deep Hubble Space Telescope (HST) Wide Field Camera 3 (WFC3) observations of the MUSE Ultra Deep Field (MUDF). This unique region of the sky contains two quasa…

astro-ph.GA2023★ 48 cited

The AGNIFS survey: spatially resolved observations of hot molecular and ionised outflows in nearby active galaxies

R. A. Riffel, T. Storchi-Bergmann, R. Riffel +17

We present the hot molecular and warm ionised gas kinematics for 33 nearby () X-ray selected active galaxies using the Hm and Br emiss…

astro-ph.GA2023★ 28 cited

A Catalog of 71 Coronal Line Galaxies in MaNGA: [NeV] is an Effective AGN Tracer

James Negus, Julia M. Comerford, Francisco Muller Sanchez +5

Despite the importance of AGN in galaxy evolution, accurate AGN identification is often challenging, as common AGN diagnostics can be confused by contributions from star formation…

astro-ph.GA2022★ 23 cited

Investigating the Narrow Line Region Dynamics in Nearby Active Galaxies

Beena Meena, D. Michael Crenshaw, Henrique R. Schmitt +7

We present dynamical models of the narrow line region (NLR) outflows in the nearby Seyfert galaxies Mrk 3, Mrk 78, NGC 1068, and NGC 4151 using observations from the Hubble Space T…

astro-ph.GA2022★ 1 cited

Hubble Space Telescope Observations of Tadpole Galaxies Kiso 3867, SBS0, SBS1, and UM461

Debra Meloy Elmegreen, Bruce G. Elmegreen, John S. Gallagher +8

Tadpole galaxies are metal-poor dwarfs with typically one dominant star-forming region, giving them a head-tail structure when inclined. A metallicity drop in the head suggests tha…

astro-ph.GA2022★ 8 cited

Jansky Very Large Array detections of CO(1-0) emission in HI-absorption-selected galaxies at

Balpreet Kaur, Nissim Kanekar, Marc Rafelski +3

We report a Karl G. Jansky Very Large Array search for redshifted CO(1-0) emission from three HI-absorption-selected galaxies at , identified earlier in their CO(3-2)…

astro-ph.GA2022★ 9 cited

A Massive, Dusty HI-Absorption-Selected Galaxy at Identified in a CO Emission Survey

Balpreet Kaur, Nissim Kanekar, Mitchell Revalski +4

We report a NOrthern Extended Millimeter Array (NOEMA) and Atacama Large Millimeter/submillimeter Array (ALMA) search for redshifted CO emission from the galaxies associated with s…

astro-ph.GA2022

Quantifying Feedback from Narrow Line Region Outflows in Nearby Active Galaxies. IV. The Effects of Different Density Estimates on the Ionized Gas Masses and Outflow Rates

Mitchell Revalski, D. Michael Crenshaw, Marc Rafelski +9

Active galactic nuclei (AGN) can launch outflows of ionized gas that may influence galaxy evolution, and quantifying their full impact requires spatially resolved measurements of t…

astro-ph.GA2021★ 8 cited

Tracking X-ray Outflows with Optical/IR Footprint Lines

Anna Trindade Falcao, S. B. Kraemer, D. M. Crenshaw +5

We use Cloudy photoionisation models to predict the flux profiles for optical/IR emission lines that trace the footprint of X-ray gas, such as [Fe X] 6375A and [Si X] 1.43m. The…

astro-ph.GA2021★ 21 cited

Lyman Continuum Galaxy Candidates in COSMOS

Laura J. Prichard, Marc Rafelski, Jeff Cooke +11

Star-forming galaxies are the sources likely to have reionized the universe. As we cannot observe them directly due to the opacity of the intergalactic medium at , we st…

astro-ph.GA2021★ 14 cited

The nature of H{\sc i}-absorption-selected galaxies at

B. Kaur, N. Kanekar, M. Rafelski +3

We report a Karl G. Jansky Very Large Array (JVLA) search for redshifted CO(1-0) or CO(2-1) emission, and a Hubble Space Telescope Wide Field Camera~3 (HST-WFC3) search for rest-fr…