activity
19992026
most citedSpitzer view on the evolution of star-forming galaxies from z=0 to z~3

503 citations · 1.9k across the 24 of their papers we have counts for

collaborators

25 papers

astro-ph.GA2026

Multiphase Analysis of (U)LIRG Nuclear Activity (MAUNA). I. Spatially Resolved Optical Emission-Line Diagnostics

Justin A. Kader, Vivian U, Marina Bianchin +33

We present resolved optical integral-field spectroscopy of the 32 luminous and ultraluminous infrared galaxy systems of the Multiphase Analysis of (U)LIRG Nuclear Activity (MAUNA)…

astro-ph.IM2021

End-to-end ground calibration and in-flight performance of the FIREBall-2 instrument

Vincent Picouet, Bruno Milliard, Gillian Kyne +18

The payload of the Faint Intergalactic Redshifted Emission Balloon (FIREBall-2), the second generation of the FIREBall instrument (PI: C. Martin, Caltech), has been calibrated and…

astro-ph.GA2021★ 31 cited

Spatially Resolved Stellar Spectroscopy of the Ultra-diffuse Galaxy Dragonfly 44. III. Evidence for an Unexpected Star-Formation History

Alexa Villaume, Aaron J. Romanowsky, Jean Brodie +6

We use the Keck Cosmic Web Imager integral-field unit spectrograph to: 1) measure the global stellar population parameters for the ultra-diffuse galaxy (UDG) Dragonfly 44 (DF44) to…

astro-ph.GA2020★ 40 cited

Spectroscopic Confirmation of a Coma Cluster Progenitor at z ~ 2.2

Behnam Darvish, Nick Z. Scoville, Christopher Martin +17

We report the spectroscopic confirmation of a new protocluster in the COSMOS field at 2.2, COSMOS Cluster 2.2 (CC2.2), originally identified as an overdensity of narrowb…

astro-ph.GA2019★ 40 cited

The Dark Matter Distributions in Low-Mass Disk Galaxies. II. The Inner Density Profiles

Nicole C. Relatores, Andrew B. Newman, Joshua D. Simon +8

Dark matter-only simulations predict that dark matter halos have steep, cuspy inner density profiles, while observations of dwarf galaxies find a range of inner slopes that are oft…

astro-ph.GA2019★ 49 cited

The FLASHES Survey I: Integral Field Spectroscopy of the CGM around 48 QSOs

Donal O'Sullivan, Christopher Martin, Mateusz Matuszewski +5

We present the pilot study component of the Fluorescent Lyman-Alpha Structures in High-z Environments (FLASHES) Survey; the largest integral-field spectroscopy survey to date of th…

astro-ph.GA2019★ 53 cited

Spatially Resolved Stellar Kinematics of the Ultra-Diffuse Galaxy Dragonfly 44: II. Constraints on Fuzzy Dark Matter

Asher Wasserman, Pieter van Dokkum, Aaron J. Romanowsky +9

Given the absence of directly detected dark matter (DM) as weakly interacting massive particles, there is strong interest in the possibility that DM is an ultra-light scalar field,…

astro-ph.IM2019

FIREBall-2: advancing TRL while doing proof-of-concept astrophysics on a suborbital platform

Erika T. Hamden, Keri Hoadley, D. Christopher Martin +32

Here we discuss advances in UV technology over the last decade, with an emphasis on photon counting, low noise, high efficiency detectors in sub-orbital programs. We focus on the u…

astro-ph.GA2019★ 112 cited

Spatially-resolved stellar kinematics of the ultra diffuse galaxy Dragonfly 44. I. Observations, kinematics, and cold dark matter halo fits

Pieter van Dokkum, Asher Wasserman, Shany Danieli +8

We present spatially-resolved stellar kinematics of the well-studied ultra diffuse galaxy (UDG) Dragonfly 44, as determined from 25.3 hrs of observations with the Keck Cosmic Web I…

astro-ph.GA2019★ 10 cited

The Dark Matter Distributions in Low-Mass Disk Galaxies. I. H Observations Using the Palomar Cosmic Web Imager

Nicole C. Relatores, Andrew B. Newman, Joshua D. Simon +6

Dark-matter-only simulations predict that dark matter halos have cusp-like inner density profiles, while observations of low-mass galaxies have found a range of inner slopes that a…

astro-ph.HE2018★ 22 cited

Supernova PTF12glz: a possible shock breakout driven through an aspherical wind

Maayane T. Soumagnac, Eran O. Ofek, Avishay Gal-Yam +21

We present visible-light and ultraviolet (UV) observations of the supernova PTF12glz. The SN was discovered and monitored in near-UV and R bands as part of a joint GALEX and Paloma…

astro-ph.GA2018★ 34 cited

Similar Scaling Relations for the Gas Content of Galaxies across Environments to z ~ 3.5

Behnam Darvish, Nick Z. Scoville, Christopher Martin +3

We study the effects of the local environment on the molecular gas content of a large sample of log(/) 10 star-forming and starburst galaxies with speci…

astro-ph.GA2018★ 63 cited

Keck/Palomar Cosmic Web Imagers (KCWI/PCWI) Reveal an Enormous Ly Nebula in an Extremely Overdense QSO Pair Field at

Zheng Cai, Erika Hamden, Matt Matuszewski +10

Enormous Ly nebulae (ELANe) represent the extrema of Ly nebulosities. They have detected extents of kpc in Ly and Ly luminosities erg s. The EL…

astro-ph.GA2018★ 24 cited

Quenching or Bursting: the Role of Stellar Mass, Environment, and Specific Star Formation Rate to 1

Behnam Darvish, Christopher Martin, Thiago S. Gonçalves +3

Using a novel approach, we study the quenching and bursting of galaxies as a function of stellar mass (), local environment (), and specific star-formation rate (sSFR) us…

astro-ph.SR2012★ 57 cited

AT Cnc: A Second Dwarf Nova with a Classical Nova Shell

Michael M. Shara, Trisha Mizusawa, Peter Wehinger +5

We are systematically surveying all known and suspected Z Cam-type dwarf novae for classical nova shells. This survey is motivated by the discovery of the largest known classical n…

astro-ph.CO2012★ 28 cited

Halo Occupation Distribution Modeling of Green Valley Galaxies

Elisabeth Krause, Christopher M. Hirata, Christopher Martin +2

We present a clustering analysis of near ultraviolet (NUV) - optical color selected luminosity bin samples of green valley galaxies. These galaxy samples are constructed by matchin…

astro-ph.SR2012★ 32 cited

The Inter-Eruption Timescale of Classical Novae from Expansion of the Z Camelopardalis Shell

Michael M. Shara, Trisha Mizusawa, David Zurek +3

The dwarf nova Z Camelopardalis is surrounded by the largest known classical nova shell. This shell demonstrates that at least some dwarf novae must have undergone classical nova e…

astro-ph.CO2011★ 14 cited

SSGSS: The Spitzer-SDSS-GALEX Spectroscopic Survey

Matthew J. O'Dowd, David Schiminovich, Benjamin D. Johnson +8

The Spitzer-SDSS-GALEX Spectroscopic Survey (SSGSS) provides a new sample of 101 star-forming galaxies at z < 0.2 with unprecedented multi-wavelength coverage. New mid- to far-infr…

astro-ph.SR2010★ 125 cited

Catalogs of Hot White Dwarfs in the Milky Way from GALEX's Ultraviolet Sky Surveys. Constraining Stellar Evolution

Luciana Bianchi, Boryana Efremova, James Herald +4

We present comprehensive catalogs of hot star candidates in the Milky Way, selected from GALEX far-UV (FUV, 1344-1786 AA) and near-UV (NUV, 1771-2831 AA) imaging. The FUV and NUV p…

astro-ph.CO2010★ 129 cited

The GALEX Arecibo SDSS Survey II: The Star Formation Efficiency of Massive Galaxies

David Schiminovich, Barbara Catinella, Guinevere Kauffmann +23

We use measurements of the HI content, stellar mass and star formation rates in ~190 massive galaxies with stellar masses greater than 10^10 Msun, obtained from the Galex Arecibo S…

astro-ph.CO2009★ 424 cited

The GALEX Arecibo SDSS Survey. I. Gas Fraction Scaling Relations of Massive Galaxies and First Data Release

Barbara Catinella, David Schiminovich, Guinevere Kauffmann +23

We introduce the GALEX Arecibo SDSS Survey (GASS), an on-going large program that is gathering high quality HI-line spectra using the Arecibo radio telescope for an unbiased sample…

astro-ph.IM2009★ 5 cited

A Vigorous Explorer Program

Martin Elvis, Matthew Beasley, Roger Brissenden +47

Explorers have made breakthroughs in many fields of astrophysics. The science from both these missions contributed to three Nobel Prizes - Giacconi (2002), Mather, and Smoot (2006)…

astro-ph.CO2009★ 77 cited

Polycyclic Aromatic Hydrocarbons in Galaxies at z~0.1: the Effect of Star Formation and AGN

Matthew J. O'Dowd, David Schiminovich, Benjamin D. Johnson +8

We present the analysis of the Polycyclic Aromatic Hydrocarbon (PAH) spectra of a sample of 92 typical star forming galaxies at 0.03 < z < 0.2 observed with the Spitzer IRS. We com…

astro-ph2005★ 503 cited

Spitzer view on the evolution of star-forming galaxies from z=0 to z~3

Pablo G. Perez-Gonzalez, George H. Rieke, Eiichi Egami +11

We use a 24 micron selected sample containing more than 8,000 sources to study the evolution of star-forming galaxies in the redshift range from z=0 to z~3. We obtain photometric r…