Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- California Institute of TechnologyUS2.6k papers
- Centre National de la Recherche ScientifiqueFR2k papers
- Massachusetts Institute of TechnologyUS1.9k papers
- University of FloridaUS1.8k papers
- Carnegie Mellon UniversityUS1.7k papers
- Princeton UniversityUS1.7k papers
- University of RochesterUS1.7k papers
- Purdue University West LafayetteUS1.6k papers
- Johns Hopkins UniversityUS1.6k papers
- University of Maryland, College ParkUS1.6k papers
- The Ohio State UniversityUS1.6k papers
- University of California, Santa BarbaraUS1.6k papers
44 papers · 2 filters
The Effects of Grain Size and Temperature Distributions on the Formation of Interstellar Ice Mantles
Tyler Pauly, Robin T. Garrod
Computational models of interstellar gas-grain chemistry have historically adopted a single dust-grain size of 0.1 micron, assumed to be representative of the size distribution pre…
Velocity resolved [CII] spectroscopy of the center and the BCLMP302 region of M33 (HerM33es)
B. Mookerjea, F. Israel, C. Kramer +8
We aim to understand the contribution of the ionized, atomic and molecular phases of the ISM to the [CII] emission from clouds near the dynamical center and the BCLMP302 HII region…
Multi-wavelength lens reconstruction of a -detected star-bursting galaxy
Nicholas Timmons, Asantha Cooray, Dominik A. Riechers +21
We present a source-plane reconstruction of a and -detected gravitationally-lensed dusty star-forming galaxy (DSFG) at using {\it Hubble}, S…
Leo P: How Many Metals can a Very Low-Mass, Isolated Galaxy Retain?
Kristen B. W. McQuinn, Evan D. Skillman, Andrew Dolphin +7
Leo P is a gas-rich dwarf galaxy with an extremely low gas-phase oxygen abundance (3% solar). The isolated nature of Leo P enables a quantitative measurement of metals lost solely…
Intermittent Self-Sustaining Star Formation in Low-Redshift Galaxies Exhibiting a Peak Metallicity Plateau
Martin Harwit
The decline of star formation in massive low-redshift galaxies, often referred to as quenching, has been attributed to a variety of factors. Some proposals suggest that erupting ac…
The Infrared Database of Extragalactic Observables from Spitzer I: the redshift catalog
Antonio Hernán-Caballero, Henrik W. W. Spoon, Vianney Lebouteiller +2
This is the first of a series of papers on the Infrared Database of Extragalactic Observables from Spitzer (IDEOS). In this work we describe the identification of optical counterpa…
Dusty Galaxies at the Highest Redshifts
David L Clements, Josh Greenslade, Dominik A. Riechers +5
We show that the use of red colour as the basis for selecting candidate high redshift dusty galaxies from surveys made with Herschel has proved highly successful. The highest redsh…
On the redshift distribution and physical properties of ACT-selected DSFGs
T. Su, T. A. Marriage, V. Asboth +25
We present multi-wavelength detections of nine candidate gravitationally-lensed dusty star-forming galaxies (DSFGs) selected at 218GHz (1.4mm) from the ACT equatorial survey. Among…
Next Generation Very Large Array Memo No. 8 Science Working Group 3: Galaxy Assembly through Cosmic Time
Caitlin M. Casey, Jacqueline A. Hodge, Mark Lacy +14
The Next-Generation Very Large Array (ngVLA) will be critical for understanding how galaxies are built and evolve at the earliest epochs. The sensitivity and frequency coverage wil…
Extragalactic HI Surveys
Riccardo Giovanelli, Martha P. Haynes
We review the results of HI line surveys of extragalactic sources in the local Universe. In the last two decades major efforts have been made in establishing on firm statistical gr…
When is Stacking Confusing?: The Impact of Confusion on Stacking in Deep HI Galaxy Surveys
Michael G. Jones, Martha P. Haynes, Riccardo Giovanelli +1
We present an analytic model to predict the HI mass contributed by confused sources to a stacked spectrum in a generic HI survey. Based on the ALFALFA correlation function, this mo…
CARMA CO Observations of Three Extremely Metal-Poor, Star-Forming Galaxies
Steven R. Warren, Edward Molter, John M. Cannon +11
We present sensitive CO (J = 1 - 0) emission line observations of three metal-poor dwarf irregular galaxies Leo P (Z ~ 3% Z_Solar), Sextans A (Z ~ 7.5% Z_Solar), and Sextans B (Z ~…
Environmental dependence of the HI mass function in the ALFALFA 70% catalogue
Michael G. Jones, Emmanouil Papastergis, Martha P. Haynes +1
We search for environmental dependence of the HI mass function in the ALFALFA 70% catalogue. The catalogue is split into quartiles of environment density based on the projected nei…
Evidence for the Thermal Sunyaev-Zel'dovich Effect Associated with Quasar Feedback
Devin Crichton, Megan B. Gralla, Kirsten Hall +20
Using a radio-quiet subsample of the Sloan Digital Sky Survey spectroscopic quasar catalogue, spanning redshifts 0.5-3.5, we derive the mean millimetre and far-infrared quasar spec…
The NANOGrav Nine-year Data Set: Astrometric Measurements of 37 Millisecond Pulsars
Allison M. Matthews, David J. Nice, Emmanuel Fonseca +18
Using the nine-year radio-pulsar timing data set from the North American Nanohertz Observatory for Gravitational Waves (NANOGrav), collected at Arecibo Observatory and the Green Ba…
Simultaneously modelling far-infrared dust emission and its relation to CO emission in star forming galaxies
Rahul Shetty, Julia Roman-Duval, Sacha Hony +6
We present a method to simultaneously model the dust far-infrared spectral energy distribution (SED) and the total infrared carbon monoxide (CO) integrated intensity $(S_{\rm I…
The JCMT Plane Survey: early results from the l = 30 degree field
T. J. T. Moore, R. Plume, M. A. Thompson +55
We present early results from the JCMT Plane Survey (JPS), which has surveyed the northern inner Galactic plane between longitudes l=7 and l=63 degrees in the 850-μm continuum with…
The Optical Luminosity Function of Void Galaxies in the SDSS and ALFALFA Surveys
Crystal M. Moorman, Michael S. Vogeley, Fiona Hoyle +3
We measure the r-band galaxy luminosity function (LF) across environments over the redshift range 0<<0.107 using the SDSS. We divide our sample into galaxies residing in large s…
The NANOGrav Nine-year Data Set: Limits on the Isotropic Stochastic Gravitational Wave Background
Zaven Arzoumanian, Adam Brazier, Sarah Burke-Spolaor +45
We compute upper limits on the nanohertz-frequency isotropic stochastic gravitational wave background (GWB) using the 9-year data release from the North American Nanohertz Observat…
Searching for Optical Counterparts to Ultra-compact High Velocity Clouds: Possible Detection of a Counterpart to AGC 198606
William Janesh, Katherine L. Rhode, John J. Salzer +6
We report on initial results from a campaign to obtain optical imaging of a sample of Ultra Compact High Velocity Clouds (UCHVCs) discovered by the ALFALFA neutral hydrogen (HI) su…
Numerical MHD Codes for Modeling Astrophysical Flows
A. V. Koldoba, G. V. Ustyugova, P. S. Lii +4
We describe a Godunov-type magnetohydrodynamic (MHD) code based on the Miyoshi and Kusano (2005) solver which can be used to solve various astrophysical hydrodynamic and MHD proble…
AGC 226067: A possible interacting low-mass system
E. A. K. Adams, J. M. Cannon, K. L. Rhode +8
We present Arecibo, GBT, VLA and WIYN/pODI observations of the ALFALFA source AGC 226067. Originally identified as an ultra-compact high velocity cloud and candidate Local Group ga…
From HI to Stars: HI Depletion in Starbursts and Star-Forming Galaxies in the ALFALFA H-alpha Survey
A. E. Jaskot, M. S. Oey, J. J. Salzer +3
HI in galaxies traces the fuel for future star formation and reveals the effects of feedback on neutral gas. Using a statistically uniform, HI-selected sample of 565 galaxies from…
The Effect of Structure and Star Formation on the Gas Content of Nearby Galaxies
Toby Brown, Barbara Catinella, Luca Cortese +3
We revisit the main HI-to-stellar mass ratio (gas fraction) scaling relations, taking advantage of the HI spectral stacking technique to understand the dependence of gas content on…