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20022009
most citedFive-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation

5.7k citations

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12 papers · 1 filter

astro-ph.CO200913 cited

Probing the Intermediate-Age Globular Clusters in NGC 5128 from Ultraviolet Observations

Soo-Chang Rey, Sangmo T. Sohn, Michael A. Beasley +23

We explore the age distribution of the globular cluster (GC) system of the nearby elliptical galaxy NGC 5128 using ultraviolet (UV) photometry from Galaxy Evolution Explorer (GALEX…

astro-ph.CO200994 cited

Ultraviolet Spectroscopy of Supernovae: The First Two Years of Swift Observations

F. Bufano, S. Immler, M. Turatto +13

We present the entire sample of ultraviolet (UV) spectra of supernovae (SNe) obtained with the Ultraviolet/Optical Telescope (UVOT) on board the Swift satellite during the first 2…

astro-ph.CO200929 cited

Structures of Local Galaxies Compared to High Redshift Star-forming Galaxies

Sara M. Petty, Duilia F. de Mello, John S. Gallagher +4

The rest-frame far-ultraviolet (FUV) morphologies of 8 nearby interacting and starburst galaxies (Arp 269, M 82, Mrk 8, NGC 520, NGC 1068, NGC 3079, NGC 3310, NGC 7673) are compare…

astro-ph.CO200957 cited

GALEX-SDSS Catalogs for Statistical Studies

T. Budavari, S. Heinis, A. S. Szalay +23

We present a detailed study of the Galaxy Evolution Explorer's photometric catalogs with special focus on the statistical properties of the All-sky and Medium Imaging Surveys. We i…

astro-ph.CO200929 cited

The Radio Luminosity Function and Galaxy Evolution in the Coma Cluster

Neal A. Miller, Ann E. Hornschemeier, Bahram Mobasher +4

We investigate the radio luminosity function (RLF) and radio source population for two fields within the Coma cluster of galaxies. Our VLA data reach down to log(L) = 20.23 W/Hz fo…

astro-ph.CO200925 cited

A Deep VLA Radio Continuum Study of the Core and Outskirts of the Coma Cluster

Neal A. Miller, Ann E. Hornschemeier, Bahram Mobasher

We present deep 1.4GHz Very Large Array (VLA) radio continuum observations of two ~half square degree fields in the Coma cluster of galaxies. The two fields, "Coma 1" and "Coma 3,"…