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20042026
most citedAn ultraviolet-optical flare from the tidal disruption of a helium-rich stellar core

469 citations · 9.1k across the 215 of their papers we have counts for

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Showing 2011Show all

9 papers · 1 filter

astro-ph.GA2011★ 347 cited

Toward a Unification of Star Formation Rate Determinations in the Milky Way and Other Galaxies

Laura Chomiuk, Matthew S. Povich

The star formation rate (SFR) of the Milky Way remains poorly known, with often-quoted values ranging from 1 to 10 solar masses per year. This situation persists despite the potent…

astro-ph.HE2011★ 47 cited

SN 2010ay is a Luminous and Broad-lined Type Ic Supernova within a Low-metallicity Host Galaxy

Nathan E. Sanders, A. M. Soderberg, S. Valenti +38

We report on our serendipitous pre-discovery detection and detailed follow-up of the broad-lined Type Ic supernova (SN) 2010ay at z = 0.067 imaged by the Pan-STARRS1 3pi survey jus…

astro-ph.HE2011★ 23 cited

EVLA Nova Project Observations of the Classical Nova V1723 Aquilae

Miriam I. Krauss, Laura Chomiuk, Michael Rupen +8

We present radio light curves and spectra of the classical nova V1723 Aql obtained with the Expanded Very Large Array (EVLA). This is the first paper to showcase results from the E…

astro-ph.HE2011★ 200 cited

Pan-STARRS1 Discovery of Two Ultra-Luminous Supernovae at z ~ 0.9

L. Chomiuk, R. Chornock, A. M. Soderberg +29

We present the discovery of two ultra-luminous supernovae (SNe) at z ~ 0.9 with the Pan-STARRS1 Medium-Deep Survey. These SNe, PS1-10ky and PS1-10awh, are amongst the most luminous…

astro-ph.HE2011★ 136 cited

Panchromatic Observations of SN 2011dh Point to a Compact Progenitor Star

Alicia M. Soderberg, R. Margutti, B. A. Zauderer +32

We report the discovery and detailed monitoring of X-ray emission associated with the Type IIb SN 2011dh using data from the Swift and Chandra satellites, placing it among the best…

astro-ph.CO2011★ 19 cited

The X-ray properties of typical high-redshift radio-loud quasars

C. Saez, W. N. Brandt, O. Shemmer +5

We report spectral, imaging, and variability results from four new XMM-Newton observations and two new Chandra observations of high-redshift (z > 4) radio-loud quasars (RLQs). Our…