activity
20082023
most citedLSST: from Science Drivers to Reference Design and Anticipated Data Products

3.5k citations · 11.1k across the 101 of their papers we have counts for

collaborators
Showing 2015Show all

12 papers · 1 filter

astro-ph.GA2015★ 53 cited

SN Refsdal: Classification as a Luminous and Blue SN 1987A-like Type II Supernova

P. L. Kelly, G. Brammer, J. Selsing +19

We have acquired Hubble Space Telescope (HST) and Very Large Telescope near-infrared spectra and images of supernova (SN) Refsdal after its discovery as an Einstein cross in Fall 2…

astro-ph.SR2015★ 34 cited

The Persistent Eruption of UGC~2773-OT: Finally, a Decade-Long Extragalactic Eta Carinae Analog

Nathan Smith, Jennifer E. Andrews, Jon C. Mauerhan +4

While SN impostors resemble the Great Eruption of eta Car in the sense that their spectra show narrow H lines and they have typical peak absolute magnitudes of -13 to -14 mag, most…

astro-ph.SR2015★ 64 cited

Extensive Spectroscopy and Photometry of the Type IIP Supernova 2013ej

G. Dhungana, R. Kehoe, J. Vinko +32

We present extensive optical (, , and open CCD) and near-infrared () photometry for the very nearby Type IIP SN ~2013ej extending from +1 to +461 days after…

astro-ph.HE2015★ 93 cited

Measuring nickel masses in Type Ia supernovae using cobalt emission in nebular phase spectra

Michael J. Childress, D. John Hillier, Ivo Seitenzahl +34

The light curves of Type Ia supernovae (SNe Ia) are powered by the radioactive decay of Ni to Co at early times, and the decay of Co to Fe from ~60 days…

astro-ph.SR2015★ 157 cited

SN~2012cg: Evidence for Interaction Between a Normal Type Ia Supernova and a Non-Degenerate Binary Companion

G. H. Marion, Peter J. Brown, Jozsef Vinkó +26

We report evidence for excess blue light from the Type Ia supernova SN 2012cg at fifteen and sixteen days before maximum B-band brightness. The emission is consistent with predicti…

astro-ph.HE2015★ 82 cited

The Double-Peaked SN2013ge: a Type Ib/c SN with an Asymmetric Mass Ejection or an Extended Progenitor Envelope

M. R. Drout, D. Milisavljevic, J. Parrent +17

We present extensive observations of the Type Ib/c SN2013ge from -13 to +457 days, including spectra and Swift UV-optical photometry beginning 2-4 days post-explosion. This data se…