activity
20122026
most citedThe Baryon Oscillation Spectroscopic Survey of SDSS-III

2.1k citations · 3.1k across the 15 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

6 papers · 1 filter

astro-ph.SR2016★ 80 cited

Far-Ultraviolet to Near-Infrared Spectroscopy of A Nearby Hydrogen Poor Superluminous Supernova Gaia16apd

Lin Yan, R. Quimby, A. Gal-Yam +8

We report the first maximum-light far-Ultraviolet to near-infrared spectra (1000A - 1.62um, rest) of a H-poor superluminous supernova, Gaia16apd. At z=0.1018, it is one of the clos…

astro-ph.SR2016★ 25 cited

Optical and Ultraviolet Observations of the Very Young Type IIP SN 2014cx in NGC 337

Fang Huang, Xiaofeng Wang, Luca Zampieri +15

Extensive photometric and spectroscopic observations are presented for SN 2014cx, a type IIP supernova (SN) exploding in the nearby galaxy NGC 337. The observations are performed i…

astro-ph.SR2016★ 84 cited

Dead or Alive? Long-term evolution of SN 2015bh (SNhunt275)

N. Elias-Rosa, A. Pastorello, S. Benetti +37

Supernova (SN) 2015bh (or SNhunt275) was discovered in NGC 2770 on 2015 February with an absolute magnitude of Mr ~ -13.4 mag, and was initially classified as a SN impostor. Here w…

astro-ph.SR2016★ 366 cited

The diversity of Type II supernova versus the similarity in their progenitors

S. Valenti, D. A. Howell, M. D. Stritzinger +19

High-quality collections of Type II supernova (SN) light curves are scarce because they evolve for hundreds of days, making follow-up observations time consuming and often extendin…

astro-ph.SR2016★ 100 cited

DES14X3taz: A Type I Superluminous Supernova Showing a Luminous, Rapidly Cooling Initial Pre-Peak Bump

M. Smith, M. Sullivan, C. B. D'Andrea +81

We present DES14X3taz, a new hydrogen-poor super luminous supernova (SLSN-I) discovered by the Dark Energy Survey (DES) supernova program, with additional photometric data provided…

astro-ph.SR2015★ 84 cited

Massive stars exploding in a He-rich circumstellar medium. IV. Transitional Type Ibn Supernovae

A. Pastorello, S. Benetti, P. J. Brown +30

We present ultraviolet, optical and near-infrared data of the Type Ibn supernovae (SNe) 2010al and 2011hw. SN 2010al reaches an absolute magnitude at peak of M(R) = -18.86 +- 0.21.…