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20052026
most citedThe Zwicky Transient Facility: Data Processing, Products, and Archive

1.2k citations · 20.5k across the 286 of their papers we have counts for

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Showing 2016Show all

11 papers · 1 filter

astro-ph.HE2016★ 79 cited

Two New Calcium-Rich Gap Transients in Group and Cluster Environments

R. Lunnan, M. M. Kasliwal, Y. Cao +20

We present the Palomar Transient Factory discoveries and the photometric and spectroscopic observations of PTF11kmb and PTF12bho. We show that both transients have properties consi…

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.CO2016★ 246 cited

iPTF16geu: A multiply imaged, gravitationally lensed type Ia supernova

A. Goobar, R. Amanullah, S. R. Kulkarni +31

We report the discovery of a multiply-imaged gravitationally lensed Type Ia supernova, iPTF16geu (SN 2016geu), at redshift . This phenomenon could be identified because th…

astro-ph.HE2016★ 23 cited

Radio follow-up of gravitational wave triggers during Advanced LIGO O1

N. T. Palliyaguru, A. Corsi, M. M. Kasliwal +8

We present radio follow-up observations carried out with the Karl G. Jansky Very Large Array during the first observing run (O1) of the Advanced Laser Interferometer Gravitational-…

astro-ph.SR2016★ 24 cited

Rising from the Ashes: Mid-Infrared Re-Brightening of the Impostor SN 2010da in NGC 300

Ryan M. Lau, Mansi M. Kasliwal, Howard E. Bond +16

We present multi-epoch mid-infrared (IR) photometry and the optical discovery observations of the "impostor" supernova (SN) 2010da in NGC 300 using new and archival Spitzer Space T…

astro-ph.HE2016★ 59 cited

iPTF15dtg: a double-peaked Type Ic Supernova from a massive progenitor

F. Taddia, C. Fremling, J. Sollerman +9

Type Ic supernovae (SNe Ic) arise from the core-collapse of H (and He) poor stars, which could be either single WR stars or lower-mass stars stripped of their envelope by a compani…