activity
20142026
most citedThe Zwicky Transient Facility: Science Objectives

850 citations · 6.8k across the 104 of their papers we have counts for

collaborators
Showing 2017Show all

9 papers · 1 filter

astro-ph.HE2017★ 148 cited

Energetic eruptions leading to a peculiar hydrogen-rich explosion of a massive star

Iair Arcavi, D. Andrew Howell, Daniel Kasen +50

Every supernova hitherto observed has been considered to be the terminal explosion of a star. Moreover, all supernovae with absorption lines in their spectra show those lines decre…

astro-ph.HE2017★ 822 cited

Illuminating Gravitational Waves: A Concordant Picture of Photons from a Neutron Star Merger

M. M. Kasliwal, E. Nakar, L. P. Singer +78

Merging neutron stars offer an exquisite laboratory for simultaneously studying strong-field gravity and matter in extreme environments. We establish the physical association of an…

astro-ph.IM2017★ 242 cited

The SED Machine: a robotic spectrograph for fast transient classification

Nadejda Blagorodnova, James D. Neill, Richard Walters +13

Current time domain facilities are finding several hundreds of transient astronomical events a year. The discovery rate is expected to increase in the future as soon as new surveys…

astro-ph.HE2017★ 181 cited

The first direct double neutron star merger detection: implications for cosmic nucleosynthesis

S. Rosswog, J. Sollerman, U. Feindt +4

The astrophysical r-process site where about half of the elements heavier than iron are produced has been a puzzle for several decades. Here we discuss the role of neutron star mer…

astro-ph.CO2017★ 38 cited

PTF11mnb: the first analog of supernova 2005bf

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

We study PTF11mnb, a He-poor supernova (SN) whose pre-peak light curves (LCs) resemble those of SN 2005bf, a peculiar double-peaked stripped-envelope (SE) SN. LCs, colors and spect…

astro-ph.GA2017★ 12 cited

Probing gas and dust in the tidal tail of NGC 5221 with the type Ia supernova iPTF16abc

R. Ferretti, R. Amanullah, A. Goobar +8

Context. Type Ia supernovae (SNe Ia) can be used to address numerous questions in astrophysics and cosmology. Due to their well known spectral and photometric properties, SNe Ia ar…

astro-ph.HE2017★ 63 cited

Early Observations of the Type Ia Supernova iPTF 16abc: A Case of Interaction with Nearby, Unbound Material and/or Strong Ejecta Mixing

A. A. Miller, Y. Cao, A. L. Piro +19

Early observations of Type Ia supernovae (SNe Ia) provide a unique probe of their progenitor systems and explosion physics. Here we report the intermediate Palomar Transient Factor…

astro-ph.SR2017★ 63 cited

The bumpy light curve of supernova iPTF13z

A. Nyholm, J. Sollerman, F. Taddia +10

A Type IIn supernova (SN) is dominated by the interaction of SN ejecta with the circumstellar medium (CSM). Some SNe IIn (e.g., SN 2006jd) have episodes of re-brightening ("bumps")…

astro-ph.HE2017★ 165 cited

Revisiting optical tidal disruption events with iPTF16axa

T. Hung, S. Gezari, N. Blagorodnova +12

We report the discovery by the intermediate Palomar Transient Factory (iPTF) of a candidate tidal disruption event (TDE) iPTF16axa at , and present its broadband photometr…