activity
20152026
most citedThe Astropy Project: Building an inclusive, open-science project and status of the v2.0 core package

7.7k citations · 22k across the 207 of their papers we have counts for

collaborators
Showing 2017Show all

15 papers · 1 filter

astro-ph.HE2017★ 126 cited

The early detection and follow-up of the highly obscured Type II supernova 2016ija/DLT16am

L. Tartaglia, D. J. Sand, S. Valenti +45

We present our analysis of the Type II supernova DLT16am (SN~2016ija). The object was discovered during the ongoing (DLT40) one day cadence supernova search a…

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★ 152 cited

The Rapid Reddening and Featureless Optical Spectra of the optical counterpart of GW170817, AT 2017gfo, During the First Four Days

Curtis McCully, Daichi Hiramatsu, D. Andrew Howell +17

We present the spectroscopic evolution of AT 2017gfo, the optical counterpart of the first binary neutron star (BNS) merger detected by LIGO and Virgo, GW170817. While models have…

astro-ph.HE2017★ 622 cited

Optical emission from a kilonova following a gravitational-wave-detected neutron-star merger

Iair Arcavi, Griffin Hosseinzadeh, D. Andrew Howell +8

The merger of two neutron stars has been predicted to produce an optical-infrared transient (lasting a few days) known as a 'kilonova', powered by the radioactive decay of neutron-…

astro-ph.HE2017★ 109 cited

Optical Follow-up of Gravitational-wave Events with Las Cumbres Observatory

Iair Arcavi, Curtis McCully, Griffin Hosseinzadeh +11

We present an implementation of the Gehrels et al. (2016) galaxy-targeted strategy for gravitational-wave (GW) follow-up using the Las Cumbres Observatory global network of telesco…

astro-ph.HE2017★ 54 cited

SN 2016coi/ASASSN-16fp: An example of residual helium in a type Ic supernova?

S. J. Prentice, C. Ashall, P. A. Mazzali +35

The optical observations of Ic-4 supernova (SN) 2016coi/ASASSN-16fp, from to days after explosion, are presented along with analysis of its physical properties.…

astro-ph.HE2017★ 72 cited

Nebular-Phase Spectra of Nearby Type Ia Supernovae

Melissa L. Graham, Sahana Kumar, Griffin Hosseinzadeh +8

We present late-time spectra of eight Type Ia supernovae (SNe Ia) obtained at days after peak brightness using the Gemini South and Keck telescopes. All of the SNe Ia in our…

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.HE2017★ 81 cited

Gaia17biu/SN 2017egm in NGC 3191: The closest hydrogen-poor superluminous supernova to date is in a "normal", massive, metal-rich spiral galaxy

Subhash Bose, Subo Dong, A. Pastorello +55

Hydrogen-poor superluminous supernovae (SLSNe-I) have been predominantly found in low-metallicity, star-forming dwarf galaxies. Here we identify Gaia17biu/SN 2017egm as an SLSN-I o…

astro-ph.HE2017★ 16 cited

LSQ14efd: observations of the cooling of a shock break-out event in a type Ic Supernova

C. Barbarino, M. T. Botticella, M. Dall'Ora +29

We present the photometric and spectroscopic evolution of the type Ic supernova LSQ14efd, discovered by the La Silla QUEST survey and followed by PESSTO. LSQ14efd was discovered fe…

astro-ph.HE2017★ 140 cited

Early Blue Excess from the Type Ia Supernova 2017cbv and Implications for Its Progenitor

Griffin Hosseinzadeh, David J. Sand, Stefano Valenti +11

We present very early, high-cadence photometric observations of the nearby Type Ia SN 2017cbv. The light curve is unique in that it has a blue bump during the first five days of ob…

astro-ph.HE2017★ 30 cited

Clues to the Nature of SN 2009ip II: The Continuing Photometric and Spectroscopic Evolution to 1000 Days

Melissa L. Graham, Andrew Bigley, Jon C. Mauerhan +6

The 2012 brightening of SN 2009ip was dominated by emission from the interaction of ejecta with the surrounding circumstellar material (CSM) produced by episodic mass loss from the…

astro-ph.HE2017★ 114 cited

Hydrogen-poor Superluminous Supernovae With Late-time H-alpha Emission: Three Events From the Intermediate Palomar Transient Factory

Lin Yan, R. Lunnan, D. Perley +20

We present observations of two new hydrogen-poor superluminous supernovae (SLSN-I), iPTF15esb and iPTF16bad, showing late-time H-alpha emission with line luminosities of (1-3)e+41…

astro-ph.HE2017★ 154 cited

iPTF16fnl: a faint and fast tidal disruption event in an E+A galaxy

N. Blagorodnova, S. Gezari, T. Hung +30

We present ground-based and \textit{Swift} observations of iPTF16fnl, a likely tidal disruption event (TDE) discovered by the intermediate Palomar Transient Factory (iPTF) survey a…

astro-ph.HE2017★ 51 cited

Multiwavelength follow-up of a rare IceCube neutrino multiplet

M. G. Aartsen, M. Ackermann, J. Adams +501

On February 17 2016, the IceCube real-time neutrino search identified, for the first time, three muon neutrino candidates arriving within 100 s of one another, consistent with comi…