activity
20092024
most citedNew Parallaxes of Galactic Cepheids from Spatially Scanning the Hubble Space Telescope: Implications for the Hubble Constant

538 citations · 7.2k across the 77 of their papers we have counts for

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18 papers · 1 filter

astro-ph.HE2022★ 15 cited

The Lick Observatory Supernova Search follow-up program: photometry data release of 70 stripped-envelope supernovae

WeiKang Zheng, Benjamin E. Stahl, Thomas de Jaeger +85

We present BVRI and unfiltered Clear light curves of 70 stripped-envelope supernovae (SESNe), observed between 2003 and 2020, from the Lick Observatory Supernova Search (LOSS) foll…

astro-ph.HE2019★ 75 cited

The Berkeley sample of Type II supernovae: BVRI light curves and spectroscopy of 55 SNe II

T. de Jaeger, W. Zheng, B. E. Stahl +58

In this work, BV RI light curves of 55 Type II supernovae (SNe II) from the Lick Observatory Supernova Search program obtained with the Katzman Automatic Imaging Telescope and the…

astro-ph.HE2018★ 40 cited

Oxygen and helium in stripped-envelope supernovae

C. Fremling, J. Sollerman, M. M. Kasliwal +23

We present an analysis of 507 spectra of 173 stripped-envelope (SE) supernovae (SNe) discovered by the untargeted Palomar Transient Factory (PTF) and intermediate PTF (iPTF) survey…

astro-ph.HE2018★ 54 cited

SN2013fs and SN2013fr: Exploring the circumstellar-material diversity in Type II supernovae

Christopher Bullivant, Nathan Smith, G. Grant Williams +12

We present photometry and spectroscopy of SN2013fs and SN2013fr in the first 100 days post-explosion. Both objects showed transient, relatively narrow H emission lines character…

astro-ph.HE2016★ 129 cited

Type Ibn Supernovae Show Photometric Homogeneity and Spectral Diversity at Maximum Light

Griffin Hosseinzadeh, Iair Arcavi, Stefano Valenti +34

Type Ibn supernovae (SNe) are a small yet intriguing class of explosions whose spectra are characterized by low-velocity helium emission lines with little to no evidence for hydrog…

astro-ph.HE2015★ 94 cited

Type II supernova energetics and comparison of light curves to shock-cooling models

Adam Rubin, Avishay Gal-Yam, Annalisa De Cia +37

During the first few days after explosion, Type II supernovae (SNe) are dominated by relatively simple physics. Theoretical predictions regarding early-time SN light curves in the…

astro-ph.HE2015★ 58 cited

Optical and near-infrared observations of SN 2013dx associated with GRB 130702A

V. L. Toy, S. B. Cenko, J. M. Silverman +33

We present optical and near-infrared light curves and optical spectra of SN 2013dx, associated with the nearby (redshift 0.145) gamma-ray burst GRB 130702A. The prompt isotropic ga…

astro-ph.HE2015★ 100 cited

Nebular spectra and abundance tomography of the type Ia supernova SN 2011fe: a normal SN Ia with a stable Fe core

P. A. Mazzali, M. Sullivan, A. V. Filippenko +10

A series of optical and one near-infrared nebular spectra covering the first year of the Type Ia supernova SN 2011fe are presented and modelled. The density profile that proved bes…

astro-ph.HE2015★ 62 cited

500 Days of SN 2013dy: spectra and photometry from the ultraviolet to the infrared

Y. -C. Pan, R. J. Foley, M. Kromer +23

SN 2013dy is a Type Ia supernova for which we have compiled an extraordinary dataset spanning from 0.1 to ~ 500 days after explosion. We present 10 epochs of ultraviolet (UV) throu…

astro-ph.HE2015★ 169 cited

PTF11iqb: Cool supergiant mass loss that bridges the gap between Type IIn and normal supernovae

Nathan Smith, Jon C. Mauerhan, S. Bradley Cenko +16

PTF11iqb was initially classified as a TypeIIn event caught very early after explosion. It showed narrow Wolf-Rayet (WR) spectral features on day 2, but the narrow emission weakene…

astro-ph.HE2014★ 42 cited

On the Progenitor System of the Type Iax Supernova 2014dt in M61

Ryan J. Foley, Schuyler D. Van Dyk, Saurabh W. Jha +5

We present pre-explosion and post-explosion Hubble Space Telescope images of the Type Iax supernova (SN Iax) 2014dt in M61. After astrometrically aligning these images, we do not d…

astro-ph.HE2014★ 113 cited

The hydrogen-poor superluminous supernova iPTF13ajg and its host galaxy in absorption and emission

Paul M. Vreeswijk, Sandra Savaglio, Avishay Gal-Yam +24

We present imaging and spectroscopy of a hydrogen-poor superluminous supernova (SLSN) discovered by the intermediate Palomar Transient Factory: iPTF13ajg. At a redshift of z=0.7403…

astro-ph.HE2014★ 46 cited

Twins for life? A comparative analysis of the Type Ia supernovae 2011fe and 2011by

Melissa L. Graham, Ryan J. Foley, Weikang Zheng +6

The nearby Type Ia supernovae (SNe Ia) 2011fe and 2011by had nearly identical photospheric phase optical spectra, light-curve widths, and photometric colours, but at peak brightnes…

astro-ph.HE2014★ 103 cited

Exploring the spectral diversity of low-redshift Type Ia supernovae using the Palomar Transient Factory

Kate Maguire, Mark Sullivan, Yen-Chen Pan +15

We present an investigation of the optical spectra of 264 low-redshift (z < 0.2) Type Ia supernovae (SNe Ia) discovered by the Palomar Transient Factory, an untargeted transient su…

astro-ph.HE2014★ 93 cited

Estimating the First-Light Time of the Type Ia Supernova 2014J in M82

WeiKang Zheng, Isaac Shivvers, Alexei V. Filippenko +6

The Type Ia supernova (SN Ia) 2014J in M82 (d~3.5 Mpc) was serendipitously discovered by S. Fossey's group on 2014 Jan. 21 UT and has been confirmed to be the nearest known SN Ia s…

astro-ph.HE2014★ 5 cited

Two active states of the narrow-line gamma-ray-loud AGN GB 1310+487

K. V. Sokolovsky, F. K. Schinzel, Y. T. Tanaka +49

Previously unremarkable, the extragalactic radio source GB 1310+487 showed a gamma-ray flare on 2009 November 18, reaching a daily flux of ~10^-6 photons/cm^2/s at energies E>100 M…

astro-ph.HE2013★ 223 cited

The Afterglow of GRB 130427A from 1 to 10^16 GHz

D. A. Perley, S. B. Cenko, A. Corsi +31

We present multiwavelength observations of the afterglow of GRB 130427A, the brightest (in total fluence) gamma-ray burst of the past 29 years. Optical spectroscopy from Gemini-Nor…

astro-ph.HE2013★ 38 cited

Nebular spectroscopy of the nearby type IIb supernova 2011dh

Isaac Shivvers, Paolo Mazzali, Jeffrey M. Silverman +6

We present nebular spectra of the nearby Type IIb supernova (SN) 2011dh taken between 201 and 678 days after core collapse. At these late times, SN 2011dh exhibits strong emission…