activity
20152021
most citedPTF12os and iPTF13bvn. Two stripped-envelope supernovae from low-mass progenitors in NGC 5806

193 citations · 1.2k across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.SR2021★ 29 cited

Photometric and spectroscopic evolution of the interacting transient AT 2016jbu (Gaia16cfr)

S. J. Brennan, M. Fraser, J. Johansson +68

We present the results from a high cadence, multi-wavelength observation campaign of AT 2016jbu (aka Gaia16cfr), an interacting transient. This dataset complements the current lite…

astro-ph.SR2020★ 4 cited

Type Ic supernovae from the (intermediate) Palomar Transient Factory

C. Barbarino, J. Sollerman, F. Taddia +8

Type Ic supernovae represent the explosions of the most stripped massive stars, but their progenitors and explosion mechanisms remain unclear. Larger samples of observed supernovae…

astro-ph.GA2020★ 131 cited

The Palomar Transient Factory Core-Collapse Supernova Host-Galaxy Sample. I. Host-Galaxy Distribution Functions and Environment-Dependence of CCSNe

Steve Schulze, Ofer Yaron, Jesper Sollerman +51

Several thousand core-collapse supernovae (CCSNe) of different flavors have been discovered so far. However, identifying their progenitors has remained an outstanding open question…

astro-ph.SR2020★ 39 cited

The Carnegie Supernova Project II. The shock wave revealed through the fog: The strongly interacting Type IIn SN 2013L

F. Taddia, M. D. Stritzinger, C. Fransson +21

We present ultra-violet to mid-infrared observations of the long-lasting Type IIn supernova (SN) 2013L obtained by the Carnegie Supernova Project II (CSP-II). The spectra of SN 201…

astro-ph.HE2019★ 53 cited

The long-lived Type IIn SN 2015da: Infrared echoes and strong interaction within an extended massive shell

L. Tartaglia, A. Pastorello, J. Sollerman +41

In this paper we report the results of the first four years of spectroscopic and photometric monitoring of the Type IIn supernova SN 2015da (also known as PSN J13522411+39412…

astro-ph.HE2019★ 10 cited

The optical and near-infrared spectrum of the Crab pulsar with X-shooter

J. Sollerman, J. Selsing, P. M. Vreeswijk +2

Pulsars are well studied all over the electromagnetic spectrum, and the Crab pulsar may be the most studied object in the sky. Nevertheless, a high-quality optical to near-infrared…

astro-ph.SR2019★ 88 cited

Type IIn supernova light-curve properties measured from an untargeted survey sample

A. Nyholm, J. Sollerman, L. Tartaglia +19

We present a sample of supernovae Type IIn (SNe IIn) from the untargeted, magnitude-limited surveys of the Palomar Transient Factory (PTF) and its successor, the intermediate PTF (…

astro-ph.HE2018★ 23 cited

R-band light-curve properties of Type Ia supernovae from the (intermediate) Palomar Transient Factory

S. Papadogiannakis, A. Goobar, R. Amanullah +15

We present the best 265 sampled R-band light curves of spectroscopically identified Type Ia supernovae (SNe) from the Palomar Transient Factory (PTF; 2009-2012) survey and the inte…

astro-ph.HE2018★ 117 cited

Analysis of broad-lined Type Ic supernovae from the (intermediate) Palomar Transient Factory

F. Taddia, J. Sollerman, C. Fremling +18

We study 34 Type Ic supernovae that have broad spectral features (SNe Ic-BL). We obtained our photometric data with the Palomar Transient Factory (PTF) and its continuation, the in…

astro-ph.HE2018★ 2 cited

A UV Resonance Line Echo from a Shell Around a Hydrogen-Poor Superluminous Supernova

R. Lunnan, C. Fransson, P. M. Vreeswijk +21

Hydrogen-poor superluminous supernovae (SLSN-I) are a class of rare and energetic explosions discovered in untargeted transient surveys in the past decade. The progenitor stars and…

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.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.GA2017★ 19 cited

AGN luminosity and stellar age -- two missing ingredients for AGN unification as seen with iPTF supernovae

Beatriz Villarroel, Anders Nyholm, Torgny Karlsson +4

Active Galactic Nuclei (AGN) are extremely powerful cosmic objects, driven by accretion of hot gas upon super-massive black holes. The zoo of AGN classes are divided into two major…

astro-ph.HE2016★ 29 cited

SN 2012aa - a transient between Type Ibc core-collapse and superluminous supernovae

R. Roy, J. Sollerman, J. M. Silverman +21

Context: Research on supernovae (SNe) over the past decade has confirmed that there is a distinct class of events which are much more luminous (by mag) than canonical core-…

astro-ph.HE2016★ 193 cited

PTF12os and iPTF13bvn. Two stripped-envelope supernovae from low-mass progenitors in NGC 5806

C. Fremling, J. Sollerman, F. Taddia +19

We investigate two stripped-envelope supernovae (SNe) discovered in the nearby galaxy NGC 5806 by the (i)PTF. These SNe, designated PTF12os/SN 2012P and iPTF13bvn, exploded at a si…

astro-ph.GA2015★ 70 cited

Extragalactic SETI: The Tully-Fisher relation as a probe of Dysonian astroengineering in disk galaxies

E. Zackrisson, P. Calissendorff, S. Asadi +1

If advanced extraterrestrial civilizations choose to construct vast numbers of Dyson spheres to harvest radiation energy, this could affect the characteristics of their host galaxi…

astro-ph.HE2015★ 83 cited

Metallicity at the explosion sites of interacting transients

F. Taddia, J. Sollerman, C. Fremling +8

Context. Some circumstellar-interacting (CSI) supernovae (SNe) are produced by the explosions of massive stars that have lost mass shortly before the SN explosion. There is evidenc…

astro-ph.HE2015★ 76 cited

No trace of a single-degenerate companion in late spectra of SNe 2011fe and 2014J

P. Lundqvist, A. Nyholm, F. Taddia +9

Left-over, ablated material from a possible non-degenerate companion can reveal itself after about one year in spectra of Type Ia SNe (SNe Ia). We have searched for such material i…