activity
20132026
most citedA kilonova as the electromagnetic counterpart to a gravitational-wave source

888 citations · 6.4k across the 167 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

23 papers · 1 filter

astro-ph.SR2025

SN 2021ukt: A Transitional Supernova with a Short Plateau and Persistent Interaction

Neil R. Pichay, Sergiy S. Vasylyev, Audrey M. Liddle +21

We present spectroscopic and photometric observations of supernova (SN) 2021ukt, a peculiar short-plateau object that was originally identified as a Type IIn SN and later underwent…

astro-ph.SR2025★ 2 cited

SN 2016iog: A fast declining Type II-L supernova with an ultra-faint tail, persistently interacting with circumstellar material

Z. -H. Peng, S. Benetti, Y. -Z. Cai +26

We present optical photometric and spectroscopic observations of the rapidly declining Type IIL supernova (SN) 2016iog. SN 2016iog reached its peak 14 days after explosion,…

astro-ph.SR2025★ 6 cited

SN 2022xlp: The second-known well-observed, intermediate-luminosity Iax supernova

D. Bánhidi, B. Barna, T. Szalai +17

We present a detailed analysis of type Iax supernova SN 2022xlp. With a V-band absolute magnitude light curve peaking at mag, this object is regarded…

astro-ph.SR2025★ 6 cited

A long-lasting eruption heralds SN 2023ldh, a clone of SN 2009ip

A. Pastorello, A. Reguitti, L. Tartaglia +46

We discuss the results of the spectroscopic and photometric monitoring of the type IIn supernova (SN) 2023ldh. Survey archive data show that the SN progenitor experienced some erra…

astro-ph.SR2024★ 2 cited

The story of SN 2021aatd -- a peculiar 1987A-like supernova with an early-phase luminosity excess

T. Szalai, R. Könyves-Tóth, A. P. Nagy +20

There is a growing number of peculiar events that cannot be assigned to any of the main supernova (SN) classes. SN 1987A and a handful of similar objects, thought to be explosive o…

astro-ph.SR2022★ 26 cited

Observations of the luminous red nova AT 2021biy in the nearby galaxy NGC 4631

Y. -Z. Cai, A. Pastorello, M. Fraser +73

We present an observational study of the luminous red nova (LRN) AT\,2021biy in the nearby galaxy NGC\,4631. The field of the object was routinely imaged during the pre-eruptive st…

astro-ph.SR2021★ 67 cited

The Early Phases of Supernova 2020pni: Shock-Ionization of the Nitrogen-Enriched Circumstellar Material

G. Terreran, W. V. Jacobson-Galan, J. H. Groh +20

We present multiwavelength observations of the Type II SN 2020pni. Classified at days after explosion, the object showed narrow (FWHM $<250\,\textrm{km}\,\textrm{s}^{-1}…

astro-ph.SR2019★ 18 cited

Observations of Type Ia Supernova 2014J for Nearly 900 Days and Constraints on Its Progenitor System

Wenxiong Li, Xiaofeng Wang, Maokai Hu +18

We present extensive ground-based and () photometry of the highly reddened, very nearby type Ia supernova (SN Ia) 2014J in M82, covering the phases fr…

astro-ph.SR2019★ 129 cited

Luminous Red Novae: Stellar Mergers or Giant Eruptions?

A. Pastorello, E. Mason, S. Taubenberger +36

We present extensive datasets for a class of intermediate-luminosity optical transients known as "luminous red novae" (LRNe). They show double-peaked light curves, with an initial…

astro-ph.SR2018★ 5 cited

SN 2014J in M82: New Insights On the Spectral Diversity of Type Ia Supernovae

Kaicheng Zhang, Xiaofeng Wang, JuJia Zhang +25

We present extensive spectroscopic observations for one of the closest type Ia supernovae (SNe Ia), SN 2014J discovered in M82, ranging from 10.4 days before to 473.2 days after B-…

astro-ph.SR2018★ 15 cited

ASASSN-15no: The Supernova that plays hide-and-seek

S. Benetti, L. Zampieri, A. Pastorello +11

We report the results of our follow-up campaign of the peculiar supernova ASASSN-15no, based on optical data covering ~300 days of its evolution. Initially the spectra show a pure…

astro-ph.SR2018★ 12 cited

SNhunt151: an explosive event inside a dense cocoon

N. Elias-Rosa, S. Benetti, E. Cappellaro +20

SNhunt151 was initially classified as a supernova (SN) impostor (nonterminal outburst of a massive star). It exhibited a slow increase in luminosity, lasting about 450 d, followed…

astro-ph.SR2017

Hydrogen-rich supernovae beyond the neutrino-driven core-collapse paradigm

G. Terreran, M. L. Pumo, T. -W. Chen +41

We present our study of OGLE-2014-SN-073, one of the brightest Type II SN ever discovered, with an unusually broad lightcurve combined with high ejecta velocities. From our hydrody…

astro-ph.SR2017★ 78 cited

Supernovae 2016bdu and 2005gl, and their link with SN 2009ip-like transients: another piece of the puzzle

A. Pastorello, C. S. Kochanek, M. Fraser +52

Supernova (SN) 2016bdu is an unusual transient resembling SN 2009ip. SN 2009ip-like events are characterized by a long-lasting phase of erratic variability which ends with two lumi…

astro-ph.SR2016★ 117 cited

Common Envelope ejection for a Luminous Red Nova in M101

N. Blagorodnova, R. Kotak, J. Polshaw +30

We present the results of optical, near-infrared, and mid-infrared observations of M101 OT2015-1 (PSN J14021678+5426205), a luminous red transient in the Pinwheel galaxy (M101), sp…

astro-ph.SR2016★ 84 cited

Dead or Alive? Long-term evolution of SN 2015bh (SNhunt275)

N. Elias-Rosa, A. Pastorello, S. Benetti +37

Supernova (SN) 2015bh (or SNhunt275) was discovered in NGC 2770 on 2015 February with an absolute magnitude of Mr ~ -13.4 mag, and was initially classified as a SN impostor. Here w…

astro-ph.SR2016★ 80 cited

450 Days of Type II SN 2013ej in Optical and Near-Infrared

Fang Yuan, A. Jerkstrand, S. Valenti +31

We present optical and near-infrared photometric and spectroscopic observations of SN 2013ej, in galaxy M74, from 1 to 450 days after the explosion. SN 2013ej is a hydrogen-rich su…

astro-ph.SR2016★ 93 cited

The multi-faceted Type II-L supernova 2014G from pre-maximum to nebular phase

G. Terreran, A. Jerkstrand, S. Benetti +18

We present multi-band ultraviolet, optical, and near-infrared photometry, along with visual-wavelength spectroscopy, of supernova (SN) 2014G in the nearby galaxy NGC 3448 (25 Mpc).…

astro-ph.SR2016★ 366 cited

The diversity of Type II supernova versus the similarity in their progenitors

S. Valenti, D. A. Howell, M. D. Stritzinger +19

High-quality collections of Type II supernova (SN) light curves are scarce because they evolve for hundreds of days, making follow-up observations time consuming and often extendin…

astro-ph.SR2015★ 24 cited

Massive stars exploding in a He-rich circumstellar medium - VIII. PSN J07285387+3349106, a highly reddened supernova Ibn

A. Pastorello, L. Tartaglia, N. Elias-Rosa +16

We present spectroscopic and photometric observations for the Type Ibn supernova (SN) dubbed PSN J07285387+3349106. Using data provided by amateur astronomers, we monitored the pho…

astro-ph.SR2015★ 31 cited

Massive stars exploding in a He-rich circumstellar medium - VII. The metamorphosis of ASASSN-15ed from a narrow line Type Ibn to a normal Type Ib Supernova

A. Pastorello, J. L. Prieto, N. Elias-Rosa +39

We present the results of the spectroscopic and photometric monitoring campaign of ASASSN-15ed. The transient was discovered quite young by the All Sky Automated Survey for SuperNo…

astro-ph.SR2015★ 80 cited

Massive stars exploding in a He-rich circumstellar medium - IX. SN 2014av, and characterization of Type Ibn SNe

A. Pastorello, X. -F. Wang, F. Ciabattari +18

We present spectroscopic and photometric data of the Type Ibn supernova (SN) 2014av, discovered by the Xingming Observatory Sky Survey. Stringent pre-discovery detection limits ind…

astro-ph.SR2014★ 361 cited

PESSTO : survey description and products from the first data release by the Public ESO Spectroscopic Survey of Transient Objects

S. J. Smartt, S. Valenti, M. Fraser +99

The Public European Southern Observatory Spectroscopic Survey of Transient Objects (PESSTO) began as a public spectroscopic survey in April 2012. We describe the data reduction str…