activity
20092023
most citedCharacterizing the V-band light-curves of hydrogen-rich type II supernovae

377 citations · 3.6k across the 70 of their papers we have counts for

collaborators
Showing 2020Show all

16 papers · 1 filter

astro-ph.GA2020★ 21 cited

The delay time distribution of supernovae from integral-field spectroscopy of nearby galaxies

Asier Castrillo, Yago Ascasibar, Lluís Galbany +6

Constraining the delay-time distribution (DTD) of different supernova (SN) types can shed light on the timescales of galaxy chemical enrichment and feedback processes affecting gal…

astro-ph.HE2020★ 48 cited

Accretion disc cooling and narrow absorption lines in the tidal disruption event AT 2019dsg

G. Cannizzaro, T. Wevers, P. G. Jonker +23

We present the results of a large multi-wavelength follow-up campaign of the Tidal Disruption Event (TDE) \dsg, focusing on low to high resolution optical spectroscopy, X-ray, and…

astro-ph.GA2020★ 63 cited

A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE).IX. The effects of ram pressure stripping down to the scale of individual HII regions in the dwarf galaxy IC 3476

A. Boselli, A. Lupi, B. Epinat +25

We study the IB(s)m galaxy IC 3476 observed in the context of VESTIGE, a blind narrow-band Halpha+[NII] imaging survey of the Virgo cluster. The deep narrow-band (NB) image reveals…

astro-ph.HE2020★ 29 cited

SN 2019muj -- a well-observed Type Iax supernova that bridges the luminosity gap of the class

Barnabás Barna, Tamás Szalai, Saurabh W. Jha +38

We present early-time ( days) observations of SN 2019muj (= ASASSN-19tr), one of the best-observed members of the peculiar SN Iax class. Ultraviolet and optical photometri…

astro-ph.GA2020★ 19 cited

An Amusing Look at the Host of the Periodic Nuclear Transient ASASSN-14ko Reveals a Second AGN

M. A. Tucker, B. J. Shappee, J. T. Hinkle +10

We present Multi-Unit Spectroscopic Explorer (MUSE) integral-field spectroscopy of ESO 253G003, which hosts a known Active Galactic Nucleus (AGN) and the periodic nuclear transi…

astro-ph.HE2020★ 71 cited

Luminous Type II Short-Plateau Supernovae 2006Y, 2006ai, and 2016egz: A Transitional Class from Stripped Massive Red Supergiants

Daichi Hiramatsu, D. Andrew Howell, Takashi J. Moriya +21

The diversity of Type II supernovae (SNe II) is thought to be driven mainly by differences in their progenitor's hydrogen-rich (H-rich) envelope mass, with SNe IIP having long plat…

astro-ph.HE2020★ 19 cited

Optical and Near-Infrared Observations of the Nearby Type Ia Supernova 2017cbv

Lingzhi Wang, Carlos Contreras, Maokai Hu +28

Supernova (SN) 2017cbv in NGC 5643 is one of a handful of type Ia supernovae (SNe~Ia) reported to have excess blue emission at early times. This paper presents extensive $BVRIYJHK_…

astro-ph.SR2020★ 11 cited

Direct evidence of two-component ejecta in supernova 2016gkg from nebular spectroscopy

Hanindyo Kuncarayakti, Gaston Folatelli, Keiichi Maeda +17

Spectral observations of the type-IIb supernova (SN) 2016gkg at 300-800 days are reported. The spectra show nebular characteristics, revealing emission from the progenitor star's m…

astro-ph.HE2020★ 70 cited

SN 2019ehk: A Double-Peaked Ca-rich Transient with Luminous X-ray Emission and Shock-Ionized Spectral Features

Wynn V. Jacobson-Galán, Raffaella Margutti, Charles D. Kilpatrick +64

We present panchromatic observations and modeling of the Calcium-rich supernova 2019ehk in the star-forming galaxy M100 (d16.2 Mpc) starting 10 hours after explosion and c…

astro-ph.HE2020★ 22 cited

The low-luminosity type II SN\,2016aqf: A well-monitored spectral evolution of the Ni/Fe abundance ratio

Tomás E. Müller-Bravo, Claudia P. Gutiérrez, Mark Sullivan +20

Low-luminosity type II supernovae (LL SNe~II) make up the low explosion energy end of core-collapse SNe, but their study and physical understanding remain limited. We present SN\,2…

astro-ph.HE2020★ 21 cited

PS15cey and PS17cke: prospective candidates from the Pan-STARRS Search for Kilonovae

Owen R. McBrien, Stephen J. Smartt, Mark E. Huber +22

Time domain astronomy was revolutionised with the discovery of the first kilonova, AT2017gfo, in August 2017 which was associated with the gravitational wave signal GW170817. Since…

astro-ph.IM2020★ 356 cited

Design and operation of the ATLAS Transient Science Server

K. W. Smith, S. J. Smartt, D. R. Young +19

The Asteroid Terrestrial impact Last Alert System (ATLAS) system consists of two 0.5m Schmidt telescopes with cameras covering 29 square degrees at plate scale of 1.86 arcsec per p…

astro-ph.HE2020★ 62 cited

The Tidal Disruption Event AT 2018hyz II: Light Curve Modeling of a Partially Disrupted Star

Sebastian Gomez, Matt Nicholl, Philip Short +18

AT 2018hyz (=ASASSN-18zj) is a tidal disruption event (TDE) located in the nucleus of a quiescent E+A galaxy at a redshift of , first detected by the All-Sky Automated…

astro-ph.GA2020★ 101 cited

The AMUSING++ Nearby Galaxy Compilation: I. Full Sample Characterization and Galactic--Scale Outflows Selection

Carlos López-Cobá, Sebastián F. Sánchez, Joseph P. Anderson +6

We present here AMUSING\textrm{++}; the largest compilation of nearby galaxies observed with the MUSE integral field spectrograph so far. This collection consists of 635 galaxies f…

astro-ph.HE2020★ 36 cited

Stripped-envelope core-collapse supernova Ni masses: Persistently larger values than supernovae type II

Nicolás Meza, J. P. Anderson

The mass of synthesised radioactive material is an important power source for all supernova (SN) types. Anderson 2019 recently compiled literature values and obtained Ni dis…

astro-ph.GA2020★ 33 cited

Arm-interarm gas abundance variations explored with MUSE: the role of spiral structure in the chemical enrichment of galaxies

Laura Sánchez-Menguiano, Sebastián F. Sánchez, Isabel Pérez +4

Spiral arms are the most characteristic features of disc galaxies, easily distinguishable due to their association with ongoing star formation. However, the role of spiral structur…