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20172026
most cited1ES 1927+654: An AGN Caught Changing Look on a Timescale of Months

193 citations · 4.4k across the 184 of their papers we have counts for

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13 papers · 1 filter

astro-ph.HE2019★ 35 cited

Flash ionization signatures in the type Ibn supernova SN 2019uo

Anjasha Gangopadhyay, Kuntal Misra, Daichi Hiramatsu +26

We present photometric and spectroscopic observations of the type Ibn supernova (SN) 2019uo, the second ever SN Ibn with flash ionization (He II, C III, N III) features in its earl…

astro-ph.SR2019★ 15 cited

SN 2017cfd: A Normal Type Ia Supernova Discovered Very Young

Xuhui Han, WeiKang Zheng, Benjamin E. Stahl +22

The Type~Ia supernova (SN~Ia) 2017cfd in IC~0511 (redshift z = 0.01209+- 0.00016$) was discovered by the Lick Observatory Supernova Search 1.6+-0.7 d after the fitted first-light t…

astro-ph.HE2019★ 28 cited

Discovery and Rapid Follow-up Observations of the Unusual Type II SN 2018ivc in NGC 1068

K. A. Bostroem, S. Valenti, D. J. Sand +44

We present the discovery and high-cadence follow-up observations of SN 2018ivc, an unusual Type II supernova that exploded in NGC 1068 (D=10.1 Mpc). The light curve of SN 2018ivc d…

astro-ph.HE2019★ 53 cited

SN 2017gmr: An energetic Type II-P supernova with asymmetries

Jennifer E. Andrews, D. J. Sand, S. Valenti +77

We present high-cadence ultraviolet (UV), optical, and near-infrared (NIR) data on the luminous Type II-P supernova SN 2017gmr from hours after discovery through the first 180 days…

astro-ph.SR2019★ 20 cited

A luminous stellar outburst during a long-lasting eruptive phase first, and then SN IIn 2018cnf

A. Pastorello, A. Reguitti, A. Morales-Garoffolo +45

We present the results of the monitoring campaign of the Type IIn supernova (SN) 2018cnf (aka ASASSN-18mr). It was discovered about 10 days before the maximum light (on MJD = 58293…

astro-ph.SR2019★ 49 cited

On the Ca-strong 1991bg-like type Ia supernova 2016hnk: evidence for a Chandrasekhar-mass explosion

Lluís Galbany, Chris Ashall, Peter Hoeflich +46

We present a comprehensive dataset of optical and near-infrared photometry and spectroscopy of type~Ia supernova (SN) 2016hnk, combined with integral field spectroscopy (IFS) of it…

astro-ph.HE2019★ 46 cited

The Young and Nearby Normal Type Ia Supernova 2018gv: UV-Optical Observations and the Earliest Spectropolarimetry

Yi Yang, Peter A. Hoeflich, Dietrich Baade +25

The non-detection of companion stars in Type Ia supernova (SN) progenitor systems lends support to the notion of double-degenerate (DD) systems and explosions triggered by the merg…

astro-ph.HE2019★ 86 cited

The Type II-P Supernova 2017eaw: from explosion to the nebular phase

Tamás Szalai, József Vinkó, Réka Könyves-Tóth +36

The nearby SN 2017eaw is a Type II-P (``plateau') supernova showing early-time, moderate CSM interaction. We present a comprehensive study of this SN including the analysis of high…

astro-ph.HE2019

Gravity and Light: Combining Gravitational Wave and Electromagnetic Observations in the 2020s

R. J. Foley, K. D. Alexander, I. Andreoni +110

As of today, we have directly detected exactly one source in both gravitational waves (GWs) and electromagnetic (EM) radiation, the binary neutron star merger GW170817, its associa…

astro-ph.GA2019★ 193 cited

1ES 1927+654: An AGN Caught Changing Look on a Timescale of Months

Benny Trakhtenbrot, Iair Arcavi, Chelsea L. MacLeod +21

We study the sudden optical and ultraviolet (UV) brightening of 1ES 1927+654, which until now was known as a narrow-line active galactic nucleus (AGN). 1ES 1927+654 was part of the…

astro-ph.GA2019★ 23 cited

Nebular H Limits for Fast Declining Type Ia Supernovae

D. J. Sand, R. C. Amaro, M. Moe +16

One clear observational prediction of the single degenerate progenitor scenario as the origin of type Ia supernovae (SNe) is the presence of relatively narrow (1000 km s$^…

astro-ph.HE2019★ 123 cited

The spectral evolution of AT 2018dyb and the presence of metal lines in tidal disruption events

Giorgos Leloudas, Lixin Dai, Iair Arcavi +29

We present light curves and spectra of the tidal disruption event (TDE) ASASSN-18pg / AT 2018dyb spanning a period of one year. The event shows a plethora of strong emission lines,…

astro-ph.HE2019★ 51 cited

Type Ibn Supernovae May not all Come from Massive Stars

Griffin Hosseinzadeh, Curtis McCully, Ann I. Zabludoff +5

Because core-collapse supernovae are the explosions of massive stars, which have relatively short lifetimes, they occur almost exclusively in galaxies with active star formation. O…