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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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astro-ph.HE2024

A Multiwavelength Autopsy of the Interacting IIn Supernova 2020ywx: Tracing its Progenitor Mass-Loss History for 100 Years before Death

Raphael Baer-Way, Poonam Chandra, Maryam Modjaz +31

While the subclass of interacting supernovae with narrow hydrogen emission lines (SNe IIn) consists of some of the longest-lasting and brightest SNe ever discovered, their progenit…

astro-ph.HE2024★ 12 cited

Luminous Type II Short-Plateau SN 2023ufx: Asymmetric Explosion of a Partially-Stripped Massive Progenitor

Aravind P. Ravi, Stefano Valenti, Yize Dong +34

We present supernova (SN) 2023ufx, a unique Type IIP SN with the shortest known plateau duration ( 47 days), a luminous V-band peak ( = 18.42 0…

astro-ph.HE2024★ 5 cited

Type IIn Supernovae. I. Uniform Light-curve Characterization and a Bimodality in the Radiated Energy Distribution

Daichi Hiramatsu, Edo Berger, Sebastian Gomez +3

We present the largest uniform study to date of Type IIn supernovae (SNe IIn), focusing in this first paper on the multiband optical light curves of 490 SNe IIn. The sample, constr…

astro-ph.HE2024

Circumstellar Interaction in the Ultraviolet Spectra of SN 2023ixf 14-66 Days After Explosion

K. Azalee Bostroem, David J. Sand, Luc Dessart +20

SN 2023ixf was discovered in M101 within a day of explosion and rapidly classified as a Type II supernova with flash features. Here we present ultraviolet (UV) spectra obtained wit…

astro-ph.HE2024★ 5 cited

Eruptive mass loss less than a year before the explosion of superluminous supernovae: I. The cases of SN 2020xga and SN 2022xgc

A. Gkini, C. Fransson, R. Lunnan +47

We present photometric and spectroscopic observations of SN 2020xga and SN 2022xgc, two hydrogen-poor superluminous supernovae (SLSNe-I) at and , respectiv…

astro-ph.HE2024★ 8 cited

Spectral dataset of young type Ib supernovae and their time evolution

N. Yesmin, C. Pellegrino, M. Modjaz +11

Due to high-cadence automated surveys, we can now detect and classify supernovae (SNe) within a few days after explosion, if not earlier. Early-time spectra of young SNe directly p…

astro-ph.HE2024

SN 2021foa: the bridge between SN IIn and Ibn

Anjasha Gangopadhyay, Naveen Dukiya, Takashi J Moriya +26

We present the long-term photometric and spectroscopic analysis of a transitioning SN~IIn/Ibn from 10.8 d to 150.7 d post -band maximum. SN~2021foa shows prominent He {\sc i}…

astro-ph.HE2024

Ejecta masses in Type Ia Supernovae -- Implications for the Progenitor and the Explosion Scenario

Zsófia Bora, Réka Könyves-Tóth, József Vinkó +35

The progenitor system(s) as well as the explosion mechanism(s) of thermonuclear (Type Ia) supernovae are long-standing issues in astrophysics. Here we present ejecta masses and oth…

astro-ph.HE2024★ 6 cited

Massive stars exploding in a He-rich circumstellar medium X. Flash spectral features in the Type Ibn SN 2019cj and observations of SN 2018jmt

Z. -Y. Wang, A. Pastorello, K. Maeda +48

We present optical and near-infrared observations of two Type Ibn supernovae (SNe), SN 2018jmt and SN 2019cj. Their light curves have rise times of about 10 days, reaching an absol…

astro-ph.HE2024

AT2023vto: An Exceptionally Luminous Helium Tidal Disruption Event from a Massive Star

Harsh Kumar, Edo Berger, Daichi Hiramatsu +10

We present optical/UV observations and the spectroscopic classification of the transient AT2023vto as a tidal disruption event (TDE) at z = 0.4846. The spectrum is dominated by a b…

astro-ph.HE2024

Finding the Fuse: Prospects for the Detection and Characterization of Hydrogen-Rich Core-Collapse Supernova Precursor Emission with the LSST

A. Gagliano, E. Berger, V. A. Villar +5

Enhanced emission in the months to years preceding explosion has been detected for several core-collapse supernovae (SNe). Though the physical mechanisms driving the emission remai…

astro-ph.HE2024★ 10 cited

One Year of SN 2023ixf: Breaking Through the Degenerate Parameter Space in Light-Curve Models with Pulsating Progenitors

Brian Hsu, Nathan Smith, Jared A. Goldberg +21

We present and analyze the extensive optical broadband photometry of the Type II SN 2023ixf up to one year after explosion. We find that, when compared to two pre-existing model gr…

astro-ph.SR2024★ 6 cited

A study in scarlet -- II. Spectroscopic properties of a sample of Intermediate Luminosity Red Transients

G. Valerin, A. Pastorello, E. Mason +65

We investigate the spectroscopic characteristics of Intermediate Luminosity Red Transients (ILRTs), a class of elusive objects with peak luminosity between that of classical novae…

astro-ph.SR2024★ 8 cited

A study in scarlet -- I. Photometric properties of a sample of Intermediate Luminosity Red Transients

G. Valerin, A. Pastorello, A. Reguitti +57

We investigate the photometric characteristics of a sample of Intermediate Luminosity Red Transients (ILRTs), a class of elusive objects with peak luminosity between that of classi…

astro-ph.HE2024

The Type I Superluminous Supernova Catalog I: Light Curve Properties, Models, and Catalog Description

Sebastian Gomez, Matt Nicholl, Edo Berger +25

We present the most comprehensive catalog to date of Type I Superluminous Supernovae (SLSNe), a class of stripped envelope supernovae (SNe) characterized by exceptionally high lumi…

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.HE2024

WTP19aalnxx: Discovery of a bright mid-infrared transient in the emerging class of low luminosity supernovae revealed by delayed circumstellar interaction

Charlotte Myers, Kishalay De, Lin Yan +11

While core-collapse supernovae (SNe) often show early and consistent signs of circumstellar (CSM) interaction, some exhibit delayed signatures due to interaction with distant mater…

astro-ph.HE2024

Extended Shock Breakout and Early Circumstellar Interaction in SN 2024ggi

Manisha Shrestha, K. Azalee Bostroem, David J. Sand +40

We present high-cadence photometric and spectroscopic observations of supernova (SN) 2024ggi, a Type II SN with flash spectroscopy features which exploded in the nearby galaxy NGC…

astro-ph.HE2024★ 1 cited

SN2023fyq: A Type Ibn Supernova With Long-standing Precursor Activity Due to Binary Interaction

Yize Dong, Daichi Tsuna, Stefano Valenti +29

We present photometric and spectroscopic observations of SN 2023fyq, a type Ibn supernova in the nearby galaxy NGC 4388 (D18~Mpc). In addition, we trace long-standing precu…

astro-ph.HE2024★ 2 cited

Final Moments II: Observational Properties and Physical Modeling of CSM-Interacting Type II Supernovae

W. V. Jacobson-Galán, L. Dessart, K. W. Davis +52

We present ultraviolet/optical/near-infrared observations and modeling of Type II supernovae (SNe II) whose early-time ( days) spectra show transient, narrow emission lines…

astro-ph.HE2024★ 8 cited

SN 2019nyk: A rapidly declining Type II supernova with early interaction signatures

Raya Dastidar, Giuliano Pignata, Naveen Dukiya +9

We present an optical photometric and spectroscopic analysis of the fast-declining hydrogen-rich Type II supernova (SN) 2019nyk. The light curve properties of SN 2019nyk align well…

astro-ph.HE2024★ 2 cited

A Robust Light-Curve Diagnostic for Electron-Capture Supernovae and Low-Mass Fe-Core-Collapse Supernovae

Masato Sato, Nozomu Tominaga, Sergei I. Blinnikov +3

Core-collapse supernovae (CCSNe) are the terminal explosions of massive stars. While most massive stars explode as iron-core-collapse supernovae (FeCCSNe), slightly less massive st…

astro-ph.HE2024★ 2 cited

SN 2020udy: A new piece of the homogeneous bright group in the diverse Iax subclass

Mridweeka Singh, Devendra K. Sahu, Barnabas Barna +23

We present optical observations and analysis of a bright type Iax SN~2020udy hosted by NGC 0812. The light curve evolution of SN~2020udy is similar to other bright Iax SNe. Analyti…

astro-ph.HE2024★ 3 cited

Circumstellar interaction signatures in the low luminosity type II SN 2021gmj

Nicolas Meza-Retamal, Yize Dong, K. Azalee Bostroem +25

We present comprehensive optical observations of SN~2021gmj, a Type II supernova (SN~II) discovered within a day of explosion by the Distance Less Than 40~Mpc (DLT40) survey. Follo…