activity
20152026
most citedThe Astropy Project: Building an inclusive, open-science project and status of the v2.0 core package

7.7k citations · 22k across the 207 of their papers we have counts for

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Showing 2024Show all

17 papers · 1 filter

astro-ph.SR2024

Spectroscopy of AT 2016blu's recurring supernova impostor outbursts

Mojgan Aghakhanloo, Nathan Smith, Jennifer E. Andrews +7

We present spectra of the supernova (SN) impostor AT 2016blu spanning over a decade. This transient exhibits quasiperiodic outbursts with a 113 d period, likely triggered by…

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.IM2024★ 6 cited

Rubin ToO 2024: Envisioning the Vera C. Rubin Observatory LSST Target of Opportunity program

Igor Andreoni, Raffaella Margutti, John Banovetz +86

The Legacy Survey of Space and Time (LSST) at Vera C. Rubin Observatory is planned to begin in the Fall of 2025. The LSST survey cadence has been designed via a community-driven pr…

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★ 13 cited

Asymmetries and Circumstellar Interaction in the Type II SN 2024bch

Jennifer E. Andrews, Manisha Shrestha, K. Azalee Bostroem +29

We present a comprehensive multi-epoch photometric and spectroscopic study of SN 2024bch, a nearby (19.9 Mpc) Type II supernova (SN) with prominent early high ionization emission l…

astro-ph.HE2024★ 1 cited

Spectropolarimetry of SN 2023ixf reveals both circumstellar material and helium core to be aspherical

Manisha Shrestha, Sabrina DeSoto, David J. Sand +33

We present multi-epoch optical spectropolarimetric and imaging polarimetric observations of the nearby Type II supernova (SN) 2023ixf discovered in M101 at a distance of 6.85 Mpc.…

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★ 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★ 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.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.HE2024

Mapping the Inner 0.1 pc of a Supermassive Black Hole Environment with the Tidal Disruption Event and Extreme Coronal Line Emitter AT 2022upj

Megan Newsome, Iair Arcavi, D. Andrew Howell +10

Extreme coronal line emitters (ECLEs) are objects showing transient high-ionization lines in the centers of galaxies. They have been attributed to echoes of high-energy flares of i…

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★ 9 cited

Probing the Circumstellar Environment of highly luminous type IIn SN ASASSN-14il

Naveen Dukiya, Anjasha Gangopadhyay, Kuntal Misra +8

We present long-term photometric and spectroscopic studies of Circumstellar Material (CSM)-Ejecta interacting supernova (SN) ASASSN-14il in the galaxy PGC 3093694. The SN reaches a…

astro-ph.HE2024★ 3 cited

Superphot+: Realtime Fitting and Classification of Supernova Light Curves

Kaylee M. de Soto, Ashley Villar, Edo Berger +9

Photometric classifications of supernova (SN) light curves have become necessary to utilize the full potential of large samples of observations obtained from wide-field photometric…

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★ 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…