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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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23 papers · 1 filter

astro-ph.HE2022★ 13 cited

The Type Ibn Supernova 2019kbj -- Indications for Diversity in Type Ibn Supernova Progenitors

Tom Ben-Ami, Iair Arcavi, Megan Newsome +9

Type Ibn supernovae (SNe) are a rare class of stellar explosions whose progenitor systems are not yet well determined. We present and analyze observations of the Type Ibn SN 2019kb…

astro-ph.HE2022★ 15 cited

Photometric and spectroscopic analysis of the Type II SN 2020jfo with a short plateau

B. Ailawadhi, R. Dastidar, K. Misra +34

We present high-cadence photometric and spectroscopic observations of SN~2020jfo in ultraviolet and optical/near-infrared bands starting from to days after the…

astro-ph.HE2022★ 36 cited

A JWST Near- and Mid-Infrared Nebular Spectrum of the Type Ia Supernova 2021aefx

Lindsey A. Kwok, Saurabh W. Jha, Tea Temim +55

We present JWST near- and mid-infrared spectroscopic observations of the nearby normal Type Ia supernova SN 2021aefx in the nebular phase at days past maximum light. Our Nea…

astro-ph.HE2022★ 13 cited

The First Two Years of FLEET: an Active Search for Superluminous Supernovae

Sebastian Gomez, Edo Berger, Peter K. Blanchard +5

In November 2019 we began operating FLEET (Finding Luminous and Exotic Extragalactic Transients), a machine learning algorithm designed to photometrically identify Type I superlumi…

astro-ph.HE2022★ 8 cited

JWST Imaging of the Cartwheel Galaxy Reveals Dust Associated with SN 2021afdx

Griffin Hosseinzadeh, David J. Sand, Jacob E. Jencson +12

We present near- and mid-infrared (0.9-18 m) photometry of supernova (SN) 2021afdx, which was imaged serendipitously with the James Webb Space Telescope (JWST) as part of its Ea…

astro-ph.HE2022★ 18 cited

Using 1991T/1999aa-like Type Ia Supernovae as Standardizable Candles

Jiawen Yang, Lifan Wang, Nicholas Suntzeff +13

We present the photometry of 16 91T/99aa-like Type Ia Supernovae (SNe Ia) observed by the Las Cumbres Observatory. We also use an additional set of 21 91T/99aa-like SNe Ia and 87 n…

astro-ph.HE2022★ 3 cited

Companion Shocking Fits to the 2018 ZTF Sample of SNe Ia Are Consistent with Single-Degenerate Progenitor Systems

J. Burke, D. A. Howell, D. J. Sand +1

The early lightcurves of Type Ia supernovae (SNe Ia) can be used to test predictions about their progenitor systems. If the progenitor system consists of a single white dwarf in a…

astro-ph.HE2022★ 32 cited

Circumstellar Medium Interaction in SN 2018lab, A Low-Luminosity II-P Supernova observed with TESS

Jeniveve Pearson, Griffin Hosseinzadeh, David J. Sand +21

We present photometric and spectroscopic data of SN 2018lab, a low luminosity type IIP supernova (LLSN) with a V-band peak luminosity of mag. SN 2018lab was discovere…

astro-ph.HE2022★ 6 cited

Early Lightcurves of Type Ia Supernovae are Consistent with Nondegenerate Progenitor Companions

J. Burke, D. A. Howell, D. J. Sand +16

If Type Ia supernovae (SNe~Ia) result from a white dwarf being ignited by Roche lobe overflow from a nondegenerate companion, then as the supernova explosion runs into the companio…

astro-ph.IM2022★ 5k cited

The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package

The Astropy Collaboration, Adrian M. Price-Whelan, Pey Lian Lim +133

The Astropy Project supports and fosters the development of open-source and openly-developed Python packages that provide commonly needed functionality to the astronomical communit…

astro-ph.SR2022★ 17 cited

SN 2016dsg: A Thermonuclear Explosion Involving A Thick Helium Shell

Yize Dong, Stefano Valenti, Abigail Polin +29

A thermonuclear explosion triggered by a helium-shell detonation on a carbon-oxygen white dwarf core has been predicted to have strong UV line blanketing at early times due to the…

astro-ph.SR2022★ 20 cited

The origin and evolution of the normal Type Ia SN 2018aoz with infant-phase reddening and excess emission

Yuan Qi Ni, Dae-Sik Moon, Maria R. Drout +40

SN~2018aoz is a Type Ia SN with a -band plateau and excess emission in the infant-phase light curves 1 day after first light, evidencing an over-density of surface ir…

astro-ph.SR2022★ 3 cited

High Cadence TESS and ground-based data of SN 2019esa, the less energetic sibling of SN 2006gy

Jennifer E. Andrews, Jeniveve Pearson, M. J. Lundquist +16

We present photometric and spectroscopic observations of the nearby ( Mpc) interacting supernova (SN) 2019esa, discovered within hours of explosion and serendipitously…

astro-ph.HE2022★ 52 cited

The Diverse Properties of Type Icn Supernovae Point to Multiple Progenitor Channels

C. Pellegrino, D. A. Howell, G. Terreran +16

We present a sample of Type Icn supernovae (SNe Icn), a newly-discovered class of transients characterized by their interaction with H- and He-poor circumstellar material (CSM). Th…

astro-ph.HE2022★ 36 cited

Constraining the Progenitor System of the Type Ia Supernova 2021aefx

Griffin Hosseinzadeh, David J. Sand, Peter Lundqvist +25

We present high-cadence optical and ultraviolet light curves of the normal Type Ia supernova (SN) 2021aefx, which shows an early bump during the first two days of observation. This…

astro-ph.HE2022★ 47 cited

Luminous Supernovae: Unveiling a Population Between Superluminous and Normal Core-collapse Supernovae

Sebastian Gomez, Edo Berger, Matt Nicholl +2

Stripped-envelope core-collapse supernovae can be divided into two broad classes: the common Type Ib/c supernovae (SNe Ib/c), powered by the radioactive decay of Ni, and the…

astro-ph.HE2022★ 8 cited

Photometrically-Classified Superluminous Supernovae from the Pan-STARRS1 Medium Deep Survey: A Case Study for Science with Machine Learning-Based Classification

Brian Hsu, Griffin Hosseinzadeh, V. Ashley Villar +1

With the upcoming Vera C.~Rubin Observatory Legacy Survey of Space and Time (LSST), it is expected that only of all transients will be classified spectroscopically. To…

astro-ph.HE2022★ 12 cited

Evolution of A Peculiar Type Ibn Supernova SN 2019wep

Anjasha Gangopadhyay, Kuntal Misra, Griffin Hosseinzadeh +14

We present a high-cadence short term photometric and spectroscopic monitoring campaign of a type Ibn SN 2019wep, which is one of the rare SN Ibn after SNe 2010al and 2019uo to disp…

astro-ph.HE2022★ 1 cited

Weak Mass Loss from the Red Supergiant Progenitor of the Type II SN 2021yja

Griffin Hosseinzadeh, Charles D. Kilpatrick, Yize Dong +56

We present high-cadence optical, ultraviolet (UV), and near-infrared data of the nearby ( Mpc) Type II supernova (SN) 2021yja. Many Type II SNe show signs of interactio…

astro-ph.HE2022★ 32 cited

Infant-phase reddening by surface Fe-peak elements in a normal Type Ia Supernova

Yuan Qi Ni, Dae-Sik Moon, Maria R. Drout +41

Type Ia Supernovae are thermonuclear explosions of white dwarf stars. They play a central role in the chemical evolution of the Universe and are an important measure of cosmologica…

astro-ph.HE2022★ 21 cited

A Systematic Exploration of Kilonova Candidates from Neutron Star Mergers During the Third Gravitational Wave Observing Run

J. Rastinejad, K. Paterson, W. Fong +9

We present a comprehensive analysis of 653 optical candidate counterparts reported during the third gravitational wave (GW) observing run. Our sample concentrates on candidates fro…

astro-ph.HE2022★ 16 cited

Nebular-Phase Spectra of Type Ia Supernovae from the Las Cumbres Observatory Global Supernova Project

M. L. Graham, T. D. Kennedy, S. Kumar +17

The observed diversity in Type Ia supernovae (SNe Ia) -- the thermonuclear explosions of carbon-oxygen white dwarf stars used as cosmological standard candles -- is currently met w…

astro-ph.HE2022

Constraining the Time of Gravitational Wave Emission from Core-Collapse Supernovae

Kiranjyot Gill, Griffin Hosseinzadeh, Edo Berger +2

The advent of sensitive gravitational wave (GW) detectors, coupled with wide-field, high cadence optical time-domain surveys, raises the possibility of the first joint GW-electroma…