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researcher

B. Shappee

97 papers hereh-index 236.1k citations113 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author81
  • last author6

Across the 87 of 97 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE52
  • astro-ph.SR14
  • astro-ph.CO11
  • astro-ph.GA10
  • astro-ph.EP8
  • astro-ph.IM2
same name
  • B. Shappee — 181 papers, h 53

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20152026
most citedSwope Supernova Survey 2017a (SSS17a), the Optical Counterpart to a Gravitational Wave Source

1.2k citations · 2.5k across the 85 of their papers we have counts for

collaborators
Showing 2025 · astro-ph.SRShow all

3 papers · 2 filters

astro-ph.SR2025

JWST Observations of SN 2024ggi II: NIRSpec Spectroscopy and CO Modeling at 285 and 385 Days Past the Explosion

T. Mera, C. Ashall, P. Hoeflich +20

We present James Webb Space Telescope (JWST) NIRSpec observations of SN~2024ggi, spanning wavelengths of 1.7--5.5 micron at +285.51 and +385.27 days post-explosion. These nebular s…

astro-ph.SR2025★ 5 cited

The nebular phase of SN 2024ggi: a low-mass progenitor with no signs of interaction

L. Ferrari, G. Folatelli, K. Ertini +14

Context: SN 2024ggi is a Type II supernova (SN) discovered in the nearby galaxy NGC 3621 (D ≈6.7±0.d Mpc) on 2024 April 03.21 UT. Its proximity enabled a detailed investi…

astro-ph.SR2025

JWST Observations of SN 2024ggi I: Interpretation and Model Comparison of the Type II Supernova 2024ggi at 55 days Past Explosion

E. Baron, C. Ashall, J. M. DerKacy +40

We present panchromatic 0.4-21 microns observations of the nearby (about 7.2 Mpc) Type II supernova 2024ggi, obtained during the plateau phase at about 55 d past explosion. Our dat…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.