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J. S. Bloom

11 papers here

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

author position
  • middle author8
  • last author1

Across the 9 of 11 papers where every author was matched, so the position is known.

fields
  • astro-ph9
  • astro-ph.CO1
  • astro-ph.GA1
ORCID 0000-0002-7777-216X
same name
  • J. S. Bloom — 12 papers, h 9

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
19982019
most citedEchelle Spectroscopy of a GRB Afterglow at z=3.969: A New Probe of the Interstellar and Intergalactic Media in the Young Universe

138 citations · 640 across the 11 of their papers we have counts for

collaborators
Showing 2005Show all

3 papers · 1 filter

astro-ph2005★ 117 cited

The Unique Type Ib Supernova 2005bf: A WN Star Explosion Model for Peculiar Light Curves and Spectra

N. Tominaga, M. Tanaka, K. Nomoto +22

Observations and modeling for the light curve (LC) and spectra of supernova (SN) 2005bf are reported. This SN showed unique features: the LC had two maxima, and declined rapidly af…

astro-ph2005★ 138 cited

Echelle Spectroscopy of a GRB Afterglow at z=3.969: A New Probe of the Interstellar and Intergalactic Media in the Young Universe

Hsiao-Wen Chen, Jason X. Prochaska, Joshua S. Bloom +1

We present an echelle spectrum of the Swift GRB 050730, obtained four hours after the burst using the MIKE spectrograph on the Magellan Clay Telescope when the afterglow was at R=1…

astro-ph2005★ 49 cited

The Calibration of the Swift/UVOT Optical Observations: A Recipe for Photometry

Weidong Li, Saurabh Jha, Alexei V. Filippenko +4

Swift/UVOT has the capability to provide critical insight into the physics of the early afterglows of gamma-ray bursts (GRBs). But without precise calibration of the UVOT to standa…

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