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researcher

B. Kelly

53 papers hereh-index 415.9k citations82 works total

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

author position
  • sole author2
  • first author16
  • middle author26
  • last author7

Across the 51 of 53 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO19
  • astro-ph14
  • astro-ph.GA8
  • astro-ph.HE6
  • astro-ph.IM5
  • astro-ph.SR1
same name
  • B. Kelly — 41 papers, h 27
  • B. Kelly — 9 papers, h 5
  • B. Kelly — 5 papers, h 2
  • B. Kelly — 4 papers, h 2
  • B. Kelly — 2 papers, h 2
  • B. Kelly — 2 papers

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
20032021
most citedSome Aspects of Measurement Error in Linear Regression of Astronomical Data

1.3k citations · 7.5k across the 52 of their papers we have counts for

collaborators
Showing 2012 · astro-ph.GAShow all

3 papers · 2 filters

astro-ph.GA2012★ 29 cited

A Quasar-Galaxy Mixing Diagram: Quasar Spectral Energy Distribution Shapes in the Optical to Near-Infrared

Heng Hao, Martin Elvis, Angela Bongiorno +19

We define a quasar-galaxy mixing diagram using the slopes of their spectral energy distributions (SEDs) from 1μm to 3000Å and from 1μm to 3μm in the rest frame. The mixing diagram…

astro-ph.GA2012★ 85 cited

Disclosing the Radio Loudness Distribution Dichotomy in Quasars: An Unbiased Monte Carlo Approach Applied to the SDSS-FIRST Quasar Sample

Mislav Balokovic, Vernesa Smolcic, Zeljko Ivezic +3

We investigate the dichotomy in the radio loudness distribution of quasars by modelling their radio emission and various selection effects using a Monte Carlo approach. The existen…

astro-ph.GA2012★ 134 cited

The linewidth-size relationship in the dense ISM of the Central Molecular Zone

Rahul Shetty, Christopher N. Beaumont, Michael G. Burton +2

The linewidth (sigma) - size (R) relationship has been extensively measured and analysed, in both the local ISM and in nearby normal galaxies. Generally, a power-law describes the…

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