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C. Blake

93 papers hereh-index 339k citations152 works total

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

author position
  • sole author1
  • first author9
  • middle author53
  • last author9

Across the 72 of 93 papers where every author was matched, so the position is known.

fields
  • astro-ph.IM26
  • astro-ph25
  • astro-ph.EP19
  • astro-ph.SR19
  • astro-ph.HE3
  • astro-ph.CO1
same name
  • C. Blake — 146 papers, h 61
  • C. Blake — 24 papers, h 5
  • C. Blake — 12 papers, h 13
  • C. Blake — 4 papers, h 4
  • C. Blake — 3 papers, h 3
  • C. Blake — 2 papers, h 2

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
20012023
most citedThe Eleventh and Twelfth Data Releases of the Sloan Digital Sky Survey: Final Data from SDSS-III

2.5k citations · 11k across the 91 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

3 papers · 1 filter

astro-ph.HE2014★ 79 cited

CfAIR2: Near Infrared Light Curves of 94 Type Ia Supernovae

Andrew S. Friedman, W. M. Wood-Vasey, G. H. Marion +18

CfAIR2 is a large homogeneously reduced set of near-infrared (NIR) light curves for Type Ia supernovae (SN Ia) obtained with the 1.3m Peters Automated InfraRed Imaging TELescope (P…

astro-ph.HE2010★ 87 cited

Multi-wavelength Observations of the Flaring Gamma-ray Blazar 3C 66A in 2008 October

LAT collaboration, A. A. Abdo et al., the VERITAS collaboration +4

The BL Lacertae object 3C 66A was detected in a flaring state by the Fermi Large Area Telescope (LAT) and VERITAS in 2008 October. In addition to these gamma-ray observations, F-GA…

astro-ph.HE2010★ 36 cited

The Double-Peaked 2008 Outburst of the Accreting Milli-Second X-ray Pulsar, IGR J00291+5934

F. Lewis, D. M. Russell, P. G. Jonker +18

In August 2008, the accreting milli-second X-ray pulsar (AMXP), IGR J00291+5934, underwent an outburst lasting ~ 100 days, the first since its discovery in 2004. We present data fr…

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