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M. Krockenberger

4 papers hereh-index 8556 citations18 works total

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

author position
  • first author2
  • middle author1

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph4
same name
  • M. Krockenberger — 9 papers, h 37

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
19952005
most citedUBVRI Light Curves of 44 Type Ia Supernovae

372 citations · 598 across the 4 of their papers we have counts for

collaborators
Showing astro-phShow all

4 papers · 1 filter

astro-ph2005★ 372 cited

UBVRI Light Curves of 44 Type Ia Supernovae

Saurabh Jha, Robert P. Kirshner, Peter Challis +2

We present UBVRI photometry of 44 type-Ia supernovae (SN Ia) observed from 1997 to 2001 as part of a continuing monitoring campaign at the Fred Lawrence Whipple Observatory of the…

astro-ph1997★ 173 cited

A Planet Orbiting the Star Rho Coronae Borealis

R. W. Noyes, S. Jha, S. G. Korzennik +5

We report the discovery of near-sinusoidal radial velocity variations of the G0V star rhoCrB, with period 39.6 days and amplitude 67 m/s. These variations are consistent with the e…

astro-ph1996★ 32 cited

Radii and Distances of Cepheids, I., Method and Measurement Errors

Martin Krockenberger, Dimitar D. Sasselov, Robert W. Noyes

We develop a formulation of the Baade-Wesselink method which uses the Fourier coefficients of the observables. We derive an explicit, analytic expression to determine the mean radi…

astro-ph1995★ 21 cited

Discovery of Diffuse X-ray Emission in 47 Tuc

Martin Krockenberger, J. Grindlay

We present the results of a search for diffuse x-ray sources in a 65 ksec ROSAT PSPC exposure of 47 Tuc. There is faint, soft emission on the NE side of the cluster at a distance o…

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