J
J. Patrick Henry
Researcher at University of Hawaii
Publications - 77
Citations - 5336
J. Patrick Henry is an academic researcher from University of Hawaii. The author has contributed to research in topics: Galaxy cluster & Galaxy. The author has an hindex of 35, co-authored 77 publications receiving 5255 citations. Previous affiliations of J. Patrick Henry include Max Planck Society & Centre national de la recherche scientifique.
Papers
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Journal ArticleDOI
The Einstein Observatory Extended Medium-Sensitivity Survey. II - The optical identifications
John T. Stocke,Simon L. Morris,Isabella M. Gioia,Tommaso Maccacaro,Rudolph E. Schild,Anna Wolter,Thomas A. Fleming,J. Patrick Henry +7 more
TL;DR: In this article, the authors presented the optical identifications of the Einstein Extended Medium-Sensitivity Survey (EMSS), including the methodology used to optically identify the EMSS sources and the uncertainties involved with that process.
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Twenty-Three High-Redshift Supernovae from the Institute for Astronomy Deep Survey: Doubling the Supernova Sample at z > 0.7 * **
Brian J. Barris,John L. Tonry,Stephane Blondin,Peter Challis,Ryan Chornock,Alejandro Clocchiatti,Alexei V. Filippenko,Peter M. Garnavich,Stephen T. Holland,Saurabh Jha,Robert P. Kirshner,Kevin Krisciunas,Bruno Leibundgut,Weidong Li,Thomas Matheson,Gajus Miknaitis,Adam G. Riess,Brian P. Schmidt,R. Chris Smith,Jesper Sollerman,Jason Spyromilio,Christopher W. Stubbs,Nicholas B. Suntzeff,Herve Aussel,K. C. Chambers,M. S. Connelley,David Donovan,J. Patrick Henry,Nick Kaiser,Michael C. Liu,Eduardo L. Martín,Richard J. Wainscoat +31 more
TL;DR: In this article, photometric and spectroscopic observations of 23 high-redshift supernovae (SNe) spanning a range of z = 0.34-1.03, nine of which are unambiguously classified as Type Ia.
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Measuring Cosmological Parameters from the Evolution of Cluster X-Ray Temperatures
TL;DR: In this article, the authors derived the cluster X-ray temperature function from two flux-and redshift-limited samples of clusters and performed maximum likelihood fits of cluster evolution models to these data in order to constrain cosmological parameters.
Journal ArticleDOI
A measurement of the mass fluctuation spectrum from the cluster X-ray temperature function
J. Patrick Henry,Keith A. Arnaud +1 more
TL;DR: In this article, a statistically complete sample of galaxy clusters is presented which also has complete X-ray temperature information, and the cluster bolometric luminosity and temperature functions are derived.
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Joint Analysis of Cluster Observations: II. Chandra/XMM-Newton X-ray and Weak Lensing Scaling Relations for a Sample of 50 Rich Clusters of Galaxies
TL;DR: In this article, the authors present a study of multiwavelength X-ray and weak lensing scaling relations for a sample of 50 clusters of galaxies using an energy-dependent cross-calibration.