Louis R. Levenson, Ph.D.

Affiliations: 
2008 University of California, Los Angeles, Los Angeles, CA 
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"Louis Levenson"
Mean distance: 14.38
 
SNBCP

Parents

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Edward L. Wright grad student 2008 UCLA
 (Intensity, isotropy and origin of the cosmic infrared background.)
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Publications

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Matsuura S, Arai T, Bock JJ, et al. (2017) New Spectral Evidence of an Unaccounted Component of the Near-infrared Extragalactic Background Light from theCIBER The Astrophysical Journal. 839: 7
Gruppioni C, Pozzi F, Rodighiero G, et al. (2013) The Herschel* PEP/HerMES luminosity function - I. Probing the evolution of PACS selected Galaxies to z ≃ 4 Monthly Notices of the Royal Astronomical Society. 432: 23-52
Gruppioni C, Pozzi F, Rodighiero G, et al. (2013) Erratum: The Herschel★ PEP/HerMES Luminosity Function – I. Probing the Evolution of PACS selected Galaxies to z ≃ 4 Monthly Notices of the Royal Astronomical Society. 436: 2875-2876
Korngut PM, Renbarger T, Arai T, et al. (2013) The cosmic infrared background experiment (CIBER): The narrow-band spectrometer Astrophysical Journal, Supplement Series. 207
Tsumura K, Arai T, Battle J, et al. (2013) The cosmic infrared background experiment (CIBER): The low resolution spectrometer Astrophysical Journal, Supplement Series. 207
Bock J, Sullivan I, Arai T, et al. (2013) The cosmic infrared background experiment (CIBER): The wide-field imagers Astrophysical Journal, Supplement Series. 207
Zemcov M, Arai T, Battle J, et al. (2013) The cosmic infrared background experiment (CIBER): A sounding rocket payload to study the near infrared extragalactic background light Astrophysical Journal, Supplement Series. 207
Roseboom IG, Ivison RJ, Greve TR, et al. (2012) The Herschel Multi-tiered Extragalactic Survey: SPIRE-mm photometric redshifts Monthly Notices of the Royal Astronomical Society. 419: 2758-2773
Béthermin M, Le Floc'H E, Ilbert O, et al. (2012) HerMES: Deep number counts at 250 μm, 350 μm and 500 μm in the COSMOS and GOODS-N fields and the build-up of the cosmic infrared background Astronomy and Astrophysics. 542
Amblard A, Cooray A, Serra P, et al. (2011) Submillimetre galaxies reside in dark matter haloes with masses greater than 3 × 10(11) solar masses. Nature. 470: 510-2
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