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L. Levenson

Identifiers

  • name variant L. Levenson 0.60 · backfill

Papers (29)

  1. The suppression of star formation by powerful active galactic nuclei astro-ph.CO · 2013 · author #39
  2. The Herschel PEP/HerMES Luminosity Function. I: Probing the Evolution of PACS selected Galaxies to z~4 astro-ph.CO · 2013 · author #66
  3. HerMES: Cosmic Infrared Background Anisotropies and the Clustering of Dusty Star-Forming Galaxies astro-ph.CO · 2012 · author #29
  4. HerMES: Candidate Gravitationally Lensed Galaxies and Lensing Statistics at Submillimeter Wavelengths astro-ph.CO · 2012 · author #50
  5. HerMES: deep number counts at 250, 350, and 500 microns in the COSMOS and GOODS-N fields and the build-up of the cosmic infrared background astro-ph.CO · 2012 · author #29
  6. The Herschel Multi-Tiered Extragalactic Survey: SPIRE-mm Photometric Redshifts astro-ph.CO · 2011 · author #38
  7. Modeling of the HERMES J105751.1+573027 submillimeter source lensed by a dark matter dominated foreground group of galaxies astro-ph.CO · 2011 · author #39
  8. Discovery of a Multiply-Lensed Submillimeter Galaxy in Early HerMES Herschel/SPIRE Data astro-ph.CO · 2011 · author #43
  9. Sub-millimetre galaxies reside in dark matter halos with masses greater than 3x10^11 solar masses astro-ph.CO · 2011 · author #34
  10. HerMES: SPIRE Science Demonstration Phase Maps astro-ph.CO · 2010 · author #1
  11. HerMES: Deep Galaxy Number Counts from a P(D) Fluctuation Analysis of SPIRE Science Demonstration Phase Observations astro-ph.CO · 2010 · author #35
  12. HerMES: Herschel-SPIRE observations of Lyman Break Galaxies astro-ph.CO · 2010 · author #33
  13. The Herschel Multi-Tiered Extragalactic Survey: Source Extraction and Cross-Identifications in Confusion-Dominated SPIRE Images astro-ph.CO · 2010 · author #45
  14. The Deep SPIRE HerMES Survey: Spectral Energy Distributions and their Astrophysical Indications at High Redshift astro-ph.CO · 2010 · author #34
  15. Evolution of Dust Temperature of Galaxies through Cosmic Time as seen by Herschel astro-ph.CO · 2010 · author #59
  16. Measures of star formation rates from Infrared (Herschel) and UV (GALEX) emissions of galaxies in the HerMES fields astro-ph.CO · 2010 · author #35
  17. Contribution of Lensed SCUBA Galaxies to the Cosmic Infrared Background astro-ph.CO · 2010 · author #4
  18. The Herschel-SPIRE instrument and its in-flight performance astro-ph.IM · 2010 · author #84
  19. In-flight calibration of the Herschel-SPIRE instrument astro-ph.IM · 2010 · author #26
  20. HerMES: Halo Occupation Number and Bias Properties of Dusty Galaxies from Angular Clustering Measurements astro-ph.CO · 2010 · author #37
  21. HerMES: The Submillimeter Spectral Energy Distributions of Herschel/SPIRE-Detected Galaxies astro-ph.CO · 2010 · author #37
  22. HerMES: The SPIRE confusion limit astro-ph.CO · 2010 · author #4
  23. HerMES: Far-infrared properties of known AGN in the HerMES fields astro-ph.CO · 2010 · author #38
  24. First results from HerMES on the evolution of the submillimetre luminosity function astro-ph.CO · 2010 · author #41
  25. The HerMES SPIRE submillimeter local luminosity function astro-ph.CO · 2010 · author #40
  26. HerMES: SPIRE galaxy number counts at 250, 350 and 500 microns astro-ph.CO · 2010 · author #37
  27. FIR colours and SEDs of nearby galaxies observed with Herschel astro-ph.CO · 2010 · author #44
  28. The far-infrared/radio correlation as probed by Herschel astro-ph.CO · 2010 · author #48
  29. The Herschel Reference Survey astro-ph.CO · 2010 · author #28

Mentions

  • 1310.4147 #39 · backfill · confidence 0.70 L. Levenson
  • 1302.5209 #66 · backfill · confidence 0.70 L. Levenson
  • 1208.5049 #29 · backfill · confidence 0.70 L. Levenson
  • 1205.3778 #50 · backfill · confidence 0.70 L. Levenson
  • 1203.1925 #29 · backfill · confidence 0.70 L. Levenson
  • 1109.2887 #38 · backfill · confidence 0.70 L. Levenson
  • 1104.4119 #39 · backfill · confidence 0.70 L. Levenson
  • 1104.4113 #43 · backfill · confidence 0.70 L. Levenson
  • 1101.1080 #34 · backfill · confidence 0.70 L. Levenson
  • 1010.0020 #1 · backfill · confidence 0.70 L. Levenson
  • 1009.5675 #35 · backfill · confidence 0.70 L. Levenson
  • 1009.2715 #33 · backfill · confidence 0.70 L. Levenson
  • 1009.1658 #45 · backfill · confidence 0.70 L. Levenson
  • 1009.1371 #34 · backfill · confidence 0.70 L. Levenson
  • 1009.1058 #59 · backfill · confidence 0.70 L. Levenson
  • 1007.1857 #35 · backfill · confidence 0.70 L. Levenson
  • 1006.1360 #4 · backfill · confidence 0.70 L. Levenson
  • 1005.5123 #84 · backfill · confidence 0.70 L. Levenson
  • 1005.5073 #26 · backfill · confidence 0.70 L. Levenson
  • 1005.3303 #37 · backfill · confidence 0.70 L. Levenson
  • 1005.2396 #37 · backfill · confidence 0.70 L. Levenson
  • 1005.2207 #4 · backfill · confidence 0.70 L. Levenson
  • 1005.2192 #38 · backfill · confidence 0.70 L. Levenson
  • 1005.2189 #41 · backfill · confidence 0.70 L. Levenson
  • 1005.2187 #40 · backfill · confidence 0.70 L. Levenson
  • 1005.2184 #37 · backfill · confidence 0.70 L. Levenson
  • 1005.1537 #44 · backfill · confidence 0.70 L. Levenson
  • 1005.1072 #48 · backfill · confidence 0.70 L. Levenson
  • 1001.5136 #28 · backfill · confidence 0.70 L. Levenson

Frequent Coauthors