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C.D. Dowell

Identifiers

  • name variant C.D. Dowell 0.60 · backfill

Papers (31)

  1. The HerMES sub-millimetre local and low-redshift luminosity functions astro-ph.GA · 2015 · author #15
  2. Self-Calibration of BICEP1 Three-Year Data and Constraints on Astrophysical Polarization Rotation astro-ph.IM · 2013 · author #15
  3. The suppression of star formation by powerful active galactic nuclei astro-ph.CO · 2013 · author #20
  4. A Dust-Obscured Massive Maximum-Starburst Galaxy at a Redshift of 6.34 astro-ph.CO · 2013 · author #5
  5. HerMES: A Deficit in the Surface Brightness of the Cosmic Infrared Background Due to Galaxy Cluster Gravitational Lensing astro-ph.CO · 2013 · author #9
  6. The Herschel PEP/HerMES Luminosity Function. I: Probing the Evolution of PACS selected Galaxies to z~4 astro-ph.CO · 2013 · author #55
  7. The Herschel census of infrared SEDs through cosmic time astro-ph.CO · 2013 · author #16
  8. Optimization and sensitivity of the Keck Array astro-ph.IM · 2012 · author #12
  9. 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 #18
  10. HerMES: point source catalogues from deep Herschel-SPIRE observations astro-ph.CO · 2011 · author #13
  11. The Herschel Multi-Tiered Extragalactic Survey: SPIRE-mm Photometric Redshifts astro-ph.CO · 2011 · author #24
  12. Modeling of the HERMES J105751.1+573027 submillimeter source lensed by a dark matter dominated foreground group of galaxies astro-ph.CO · 2011 · author #21
  13. Discovery of a Multiply-Lensed Submillimeter Galaxy in Early HerMES Herschel/SPIRE Data astro-ph.CO · 2011 · author #25
  14. Redshift Determination and CO Line Excitation Modeling for the Multiply-Lensed Galaxy HLSW-01 astro-ph.CO · 2011 · author #19
  15. Dynamical Structure of the Molecular Interstellar Medium in an Extremely Bright, Multiply Lensed z~3 Submillimeter Galaxy Discovered with Herschel astro-ph.CO · 2011 · author #21
  16. Sub-millimetre galaxies reside in dark matter halos with masses greater than 3x10^11 solar masses astro-ph.CO · 2011 · author #18
  17. HerMES: SPIRE Science Demonstration Phase Maps astro-ph.CO · 2010 · author #10
  18. HerMES: Deep Galaxy Number Counts from a P(D) Fluctuation Analysis of SPIRE Science Demonstration Phase Observations astro-ph.CO · 2010 · author #19
  19. HerMES: Herschel-SPIRE observations of Lyman Break Galaxies astro-ph.CO · 2010 · author #19
  20. The Herschel Multi-Tiered Extragalactic Survey: Source Extraction and Cross-Identifications in Confusion-Dominated SPIRE Images astro-ph.CO · 2010 · author #25
  21. The Deep SPIRE HerMES Survey: Spectral Energy Distributions and their Astrophysical Indications at High Redshift astro-ph.CO · 2010 · author #19
  22. Evolution of Dust Temperature of Galaxies through Cosmic Time as seen by Herschel astro-ph.CO · 2010 · author #34
  23. Measures of star formation rates from Infrared (Herschel) and UV (GALEX) emissions of galaxies in the HerMES fields astro-ph.CO · 2010 · author #19
  24. Deep Herschel view of obscured star formation in the Bullet cluster astro-ph.CO · 2010 · author #22
  25. HerMES: Halo Occupation Number and Bias Properties of Dusty Galaxies from Angular Clustering Measurements astro-ph.CO · 2010 · author #20
  26. HerMES: The Submillimeter Spectral Energy Distributions of Herschel/SPIRE-Detected Galaxies astro-ph.CO · 2010 · author #21
  27. The HerMES SPIRE submillimeter local luminosity function astro-ph.CO · 2010 · author #22
  28. Simultaneous Multi-Wavelength Observations of Sgr A* during 2007 April 1-11 astro-ph.GA · 2009 · author #6
  29. Structure of the outer layers of cool standard stars astro-ph.SR · 2009 · author #7
  30. A Multi-Wavelength Study of Sgr A*: The Role of Near-IR Flares in Production of X-ray, Soft $\gamma$-ray and Sub-millimeter Emission astro-ph · 2005 · author #3
  31. Submillimeter Imaging of NGC 891 with SHARC astro-ph · 1998 · author #3

Mentions

  • 1312.7877 #15 · backfill · confidence 0.70 C.D. Dowell
  • 1310.4147 #20 · backfill · confidence 0.70 C.D. Dowell
  • 1304.4256 #5 · backfill · confidence 0.70 C.D. Dowell
  • 1303.6725 #9 · backfill · confidence 0.70 C.D. Dowell
  • 1302.5209 #55 · backfill · confidence 0.70 C.D. Dowell
  • 1302.4895 #16 · backfill · confidence 0.70 C.D. Dowell
  • 1208.0857 #12 · backfill · confidence 0.70 C.D. Dowell
  • 1203.1925 #18 · backfill · confidence 0.70 C.D. Dowell
  • 1109.5186 #13 · backfill · confidence 0.70 C.D. Dowell
  • 1109.2887 #24 · backfill · confidence 0.70 C.D. Dowell
  • 1104.4119 #21 · backfill · confidence 0.70 C.D. Dowell
  • 1104.4116 #21 · backfill · confidence 0.70 C.D. Dowell
  • 1104.4115 #19 · backfill · confidence 0.70 C.D. Dowell
  • 1104.4113 #25 · backfill · confidence 0.70 C.D. Dowell
  • 1101.1080 #18 · backfill · confidence 0.70 C.D. Dowell
  • 1010.0020 #10 · backfill · confidence 0.70 C.D. Dowell
  • 1009.5675 #19 · backfill · confidence 0.70 C.D. Dowell
  • 1009.2715 #19 · backfill · confidence 0.70 C.D. Dowell
  • 1009.1658 #25 · backfill · confidence 0.70 C.D. Dowell
  • 1009.1371 #19 · backfill · confidence 0.70 C.D. Dowell
  • 1009.1058 #34 · backfill · confidence 0.70 C.D. Dowell
  • 1007.1857 #19 · backfill · confidence 0.70 C.D. Dowell
  • 1005.3822 #22 · backfill · confidence 0.70 C.D. Dowell
  • 1005.3303 #20 · backfill · confidence 0.70 C.D. Dowell
  • 1005.2396 #21 · backfill · confidence 0.70 C.D. Dowell
  • 1005.2187 #22 · backfill · confidence 0.70 C.D. Dowell
  • 0907.3786 #6 · backfill · confidence 0.70 C.D. Dowell
  • 0905.1240 #7 · backfill · confidence 0.70 C.D. Dowell

Frequent Coauthors