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Calvin B. Netterfield

Identifiers

  • name variant Calvin B. Netterfield 0.60 · backfill

Papers (32)

  1. Submillimeter Polarization Spectrum of the Carina Nebula astro-ph.GA · 2018 · author #19
  2. Relative Alignment Between the Magnetic Field and Molecular Gas Structure in the Vela C Giant Molecular Cloud using Low and High Density Tracers astro-ph.GA · 2018 · author #26
  3. First Observation of the Submillimeter Polarization Spectrum in a Translucent Molecular Cloud astro-ph.GA · 2017 · author #18
  4. Comparing submillimeter polarized emission with near-infrared polarization of background stars for the Vela C molecular cloud astro-ph.GA · 2016 · author #19
  5. Submillimeter Polarization Spectrum in the Vela C Molecular Cloud astro-ph.IM · 2015 · author #18
  6. Lupus I Observations from the 2010 Flight of the Balloon-borne Large Aperture Submillimeter Telescope for Polarimetry astro-ph.GA · 2013 · author #17
  7. The Atacama Cosmology Telescope: Data Characterization and Map Making astro-ph.IM · 2012 · author #54
  8. Evidence for Environmental Changes in the Submillimeter Dust Opacity astro-ph.GA · 2011 · author #18
  9. Correlations in the (Sub)millimeter background from ACTxBLAST astro-ph.CO · 2011 · author #32
  10. Deconvolution of Images from BLAST 2005: Insight into the K3-50 and IC 5146 Star-Forming Regions astro-ph.GA · 2010 · author #19
  11. The Atacama Cosmology Telescope: Cosmology from Galaxy Clusters Detected via the Sunyaev-Zel'dovich Effect astro-ph.CO · 2010 · author #52
  12. The Balloon-Borne Large Aperture Submillimeter Telescope (BLAST) 2005: A 10 deg^2 Survey of Star Formation in Cygnus X astro-ph.GA · 2010 · author #19
  13. The BLAST View of the Star Forming Region in Aquila (ell=45deg,b=0deg) astro-ph.GA · 2010 · author #16
  14. The Atacama Cosmology Telescope: A Measurement of the Cosmic Microwave Background Power Spectrum at 148 and 218 GHz from the 2008 Southern Survey astro-ph.CO · 2010 · author #48
  15. The Atacama Cosmology Telescope: Calibration with WMAP Using Cross-Correlations astro-ph.CO · 2010 · author #48
  16. Measuring star formation in high-z massive galaxies: A mid-infrared to submillimeter study of the GOODS NICMOS Survey sample astro-ph.CO · 2010 · author #11
  17. A panchromatic study of BLAST counterparts: total star-formation rate, morphology, AGN fraction and stellar mass astro-ph.CO · 2010 · author #13
  18. A joint analysis of BLAST 250--500um and LABOCA 870um observations in the Extended Chandra Deep Field South astro-ph.CO · 2010 · author #13
  19. Submillimetre observations of galaxy clusters with BLAST: the star-formation activity in Abell 3112 astro-ph.CO · 2010 · author #16
  20. The BLAST Survey of the Vela Molecular Cloud: Physical Properties of the Dense Cores in Vela-D astro-ph.GA · 2009 · author #24
  21. BLAST: the far-infrared/radio correlation in distant galaxies astro-ph.CO · 2009 · author #19
  22. BLAST05: Power Spectra of Bright Galactic Cirrus at Submillimeter Wavelengths astro-ph.GA · 2009 · author #17
  23. Temperature Profiles and the Effect of AGN on Submillimeter Emission from BLAST Observations of Resolved Galaxies astro-ph.GA · 2009 · author #16
  24. BLAST: the Redshift Survey astro-ph.CO · 2009 · author #10
  25. Submillimeter Number Counts From Statistical Analysis of BLAST Maps astro-ph.CO · 2009 · author #16
  26. A Bright Submillimeter Source in the Bullet Cluster (1E0657--56) Field Detected with BLAST astro-ph.CO · 2009 · author #18
  27. BLAST: A Far-Infrared Measurement of the History of Star Formation astro-ph.CO · 2009 · author #17
  28. BLAST: Resolving the Cosmic Submillimeter Background astro-ph.CO · 2009 · author #16
  29. BLAST: Correlations in the Cosmic Far-Infrared Background at 250, 350, and 500 microns Reveal Clustering of Star-Forming Galaxies astro-ph.CO · 2009 · author #18
  30. Radio and mid-infrared identification of BLAST source counterparts in the Chandra Deep Field South astro-ph.CO · 2009 · author #18
  31. The Balloon-borne Large Aperture Submillimeter Telescope (BLAST) 2006: Calibration and Flight Performance astro-ph.IM · 2009 · author #17
  32. Over half of the far-infrared background light comes from galaxies at z >= 1.2 astro-ph.CO · 2009 · author #16

Mentions

  • 1307.5853 #17 · backfill · confidence 0.70 Calvin B. Netterfield
  • 1208.0050 #54 · backfill · confidence 0.70 Calvin B. Netterfield
  • 1112.5433 #18 · backfill · confidence 0.70 Calvin B. Netterfield
  • 1101.1517 #32 · backfill · confidence 0.70 Calvin B. Netterfield
  • 1010.4605 #19 · backfill · confidence 0.70 Calvin B. Netterfield
  • 1010.1025 #52 · backfill · confidence 0.70 Calvin B. Netterfield
  • 1009.2972 #19 · backfill · confidence 0.70 Calvin B. Netterfield
  • 1009.1296 #16 · backfill · confidence 0.70 Calvin B. Netterfield
  • 1009.0847 #48 · backfill · confidence 0.70 Calvin B. Netterfield
  • 1009.0777 #48 · backfill · confidence 0.70 Calvin B. Netterfield
  • 1008.4359 #11 · backfill · confidence 0.70 Calvin B. Netterfield
  • 1008.1542 #13 · backfill · confidence 0.70 Calvin B. Netterfield
  • 1003.2647 #13 · backfill · confidence 0.70 Calvin B. Netterfield
  • 1003.2629 #16 · backfill · confidence 0.70 Calvin B. Netterfield
  • 0910.1097 #24 · backfill · confidence 0.70 Calvin B. Netterfield
  • 0910.1095 #17 · backfill · confidence 0.70 Calvin B. Netterfield
  • 0910.1091 #19 · backfill · confidence 0.70 Calvin B. Netterfield
  • 0907.4156 #10 · backfill · confidence 0.70 Calvin B. Netterfield
  • 0907.4154 #16 · backfill · confidence 0.70 Calvin B. Netterfield
  • 0906.0981 #16 · backfill · confidence 0.70 Calvin B. Netterfield
  • 0904.1206 #17 · backfill · confidence 0.70 Calvin B. Netterfield
  • 0904.1205 #16 · backfill · confidence 0.70 Calvin B. Netterfield
  • 0904.1204 #18 · backfill · confidence 0.70 Calvin B. Netterfield
  • 0904.1203 #18 · backfill · confidence 0.70 Calvin B. Netterfield
  • 0904.1202 #17 · backfill · confidence 0.70 Calvin B. Netterfield
  • 0904.1201 #16 · backfill · confidence 0.70 Calvin B. Netterfield
  • 0904.1200 #18 · backfill · confidence 0.70 Calvin B. Netterfield

Frequent Coauthors