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B.P. Crill

Identifiers

  • name variant B.P. Crill 0.60 · backfill

Papers (30)

  1. Attitude determination for balloon-borne experiments astro-ph.IM · 2014 · author #11
  2. Impact of particles on the Planck HFI detectors: Ground-based measurements and physical interpretation astro-ph.IM · 2014 · author #10
  3. Inflation Physics from the Cosmic Microwave Background and Large Scale Structure astro-ph.CO · 2013 · author #19
  4. SPIDER: a balloon-borne CMB polarimeter for large angular scales astro-ph.CO · 2011 · author #13
  5. Planck early results. IX. XMM-Newton follow-up for validation of Planck cluster candidates astro-ph.CO · 2011 · author #42
  6. Planck early results XIV: ERCSC validation and extreme radio sources astro-ph.CO · 2011 · author #40
  7. Measuring Planck beams with planets astro-ph.CO · 2010 · author #2
  8. Searching for non Gaussian signals in the BOOMERanG 2003 CMB maps astro-ph · 2007 · author #9
  9. Maps of the millimetre sky from the BOOMERanG experiment astro-ph · 2003 · author #10
  10. Measuring CMB Polarization with BOOMERANG astro-ph · 2003 · author #10
  11. Observations of Galactic and Extra-galactic Sources From the BOOMERANG and SEST Telescopes astro-ph · 2003 · author #8
  12. The trispectrum of the Cosmic Microwave Background on sub-degree angular scales: an analysis of the BOOMERanG data astro-ph · 2003 · author #7
  13. Ellipticity analysis of the BOOMERanG CMB maps astro-ph · 2002 · author #7
  14. BOOMERANG: A Balloon-borne Millimeter Wave Telescope and Total Power Receiver for Mapping Anisotropy in the Cosmic Microwave Background astro-ph · 2002 · author #1
  15. The BOOMERanG experiment and the curvature of the Universe astro-ph · 2002 · author #9
  16. Search for non-gaussian signals in the BOOMERanG maps: pixel-space analysis astro-ph · 2002 · author #8
  17. Multiple Peaks in the Angular Power Spectrum of the Cosmic Microwave Background: Significance and Consequences for Cosmology astro-ph · 2001 · author #9
  18. The BOOMERANG North America Instrument: a balloon-borne bolometric radiometer optimized for measurements of cosmic background radiation anisotropies from 0.3 to 4 degrees astro-ph · 2001 · author #7
  19. A measurement by BOOMERANG of multiple peaks in the angular power spectrum of the cosmic microwave background astro-ph · 2001 · author #9
  20. High latitude Galactic dust emission in the BOOMERanG maps astro-ph · 2001 · author #5
  21. Noise estimation in CMB time-streams and fast map-making. Application to the BOOMERanG98 data astro-ph · 2001 · author #8
  22. Foregrounds in the BOOMERANG-LDB data: a preliminary rms analysis astro-ph · 2000 · author #5
  23. First results from the BOOMERanG experiment astro-ph · 2000 · author #8
  24. Detection of anisotropy in the Cosmic Microwave Background at horizon and sub-horizon scales with the BOOMERanG experiment astro-ph · 2000 · author #8
  25. Cosmology from Maxima-1, Boomerang and COBE/DMR CMB Observations astro-ph · 2000 · author #9
  26. Iterative map-making for scanning experiments astro-ph · 2000 · author #4
  27. First Estimations of Cosmological Parameters From BOOMERANG astro-ph · 2000 · author #8
  28. BOOMERanG: a scanning telescope for 10 arcminutes resolution CMB maps astro-ph · 1999 · author #6
  29. Measurement of a Peak in the Cosmic Microwave Background Power Spectrum from the North American test flight of BOOMERANG astro-ph · 1999 · author #7
  30. A measurement of Omega from the North American test flight of BOOMERANG astro-ph · 1999 · author #7

Mentions

  • 1407.1883 #11 · backfill · confidence 0.70 B.P. Crill
  • 1403.6592 #10 · backfill · confidence 0.70 B.P. Crill
  • 1309.5381 #19 · backfill · confidence 0.70 B.P. Crill
  • 1106.2158 #13 · backfill · confidence 0.70 B.P. Crill
  • 1101.2025 #42 · backfill · confidence 0.70 B.P. Crill
  • 1101.1721 #40 · backfill · confidence 0.70 B.P. Crill
  • 1007.3468 #2 · backfill · confidence 0.70 B.P. Crill
  • 0705.1615 #9 · backfill · confidence 0.70 B.P. Crill

Frequent Coauthors