Brendan P. Crill, Ph.D.
Affiliations: | 2001 | California Institute of Technology, Pasadena, CA |
Area:
cosmic microwave backgroundGoogle:
"Brendan Crill"Mean distance: 14.8 | S | N | B | C | P |
Parents
Sign in to add mentor| Andrew Evan Lange | grad student | 2001 | Caltech | |
| (A measurement of the angular power spectrum of the cosmic microwave background with a long duration balloon -borne receiver.) | ||||
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Publications
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| Aghanim N, Polastri L, Rubiño-Martín JA, et al. (2020) Planck 2018 results. VI. Cosmological parameters Astronomy and Astrophysics. 641 |
| Aghanim N, Akrami Y, Alves MIR, et al. (2020) Planck 2018 results. XII. Galactic astrophysics using polarized dust emission Astronomy and Astrophysics. 641 |
| Aghanim N, Akrami Y, Ashdown M, et al. (2020) Planck 2018 results. III. High frequency instrument data processing and frequency maps Astronomy and Astrophysics. 641 |
| Tauber JA, Nielsen PH, Martín-Polegre A, et al. (2019) Characterization of the in-flight properties of the Planck telescope Astronomy & Astrophysics. 622: A55 |
| Ade PAR, Ahmed Z, Aikin RW, et al. (2018) Constraints on Primordial Gravitational Waves Using Planck, WMAP, and New BICEP2/Keck Observations through the 2015 Season. Physical Review Letters. 121: 221301 |
| Akrami Y, Arguëso F, Ashdown M, et al. (2018) Planck intermediate results LIV. The Planck multi-frequency catalogue of non-thermal sources Astronomy and Astrophysics. 619: 1-22 |
| Suzuki A, Ade PAR, Akiba Y, et al. (2018) The LiteBIRD Satellite Mission: Sub-Kelvin Instrument Journal of Low Temperature Physics. 193: 1048-1056 |
| Akrami Y, Ashdown M, Aumont J, et al. (2017) Planck intermediate results LII. Planet flux densities Astronomy and Astrophysics. 607: 1-20 |
| Aghanim N, Ashdown M, Aumont J, et al. (2017) Planck intermediate results L. Evidence of spatial variation of the polarized thermal dust spectral energy distribution and implications for CMB B-mode analysis Astronomy and Astrophysics. 599: 1-15 |
| Ade PA, Ahmed Z, Aikin RW, et al. (2016) Improved Constraints on Cosmology and Foregrounds from BICEP2 and Keck Array Cosmic Microwave Background Data with Inclusion of 95 GHz Band. Physical Review Letters. 116: 031302 |