Zobrazeno 1 - 10
of 44
pro vyhledávání: '"Francesco De Bernardis"'
Autor:
Laura Newburgh, Edward J. Wollack, Kavilan Moodley, Arthur Kosowsky, Blake D. Sherwin, Suzanne T. Staggs, Michael D. Niemack, Alexander van Engelen, Jeff McMahon, Thibaut Louis, Renée Hlozek, Mark J. Devlin, Joanna Dunkley, Patricio A. Gallardo, David N. Spergel, Rupert Allison, Erminia Calabrese, Shawn W. Henderson, J. Richard Bond, Bruce Partridge, Lyman A. Page, Sam N. Lindsay, Francesco De Bernardis, Sigurd Naess, Matt J. Jarvis, Mathew S. Madhavacheril, Adam D. Hincks, Neelima Sehgal
Publikováno v:
Monthly Notices Of The Royal Astronomical Society
Artículos CONICYT
CONICYT Chile
instacron:CONICYT
Artículos CONICYT
CONICYT Chile
instacron:CONICYT
We correlate the positions of radio galaxies in the FIRST survey with the CMB lensing convergence estimated from the Atacama Cosmology Telescope over 470 square degrees to determine the bias of these galaxies. We remove optically cross-matched source
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1a28219747cde5f8de28245e839b0955
https://doi.org/10.1093/mnras/stv991
https://doi.org/10.1093/mnras/stv991
Autor:
Renée Hložek, Laura Newburgh, Kavilan Moodley, Arthur Kosowsky, J. Richard Bond, Suzanne T. Staggs, Thibaut Louis, J. Colin Hill, David N. Spergel, Edward J. Wollack, Shawn W. Henderson, Bruce Partridge, Jeff McMahon, Jonathan Sievers, Neelima Sehgal, Erminia Calabrese, Francesco De Bernardis, Amir Hajian, Hy Trac, Mark J. Devlin, Lyman A. Page, Nick Battaglia, Eric R. Switzer, Michael D. Niemack
Future arcminute resolution polarization data from ground-based Cosmic Microwave Background (CMB) observations can be used to estimate the contribution to the temperature power spectrum from the primary anisotropies and to uncover the signature of re
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cf05f8e7bc27b0fbb971310114b6077f
https://ora.ox.ac.uk/objects/uuid:561a08f3-4150-4dbb-b74e-03626ab1bbbe
https://ora.ox.ac.uk/objects/uuid:561a08f3-4150-4dbb-b74e-03626ab1bbbe
Autor:
Katherine N. Quinn, Francesco De Bernardis, James P. Sethna, Colin B. Clement, Michael D. Niemack
Publikováno v:
Proceedings of the National Academy of Sciences of the United States of America. 116(28)
Unsupervised learning makes manifest the underlying structure of data without curated training and specific problem definitions. However, the inference of relationships between data points is frustrated by the “curse of dimensionality” in high di
Autor:
Johannes Hubmayr, Francesco De Bernardis, Christopher Groppi, Enzo Pascale, Seth Hillbrand, Douglas Scott, Jeff McMahon, Giampaolo Pisano, Michael D. Niemack, Giles Novak, Juan D. Soler, Peter A. R. Ade, Shawn W. Henderson, Sean Bryan, Mark J. Devlin, Marc-Antoine Miville-Deschênes, Stephen Anthony Eales, Philip Daniel Mauskopf, Carole Tucker, Haley Louise Gomez, Joanna Dunkley, Francois Boulanger
Publikováno v:
Journal of Low Temperature Physics
The B-mode Foreground Experiment (BFORE) is a proposed NASA balloon project designed to make optimal use of the sub-orbital platform by concentrating on three dust foreground bands (270, 350, and 600 GHz) that complement ground-based cosmic microwave
Autor:
Brian J. Koopman, Jeff McMahon, Kavilan Moodley, Joanna Dunkley, Felipe Menanteau, David N. Spergel, Simon Muya Kasanda, Jesse Treu, Graeme E. Addison, J. Richard Bond, Shawn W. Henderson, Sara M. Simon, Simone Aiola, John P. Hughes, Matt Hilton, Joseph W. Britton, Alexander van Engelen, Tobias A. Marriage, Jonathan T. Ward, Robert Thornton, Michael R. Nolta, Christine G. Pappas, Rahul Datta, Peter A. R. Ade, Gene C. Hilton, Jeff Klein, Nicholas Battaglia, Mathew S. Madhavacheril, Matthew Hasselfield, Arthur Kosowsky, Benjamin L. Schmitt, Devin Crichton, Charles Munson, Thibaut Louis, Zhiqi Huang, Erminia Calabrese, Kevin Coughlin, Francesco De Bernardis, Neelima Sehgal, Megan Gralla, Kent D. Irwin, Hsiao-Mei Cho, J. Colin Hill, Edward J. Wollack, Michael D. Niemack, Steve K. Choi, Loïc Maurin, Lyman A. Page, Suzanne T. Staggs, S. P. Patty Ho, Federico Nati, Mandana Amiri, Kevin M. Huffenberger, Emmanuel Schaan, Johannes Hubmayr, Eric R. Switzer, Elio Angile, Mark Halpern, Simone Ferraro, James A. Beall, Kevin T. Crowley, Hy Trac, Mark J. Devlin, Patricio A. Gallardo, R. Allison, Simon Dicker, Sigurd Naess, Leopoldo Infante, Laura Newburgh, Dale Li, Adam D. Hincks, Carole Tucker, Bruce Partridge, Anna E. Fox, Jon Sievers, Renée Hlozek, E. Grace, Felipe Rojas, Rolando Dünner, John P. Nibarger, Marius Lungu, Carolina Núñez, Blake D. Sherwin
Publikováno v:
JCAP
JCAP, 2017, 06 (06), pp.031. 〈10.1088/1475-7516/2017/06/031〉
JCAP, 2017, 06, pp.031. ⟨10.1088/1475-7516/2017/06/031⟩
Journal of Cosmology and Astroparticle Physics, vol 2017, iss 6
NASA Astrophysics Data System
Journal of Cosmology and Astroparticle Physics, vol 2017, iss 06
Journal of Cosmology and Astroparticle Physics
Artículos CONICYT
CONICYT Chile
instacron:CONICYT
JCAP, 2017, 06 (06), pp.031. 〈10.1088/1475-7516/2017/06/031〉
JCAP, 2017, 06, pp.031. ⟨10.1088/1475-7516/2017/06/031⟩
Journal of Cosmology and Astroparticle Physics, vol 2017, iss 6
NASA Astrophysics Data System
Journal of Cosmology and Astroparticle Physics, vol 2017, iss 06
Journal of Cosmology and Astroparticle Physics
Artículos CONICYT
CONICYT Chile
instacron:CONICYT
We present the temperature and polarization angular power spectra measured by the Atacama Cosmology Telescope Polarimeter (ACTPol). We analyze night-time data collected during 2013-14 using two detector arrays at 149 GHz, from 548 deg$^2$ of sky on t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b0613dfc311ba3fabc5b75891e4adc6c
https://hal.archives-ouvertes.fr/hal-01554436
https://hal.archives-ouvertes.fr/hal-01554436
Autor:
Nicholas Battaglia, Daniel Green, Kam Arnold, Blake D. Sherwin, Joaquin Vieira, Tijmen de Haan, Marilena LoVerde, M. Lilley, Marco Peloso, Raphael Flauger, John M Kovac, Josquin Errard, Scott Watson, Cora Dvorkin, Tristan L. Smith, Stephen M. Feeney, P. D. Meerburg, Sperello di Serego Alighieri, Akito Kusaka, J. Colin Hill, Glenn D. Starkman, Zeeshan Ahmed, W. L. Holzapfel, George M. Fuller, Julian B. Muñoz, Maude Le Jeune, Chao-Lin Kuo, Nathan Whitehorn, Adam Mantz, Reijo Keskitalo, Marcel Schmittfull, Christian L. Reichardt, Julian Borrill, Victor Buza, Michael D. Niemack, Emmanuel Schaan, Giulio Fabbian, Simone Ferraro, T. M. Crawford, Lorenzo Sorbo, Mathew S. Madhavacheril, Jeff McMahon, Ely D. Kovetz, Kevork N. Abazajian, James G. Bartlett, Jason W. Henning, Lloyd Knox, Evan Grohs, J. Peloton, K. T. Story, Robert R. Caldwell, Erminia Calabrese, Francesco De Bernardis, Wayne Hu, Steven W. Allen, Levon Pogosian, Sarah Shandera, David J. E. Marsh, Amber Miller, Joel Meyers, Arthur Kosowsky, John E. Carlstrom, Carlo Baccigalupi, Joanna Dunkley, Kevin M. Huffenberger, C. Pryke, Jeffrey P. Filippini, Alexander van Engelen, Francis-Yan Cyr-Racine, Bradford Benson, Marco Raveri, Daniel Grin, Colin A. Bischoff, Ho Nam Nguyen, Neelima Sehgal, Aditya Rotti, C. L. Chang, Vera Gluscevic, Douglas Scott, W. L. Kimmy Wu, David Alonso, Adrian T. Lee, Renée Hlozek, Graca Rocha, Peter Adshead, Gilbert Holder
This book lays out the scientific goals to be addressed by the next-generation ground-based cosmic microwave background experiment, CMB-S4, envisioned to consist of dedicated telescopes at the South Pole, the high Chilean Atacama plateau and possibly
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0c3355cd5448743e76305fa52aa7ea5e
https://doi.org/10.2172/1352047
https://doi.org/10.2172/1352047
Autor:
Simone Aiola, Mathew S. Madhavacheril, Benjamin L. Schmitt, Matthew Hasselfield, Neelima Sehgal, J. Colin Hill, Loïc Maurin, Kent D. Irwin, Suzanne T. Staggs, Edward J. Wollack, Kavilan Moodley, M. Lungu, Michael D. Niemack, Bruce Partridge, Laura Newburgh, J. Richard Bond, Brian J. Koopman, Jeff McMahon, Jonathan Sievers, Dale Li, Francesco De Bernardis, Hsiao-Mei Cho, David N. Spergel, Sigurd Naess, Thibaut Louis, Adam D. Hincks, Mariana Vargas-Magaña, Arthur Kosowsky, Shawn W. Henderson, Christine G. Pappas, Erminia Calabrese, Lyman A. Page, John P. Hughes, Emmanuel Schaan, Johannes Hubmayr, Simone Ferraro, Mark J. Devlin, Patricio A. Gallardo, Nicholas Battaglia, Federico Nati, Shirley Ho, Blake D. Sherwin, Joanna Dunkley, Alexander van Engelen, Renée Hlozek, Kendrick M. Smith
Publikováno v:
Physical Review D, vol 93, iss 8
Physical Review D
Artículos CONICYT
CONICYT Chile
instacron:CONICYT
Schaan, E; Ferraro, S; Vargas-Magaña, M; Smith, KM; Ho, S; Aiola, S; et al.(2016). Evidence for the kinematic Sunyaev-Zel'dovich effect with the Atacama Cosmology Telescope and velocity reconstruction from the Baryon Oscillation Spectroscopic Survey. Physical Review D, 93(8). doi: 10.1103/PhysRevD.93.082002. Lawrence Berkeley National Laboratory: Retrieved from: http://www.escholarship.org/uc/item/8qc073zh
Physical Review D
Artículos CONICYT
CONICYT Chile
instacron:CONICYT
Schaan, E; Ferraro, S; Vargas-Magaña, M; Smith, KM; Ho, S; Aiola, S; et al.(2016). Evidence for the kinematic Sunyaev-Zel'dovich effect with the Atacama Cosmology Telescope and velocity reconstruction from the Baryon Oscillation Spectroscopic Survey. Physical Review D, 93(8). doi: 10.1103/PhysRevD.93.082002. Lawrence Berkeley National Laboratory: Retrieved from: http://www.escholarship.org/uc/item/8qc073zh
Author(s): Schaan, E; Ferraro, S; Vargas-Magana, M; Smith, KM; Ho, S; Aiola, S; Battaglia, N; Bond, JR; De Bernardis, F; Calabrese, E; Cho, HM; Devlin, MJ; Dunkley, J; Gallardo, PA; Hasselfield, M; Henderson, S; Hill, JC; Hincks, AD; Hlozek, R; Hubma
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fb2ef0407cea263b2a1a529d4b944215
https://escholarship.org/uc/item/8qc073zh
https://escholarship.org/uc/item/8qc073zh
Publikováno v:
International Journal of Modern Physics: Conference Series. 12:368-379
We place a nre upper limit on the sum of neutrino masses by using measurements of luminosity-dependent galaxy bias at several different redshifts, SDSS at z = 0.05, DEEP2 at z = 1 and LBGs at z = 3.8, combined with WMAP five-year cosmic microwave bac
Publikováno v:
Journal of Cosmology and Astroparticle Physics. 2018:032-032
Galaxy cluster velocity correlations and mass distributions are sensitive probes of cosmology and the growth of structure. Upcoming microwave surveys will enable extraction of velocities and temperatures from many individual clusters for the first ti
Autor:
Francesco De Bernardis
Publikováno v:
Nuclear Physics B - Proceedings Supplements. 194:39-44
We report new constraints on the reheating temperature of the Universe by analyzing the Cosmic Microwave Background data from the WMAP five year survey. From WMAP-5 data alone we found an upper limit at 95% c.l. of T r e > 2 M e V , while including e