Zobrazeno 1 - 10
of 1 133
pro vyhledávání: '"Cosmic infrared background"'
Autor:
Kirit Karkare, Ely D. Kovetz, Jacques Delabrouille, Matthieu Béthermin, Garrett K. Keating, M. B. Silva, Azadeh Moradinezhad Dizgah, Patrick C. Breysse, José Luis Bernal
Publikováno v:
INSPIRE-HEP
Exper.Astron.
Exper.Astron., 2021, 51 (3), pp.1593-1622. ⟨10.1007/s10686-021-09755-3⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Exper.Astron.
Exper.Astron., 2021, 51 (3), pp.1593-1622. ⟨10.1007/s10686-021-09755-3⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
This paper outlines the science case for line-intensity mapping with a space-borne instrument targeting the sub-millimeter (microwaves) to the far-infrared (FIR) wavelength range. Our goal is to observe and characterize the large-scale structure in t
Publikováno v:
Astronomy Letters. 46:298-311
Sensitivity of future far infrared 10m class space telescopes will be limited by a confusion noise created by distant galaxies. Our primary goal is to create a model that will allow us to estimate the confusion noise parameters of the Millimetron mis
Autor:
H. Ikeda, Satoru Mima, G. Maekawa, Koichi Nagase, Rena Wakasa, S. H. Kim, Go Fujii, S. Nakahara, C. Asano, Kenji Kiuchi, Erik Ramberg, Takashi Iida, Ikuo Kurachi, S.B. Kim, H.J. Lee, Dmitri Sergatskov, Y.H. Kim, T. Yoshida, A. Kibayashi, R. Yamane, Shuji Matsuura, Shigetomo Shiki, Masataka Ohkubo, Masashi Hazumi, Yoshio Arai, Shoji Kawahito, P. Rubinov, Hirokazu Ishino, T. Wada, Y. Kato, Masahiro Ukibe, Y. Takeuchi
Publikováno v:
2021 International Symposium on VLSI Technology, Systems and Applications (VLSI-TSA).
The COBAND is a project of an experimental search for the cosmic background neutrino decay [1] – [9] . The existence of the cosmic background neutrino is predicted as a relic of the big bang in the theoretical cosmology. Since the neutrino is found
Publikováno v:
Physical Review D. 103
The cosmic microwave background (CMB) is gravitationally lensed by large-scale structure, which distorts observations of the primordial anisotropies in any given direction. Averaged over the sky, this important effect is routinely modelled with the l
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2021, 645, pp.A40. ⟨10.1051/0004-6361/202038790⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 645, pp.A40. ⟨10.1051/0004-6361/202038790⟩
Astronomy & Astrophysics
Astronomy and Astrophysics-A&A, 2021, 645, pp.A40. ⟨10.1051/0004-6361/202038790⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 645, pp.A40. ⟨10.1051/0004-6361/202038790⟩
Astronomy & Astrophysics
Modelling the anisotropies in the CIB on all the scales is a challenging task due to the complex nature of the galaxy evolution and thus often requires too many parameters in order to fit the observational data. In this paper, we present a new halo m
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a550112a0a96cfdf162ee84c46cf556a
https://hal.science/hal-02905907
https://hal.science/hal-02905907
Autor:
Kei Sano, Kenta Danbayashi, Shuji Matsuura, Michael Zemcov, Alicia Lanz, Phillip Korngut, Dorin Patru, Kohji Tsumura, Peter Mason, Jodi-Ann Morgan, Aoi Takahashi, Seung-Cheol Bang, Kevin Gates, Yasuhiro Yamada, Dae-Hee Lee, Kohji Takimoto, Arisa Kida, James J. Bock, Chi H. Nguyen, Ryo Hashimoto, Priyadarshini Bangale, Takehiko Wada, Masaki Furutani, Richard M. Feder, Sohta Tatsu, Hiroko Suzuki, James Parkus, Asantha Cooray, Shohta Sakai, Lunjun Liu, Shiang-Yu Wang, Won-Kee Park, Toshio Matsumoto, Viktor Hristov
Publikováno v:
Space Telescopes and Instrumentation 2020: Optical, Infrared, and Millimeter Wave.
The total integrated emission from galaxies, known as the Extragalactic Background Light (EBL), is an important observable for understanding the history of star formation over the history of the universe. Spatial fluctuations in the infrared EBL as m
Autor:
Ioana A. Zelko, Douglas P. Finkbeiner
Spectral distortions of the cosmic microwave background (CMB) are sensitive to energy injection by exotic physics in the early universe. The proposed Primordial Inflation Explorer (PIXIE) mission has the raw sensitivity to provide meaningful limits o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::72b24b66875a801d46dfa3329c6eae13
http://arxiv.org/abs/2010.06589
http://arxiv.org/abs/2010.06589
Autor:
Simone Aiola, Michael D. Niemack, Federico Nati, C. Sifon, Brian J. Koopman, Kavilan Moodley, Victoria Calafut, Graeme E. Addison, Jeff McMahon, Matthew Hasselfield, Matt Hilton, Arthur Kosowsky, Nicholas Battaglia, Erminia Calabrese, Alexander van Engelen, Edward J. Wollack, David N. Spergel, Marius Lungu, Joanna Dunkley, J. Richard Bond, Renée Hložek, Alessandro Schillaci, Suzanne T. Staggs, Eve M. Vavagiakis, Kevin M. Huffenberger, Shuay-Pwu Patty Ho, Emmanuel Schaan, Mark Halpern, Simone Ferraro, Vera Gluscevic, Mark J. Devlin, Mathew S. Madhavacheril, Patricio A. Gallardo, Thibaut Louis, Zhilei Xu, Taylor Baildon, Neelima Sehgal, Steve K. Choi, Bruce Partridge, Amanda MacInnis, Lyman A. Page, Loïc Maurin, J. Colin Hill, Naomi Robertson, Blake D. Sherwin, Rachel Bean, Emilie R. Storer, Sigurd Naess, Adam D. Hincks, Rahul Datta, Dongwon Han, Martine Lokken, John P. Hughes, Omar Darwish, Rolando Dünner, Sara M. Simon
Publikováno v:
Phys.Rev.D
Phys.Rev.D, 2020, 102 (2), pp.023534. ⟨10.1103/PhysRevD.102.023534⟩
Physical Review D, vol 102, iss 2
Phys.Rev.D, 2020, 102 (2), pp.023534. ⟨10.1103/PhysRevD.102.023534⟩
Physical Review D, vol 102, iss 2
Optimal analyses of many signals in the cosmic microwave background (CMB) require map-level extraction of individual components in the microwave sky, rather than measurements at the power spectrum level alone. To date, nearly all map-level component
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5422286fb7aed21289c2ff29e98dbb18
https://orca.cardiff.ac.uk/id/eprint/134934/1/PhysRevD.102.023534.pdf
https://orca.cardiff.ac.uk/id/eprint/134934/1/PhysRevD.102.023534.pdf
Illuminating the dark ages: Cosmic backgrounds from accretion onto primordial black hole dark matter
Autor:
Guenther Hasinger
Cold dark matter as the sum of different mass Primordial Black Holes (PBH) can explain a number of unsolved astrophysical mysteries. Here I assume a broad PBH mass distribution providing the bulk of the dark matter, consistent with all constraints an
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::aeed8a7194b079be50c92cdecbd73fca
http://arxiv.org/abs/2003.05150
http://arxiv.org/abs/2003.05150
Autor:
Roger O'Brient, John M Kovac, Kirit Karkare, T. Natoli, Kent D. Irwin, A. E. Lowitz, N. Huang, Y. Omori, Victor Buza, Robert I. Citron, S. A. Kernasovskiy, W. L. Holzapfel, Ahmed Soliman, Jeff McMahon, C. Corbett Moran, P. A. R. Ade, Lingzhen Zeng, S. Henderson, W. B. Everett, J. D. Hrubes, Jessica Avva, C. Yu, Calvin B. Netterfield, Lorenzo Moncelsi, J. R. Cheshire, Jason W. Henning, J. A. Grayson, S. Patil, K. K. Schaffer, Elizabeth George, Abigail G. Vieregg, Denis Barkats, V. G. Yefremenko, Jason E. Austermann, N. W. Halverson, A. Cukierman, H. Boenish, B. L. Schmitt, Marion Dierickx, M. Crumrine, K. W. Yoon, Joaquin Vieira, E. Young, G. Hall, Stefan Richter, C. Sievers, Toshiya Namikawa, Graeme Smecher, C. Umilta, D. V. Wiebe, S. Fliescher, T.-L. Chou, H. C. Chiang, Johannes Hubmayr, H. Yang, C. D. Sheehy, Chao-Lin Kuo, Mark Halpern, Christian L. Reichardt, Marius Millea, Joshua Montgomery, S. Kefeli, J. Cornelison, J. J. Bock, Bryan Steinbach, Howard Hui, Gensheng Wang, Andreas Bender, Neil Goeckner-Wald, J. E. Ruhl, Dale Li, C. Tucker, K. G. Megerian, T. M. Crawford, M. A. Dobbs, Mandana Amiri, V. Novosad, R. Schwarz, S. Fatigoni, S. R. Hildebrandt, S. Padin, John E. Carlstrom, E. Bullock, Chao Zhang, T. de Haan, D. C. Goldfinger, John P. Nibarger, Andrew Nadolski, J. Willmert, Carl D. Reintsema, Gene C. Hilton, N. Whitehorn, B. Racine, H. T. Nguyen, A. A. Stark, E. M. Leitch, Alessandro Schillaci, A. D. Turner, E. Karpel, T. Veach, R. Basu Thakur, K. L. Thompson, T. Prouve, A. T. Crites, C. Pryke, C. L. Wong, C. L. Chang, J. Kang, Adam Anderson, Grant Teply, Benjamin Saliwanchik, A. Wandui, Gilbert Holder, A. Manzotti, A. C. Weber, G. I. Noble, Federico Bianchini, Nikhel Gupta, Jeffrey P. Filippini, R. V. Sudiwala, Adrian T. Lee, Bradford Benson, Lloyd Knox, W. L. K. Wu, Colin A. Bischoff, S. S. Meyer, Jason Gallicchio, T. St. Germaine, S. Palladino, L. Duband, J. E. Tolan, Zeeshan Ahmed, L. M. Mocanu, Jake Connors, Kei May Lau, Sarah M. Harrison, Lindsey Bleem, R. W. Ogburn, J. A. Beall
Publikováno v:
Physical Review D
Physical Review D, 2021, 103 (2), pp.022004. ⟨10.1103/PhysRevD.103.022004⟩
Phys.Rev.D
Phys.Rev.D, 2021, 103 (2), pp.022004. ⟨10.1103/PhysRevD.103.022004⟩
Physical Review D, 2021, 103 (2), pp.022004. ⟨10.1103/PhysRevD.103.022004⟩
Phys.Rev.D
Phys.Rev.D, 2021, 103 (2), pp.022004. ⟨10.1103/PhysRevD.103.022004⟩
We present a constraint on the tensor-to-scalar ratio, $r$, derived from measurements of cosmic microwave background (CMB) polarization $B$-modes with "delensing," whereby the uncertainty on $r$ contributed by the sample variance of the gravitational
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::900b9b3521182a6f974e784c4523d6f9