LiteBIRD is a future satellite mission designed to observe the polarization of the cosmic microwave background radiation in order to probe the inflationary universe. LiteBIRD is set to observe the sky using three telescopes with transition-edge sensor bolometers. In this work we estimated the LiteBIRD instrumental sensitivity using its current design. We estimated the detector noise due to the optical loadings using physical optics and ray-tracing simulations. The noise terms associated with thermal carrier and readout noise were modeled in the detector noise calculation. We calculated the observational sensitivities over fifteen bands designed for the LiteBIRD telescopes using assumed observation time efficiency.

Hasebe, T., Ade, P., Adler, A., Allys, E., Alonso, D., Arnold, K., et al. (2022). Sensitivity modeling for LiteBIRD. JOURNAL OF LOW TEMPERATURE PHYSICS [10.1007/s10909-022-02921-7].

Sensitivity modeling for LiteBIRD

Migliaccio M.;Vittorio N.;
2022-01-01

Abstract

LiteBIRD is a future satellite mission designed to observe the polarization of the cosmic microwave background radiation in order to probe the inflationary universe. LiteBIRD is set to observe the sky using three telescopes with transition-edge sensor bolometers. In this work we estimated the LiteBIRD instrumental sensitivity using its current design. We estimated the detector noise due to the optical loadings using physical optics and ray-tracing simulations. The noise terms associated with thermal carrier and readout noise were modeled in the detector noise calculation. We calculated the observational sensitivities over fifteen bands designed for the LiteBIRD telescopes using assumed observation time efficiency.
2022
Pubblicato
Rilevanza internazionale
Articolo
Sì, ma tipo non specificato
Settore FIS/05 - ASTRONOMIA E ASTROFISICA
English
Astronomy; CMB; Cosmology; Detector noise; Satellite; Sensitivity
Hasebe, T., Ade, P., Adler, A., Allys, E., Alonso, D., Arnold, K., et al. (2022). Sensitivity modeling for LiteBIRD. JOURNAL OF LOW TEMPERATURE PHYSICS [10.1007/s10909-022-02921-7].
Hasebe, T; Ade, Par; Adler, A; Allys, E; Alonso, D; Arnold, K; Auguste, D; Aumont, J; Aurlien, R; Austermann, J; Azzoni, S; Baccigalupi, C; Banday, Aj; Banerji, R; Barreiro, Rb; Bartolo, N; Basak, S; Battistelli, E; Bautista, L; Beall, J; Beck, D; Beckman, S; Benabed, K; Bermejo-Ballesteros, J; Bersanelli, M; Bonis, J; Borrill, J; Bouchet, F; Boulanger, F; Bounissou, S; Brilenkov, M; Brown, Ml; Bucher, M; Calabrese, E; Calvo, M; Campeti, P; Carones, A; Casas, Fj; Catalano, A; Challinor, A; Chan, V; Cheung, K; Chinone, Y; Cliche, J; Columbro, F; Coulton, W; Cubas, J; Cukierman, A; Curtis, D; D'Alessandro, G; Dachlythra, K; de Bernardis, P; de Haan, T; dela Hoz, E; De Petris, M; Torre, Sd; Dickinson, C; Diego-Palazuelos, P; Dobbs, M; Dotani, T; Douillet, D; Duband, L; Ducout, A; Duff, S; Duval, Jm; Ebisawa, K; Elleflot, T; Eriksen, Hk; Errard, J; Essinger-Hileman, T; Finelli, F; Flauger, R; Franceschet, C; Fuskeland, U; Galli, S; Galloway, M; Ganga, K; Gao, Jr; Genova-Santos, Rt; Gerbino, M; Gervasi, M; Ghigna, T; Giardiello, S; Gjerlow, E; Gradziel, Ml; Grain, J; Grandsire, L; Grupp, F; Gruppuso, A; Gudmundsson, Je; Halverson, Nw; Hamilton, J; Hargrave, P; Hasegawa, M; Hattori, M; Hazumi, M; Henrot-Versille, S; Hergt, Lt; Herman, D; Herranz, D; Hill, Ca; Hilton, G; Hivon, E; Hlozek, Ra; Hoang, Td; Hornsby, Al; Hoshino, Y; Hubmayr, J; Ichiki, K; Iida, T; Imada, H; Ishimura, K; Ishino, H; Jaehnig, G; Jones, M; Kaga, T; Kashima, S; Katayama, N; Kato, A; Kawasaki, T; Keskitalo, R; Kisner, T; Kobayashi, Y; Kogiso, N; Kogut, A; Kohri, K; Komatsu, E; Komatsu, K; Konishi, K; Krachmalnicoff, N; Kreykenbohm, I; Kuo, Cl; Kushino, A; Lamagna, L; Lanen, Jv; Laquaniello, G; Lattanzi, M; Lee, At; Leloup, C; Levrier, F; Linder, E; Louis, T; Luzzi, G; Macias-Perez, J; Maciaszek, T; Maffei, B; Maino, D; Maki, M; Mandelli, S; Maris, M; Martinez-Gonzalez, E; Masi, S; Massa, M; Matarrese, S; Matsuda, Ft; Matsumura, T; Mele, L; Mennella, A; Migliaccio, M; Minami, Y; Mitsuda, K; Moggi, A; Monfardini, A; Montgomery, J; Montier, L; Morgante, G; Mot, B; Murata, Y; Murphy, Ja; Nagai, M; Nagano, Y; Nagasaki, T; Nagata, R; Nakamura, S; Nakano, R; Namikawa, T; Nati, F; Natoli, P; Nerval, S; Nishibori, T; Nishino, H; Noviello, F; O'Sullivan, C; Odagiri, K; Ogawa, H; Ogawa, H; Oguri, S; Ohsaki, H; Ohta, Is; Okada, N; Okada, N; Pagano, L; Paiella, A; Paoletti, D; Passerini, A; Patanchon, G; Pelgrim, V; Peloton, J; Piacentini, F; Piat, M; Pisano, G; Polenta, G; Poletti, D; Prouve, T; Puglisi, G; Rambaud, D; Raum, C; Realini, S; Reinecke, M; Remazeilles, M; Ritacco, A; Roudil, G; Rubino-Martin, J; Russell, M; Sakurai, H; Sakurai, Y; Sandri, M; Sasaki, M; Savini, G; Scott, D; Seibert, J; Sekimoto, Y; Sherwin, B; Shinozaki, K; Shiraishi, M; Shirron, P; Signorelli, G; Smecher, G; Spinella, F; Stever, S; Stompor, R; Sugiyama, S; Sullivan, R; Suzuki, A; Suzuki, J; Svalheim, Tl; Switzer, E; Takaku, R; Takakura, H; Takakura, S; Takase, Y; Takeda, Y; Tartari, A; Tavagnacco, D; Taylor, A; Taylor, E; Terao, Y; Thermeau, J; Thommesen, H; Thompson, Kl; Thorne, B; Toda, T; Tomasi, M; Tominaga, M; Trappe, N; Tristram, M; Tsuji, M; Tsujimoto, M; Tucker, C; Ullom, J; Vacher, L; Vermeulen, G; Vielva, P; Villa, F; Vissers, M; Vittorio, N; Wandelt, B; Wang, W; Watanuki, K; Wehus, Ik; Weller, J; Westbrook, B; Wilms, J; Winter, B; Wollack, Ej; Yamasaki, Ny; Yoshida, T; Yumoto, J; Zacchei, A; Zannoni, M; Zonca, A
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2108/316910
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