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We present the temperature power spectrum of the Cosmic Microwave Background obtained by cross-correlating maps from the Atacama Cosmology Telescope (ACT) at 148 and 218 GHz with maps from the Planck satellite at 143 and 217 GHz, in two overlapping r...
Ade, P;Aguirre, J;Ahmed, Z;Aiola, S;Ali, A;Alonso, D;Alvarez, MA;Arnold, K;Ashton, P;Austermann, J;Awan, H;Baccigalupi, C;Baildon, T;Barron, D;Battaglia, N;Battye, R;Baxter, E;Bazarko, A;Beall, JA;Bean, R;Beck, D;Beckman, S;Beringue, B;Bianchini, F;Boada, S;Boettger, D;Bond, JR;Borrill, J;Brown, ML;Bruno, SM;Bryan, S;Calabrese, E;Calafut, V;Calisse, P;Carron, J;Challinor, A;Chesmore, G;Chinone, Y;Chluba, J;Cho, H-MS;Choi, S;Coppi, G;Cothard, NF;Coughlin, K;Crichton, D;Crowley, KD;Crowley, KT;Cukierman, A;D'Ewart, JM;Dunner, R;De Haan, T;Devlin, M;Dicker, S;Didier, J;Dobbs, M;Dober, B;Duell, CJ;Duff, S;Duivenvoorden, A;Dunkley, J;Dusatko, J;Errard, J;Fabbian, G;Feeney, S;Ferraro, S;Fluxa, P;Freese, K;Frisch, JC;Frolov, A;Fuller, G;Fuzia, B;Galitzki, N;Gallardo, PA;Ghersi, JTG;Gao, J;Gawiser, E;Gerbino, M;Gluscevic, V;Goeckner-Wald, N;Golec, J;Gordon, S;Gralla, M;Green, D;Grigorian, A;Groh, J;Groppi, C;Guan, Y;Gudmundsson, JE;Han, D;Hargrave, P;Hasegawa, M;Hasselfield, M;Hattori, M;Haynes, V;Hazumi, M;He, Y;Healy, E;Henderson, SW;Hervias-Caimapo, C;Hill, CA;Hill, JC;Hilton, G;Hilton, M;Hincks, AD;Hinshaw, G;Hlozek, R;Ho, S;Ho, S-PP;Howe, L;Huang, Z;Hubmayr, J;Huffenberger, K;Hughes, JP;Ijjas, A;Ikape, M;Irwin, K;Jaffe, AH;Jain, B;Jeong, O;Kaneko, D;Karpel, ED;Katayama, N;Keating, B;Kernasovskiy, SS;Keskitalo, R;Kisner, T;Kiuchi, K;Klein, J;Knowles, K;Koopman, B;Kosowsky, A;Krachmalnicoff, N;Kuenstner, SE;Kuo, C-L;Kusaka, A;Lashner, J;Lee, A;Lee, E;Leon, D;Leung, JS-Y;Lewis, A;Li, Y;Li, Z;Limon, M;Linder, E;Lopez-Caraballo, C;Louis, T;Lowry, L;Lungu, M;Madhavacheril, M;Mak, D;Maldonado, F;Mani, H;Mates, B;Matsuda, F;Maurin, L;Mauskopf, P;May, A;McCallum, N;McKenney, C;McMahon, J;Meerburg, PD;Meyers, J;Miller, A;Mirmelstein, M;Moodley, K;Munchmeyer, M;Munson, C;Naess, S;Nati, F;Navaroli, M;Newburgh, L;Nguyen, HN;Niemack, M;Nishino, H;Orlowski-Scherer, J;Page, L;Partridge, B;Peloton, J;Perrotta, F;Piccirillo, L;Pisano, G;Poletti, D;Puddu, R;Puglisi, G;Raum, C;Reichardt, CL;Remazeilles, M;Rephaeli, Y;Riechers, D;Rojas, F;Roy, A;Sadeh, S;Sakurail, Y;Salatino, M;Rao, MS;Schaan, E;Schmittfull, M;Sehgal, N;Seibert, J;Seljak, U;Sherwin, B;Shimon, M;Sierra, C;Sievers, J;Sikhosana, P;Silva-Feaver, M;Simon, SM;Sinclair, A;Siritanasak, P;Smith, K;Smith, SR;Spergel, D;Staggs, ST;Stein, G;Stevens, JR;Stompor, R;Suzuki, A;Tajima, O;Takakura, S;Teply, G;Thomas, DB;Thorne, B;Thornton, R;Trac, H;Tsai, C;Tucker, C;Ullom, J;Vagnozzi, S;Van Engelen, A;Van Lanen, J;Van Winkle, DD;Vavagiakis, EM;Verges, C;Vissers, M;Wagoner, K;Walker, S;Ward, J;Westbrook, B;Whitehorn, N;Williams, J;Williams, J;Wollack, EJ;Xu, Z;Yu, B;Yu, C;Zago, F;Zhang, H;Zhu, N;Simons Observatory Collaboration
© 2019 IOP Publishing Ltd and Sissa Medialab. The Simons Observatory (SO) is a new cosmic microwave background experiment being built on Cerro Toco in Chile, due to begin observations in the early 2020s. We describe the scientific goals of the experi...
The Atacama Cosmology Telescope has measured the angular power spectra of microwave fluctuations to arcminute scales at frequencies of 148 and 218 GHz, from three seasons of data. At small scales the fluctuations in the primordial Cosmic Microwave Ba...
We present the temperature power spectrum of the Cosmic Microwave Background obtained by cross-correlating maps from the Atacama Cosmology Telescope (ACT) at 148 and 218 GHz with maps from the Planck satellite at 143 and 217 GHz, in two overlapping r...
We present the temperature power spectra of the cosmic microwave background (CMB) derived from the three seasons of data from the Atacama Cosmology Telescope (ACT) at 148 GHz and 218 GHz, as well as the cross-frequency spectrum between the two channe...
We present the temperature power spectrum of the Cosmic Microwave Background obtained by cross-correlating maps from the Atacama Cosmology Telescope (ACT) at 148 and 218 GHz with maps from the Planck satellite at 143 and 217 GHz, in two overlapping r...
We present multi-wavelength detections of nine candidate gravitationally-lensed dusty starforming galaxies (DSFGs) selected at 218 GHz (1.4 mm) from the ACT equatorial survey. Among the brightest ACT sources, these represent the subset of the total A...
We present C I(21) and multi-transition C-12 O observations of a dusty star-forming galaxy, ACT J2029+0120,which we spectroscopically confirm to lie at zeta = 2.64. We detect CO(3-2), CO(5-4), CO(7-6), CO(8-7), and C I(2-1) at high significance, tent...
Mass calibration uncertainty is the largest systematic effect for using clustersof galaxies to constrain cosmological parameters. We present weak lensing mass measurements from the Canada-France-Hawaii Telescope Stripe 82 Survey for galaxy clusters s...
The Atacama Cosmology Telescope has measured the angular power spectra of microwave fluctuations to arcminute scales at frequencies of 148 and 218 GHz, from three seasons of data. At small scales the fluctuations in the primordial Cosmic Microwave Ba...