First cosmology results using supernovae ia from the dark energy survey: Survey overview, performance, and supernova spectroscopy

Autor: Smith, M, D'Andrea, CB, Sullivan, M, Möller, A, Nichol, RC, Thomas, RC, Kim, AG, Sako, M, Castander, FJ, Filippenko, AV, Foley, RJ, Galbany, L, González-Gaitán, S, Kasai, E, Kirshner, RP, Lidman, C, Scolnic, D, Brout, D, Davis, TM, Gupta, RR, Hinton, Kessler, R, Lasker, J, Macaulay, E, Wolf, RC, Zhang, B, Asorey, J, Avelino, A, Bassett, BA, Calcino, J, Carollo, D, Casas, R, Challis, P, Childress, M, Clocchiatti, A, Crawford, S, Frohmaier, C, Glazebrook, K, Goldstein, DA, Graham, ML, Hoormann, JK, Kuehn, K, Lewis, GF, Mandel, KS, Morganson, E, Muthukrishna, D, Nugent, P, Pan, YC, Pursiainen, M, Sharp, R, Sommer, NE, Swann, E, Thomas, BP, Tucker, BE, Uddin, SA, Wiseman, P, Zheng, W, Abbott, TMC, Annis, J, Avila, S, Bechtol, K, Bernstein, GM, Bertin, E, Brooks, D, Burke, DL, Carnero Rosell, A, Carrasco Kind, M, Carretero, J, Cunha, CE, Da Costa, LN, Davis, C, De Vicente, J, Diehl, HT, Eifler, TF, Estrada, J, Frieman, J, García-Bellido, J, Gaztanaga, E, Gerdes, DW, Gruen, D, Gruendl, RA, Gschwend, J, Gutierrez, G, Hartley, WG, Hollowood, DL, Honscheid, K, Hoyle, B, James, DJ, Johnson, MWG, Johnson, MD, Kuropatkin, N, Li, TS, Lima, M, Maia, MAG, March, M, Marshall, JL, Martini, P, Menanteau, F, Miller, CJ, Miquel, R

Publikováno v: The Astronomical Journal, vol 160, iss 6
Astronomical Journal, vol 160, iss 6

We present details on the observing strategy, data-processing techniques, and spectroscopic targeting algorithms for the first three years of operation for the Dark Energy Survey Supernova Program (DES-SN). This five-year program using the Dark Energ

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9ab2ae6b07d52fafb21fbd99fcc4615c

First Cosmology Results Using SNe Ia from the Dark Energy Survey: Analysis, Systematic Uncertainties, and Validation

Autor: Brout, D, Scolnic, D, Kessler, R, D'Andrea, CB, Davis, TM, Gupta, RR, Hinton, SR, Kim, AG, Lasker, J, Lidman, C, Macaulay, E, Möller, A, Nichol, RC, Sako, M, Smith, M, Sullivan, M, Zhang, B, Andersen, P, Asorey, J, Avelino, A, Bassett, BA, Brown, P, Calcino, J, Carollo, D, Challis, P, Childress, M, Clocchiatti, A, Filippenko, AV, Foley, RJ, Galbany, L, Glazebrook, K, Hoormann, JK, Kasai, E, Kirshner, RP, Kuehn, K, Kuhlmann, S, Lewis, GF, Mandel, KS, March, M, Miranda, V, Morganson, E, Muthukrishna, D, Nugent, P, Palmese, A, Pan, YC, Sharp, R, Sommer, NE, Swann, E, Thomas, RC, Tucker, BE, Uddin, SA, Wester, W, Abbott, TMC, Allam, S, Annis, J, Avila, S, Bechtol, K, Bernstein, GM, Bertin, E, Brooks, D, Burke, DL, Rosell, AC, Kind, MC, Carretero, J, Castander, FJ, Cunha, CE, Da Costa, LN, Davis, C, De Vicente, J, Depoy, DL, Desai, S, Diehl, HT, Doel, P, Drlica-Wagner, A, Eifler, TF, Estrada, J, Fernandez, E, Flaugher, B, Fosalba, P, Frieman, J, García-Bellido, J, Gruen, D, Gruendl, RA, Gutierrez, G, Hartley, WG, Hollowood, DL, Honscheid, K, Hoyle, B, James, DJ, Jarvis, M, Jeltema, T, Krause, E, Lahav, O, Li, TS, Lima, M, Maia, MAG, Marriner, J, Marshall, JL, Martini, P, Menanteau, F

Publikováno v: The Astrophysical Journal, vol 874, iss 2
Astrophysical Journal, vol 874, iss 2

We present the analysis underpinning the measurement of cosmological parameters from 207 spectroscopically classified SNe Ia from the first 3 years of the Dark Energy Survey Supernova Program (DES-SN), spanning a redshift range of 0.017 < z < 0.849.

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::31465232e982884f381c247ee1e58ecd

Cosmological Constraints from Multiple Probes in the Dark Energy Survey

Autor: Abbott, TMC, Alarcon, A, Allam, S, Andersen, P, Andrade-Oliveira, F, Annis, J, Asorey, J, Avila, S, Bacon, D, Banik, N, Bassett, BA, Baxter, E, Bechtol, K, Becker, MR, Bernstein, GM, Bertin, E, Blazek, J, Bridle, SL, Brooks, D, Brout, D, Burke, DL, Calcino, J, Camacho, H, Campos, A, Carnero Rosell, A, Carollo, D, Carrasco Kind, M, Carretero, J, Castander, FJ, Cawthon, R, Challis, P, Chan, KC, Chang, C, Childress, M, Crocce, M, Cunha, CE, D'Andrea, CB, da Costa, LN, Davis, C, Davis, TM, De Vicente, J, DePoy, DL, DeRose, J, Desai, S, Diehl, HT, Dietrich, JP, Dodelson, S, Doel, P, Drlica-Wagner, A, Eifler, TF, Elvin-Poole, J, Estrada, J, Evrard, AE, Fernandez, E, Flaugher, B, Foley, RJ, Fosalba, P, Frieman, J, Galbany, L, García-Bellido, J, Gatti, M, Gaztanaga, E, Gerdes, DW, Giannantonio, T, Glazebrook, K, Goldstein, DA, Gruen, D, Gruendl, RA, Gschwend, J, Gutierrez, G, Hartley, WG, Hinton, SR, Hollowood, DL, Honscheid, K, Hoormann, JK, Hoyle, B, Huterer, D, Jain, B, James, DJ, Jarvis, M, Jeltema, T, Kasai, E, Kent, S, Kessler, R, Kim, AG, Kokron, N, Krause, E, Kron, R, Kuehn, K, Kuropatkin, N, Lahav, O, Lasker, J, Lemos, P, Lewis, GF, Li, TS, Lidman, C, Lima, M, Lin, H, Macaulay, E, MacCrann, N

Publikováno v: Physical review letters, vol 122, iss 17

The combination of multiple observational probes has long been advocated as a powerful technique to constrain cosmological parameters, in particular dark energy. The Dark Energy Survey has measured 207 spectroscopically confirmed type Ia supernova li

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::90c04e1d3701f8ee9998f13d62e2bfc6
https://escholarship.org/uc/item/63f2n75h

First Cosmology Results Using Type Ia Supernovae from the Dark Energy Survey: Photometric Pipeline and Light-curve Data Release

Autor: Brout, D, Sako, M, Scolnic, D, Kessler, R, D'Andrea, CB, Davis, TM, Hinton, SR, Kim, AG, Lasker, J, Macaulay, E, Möller, A, Nichol, RC, Smith, M, Sullivan, M, Wolf, RC, Allam, S, Bassett, BA, Brown, P, Castander, FJ, Childress, M, Foley, RJ, Galbany, L, Herner, K, Kasai, E, March, M, Morganson, E, Nugent, P, Pan, YC, Thomas, RC, Tucker, BE, Wester, W, Abbott, TMC, Annis, J, Avila, S, Bertin, E, Brooks, D, Burke, DL, Rosell, AC, Kind, MC, Carretero, J, Crocce, M, Cunha, CE, Costa, LND, Davis, C, Vicente, JD, Desai, S, Diehl, HT, Doel, P, Eifler, TF, Flaugher, B, Fosalba, P, Frieman, J, Garcia-Bellido, J, Gaztanaga, E, Gerdes, DW, Goldstein, DA, Gruen, D, Gruendl, RA, Gschwend, J, Gutierrez, G, Hartley, WG, Hollowood, DL, Honscheid, K, James, DJ, Kuehn, K, Kuropatkin, N, Lahav, O, Li, TS, Lima, M, Marshall, JL, Martini, P, Miquel, R, Nord, B, Plazas, AA, Roodman, A, Rykoff, ES, Sanchez, E, Scarpine, V, Schindler, R, Schubnell, M, Serrano, S, Sevilla-Noarbe, I, Soares-Santos, M, Sobreira, F, Suchyta, E, Swanson, MEC, Tarle, G, Thomas, D, Tucker, DL, Walker, AR, Yanny, B, Zhang, Y

Publikováno v: Brout, D; Sako, M; Scolnic, D; Kessler, R; D’Andrea, CB; Davis, TM; et al.(2019). First Cosmology Results Using Type Ia Supernovae from the Dark Energy Survey: Photometric Pipeline and Light-curve Data Release. The Astrophysical Journal, 874(1), 106-106. doi: 10.3847/1538-4357/ab06c1. Lawrence Berkeley National Laboratory: Retrieved from: http://www.escholarship.org/uc/item/5hs3g6st
The Astrophysical Journal, vol 874, iss 1
Astrophysical Journal, vol 874, iss 1

© Contribution of US Department of Energy; not subject to copyright in the United States.. We present griz light curves of 251 SNe Ia from the first 3 years of the Dark Energy Survey Supernova Program's (DES-SN) spectroscopically classified sample.

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::0f2af6a19b4692b5fbed4c455ed6a67c
http://www.escholarship.org/uc/item/5hs3g6st

An Ultra Deep Field survey with WFIRST

Autor: Koekemoer, Anton M, Foley, RJ, Spergel, DN, Bagley, M, Bezanson, R, Bianco, FB, Bouwens, R, Bradley, L, Brammer, G, Capak, P, Davidzon, I, Rosa, G De, Dickinson, ME, Doré, O, Dunlop, JS, Ellis, RS, Fan, X, Fazio, GG, Ferguson, HC, Filippenko, AV, Finkelstein, S, Frye, B, Gawiser, E, Grogin, NA, Hathi, NP, Hirata, CM, Hounsell, R, Illingworth, GD, Jansen, RA, Jauzac, M, Jha, SW, Kartaltepe, JS, Kim, AG, Kelly, P, Kruk, JW, Larson, R, Lotz, J, Lucas, R, Malhotra, S, Mandel, K, Margutti, R, Marrone, D, McLure, RJ, McQuinn, K, Melchior, P, Mobasher, B, Mould, JR, Moustakas, L, Newman, JA, Papovich, C, Peeples, MS, Perlmutter, S, Pirzkal, N, Rhoads, J, Rhodes, J, Robertson, B, Rubin, D, Ryan, R, Scolnic, D, Shapley, A, Somerville, R, Steinhardt, C, Stiavelli, M, Street, R, Trenti, M, Treu, T, Wang, L, Wang, Y, Whalen, D, Windhorst, RA, Wollack, EJ, Yan, H

Studying the formation and evolution of galaxies at the earliest cosmic times, and their role in reionization, requires the deepest imaging possible. Ultra-deep surveys like the HUDF and HFF have pushed to mag \mAB$\,\sim\,$30, revealing galaxies at

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1ba74d212ef66510584df83bdcfb75cc