Preliminary Limits on the WIMP-Nucleon Cross Section from the Cryogenic Dark Matter Search (CDMS)

Autor: Akerib, DS, Barnes Jr, PD, Bauer, DA, Brink, PL, Cabrera, B, Caldwell, DO, Clarke, RM, Da Silva, A, Davies, AK, Dougherty, BL, Irwin, KD, Gaitskell, RJ, Golwala, SR, Haller, EE, Jochum, J, Knowlton, WB, Kuzminov, V, Nam, SW, Novikov, V, Penn, MJ, Perera, TA, Ross, RR, Sadoulet, B, Schnee, RW, Shutt, T, Smith, A, Sonnenschein, AH, Spadafora, AL, Stockwell, WK, Yellin, S, Young, BA

Publikováno v: Nucl.Phys.Proc.Suppl.70:64-68,1999

We are conducting an experiment to search for WIMPs, or weakly-interacting massive particles, in the galactic halo using terrestrial detectors. This generic class of hypothetical particles, whose properties are similar to those predicted by extension

Externí odkaz: http://arxiv.org/abs/astro-ph/9712343

THE HUBBLE SPACE TELESCOPE CLUSTER SUPERNOVA SURVEY. II. THE TYPE Ia SUPERNOVA RATE IN HIGH-REDSHIFT GALAXY CLUSTERS

Autor: Barbary, K, Aldering, G, Amanullah, R, Brodwin, M, Connolly, N, Dawson, KS, Doi, M, Eisenhardt, P, Faccioli, L, Fadeyev, V, Fakhouri, HK, Fruchter, AS, Gilbank, DG, Gladders, MD, Goldhaber, G, Goobar, A, Hattori, T, Hsiao, E, Huang, X, Ihara, Y, Kashikawa, N, Koester, B, Konishi, K, Kowalski, M, Lidman, C, Lubin, L, Meyers, J, Morokuma, T, Oda, T, Panagia, N, Perlmutter, S, Postman, M, Ripoche, P, Rosati, P, Rubin, D, Schlegel, DJ, Spadafora, AL, Stanford, SA, Strovink, M, Suzuki, N, Takanashi, N, Tokita, K, Yasuda, N, Project, SC

Publikováno v: ASTROPHYSICAL JOURNAL, vol 745, iss 1
Barbary, K; Aldering, G; Amanullah, R; Brodwin, M; Connolly, N; Dawson, KS; et al.(2012). THE HUBBLE SPACE TELESCOPE CLUSTER SUPERNOVA SURVEY. II. THE TYPE Ia SUPERNOVA RATE IN HIGH-REDSHIFT GALAXY CLUSTERS. ASTROPHYSICAL JOURNAL, 745(1). doi: 10.1088/0004-637X/745/1/32. Lawrence Berkeley National Laboratory: Lawrence Berkeley National Laboratory. Retrieved from: http://www.escholarship.org/uc/item/3c29f7x3

We report a measurement of the Type Ia supernova (SN Ia) rate in galaxy clusters at 0.9 < z < 1.45 from the Hubble Space Telescope (HST) Cluster Supernova Survey. This is the first cluster SN Ia rate measurement with detected z > 0.9 SNe. Finding 8 +

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::3845ec866f732cbfc7b99c583295db71
https://escholarship.org/uc/item/3c29f7x3

Subaru FOCAS Spectroscopic Observations of High-Redshift Supernovae

Autor: Morokuma, T, Tokita, K, Lidman, C, Doi, M, Yasuda, N, Aldering, G, Amanullah, R, Barbary, K, Dawson, K, Fadeyev, V, Fakhouri, HK, Goldhaber, G, Goobar, A, Hattori, T, Hayano, J, Hook, IM, Howell, DA, Furusawa, H, Ihara, Y, Kashikawa, N, Knop, RA, Konishi, K, Meyers, J, Oda, T, Pain, R, Perlmutter, S, Rubin, D, Spadafora, AL, Suzuki, N, Takanashi, N, Totani, T, Utsunomiya, H, Wang, L, Project, SC

Publikováno v: PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN. 62(1)

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=od______1064::057045eb7bf51474042e42a6babce26e
http://ora.ox.ac.uk/objects/uuid:d3d70597-9c3d-4396-86b9-1ec563ae84a5

Improved Cosmological Constraints from New, Old and Combined Supernova Datasets

Autor: Kowalski, M, Rubin, D, Aldering, G, Agostinho, RJ, Amadon, A, Amanullah, R, Balland, C, Barbary, K, Blanc, G, Challis, PJ, Conley, A, Connolly, NV, Covarrubias, R, Dawson, KS, Deustua, SE, Ellis, R, Fabbro, S, Fadeyev, V, Fan, X, Farris, B, Folatelli, G, Frye, BL, Garavini, G, Gates, EL, Germany, L, Goldhaber, G, Goldman, B, Goobar, A, Groom, DE, Haissinski, J, Hardin, D, Hook, I, Kent, S, Kim, AG, Knop, RA, Lidman, C, Linder, EV, Mendez, J, Meyers, J, Miller, GJ, Moniez, M, Mourao, AM, Newberg, H, Nobili, S, Nugent, PE, Pain, R, Perdereau, O, Perlmutter, S, Phillips, MM, Prasad, V, Quimby, R, Regnault, N, Rich, J, Rubenstein, EP, Ruiz-Lapuente, P, Santos, FD, Schaefer, BE, Schommer, RA, Smith, RC, Soderberg, AM, Spadafora, AL, Strolger, L-G, Strovink, M, Suntzeff, NB, Suzuki, N, Thomas, RC, Walton, NA, Wang, L, Wood-Vasey, WM, Yun, JL, Project, SC

Publikováno v: The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2008, 686, pp.749-778. ⟨10.1086/589937⟩
The Astrophysical Journal, 2008, 686, pp.749-778. ⟨10.1086/589937⟩
The Astrophysical Journal, vol 686, iss 2
Kowalski, M; Rubin, D; Aldering, G; Agostinho, RJ; Amadon, A; Amanullah, R; et al.(2008). Improved cosmological constraints from new, old, and combined supernova data sets. Astrophysical Journal, 686(2), 749-778. doi: 10.1086/589937. Lawrence Berkeley National Laboratory: Retrieved from: http://www.escholarship.org/uc/item/8646z73c
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astrophysical Journal, vol 686, iss 2

30 pags., 17 figs., 12 tabs. 4 apps.
We present a new compilation of Type Ia supernovae (SNe Ia), a new data set of low-redshift nearby-Hubble-flow SNe, and new analysis procedures to work with these heterogeneous compilations. This >Union> comp

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f2a0b7fff8b0c83cc633c11ce2298984
http://hal.in2p3.fr/in2p3-00292374

Quantitative comparison between type Ia supernova spectra at low and high redshifts: A case study

Autor: Garavini, G, Folatelli, G, Nobili, S, Aldering, G, Amanullah, R, Antilogus, P, Astier, P, Blanc, G, Bronder, T, Burns, MS, Conley, A, Deustua, SE, Doi, M, Fabbro, S, Fadeyev, V, Gibbons, R, Goldhaber, G, Goobar, A, Groom, DE, Hook, I, Howell, DA, Kashikawa, N, Kim, AG, Kowalski, M, Kuznetsova, N, Lee, BC, Lidman, C, Mendez, J, Morokuma, T, Motohara, K, Nugent, PE, Pain, R, Perlmutter, S, Quimby, R, Raux, J, Regnault, N, Ruiz-Lapuente, P, Sainton, G, Schahmaneche, K, Smith, E, Spadafora, AL, Stanishev, V, Thomas, RC, Walton, NA, Wang, L, Wood-Vasey, WM, Yasuda, N, Project, SC

Publikováno v: Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2007, 470, pp.411-424. ⟨10.1051/0004-6361:20065400⟩
Astronomy and Astrophysics-A&A, 2007, 470, pp.411-424. ⟨10.1051/0004-6361:20065400⟩
Astronomy & Astrophysics, vol 470, iss 2

We develop a method to measure the strength of the absorption features in Type Ia supernova (SN Ia) spectra and use it to make a quantitative comparison between the spectra of Type Ia supernovae at low and high redshifts. In this case study, we apply

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1a024d0c5adb1f3c447712722de8d36c
http://hal.in2p3.fr/in2p3-00142917