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Dey, A;Schlegel, DJ;Lang, D;Blum, R;Burleigh, K;Fan, X;Findlay, JR;Finkbeiner, D;Herrera, D;Juneau, S;Landriau, M;Levi, M;McGreer, I;Meisner, A;Myers, AD;Moustakas, J;Nugent, P;Patej, A;Schlafly, EF;Walker, AR;Valdes, F;Weaver, BA;Yeche, C;Zou, H;Zhou, X;Abareshi, B;Abbott, TMC;Abolfathi, B;Aguilera, C;Alam, S;Allen, L;Alvarez, A;Annis, J;Ansarinejad, B;Aubert, M;Beechert, J;Bell, EF;BenZvi, SY;Beutler, F;Bielby, RM;Bolton, AS;Briceno, C;Buckley-Geer, EJ;Butler, K;Calamida, A;Carlberg, RG;Carter, P;Casas, R;Castander, FJ;Choi, Y;Comparat, J;Cukanovaite, E;Delubac, T;DeVries, K;Dey, S;Dhungana, G;Dickinson, M;Ding, Z;Donaldson, JB;Duan, Y;Duckworth, CJ;Eftekharzadeh, S;Eisenstein, DJ;Etourneau, T;Fagrelius, PA;Farihi, J;Fitzpatrick, M;Font-Ribera, A;Fulmer, L;Gansicke, BT;Gaztanaga, E;George, K;Gerdes, DW;Gontcho, SGA;Gorgoni, C;Green, G;Guy, J;Harmer, D;Hernandez, M;Honscheid, K;Huang, LW;James, DJ;Jannuzi, BT;Jiang, L;Joyce, R;Karcher, A;Karkar, S;Kehoe, R;Kneib, J-P;Kueter-Young, A;Lan, T-W;Lauer, TR;Le Guillou, L;Le Van Suu, A;Lee, JH;Lesser, M;Levasseur, LP;Li, TS;Mann, JL;Marshall, R;Martinez-Vazquez, CE;Martini, P;des Bourboux, HDM;McManus, S;Meier, TG;Menard, B;Metcalfe, N;Munoz-Gutierrez, A;Najita, J;Napier, K;Narayan, G;Newman, JA;Nie, J;Nord, B;Norman, DJ;Olsen, KAG;Paat, A;Palanque-Delabrouille, N;Peng, X;Poppett, CL;Poremba, MR;Prakash, A;Rabinowitz, D;Raichoor, A;Rezaie, M;Robertson, AN;Roe, NA;Ross, AJ;Ross, NP;Rudnick, G;Safonova, S;Saha, A;Sanchez, FJ;Savary, E;Schweiker, H;Scott, A;Seo, H-J;Shan, H;Silva, DR;Slepian, Z;Soto, C;Sprayberry, D;Staten, R;Stillman, CM;Stupak, RJ;Summers, DL;Tie, SS;Tirado, H;Vargas-Magana, M;Vivas, AK;Wechsler, RH;Williams, D;Yang, J;Yang, Q;Yapici, T;Zaritsky, D;Zenteno, A;Zhang, K;Zhang, T;Zhou, R;Zhou, Z
The DESI Legacy Imaging Surveys (http://legacysurvey.org/) are a combination of three public projects (the Dark Energy Camera Legacy Survey, the Beijing–Arizona Sky Survey, and the Mayall z-band Legacy Survey) that will jointly image ≈14,000 deg2 of ...
(The SNLS Collaboration) 40 pages, 32 figures, Accepted in A&A
We present a method using the SALT2 light curve fitter to determine the redshift of type Ia supernovae in the Supernova Legacy Survey (SNLS) based on their photometry in g', r', i' and z'. On 289 supernovae of the first three years of SNLS data, we o...
Submitted to ApJ. Data available from https://tspace.library.utoronto.ca/snls
Aihara, H.;Allende Prieto, C.;An, D.;F. Anderson, S.;Aubourg, É.;Balbinot, E.;C. Beers, T.;A. Berlind, A.;J. Bickerton, S.;Bizyaev, D.;R. Blanton, M.;Bochanski, J.J.;S. Bolton, A.;Bovy, J.;N. Brandt, W.;Brinkmann, J.;J. Brown, P.;R. Brownstein, J.;Busca, N.G.;A. Carr, M.;Chen, Y.;Chiappini, C.;Comparat, J.;Cortes, M.;C. Croft, R.A.;J. Cuesta, A.;N. Da Costa, L.;R. A. Davenport, J.;Dawson, K.;Dhital, S.;Ealet, A.;L. Ebelke, G.;Edmondson, E.M.;Eisenstein, D.J.;Escoffier, S.;Esposito, M.;L. Evans, M.;Fan, X.;Femenía Castellá, B.;Font-Ribera, A.;M. Frinchaboy, P.;Ge, J.;A. Gillespie, B.;Gilmore., G.;I. González Hernández, J.;R Gott, J.;Gould, A.;K. Grebel, E.;E. Gunn, J.;Hamilton, J.-C.;Harding, P.;Harris, D.W.;L. Hawley, S.;R. Hearty, F.;Ho, S.;W. Hogg, D.;A. Holtzman, J.;Honscheid, K.;Inada, N.;I. Ivans, I.;Jiang, Liang;A. Johnson, J.;Jordan, C.;P. Jordan, W.;A. Kazin, E.;Kirkby, D.;Klaene, M.A.;R. Knapp, G.;Kneib, J.-P.;S. Kochanek, C.;Koesterke, L.;A. Kollmeier, J.;G. Kron, R.;Lampeitl, H.;Lang, D.;Le Goff, J.-M.;Sun Lee, Y.;Lin, Y.-T.;C. Long, D.;P. Loomis, C.;Lucatello, S.;Lundgren, B.;H. Lupton, R.;Ma, Z.;Macdonald, N.;Mahadevan, S.;A. G. Maia, M.;Makler, M.;Malanushenko, E.;Malanushenko, V.;Mandelbaum, R.;Maraston, C.;Margala, D.;L. Masters, K.;K. Mcbride, C.;M. Mcgehee, P.;D. Mcgreer, I.;Ménard, B.;Miralda-Escudé, J.;L. Morrison, H.;Mullally, F.;Muna, D.;A. Munn, J.;Murayama, H.;D. Myers, A.;Naugle, T.;Fausti Neto, A.;Cuong Nguyen, D.;Nichol, R.C.;O'Connell, R.W.;L. C. Ogando, R.;D. Olmstead, M.;J. Oravetz, D.;Padmanabhan, N.;Palanque-Delabrouille, N.;Pan, K.;Pandey, P.;Pâris, I.;J. Percival, W.;Petitjean, P.;Pfaffenberger, R.;Pforr, J.;Phleps, S.;Pichon, C.;M. Pieri, M.;Prada, F.;M. Price-Whelan, A.;J. Raddick, M.;H. F. Ramos, B.;Reylé, C.;Rich, J.;T. Richards, G.;Rix, H.-W.;C. Robin, A.;J. Rocha-Pinto, H.;M. Rockosi, C.;Roe, N.A.;Rollinde, E.;J. Ross, A.;P. Ross, N.;M. Rossetto, B.;G. Sánchez, A.;Sayres, C.;J. Schlegel, D.;J. Schlesinger, K.;J. Schmidt, S.;P. Schneider, D.;Sheldon, E.;Shu, Y.;Simmerer, J.;E. Simmons, A.;Sivarani, T.;Snedden, S.A.;S. Sobeck, J.;Steinmetz, M.;A. Strauss, M.;S. Szalay, A.;Tanaka, M.;R. Thakar, A.;Thomas, D.;L. Tinker, J.;M. Tofflemire, B.;Tremonti, C.A.;Vandenberg, Jan;Vargas Magaña, M.;Verde, L.;P. Vogt, N.;A. Wake, D.;Wang, J.;A. Weaver, B.;H. Weinberg, D.;White, M.;D. M. White, S.;Yanny, B.;Yasuda, N.;Yeche, C.;Zehavi, I.
The Sloan Digital Sky Survey (SDSS) started a new phase in 2008 August, with new instrumentation and new surveys focused on Galactic structure and chemical evolution, measurements of the baryon oscillation feature in the clustering of galaxies and th...
Adhikari, R.;Agostini, M.;Anh Ky, N.;Araki, T.;Archidiacono, M.;Bahr, M.;Baur, J.;Behrens, J.;Bezrukov, F.;Bhupal Dev, P. S.;Borah, D.;Boyarsky, A.;De Gouvea, A.;Pires, C. A D S;De Vega, H. J.;Dias, A. G.;Di Bari, P.;Djurcic, Z.;Dolde, K.;Dorrer, H.;Durero, M.;Dragoun, O.;Drewes, M.;Drexlin, G.;Düllmann, Ch E.;Eberhardt, K.;Eliseev, S.;Enss, C.;Evans, N. W.;Faessler, A.;Filianin, P.;Fischer, V.;Fleischmann, A.;Formaggio, J. A.;Franse, J.;Fraenkle, F. M.;Frenk, C. S.;Fuller, G.;Gastaldo, L.;Garzilli, A.;Giunti, C.;Glück, F.;Goodman, M. C.;Gonzalez-Garcia, M. C.;Gorbunov, D.;Hamann, J.;Hannen, V.;Hannestad, S.;Hansen, S. H.;Hassel, C.;Heeck, J.;Hofmann, F.;Houdy, T.;Huber, A.;Iakubovskyi, D.;Ianni, A.;Ibarra, A.;Jacobsson, R.;Jeltema, T.;Jochum, J.;Kempf, S.;Kieck, T.;Korzeczek, M.;Kornoukhov, V.;Lachenmaier, T.;Laine, M.;Langacker, P.;Lasserre, T.;Lesgourgues, J.;Lhuillier, D.;Li, Y. F.;Liao, W.;Long, A. W.;Maltoni, M.;Mangano, G.;Mavromatos, Nikolaos;Menci, N.;Merle, A.;Mertens, S.;Mirizzi, A.;Monreal, B.;Nozik, A.;Neronov, A.;Niro, V.;Novikov, Y.;Oberauer, L.;Otten, E.;Palanque-Delabrouille, N.;Pallavicini, M.;Pantuev, V. S.;Papastergis, E.;Parke, S.;Pascoli, S.;Pastor, S.;Patwardhan, A.;Pilaftsis, A.;Radford, D. C.;Ranitzsch, P. C O;Rest, O.;Robinson, D. J.;Rodrigues Da Silva, P. S.;Ruchayskiy, O.;Sanchez, N. G.;Sasaki, M.;Saviano, N.;Schneider, A.;Schneider, F.;Schwetz, T.;Schönert, S.;Scholl, S.;Shankar, F.;Shrock, R.;Steinbrink, N.;Strigari, L.;Suekane, F.;Suerfu, B.;Takahashi, R.;Thi Hong Van, N.;Tkachev, I.;Totzauer, M.;Tsai, Y.;Tully, C. G.;Valerius, K.;Valle, J. W F;Venos, D.;Viel, M.;Vivier, M.;Wang, M. Y.;Weinheimer, C.;Wendt, K.;Winslow, L.;Wolf, J.;Wurm, M.;Xing, Z.;Zhou, S.;Zuber, K.
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