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Dawson, KS;Kneib, J-P;Percival, WJ;Alam, S;Albareti, FD;Anderson, SF;Armengaud, E;Aubourg, E;Bailey, S;Bautista, JE;Berlind, AA;Bershady, MA;Beutler, F;Bizyaev, D;Blanton, MR;Blomqvist, M;Bolton, AS;Boyy, J;Brandt, WN;Brinkmann, J;Brownstein, JR;Burtin, E;Busca, NG;Cai, Z;Chuang, C-H;Clerc, N;Comparat, J;Cope, F;Croft, RAC;Cruz-Gonzalez, I;da Costa, LN;Cousinou, M-C;Darling, J;de la Macorra, A;de la Torre, S;Delubac, T;des Bourboux, HDM;Dwelly, T;Ealet, A;Eisenstein, DJ;Eracleous, M;Escoffier, S;Fan, X;Finoguenov, A;Font-Ribera, A;Frinchaboy, P;Gaulme, P;Georgakakis, A;Green, P;Guo, H;Guy, J;Ho, S;Holder, D;Huehnerhoff, J;Hutchinson, T;Jing, Y;Jullo, E;Kamble, V;Kinemuchi, K;Kirkby, D;Kitaura, F-S;Klaene, MA;Laher, RR;Lang, D;Laurent, P;Le Goff, J-M;Li, C;Liang, Y;Lima, M;Lin, Q;Lin, W;Lin, Y-T;Long, DC;Lundgren, B;MacDonald, N;Maia, MAG;Malanushenko, E;Malanushenko, V;Mariappan, V;McBride, CK;McGreer, ID;Menard, B;Merloni, A;Meza, A;Montero-Dorta, AD;Muna, D;Myers, AD;Nandra, K;Naugle, T;Newman, JA;Noterdaeme, P;Nugent, P;Ogando, N;Olmstead, MD;Oravetz, A;Oravetz, DJ;Padmanabhan, N;Palanque-Delabrouille, N;Pan, K;Parejko, JK;Paris, I;Peacock, JA;Petitjean, P;Pieri, MM;Pisani, A;Prada, F;Prakash, A;Raichoor, A;Reid, B;Rich, J;Ridl, J;Rodriguez-Torres, S;Rosell, AC;Ross, AJ;Rossi, G;Ruan, J;Salvato, M;Sayres, C;Schneider, DP;Schlegel, DJ;Seljak, U;Seo, H-J;Sesar, B;Shandera, S;Shu, Y;Slosar, A;Sobreira, F;Streblyanska, A;Suzuki, N;Taylor, D;Tao, C;Tinker, JL;Tojeiro, R;Vargas-Magana, M;Wang, Y;Weaver, BA;Weinberg, DH;White, M;Wood-Vasey, WM;Yeche, C;Zhai, Z;Zhao, C;Zhao, G-B;Zheng, Z;Zhu, GB;Zou, H
Ade, P. A. R.;Aghanim, N.;Arnaud, M.;Ashdown, M.;Aubourg, E.;Aumont, J.;Baccigalupi, C.;Banday, A. J.;Barreiro, R. B.;Bartolo, N.;Battaner, E.;Benabed, K.;Benoit-Levy, A.;Bersanelli, M.;Bielewicz, P.;Bock, J. J.;Bonaldi, A.;Bonavera, L.;Bond, J. R.;Borrill, J.;Bouchet, F. R.;Burigana, C.;Calabrese, E.;Cardoso, J. -F.;Catalano, A.;Chamballu, A.;Chiang, H. C.;Christensen, P. R.;Clements, D. L.;Colombo, L. P. L.;Combet, C.;Crill, B. P.;Curto, A.;Cuttaia, F.;Danese, L.;Davies, R. D.;Davis, R. J.;de Bernardis, P.;de Zotti, G.;Delabrouille, J.;Dickinson, C.;Diego, J. M.;Dolag, K.;Donzelli, S.;Doré, O.;Douspis, M.;Ducout, A.;Dupac, X.;Efstathiou, G.;Elsner, F.;Ensslin, T. A.;Eriksen, H. K.;Finelli, F.;Forni, O.;Frailis, M.;Fraisse, A. A.;Franceschi, E.;Frejsel, A.;Galeotta, S.;Galli, S.;Ganga, K.;Genova-Santos, R. T.;Giard, M.;Gjerlow, E.;Gonzalez-Nuevo, J.;Gorski, K. M.;Gregorio, A.;Gruppuso, A.;Hansen, F. K.;Harrison, D. L.;Henrot-Versillé, S.;Hernandez-Monteagudo, C.;Herranz, D.;Hildebrandt, S. R.;Hivon, E.;Hobson, M.;Hornstrup, A.;Huffenberger, K. M.;Hurier, G.;Jaffe, A. H.;Jaffe, T. R.;Jones, W. C.;Juvela, M.;Keihänen, E.;Keskitalo, R.;Kitaura, F.;Kneissl, R.;Knoche, J.;Kunz, M.;Kurki-Suonio, H.;Lagache, G.;Lamarre, J. -M.;Lasenby, A.;Lattanzi, M.;Lawrence, C. R.;Leonardi, R.;Leon-Tavares, J.;Levrier, F.;Liguori, M.;Lilje, P. B.;Linden-Vornle, M.;Lopez-Caniego, M.;Lubin, P. M.;Ma, Y. -Z.;Macias-Perez, J. F.;Maffei, B.;Maino, D.;Mak, D. S. Y.;Mandolesi, N.;Mangilli, A.;Maris, M.;Martin, P. G.;Martinez-Gonzalez, E.;Masi, S.;Matarrese, S.;McGehee, P.;Melchiorri, A.;Mennella, A.;Migliaccio, M.;Miville-Deschenes, M. -A.;Moneti, A.;Montier, L.;Morgante, G.;Mortlock, D.;Munshi, D.;Murphy, J. A.;Naselsky, P.;Nati, F.;Natoli, P.;Noviello, F.;Novikov, D.;Novikov, I.;Oxborrow, C. A.;Pagano, L.;Pajot, F.;Paoletti, D.;Perdereau, O.;Perotto, L.;Pettorino, V.;Piacentini, F.;Piat, M.;Pierpaoli, E.;Pointecouteau, E.;Polenta, G.;Ponthieu, N.;Pratt, G. W.;Puget, J. -L.;Puisieux, S.;Rachen, J. P.;Racine, B.;Reach, W. T.;Reinecke, M.;Remazeilles, M.;Renault, C.;Renzi, A.;Ristorcelli, I.;Rocha, G.;Rosset, C.;Rossetti, M.;Roudier, G.;Rubino-Martin, J. A.;Rusholme, B.;Sandri, M.;Santos, D.;Savelainen, M.;Savini, G.;Scott, D.;Spencer, L. D.;Stolyarov, V.;Sudiwala, R.;Sunyaev, R.;Sutton, D.;Suur-Uski, A. -S.;Sygnet, J. -F.;Tauber, J. A.;Terenzi, L.;Toffolatti, F.;Tomasi, M.;Tucci, M.;Valenziano, L.;Väliviita, Jussi;Van Tent, B.;Vielva, P.;Villa, F.;Wade, L. A.;Wandelt, B. D.;Wang, W.;Wehus, I. K.;Yvon, D.;Zacchei, A.;Zonca, A.
By looking at the kinetic Sunyaev-Zeldovich effect (kSZ) in Planck nominal mission data, we present a significant detection of baryons participating in large-scale bulk flows around central galaxies (CGs) at redshift z approximate to 0.1. We estimate...
Ade, Peter;Aghanim, N.;Arnaud, M.;Ashdown, M.;Aubourg, E.;Aumont, J.;Baccigalupi, C.;Banday, A. J.;Barreiro, R. B.;Bartolo, N.;Battaner, E.;Benabed, K.;Benoit-Lévy, A.;Bersanelli, M.;Bielewicz, P.;Bock, J. J.;Bonaldi, A.;Bonavera, L.;Bond, J. R.;Borrill, J.;Bouchet, F. R.;Burigana, C.;Calabrese, Erminia;Cardoso, J.-F.;Catalano, A.;Chamballu, A.;Chiang, H. C.;Christensen, P. R.;Clements, D. L.;Colombo, L. P. L.;Combet, C.;Crill, B. P.;Curto, A.;Cuttaia, F.;Danese, L.;Davies, R. D.;Davis, R. J.;de Bernardis, P.;de Zotti, G.;Delabrouille, J.;Dickinson, C.;Diego, J. M.;Dolag, K.;Donzelli, S.;Doré, O.;Douspis, M.;Ducout, A.;Dupac, X.;Efstathiou, G.;Elsner, F.;Enßlin, T. A.;Eriksen, H. K.;Finelli, F.;Forni, O.;Frailis, M.;Fraisse, A. A.;Franceschi, E.;Frejsel, A.;Galeotta, S.;Galli, S.;Ganga, K.;Génova-Santos, R. T.;Giard, M.;Gjerløw, E.;González-Nuevo, J.;Górski, K. M.;Gregorio, A.;Gruppuso, A.;Hansen, F. K.;Harrison, D. L.;Henrot-Versillé, S.;Hernández-Monteagudo, C.;Herranz, D.;Hildebrandt, S. R.;Hivon, E.;Hobson, M.;Hornstrup, A.;Huffenberger, K. M.;Hurier, G.;Jaffe, A. H.;Jaffe, T. R.;Jones, W. C.;Juvela, M.;Keihänen, E.;Keskitalo, R.;Kitaura, F.;Kneissl, R.;Knoche, J.;Kunz, M.;Kurki-Suonio, H.;Lagache, G.;Lamarre, J.-M.;Lasenby, A.;Lattanzi, M.;Lawrence, C. R.;Leonardi, R.;León-Tavares, J.;Levrier, F.;Liguori, M.;Lilje, P. B.;Linden-Vørnle, M.;López-Caniego, M.;Lubin, P. M.;Ma, Y.-Z.;Macías-Pérez, J. F.;Maffei, B.;Maino, D.;Mak, D. S. Y.;Mandolesi, N.;Mangilli, A.;Maris, M.;Martin, P. G.;Martínez-González, E.;Masi, S.;Matarrese, S.;McGehee, P.;Melchiorri, A.;Mennella, A.;Migliaccio, M.;Miville-Deschênes, M.-A.;Moneti, A.;Montier, L.;Morgante, G.;Mortlock, D.;Munshi, D.;Murphy, J. A.;Naselsky, P.;Nati, F.;Natoli, P.;Noviello, F.;Novikov, D.;Novikov, I.;Oxborrow, C. A.;Pagano, L.;Pajot, F.;Paoletti, D.;Perdereau, O.;Perotto, L.;Pettorino, V.;Piacentini, F.;Piat, M.;Pierpaoli, E.;Pointecouteau, E.;Polenta, G.;Ponthieu, N.;Pratt, G. W.;Puget, J.-L.;Puisieux, S.;Rachen, J. P.;Racine, B.;Reach, W. T.;Reinecke, M.;Remazeilles, M.;Renault, C.;Renzi, A.;Ristorcelli, I.;Rocha, G.;Rosset, C.;Rossetti, M.;Roudier, G.;Rubiño-Martín, J. A.;Rusholme, B.;Sandri, M.;Santos, D.;Savelainen, M.;Savini, G.;Scott, D.;Spencer, L. D.;Stolyarov, V.;Sudiwala, R.;Sunyaev, R.;Sutton, D.;Suur-Uski, A.-S.;Sygnet, J.-F.;Tauber, J. A.;Terenzi, L.;Toffolatti, L.;Tomasi, M.;Tucci, M.;Valenziano, L.;Valiviita, J.;Van Tent, B.;Vielva, P.;Villa, F.;Wade, L. A.;Wandelt, B. D.;Wang, W.;Wehus, I. K.;Yvon, D.;Zacchei, A.;Zonca, A.
By looking at the kinetic Sunyaev-Zeldovich effect (kSZ) in Planck nominal mission data, we present a significant detection of baryons participating in large-scale bulk flows around central galaxies (CGs) at redshift z ≈ 0.1. We estimate the pairwise...
The EROS collaboration has developed a real time alert system, which was operational in 1999 and 2000. A very long binary-lensing caustic crossing event, EROS-BLG-2000-5, was found in the 2000 season and monitored by EROS. EROS photometric data for t...
Recent surveys monitoring millions of light curves of resolved stars in the LMC have discovered several microlensing events. Unresolved stars could however significantly contribute to the microlensing rate towards the LMC. Monitoring pixels, as oppos...
Since 1996 EROS 2 has surveyed 440 square degrees at high Galactic latitude in order to search for high proper motion stars in the Solar neighbourhood. We present here the analysis of 250 square degrees for which we have three years of data. No objec...
We present the EROS nearby supernova ($z \sim 0.02 - 0.2$) search and the analysis of the first year of data (1997). A total of 80 square degrees were surveyed. Eight supernov{æ} were detected, four of which were spectroscopically identified as type ...
We present the EROS nearby supernova ($z \sim 0.02 - 0.2$) search and the analysis of the first year of data (1997). A total of 80 square degrees were surveyed. Eight supernov{æ} were detected, four of which were spectroscopically identified as type ...
LAL 04-91