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Ruud, T. M.Fuskeland, U.Wehus, I. K.Vidal, M.Araujo, D.Bischoff, C.Buder, I.Chinone, Y.Cleary, K.Dumoulin, R. N.Kusaka, A.Monsalve, R.Næss, S. K.Newburgh, L. B.Reeves, R. A.Zwart, J. T. L.Bronfman Aguiló, LeonardoDavies, R. D.Davis, R.Dickinson, C.Eriksen, H. K.Gaier, T.Gundersen, J. O.Hasegawa, M.Hazumi, M.Huffenberger, K. M.Jones, M. E.Lawrence, C. R.Leitch, E. M.Limon, M.Miller, A. D.Pearson, T. J.Piccirillo, L.Radford, S. J. E.Readhead, A. C. S.Samtleben, D.Seiffert, M.Shepherd, M. C.Staggs, S. T.Tajima, O.Thompson, K. L.[The Q/U Imaging ExperimenT: Polarization Measurements of the Galactic Plane at 43 and 95 GHz]

Chiang, Yi-KuanOverzier, Roderik A.Gebhardt, KarlFinkelstein, Steven L.Chiang, Chi-TingHill, Gary J.Blanc Mendiberri, GuillermoDrory, NivChonis, Taylor S.Zeimann, Gregory R.Hagen, AlexSchneider, Donald P.Jogee, ShardhaCiardullo, RobinGronwall, Caryl[Surveying galaxy proto-clusters in emission: a large-scale structure at z = 2.44 and the outlook for hetdex]

Context. Extremely metal-poor (EMP) stars provide us with indirect information on the first generations of massive stars. The TOPoS survey has been designed to increase the census of these stars and to provide a chemical inventory that is as detailed as possible. Aims. Seven of the most iron-poor...


Bonifacio, P.Caffau, E.Spite, M.Spite, F.Sbordone, L.Monaco, L.François, P.Plez, B.Molaro, P.Gallagher, A.J.Cayrel, R.Christlieb, N.Klessen, R.S.Koch, A.Ludwig, H.-G.Steffen, M.Zaggia, S.Abate, C.[TOPoS: IV. Chemical abundances from high-resolution observations of seven extremely metal-poor stars]TOPoS: IV. Chemical abundances from high-resolution observations of seven extremely metal-poor stars

The VST Optical Imaging of the CDFS and ES1 Fields (VOICE) Survey is a Guaranteed Time programme carried out with the European Southern Observatory (ESO) VLT Survey Telescope (VST) telescope to provide deep optical imaging over two 4 deg2 patches of the sky centred on the Chandra Deep Field South...


Fu, L.Liu, D.Radovich, M.Liu, X.Pan, C.Fan, Z.Covone, G.Vaccari, M.Amaro, V.Brescia, M.Capaccioli, M.De Cicco, D.Grado, A.Limatola, L.Miller, L.Napolitano, N.R.Paolillo, M.Pignata, G.[Weak-lensing study in VOICE survey - I. Shear measurement]Weak-lensing study in VOICE survey - I. Shear measurement

Narayan, G.Rest, A.Tucker, B. E.Foley, R. J.Wood-Vasey, W. M.Challis, P.Stubbs, C.Kirshner, R. P.Aguilera, C.Becker, A. C.Blondin, S.Clocchiatti, A.Covarrubias, R.Damke, G.Davis, T. M.Filippenko, A. V.Ganeshalingam, M.Garg, A.Garnavich, P. M.Hicken, M.Jha, S. W.Krisciunas, K.Leibundgut, B.Li, W.Matheson, T.Miknaitis, G.Pignata, G.Prieto, J. L.Riess, A. G.Schmidt, B. P.Silverman, J. M.Smith, R. C.Sollerman, J.Spyromilio, J.Suntzeff, N. B.Tonry, J. L.Zenteno, A.[LIGHT CURVES OF 213 TYPE Ia SUPERNOVAE FROM THE ESSENCE SURVEY]LIGHT CURVES OF 213 TYPE Ia SUPERNOVAE FROM THE ESSENCE SURVEY

Smith, G. P.Mazzotta, P.Okabe, N.Ziparo, F.Mulroy, S. L.Babul, A.Finoguenov, A.McCarthy, I. G.Lieu, M.Bahé, Y. M.Bourdin, H.Evrard, A. E.Futamase, T.Haines, ChrisJauzac, M.Marrone, D. P.Martino, R.May, P. E.Taylor, J. E.Umetsu, K.[LoCuSS: Testing hydrostatic equilibrium in galaxy clusters]

Roukema, Boudewijn F.Buchert, ThomasFujii, HirokazuOstrowski, Jan J.[Is the baryon acoustic oscillation peak a cosmological standard ruler?]

Marchesi, StefanoTreister, Ezequiel.Civano, FrancescaElvis, MartinSalvato, M.Brusa, MarcellaComastri, A.Gilli, R.Hasinger, G.Lanzuisi, G.Miyaji, T.Urry, C. Megan[The Chandra COSMOS Legacy survey: optical/IR identifications]The Chandra COSMOS Legacy survey: optical/IR identifications

Civano, FrancescaTreister, Ezequiel.Marchesi, StefanoComastri, A.Urry, C. MeganElvis, MartinCappelluti NPuccetti, S.Brusa, MarcellaZamorani, G.Hasinger, G.[The Chandra Cosmos Legacy Survey: Overview and Point Source Catalog]The Chandra Cosmos Legacy Survey: Overview and Point Source Catalog

Mateos, S.Treister, Ezequiel.Warwick, R. S.Carrera, F J.Stewart, G. C.Ebrero, J.Della Ceca, R.Caccianiga, A.Gilli, R.Page, M. J.Tedds, J. A.Watson, M. G.Lamer, G.Saxton, R. D.Brunner, H.Page, C. G.[High precision X-ray log N - log S distributions : implications for the obscured AGN population.]High precision X-ray log N - log S distributions : implications for the obscured AGN population.

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