Showing results 59 to 78 of 91
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Publication Date | Article Title | Author(s) |
20-Feb-2019 | Mass Calibration of Optically Selected DES Clusters Using a Measurement of CMB-cluster Lensing with SPTpol Data | Raghunathan, S; Patil, S; Baxter, E; Benson, BA; Bleem, LE; et al |
Dec-2019 | Mass variance from archival X-ray properties of Dark Energy Survey Year-1 galaxy clusters | Farahi, A; Chen, X; Evrard, AE; Hollowood, DL; Wilkinson, R; et al |
May-2018 | A measurement of CMB cluster lensing with SPT and DES year 1 data | Baxter, EJ; Raghunathan, S; Crawford, TM; Fosalba, P; Hou, Z; et al |
Dec-2017 | Models of the strongly lensed quasar DES J0408-5354 | Agnello, A; Lin, H; Buckley-Geer, L; Treu, T; Bonvin, V; et al |
Apr-2019 | More out of less: an excess integrated Sachs-Wolfe signal from supervoids mapped out by the Dark Energy Survey | Kovacs, A; Sanchez, C; Garcia-Bellido, J; Elvin-Poole, J; Hamaus, N; et al |
May-2020 | Observation and confirmation of nine strong-lensing systems in Dark Energy Survey Year 1 data | Nord, B; Buckley-Geer, E; Lin, H; Kuropatkin, N; Collett, T; et al |
Aug-2019 | On the relative bias of void tracers in the Dark Energy Survey | Pollina, G; Hamaus, N; Paech, K; Dolag, K; Weller, J; et al |
Jul-2017 | Optical-SZE scaling relations for DES optically selected clusters within the SPT-SZ Survey | Saro, A; Bocquet, S; Mohr, J; Rozo, E; Benson, BA; et al |
Oct-2019 | Phenotypic redshifts with self-organizing maps: A novel method to characterize redshift distributions of source galaxies for weak lensing | Buchs, R; Davis, C; Gruen, D; DeRose, J; Alarcon, A; et al |
29-Oct-2014 | Planck 2013 results. I. Overview of products and scientific results | Planck Collaboration; Ade, PAR; Aghanim, N; Alves, MIR; Armitage-CaplanI, C; et al |
29-Oct-2014 | Planck 2013 results. XIX. The integrated Sachs-Wolfe effect | Planck Collaboration; Ade, PAR; Aghanim, N; Armitage-Caplan, C; Arnaud, M; et al |
1-Dec-2011 | Planck early results. I. The Planck mission | Ade, PAR; Aghanim, N; Arnaud, M; Ashdown, M; Aumont, J; et al |
1-Dec-2011 | Planck early results. II. The thermal performance of Planck | Ade, PAR; Aghanim, N; Arnaud, M; Ashdown, M; Aumont, J; et al |
1-Dec-2011 | Planck early results. IV. First assessment of the High Frequency Instrument in-flight performance | Ade, PAR; Aghanim, N; Ansari, R; Arnaud, M; Ashdown, M; et al |
1-Dec-2011 | Planck early results. VI. The High Frequency Instrument data processing | Ade, PAR; Aghanim, N; Ansari, R; Arnaud, M; Ashdown, M; et al |
1-Dec-2011 | Planck early results. VII. The Early Release Compact Source Catalogue | Ade, PAR; Aghanim, N; Arnaud, M; Ashdown, M; Aumont, J; et al |
1-Dec-2011 | Planck early results. VIII. The all-sky early Sunyaev-Zeldovich cluster sample | Ade, PAR; Aghanim, N; Arnaud, M; Ashdown, M; Aumont, J; et al |
1-Dec-2011 | Planck early results. XIX. All-sky temperature and dust optical depth from Planck and IRAS. Constraints on the “dark gas” in our Galaxy | Ade, PAR; Aghanim, N; Arnaud, M; Ashdown, M; Aumont, J; et al |
1-Dec-2011 | Planck early results. XVIII. The power spectrum of cosmic infrared background anisotropies | Ade, PAR; Aghanim, N; Arnaud, M; Ashdown, M; Aumont, J; et al |
1-Dec-2011 | Planck early results. XXVI. Detection with Planck and confirmation by XMM-Newton of PLCK G266.6–27.3, an exceptionally X-ray luminous and massive galaxy cluster at z ~ 1 | Aghanim, N; Arnaud, M; Ashdown, M; Atrio-Barandela, F; Aumont, J; et al |