{"paper":{"title":"Combining Dark Energy Survey Science Verification Data with Near Infrared Data from the ESO VISTA Hemisphere Survey","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","astro-ph.IM"],"primary_cat":"astro-ph.CO","authors_text":"A. Carnero, A. Kim, A. Kupcu-Yoldas, A. Merson, B. Flaugher, Carlos E. Cunha, C. Gonzalez-Fernandez, C. Lidman, C. Miller, C. Sanchez, D. A. Finley, D. Capozzi, D. Gerdes, D. Lagattuta, D. L. DePoy, D. Tucker, E. Bertin, E. Gaztanaga, E. Gonzalez-Solares, E. Neilsen, E. Sanchez, F. B. Abdalla, F. J. Castander (IEEC Barcelona), F. Yuan, G. Bernstein, G. Tarle, H. Lin (Fermilab), H. T. Diehl, I. Sevilla, J. Bernstein, Jennifer L. Marshall, J. Findlay, J. Frieman, J. Gschwend, J. Marriner, Joseph J. Mohr, J. Peoples, J. R. Lewis, J. Thaler, J. Zuntz, K. Glazebrook, K. Honscheid, K. Kuehn, L. N. da Costa, M. A. G. Maia, Manda Banerji (UCL), M. Carrasco Kind, M. Childress, M. E. C. Swanson, M. J. Irwin, M. J. Jarvis, M. Lima, M. Makler, M. Sako, M. Schubnell, M. Soares-Santos, O. Lahav (UCL), P. Doel, P. Pellegrini, R. Bernstein, R. G. McMahon (IoA/KICC Cambridge), R. Miquel, R. Ogando, R. Saglia, R. Schindler, R. Sharp, R. Wechsler, S. Allam J. Annis, S. A. Uddin, S. Desai, S. E. Bosman, S. Jouvel (UCL), S. Koposov, S. Reed, T. M. Davis, V. Scarpine, W. Wester","submitted_at":"2014-07-14T20:00:23Z","abstract_excerpt":"We present the combination of optical data from the Science Verification phase of the Dark Energy Survey (DES) with near infrared data from the ESO VISTA Hemisphere Survey (VHS). The deep optical detections from DES are used to extract fluxes and associated errors from the shallower VHS data. Joint 7-band ($grizYJK$) photometric catalogues are produced in a single 3 sq-deg DECam field centred at 02h26m$-$04d36m where the availability of ancillary multi-wavelength photometry and spectroscopy allows us to test the data quality. Dual photometry increases the number of DES galaxies with measured V"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1407.3801","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}