/ftp/cats/ii/357



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II/357        The Dark Energy Survey (DES): Data Release 1       (Abbott+, 2018)
The following files can be converted to FITS (extension .fit or fit.gz)
	des_dr1.sam
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=II/357
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drwxr-xr-x 351 cats archive 8192 Mar 25 10:13 [Up] drwxr-xr-x 5 cats archive 4096 Dec 20 22:48 [TAR file] -rw-r--r-- 1 cats archive 462 Dec 20 12:08 .message -r--r--r-- 1 cats archive 39237 Apr 9 2020 ReadMe -rw-r--r-- 1 cats archive 1513 Dec 20 12:08 +footg5.gif -rw-r--r-- 1 cats archive 9928 Dec 20 12:08 +footg8.gif -r--r--r-- 1 cats archive 478884 Mar 9 2020 des_dr1.sam.gz [Uncompressed] -rw-r--r-- 1 cats archive 60480 Aug 22 2022 tab_2357_1_II_357_des_dr1.moc.fits
Beginning of ReadMe : II/357 The Dark Energy Survey (DES): Data Release 1 (Abbott+, 2018) ================================================================================ The Dark Energy Survey: Data Release 1. Abbott T.M.C., Abdalla F.B., Allam S., Amara A., Annis J., Asorey J., Avila S., Ballester O., Banerji M., Barkhouse W., Baruah L., Baumer M., Bechtol K., Becker M.R., Benoit-Levy A., Bernstein G.M., Bertin E., Blazek J., Bocquet S., Brooks D., Brout D., Buckley-Geer E., Burke D.L., Busti V., Campisano R., Cardiel-Sas L., Rosell A.C., Kind M.C., Carretero J., Castander F.J., Cawthon R., Chang C., Chen X., Conselice C., Costa G., Crocce M., Cunha C.E., D'Andrea C.B., da Costa L.N., Das R., Daues G., Davis T.M., Davis C., De Vicente J., DePoy D.L., DeRose J., Desai S., Diehl H.T., Dietrich J.P., Dodelson S., Doel P., Drlica-Wagner A., Eifler T.F., Elliott A.E., Evrard A.E., Farahi A., Neto A.F., Fernandez E., Finley D.A., Flaugher B., Foley R.J., Fosalba P., Friedel D.N., Frieman J., Garcia-Bellido J., Gaztanaga E., Gerdes D.W., Giannantonio T., Gill M.S.S., Glazebrook K., Goldstein D.A., Gower M., Gruen D., Gruendl R.A., Gschwend J., Gupta R.R., Gutierrez G., Hamilton S., Hartley W.G., Hinton S.R., Hislop J.M., Hollowood D., Honscheid K., Hoyle B., Huterer D., Jain B., James D.J., Jeltema T., Johnson M.W.G., Johnson M.D., Kacprzak T., Kent S., Khullar G., Klein M., Kovacs A., Koziol A.M.G., Krause E., Kremin A., Kron R., Kuehn K., Kuhlmann S., Kuropatkin N., Lahav O., Lasker J., Li T.S., Li R.T., Liddle A.R., Lima M., Lin H., Lopez-Reyes P., MacCrann N., Maia M.A.G., Maloney J.D., Manera M., March M., Marriner J., Marshall J.L., Martini P., McClintock T., McKay T., McMahon R.G., Melchior P., Menanteau F., Miller C.J., Miquel R., Mohr J.J., Morganson E., Mould J., Neilsen E., Nichol R.C., Nogueira F., Nord B., Nugent P., Nunes L., Ogando R.L.C., Old L., Pace A.B., Palmese A., Paz-Chinchon F., Peiris H.V., Percival W.J., Petravick D., Plazas A.A., Poh J., Pond C., Porredon A., Pujol A., Refregier A., Reil K., Ricker P.M., Rollins R.P., Romer A.K., Roodman A., Rooney P., Ross A.J., Rykoff E.S., Sako M., Sanchez M.L., Sanchez E., Santiago B., Saro A., Scarpine V., Scolnic D., Serrano S., Sevilla-Noarbe I., Sheldon E., Shipp N., Silveira M.L., Smith M., Smith R.C., Smith J.A., Soares-Santos M., Sobreira F., Song J., Stebbins A., Suchyta E., Sullivan M., Swanson M.E.C., Tarle G., Thaler J., Thomas D., Thomas R.C., Troxel M.A., Tucker D.L., Vikram V., Vivas A.K., Walker A.R., Wechsler R.H., Weller J., Wester W., Wolf R.C., Wu H., Yanny B., Zenteno A., Zhang Y., Zuntz J., Juneau S., Fitzpatrick M., Nikutta R., Nidever D., Olsen K., Scott A. (The NOAO Data Lab) <Astrophys. J. Suppl., 239, 18 (2018)> =2018ApJS..239...18A ================================================================================ ADC_Keywords: Surveys; Photometry, ugriz; Reddening Keywords: astronomical databases: miscellaneous ; catalogs ; cosmology: observations ; surveys ; techniques: image processing ; techniques: photometric Abstract: We describe the first public data release of the Dark Energy Survey, DES DR1, consisting of reduced single-epoch images, co-added images, co-added source catalogs, and associated products and services assembled over the first 3yr of DES science operations. DES DR1 is based on optical/near-infrared imaging from 345 distinct nights (2013 August to 2016 February) by the Dark Energy Camera (DECam) mounted on the 4m Blanco telescope at the Cerro Tololo Inter-American Observatory in Chile. We release data from the DES wide-area survey covering  5000deg^2^ of the southern Galactic cap in five broad photometric bands, grizY. DES DR1 has a median delivered point-spread function of g=1.12, r=0.96, i=0.88, z=0.84, and Y=0.90" FWHM, a photometric precision of <1% in all bands, and an astrometric precision of 151mas. The median co-added catalog depth for a 1.95" diameter aperture at signal-to-noise ratio (S/N)=10 is g=24.33, r=24.08, i=23.44, z=22.69, and Y=21.44mag. DES DR1 includes nearly 400 million distinct astronomical objects detected in  10000 co-add tiles of size 0.534deg^2^ produced from  39000 individual exposures. Benchmark galaxy and stellar samples contain  310 million and  80 million objects, respectively, following a basic object quality selection. DES DR1 constitutes the largest photometric data set to date at the achieved depth and photometric precision. Acknowledging the Dark Energy Survey (DES) in publications: This project used public archival data from the Dark Energy Survey (DES). Funding for the DES Projects has been provided by the U.S. Department of Energy, the U.S. National Science Foundation, the Ministry of Science and Education of Spain, the Science and Technology Facilities Council of the United Kingdom, the Higher Education Funding Council for England, the National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign, the Kavli Institute of Cosmological Physics at the University of Chicago, the Center for Cosmology and Astro-Particle Physics at the Ohio State University, the Mitchell Institute for Fundamental Physics and Astronomy at Texas A&M University, Financiadora de Estudos e Projetos, Fundacao Carlos Chagas Filho de Amparo a Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Cientifico e Tecnologico and the Ministerio da Ciencia, Tecnologia e Inovacao, the Deutsche Forschungsgemeinschaft and the Collaborating Institutions in the Dark Energy Survey. The Collaborating Institutions are Argonne National Laboratory, the University of California at Santa Cruz, the University of Cambridge, Centro de Investigaciones Energeticas, Medioambientales y Tecnologicas-Madrid, the University of Chicago, University College London, the DES-Brazil Consortium, the University of Edinburgh, the Eidgenossische Technische Hochschule (ETH) Zurich, Fermi National Accelerator Laboratory, the University of Illinois at Urbana-Champaign, the Institut de Ciencies de l'Espai (IEEC/CSIC), the Institut de Fisica d'Altes Energies, Lawrence Berkeley National Laboratory, the Ludwig-Maximilians Universitat Munchen and the associated Excellence Cluster Universe, the University of Michigan, the National Optical Astronomy Observatory, the University of Nottingham, The Ohio State University, the OzDES Membership Consortium, the University of Pennsylvania, the University of Portsmouth, SLAC National Accelerator Laboratory, Stanford University, the University of Sussex, and Texas A&M University. Based in part on observations at Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory, which is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation. See http://des.ncsa.illinois.edu/thanks for the TeX version.