Suchergebnisse

Spanish Institute of Health Carlos III‐Ministryof Economy and Competitiveness, Grant/Award Number: INMA Network G03/176,CB06/02/0041, and FIS‐FEDER: PI03/1615,PI04/1436, PI08/1151, PI04/2018, PI04/1509, PI04/1112, PI04/1931, PI05/1079,PI05/1052, PI06/1213, PI06/0867, PI07/0314, PI09/02647, PS09/00090, PI09/02311,MS11/0178, PI13/1944, PI13/2032, PI14/00891, PI16/1288, PI16/00261 and PI17/00663; Generalitat Valenciana, Grant/AwardNumber: Conselleria de Sanitat-048/2010 and060/2010 and FISABIO‐UGP 15‐230, 15‐244,and 15‐249; Universidad de Oviedo,Fundación Cajastur‐Liberbank, Department ofHealth of the Basque Government, Grant/Award Numbers: 2005111093 and2009111069; Provincial Government ofGipuzkoa, Grant/Award Numbers: DFG06/004 and DFG08/001; Fundació Maratò TV3,Grant/Award Number: 201622 10

This study was funded by grants from the Eulji University (grant numbers ESCAPE project FP7-ENV-2007-1-211250, DENAMIC project FP7-ENV-2011-282957, HELIX project FP7-ENV-2012-308333, and MEDALL project HEALTH.2010.2.4.5-1), from the Spanish Instituto de Salud Carlos III (grant numbers Red INMA G03/176; CB06/02/0041; PI03/1615 incl. FEDER funds, PI04/1112 incl. FEDER funds, PI041436, PI04/1509 incl. FEDER funds, PI04/1931 incl. FEDER funds, PI042018 incl. FEDER funds, PI05/1079 incl. FEDER funds, PI05/1052 incl. FEDER funds, FIS-PI06/0867, PI06/1213 incl. FEDER funds, PI07/0314 incl. FEDER funds, PI081151 incl. FEDER funds, FIS-PI09/00090, PI09/02311 incl. FEDER funds, PI09/02647 incl. FEDER funds, PI11/01007 incl. FEDER funds, PI11/02591 incl. FEDER funds, PI11/02038 incl. FEDER funds, PI13/1944 incl. FEDER funds, PI13/2032 incl. FEDER funds, PI13/02429 incl. FEDER funds, PI14/00891 incl. FEDER funds, PI14/01687 incl. FEDER funds, PI15/00118 incl. FEDER funds, PI16/1288 incl. FEDER funds, and PI17/00663 incl. FEDER funds, PI18/00547 incl. FEDER funds, PI18/00909 incl. FEDER funds; CP11/00178, CP15/00025, and CPII16/00051; MS13/00054 incl. FEDER funds), CIBERESP, Department of Health of the Basque Government (grant numbers 2005111093, 2013111089), Generalitat de Catalunya-CIRIT (grant numbers 1999SGR 00241), Generalitat Valenciana: FISABIO (grant numbers UGP 15-230, UGP-15-244, and UGP-15-249), Provincial Government of Gipuzkoa (grant number DFG06/002), Alicia Koplowitz Foundation 2017, Fundació La marató de TV3 (grant number090430), Obra Social Cajastur/Fundación Liberbank, Universidad de Oviedo, and annual agreements with the municipalities of the study area of the Gipuzkoa sub-cohort (Zumarraga, Urretxu , Legazpi, Azkoitia, Azpeitia and Beasain). ISGlobal is a member of the Agency for the Research Centres of Catalonia (CERCA) Programme, Generalitat de Catalunya.

This study was funded by grants from Instituto de Salud Carlos III and the Spanish Ministry of Health (Red INMA G03/176; CB06/02/0041; FIS 97/0588; 00/0021-2; PI061756; PS0901958; FIS-FEDER 03/1615; 04/1509; 04/1112; 04/1931; 05/1079; 05/1052; 06/1213; 07/0314; 09/02647; FIS-FEDER 18/00909; FIS-PI041436; FIS-PI081151; FIS-PI06/0867; FIS-PS09/00090; FIS-PI04/2018; FIS-PI09/02311; FIS PI11/01007; FIS-PI13/02429; MS13/00054, CPII18/00018; PI12/01890; CP13/00054; PI18/00825) University of Oviedo, Conselleria de Sanitat Generalitat Valenciana, Generalitat de Catalunya-CIRIT 1999SGR 00241, Generalitat de Catalunya-AGAUR 2009 SGR 501 and 2014 SGR 822. Department of Health of the Basque Government (2005111093, 2009111069, and 201311089) the Provincial Government of Gipuzkoa (DFG06/004 and DFG08/001), annual agreements with the municipalities of the study area of Gipuzkoa (Zumarraga, Urretxu, Legazpi, Azkoitia y Azpeitia y Beasain), Fundació Marató TV3 (20162210 and 090430). ISGlobal is a member of the CERCA Programme, Generalitat de Catalunya. Spanish Ministry of Economy and Competitiveness (SAF2012-32991 incl. FEDER funds), Agence Nationale de Securite Sanitaire de l'Alimentation de l'Environnement et du Travail (1262C0010), EU Commission (261357, 308333, 603794, and 634453).

ESCAPE Project. European Community's Seventh Framework Program (FP7/2007-2011-GA#211250). INMA. This study was funded by grants from Instituto de Salud Carlos III (Red INMA G03/176, CB06/02/0041, FIS-FEDER: PI03/1615,PI04/1509, PI04/1112, PI04/1931, PI04/1436, PI04/2018, PI05/1079, PI05/1052, PI06/1213, PI06/0867, PI07/0314, PI07/0252, PI08/1151, PI09/02647, PI09/02311, PS09/00090, PI11/02591, PI11/02038, PI13/02429, PI13/1944, PI13/2032, PI14/00891, PI14/01687,PI16/00118, PI17/00663, PI18/00909, and Miguel Servet-FEDER: MS13/00054, MS11/00178, MS16/00085, MSII16/00051, and CP18/00018), Generalitat de Catalunya-CIRIT 1999SGR 00241, La FundacióLa Marató de TV3 (090430), Generalitat Valenciana (FISABIO-UGP 15-230, 15-244, and 15-249), Fundación Alicia Koplowitz, Department of Health of the Basque Government (2005111093 and 2009111069), Provincial Government of Gipuzkoa (DFG06/004 and DFG08/001), Obra Social Cajastur/Fundación Liberbank, Universidad de Oviedo, Consejería de Salud de la Junta de Andalucía (grant number 183/07), EU Commission (QLK4-1999-01422, QLK4-2002 00603, CONTAMED FP7-ENV-12502, and FP7-ENV-2011 cod 282957), and Fundación Roger Torné. ISGlobal is a member of the CERCA Programme, Generalitat de Catalunya. (.)

The Javalambre Photometric Local Universe Survey (J-PLUS) is an ongoing 12-band photometric optical survey, observing thousands of square degrees of the Northern Hemisphere from the dedicated JAST/T80 telescope at the Observatorio Astrofísico de Javalambre (OAJ). The T80Cam is a camera with a field of view of 2 deg 2 mounted on a telescope with a diameter of 83 cm, and is equipped with a unique system of filters spanning the entire optical range (3500-10 000 Å). This filter system is a combination of broad-, medium-, and narrow-band filters, optimally designed to extract the rest-frame spectral features (the 3700-4000 Å Balmer break region, Hδ, Ca H+K, the G band, and the Mg b and Ca triplets) that are key to characterizing stellar types and delivering a low-resolution photospectrum for each pixel of the observed sky. With a typical depth of AB ∼21.25 mag per band, this filter set thus allows for an unbiased and accurate characterization of the stellar population in our Galaxy, it provides an unprecedented 2D photospectral information for all resolved galaxies in the local Universe, as well as accurate photo-z estimates (at the δ z/(1 + z)∼0.005-0.03 precision level) for moderately bright (up to r∼20 mag) extragalactic sources. While some narrow-band filters are designed for the study of particular emission features ([O II]/λ3727, Hα/λ6563) up to z< 0.017, they also provide well-defined windows for the analysis of other emission lines at higher redshifts. As a result, J-PLUS has the potential to contribute to a wide range of fields in Astrophysics, both in the nearby Universe (Milky Way structure, globular clusters, 2D IFU-like studies, stellar populations of nearby and moderate-redshift galaxies, clusters of galaxies) and at high redshifts (emission-line galaxies at z≈0.77, 2.2, and 4.4, quasi-stellar objects, etc.). With this paper, we release the first ∼1000 deg 2 of J-PLUS data, containing about 4.3 million stars and 3.0 million galaxies at r< 21 mag. With a goal of 8500 deg 2 for the total J-PLUS footprint, these numbers are expected to rise to about 35 million stars and 24 million galaxies by the end of the survey. © ESO 2019. ; Funding for the J-PLUS Project has been provided by the Governments of Spain and Aragon through the Fondo de Inversiones de Teruel, by the Spanish Ministry of Economy and Competitiveness (MINECO; under grants AYA2012-30789, AYA2013-40611-P, AYA2015-66211-C2-1-P, AYA2015-66211-C2-2, AYA2016-77846-P, AYA2016-77237-C3-1-P, AYA2016-75931-C2-1-P, AYA2017-86274-P, AGAURgrantSGR-661/2017, andICTS-2009-14), byFAPERJ the Government of Aragon, through the Grupo de Investigacion E16_17R, and by European FEDER funding (FCDD10-4E-867, FCDD13-4E-2685). Further support has been provided by the Ramon y Cajal programmes RYC-2016-20254, RYC-2011-08262 and RYC-2011-08529. This research has made use of the Spanish Virtual Observatory (http://svo.cab.inta-csic.es) supported from the Spanish MINECO through grant AYA2014-55216. We also acknowledge Spanish CSIC (I-COOP+ 2016 program) through grant COOPB20263. The Brazilian agencies FAPESP and the National Observatory of Brazil have also contributed to this project. We acknowledge financial support from the Fundacao Carlos Chagas Filho de Amparo a Pesquisa do Estado do Rio de Janeiro - FAPERJ (fellowship Nota 10, PDR-10), from CNPq through BP grant 312307/2015-2 and Universal Grants 459553/20143, PQ 302037/2015-2, and PDE 200289/2017-9), FINEP grants REF. 1217/13 -01.13.0279.00 and REF 0859/10 -01.10.0663.00, from FAPERJ grant E-26/202.835/2016, and CAPES (Science without Borders program, Young Talent Fellowship, BJT) through grants A062/2013 and CAPES-PNPD 2940/2011. The FAPESP grants no. 2015/12745-6, 2014/11338-5, 2014/07684-5, 2013/04582-4 and 2009/54202-8 are also acknowledged. Finally, the authors acknowledge partial support from grant PHY 14-30152; Physics Frontier Center/JINA Center for the Evolution of the Elements (JINA-CEE), awarded by the US National Science Foundation. ; Peer Reviewed