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dc.date.accessioned2023-07-17T21:16:36Z
dc.date.accessioned2023-09-08T18:15:54Z
dc.date.available2023-07-17T21:16:36Z
dc.date.available2023-09-08T18:15:54Z
dc.date.created2023-07-17T21:16:36Z
dc.date.issued2022
dc.identifierA&A 664, A196 (2022)
dc.identifier10.1051/0004-6361/202243604
dc.identifierhttps://repositorio.uchile.cl/handle/2250/194744
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/8752980
dc.description.abstractThe Complete Calibration of the Color-Redshift Relation survey (C3R2) is a spectroscopic program designed to empirically calibrate the galaxy color-redshift relation to the Euclid depth (I-E = 24.5), a key ingredient for the success of Stage IV dark energy projects based on weak lensing cosmology. A spectroscopic calibration sample that is as representative as possible of the galaxies in the Euclid weak lensing sample is being collected, selecting galaxies from a self-organizing map (SOM) representation of the galaxy color space. Here, we present the results of a near-infrared H- and K-band spectroscopic campaign carried out using the LUCI instruments at the LBT. For a total of 251 galaxies, we present new highly reliable redshifts in the 1.3 <= z <= 1.7 and 2 <= z <= 2.7 ranges. The newly-determined redshifts populate 49 SOM cells that previously contained no spectroscopic measurements and almost twice the occupation numbers of an additional 153 SOM cells. A final optical ground-based observational effort is needed to calibrate the missing cells, in particular in the redshift range 1.7 <= z <= 2.7, which lack spectroscopic calibration. In the end, Euclid itself will deliver telluric-free near-IR spectra that can complete the calibration.
dc.languageen
dc.publisherEDP Sciences
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/us/
dc.rightsAttribution-NonCommercial-NoDerivs 3.0 United States
dc.sourceAstronomy & Astrophysics
dc.subjectGalaxies: distances and redshifts
dc.subjectCatalogs
dc.subjectSurveys
dc.titleEuclid preparation XX. The complete calibration of the color-redshift relation survey: LBT observations and data release
dc.typeArtículo de revista


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