J/MNRAS/501/281ivo://CDS.VizieR/J/MNRAS/501/281CDSSolano E.Galvez-Ortiz M.C.Martin E.L.Gomez Munoz I.M.Rodrigo C.,Burgasser A.J.Lodieu N.Bejar V.J.S.Huelamo N.Morales-Calderon M.,Bouy H.2023-11-15T06:36:27Z2023-11-15T07:32:28ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frbrown-dwarfsvisible-astronomytrigonometric-parallaxproper-motionsstellar-spectral-typesUltracool dwarfs (UCDs) encompass a wide variety of compact stellar-like objects with spectra classified as late-M, L, T, and Y. Most of them have been discovered using wide-field imaging surveys. The Virtual Observatory (VO) has proven to be of great utility to efficiently exploit these astronomical resources. We aim to validate a VO methodology designed to discover and characterize UCDs in deep extragalactic surveys like Advance Large Homogeneous Area Medium-Band Redshift Astronomical (ALHAMBRA) and Cosmological Evolution Survey (COSMOS). Three complimentary searches based on parallaxes, proper motions and colours, respectively, were carried out. A total of 897 candidate UCDs were found, with only 16 previously reported in SIMBAD. Most of the new UCDs reported here are likely late-M and L dwarfs because of the limitations imposed by the utilization of optical (Gaia DR2 and r-band) data. We complement ALHAMBRA and COSMOS photometry with other catalogues in the optical and infrared using VOSA, a VO tool that estimates effective temperatures from the spectral energy distribution fitting to collections of theoretical models. The agreement between the number of UCDs found in the COSMOS field and theoretical estimations together with the low false-negative rate (known UCDs not discovered in our search) validates the methodology proposed in this work, which will be used in the forthcoming wide and deep surveys provided by the Euclid space mission. Simulations of Euclid number counts for UCDs detectable in different photometric passbands are presented for a wide survey area of 15000deg^2^, and the limitations of applicability of Euclid data to detect UCDs using the methods employed in this paper are discussed.2021MNRAS.501..281Shttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/501/281CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toI/345 : Gaia DR2 (Gaia Collaboration, 2018)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/501/281https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/501/281http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/501/281https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/501/281https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/501/281http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/501/281GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/501/281/catalog (The SVO archive of ultracool dwarfs identified in ALHAMBRA and COSMOS)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/501/281/catalog?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/501/281/catalog?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/501/281/catalog?GETtext/xml+votable180.050000true150.7661590581.91807990.0055555555555555565/6814 6/5819 7185 10153 10155-10156 11227 11249 11252 11424-11426 17767 17772-17773 19691 19694 20036 27245 27247 273441.9867573869263685e-19 3.916500758235022e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/501/281?format=asciiOpticaldefaultJ/MNRAS/501/281/catalogThe SVO archive of ultracool dwarfs identified in ALHAMBRA and COSMOSrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRAJ2000Right ascension (J2000)degpos.eq.ra;meta.mainDEJ2000Declination (J2000)degpos.eq.dec;meta.mainDistDistance from ConeSearch center positionarcsecpos.angDistancedoubleSurveySurvey (ALHAMBRA or COSMOS)meta.notecharIDSource identifier in ALHAMBRA or COSMOSmeta.id;meta.mainGaiaDR2? Gaia DR2 source identifiermeta.idnullableplx? Gaia DR2 parallaxmaspos.parallax.trigfloatnullablee_plx? Error on plxmasstat.error;pos.parallaxfloatnullablepmRA? Gaia DR2 proper motion in right ascensionmas/yrpos.pm;pos.eq.rafloatnullablee_pmRA? Error on pmRAmas/yrstat.error;pos.pm;pos.eq.rafloatnullablepmDE? Gaia DR2 proper motion in declinationmas/yrpos.pm;pos.eq.decfloatnullablee_pmDE? Error on pmDEmas/yrstat.error;pos.pm;pos.eq.decfloatnullableGmag? Gaia DR2 G-band magnitudemagphot.mag;em.optdoublenullableRPmag? Gaia DR2 RP-band magnitudemagphot.mag;em.opt.RdoublenullableMethodMethod used to identify the source (1)meta.notecharTeffEffective temperature estimated using VOSAKphys.temperature.effectiveintSpTypeSimSpectral type from Simbadsrc.spTypecharSpTypeSDSSSpectral type from SDSSsrc.spTypecharSpectrumLink to the SDSS DR16 spectrummeta.ref.urlchar