Please use this identifier to cite or link to this item: http://repositorio.unicamp.br/jspui/handle/REPOSIP/341157
Type: Artigo
Title: Brown dwarf census with the Dark Energy Survey year 3 data and the thin disc scale height of early L types
Author: Rosell, A. C.
Santiago, B.
dal Ponte, M.
Burningham, B.
da Costa, L. N.
James, D. J.
Marshall, J. L.
McMahon, R. G.
Bechtol, K.
De Paris, L.
Li, T.
Pieres, A.
Garcia-Bellido, J.
Abbott, T. M. C.
Annis, J.
Avila, S.
Bernstein, G. M.
Brooks, D.
Burke, D. L.
Kind, M. C.
Carretero, J.
De Vicente, J.
Drlica-Wagner, A.
Fosalba, P.
Frieman, J.
Gaztanaga, E.
Gruendl, R. A.
Gschwend, J.
Gutierrez, G.
Hollowood, D. L.
Maia, M. A. G.
Menanteau, F.
Miquel, R.
Plazas, A. A.
Roodman, A.
Sanchez, E.
Scarpine, V.
Schindler, R.
Serrano, S.
Sevilla-Noarbe, I.
Smith, M.
Sobreira, F.
Soares-Santos, M.
Suchyta, E.
Swanson, M. E. C.
Tarle, G.
Vikram, V.
Walker, A. R.
Abstract: In this paper we present a catalogue of 11 745 brown dwarfs with spectral types ranging from L0 to T9, photometrically classified using data from the Dark Energy Survey (DES) year 3 release matched to the Vista Hemisphere Survey (VHS) DR3 and Wide-field Infrared Survey Explorer (WISE) data, covering approximate to 2400 deg(2) up to i(AB) = 22. The classification method follows the same phototype method previously applied to SDSS-UKIDSS-WISE data. The most significant difference comes from the use of DES data instead of SDSS, which allow us to classify almost an order of magnitude more brown dwarfs than any previous search and reaching distances beyond 400 pc for the earliest types. Next, we also present and validate the GalmodBD simulation, which produces brown dwarf number counts as a function of structural parameters with realistic photometric properties of a given survey. We use this simulation to estimate the completeness and purity of our photometric LT catalogue down to i(AB) = 22, as well as to compare to the observed number of LT types. We put constraints on the thin disc scale height for the early L (L0-L3) population to be around 450 pc, in agreement with previous findings. For completeness, we also publish in a separate table a catalogue of 20 863M dwarfs that passed our colour cut with spectral types greater than M6. Both the LT and the late M catalogues are found at DES release page https://des.ncsa.illinois.edu/releases/other/y3-mlt.
Subject: Fotometria - Técnica
Catálogos
Levantamentos
Galáxias anãs
Galáxias
Estrelas
Photometry - Technique
Catalogs
Surveys
Dwarf galaxies
Galaxies
Stars
Country: Reino Unido
Editor: Oxford University Press
Rights: aberto
Identifier DOI: 10.1093/mnras/stz2398
Address: https://academic.oup.com/mnras/article/489/4/5301/5561500
Date Issue: 2019
Appears in Collections:IFGW - Artigos e Outros Documentos

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