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arXiv · 2503.22559

Euclid Quick Data Release (Q1) Ultracool dwarfs in the Euclid Deep Field North

A. Mohandasan·R. L. Smart·C. Reylé·V. Le Brun·A. Pérez-Garrido·E. Bañados·B. Goldman·S. L. Casewell·M. R. Zapatero Osorio·T. Dupuy·M. Rejkuba·E. L. Martín·C. Dominguez-Tagle·M. {Ž}erjal·N. Huélamo·N. Lodieu·P. Cruz·R. Rebolo·M. W. Phillips·J. -Y. Zhang·N. Aghanim·B. Altieri·A. Amara·S. Andreon·N. Auricchio·C. Baccigalupi·M. Baldi·A. Balestra·S. Bardelli·P. Battaglia·A. Biviano·A. Bonchi·E. Branchini·M. Brescia·J. Brinchmann·S. Camera·G. Cañas-Herrera·V. Capobianco·C. Carbone·J. Carretero·S. Casas·M. Castellano·G. Castignani·S. Cavuoti·K. C. Chambers·A. Cimatti·C. Colodro-Conde·G. Congedo·C. J. Conselice·L. Conversi·Y. Copin·A. Costille·F. Courbin·H. M. Courtois·M. Cropper·A. Da Silva·H. Degaudenzi·G. De Lucia·H. Dole·M. Douspis·F. Dubath·X. Dupac·S. Dusini·S. Escoffier·M. Farina·F. Faustini·S. Ferriol·S. Fotopoulou·M. Frailis·E. Franceschi·S. Galeotta·K. George·W. Gillard·B. Gillis·C. Giocoli·J. Gracia-Carpio·B. R. Granett·A. Grazian·F. Grupp·S. V. H. Haugan·J. Hoar·W. Holmes·I. M. Hook·F. Hormuth·A. Hornstrup·K. Jahnke·M. Jhabvala·E. Keihänen·S. Kermiche·A. Kiessling·B. Kubik·K. Kuijken·M. Kümmel·M. Kunz·H. Kurki-Suonio·Q. Le Boulc'h·A. M. C. Le Brun·D. Le Mignant·S. Ligori·P. B. Lilje
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Abstract

Ultracool dwarfs (UCDs) encompass the lowest mass stars and brown dwarfs, defining the stellar substellar boundary. They have significant potential for advancing the understanding of substellar physics; however, these objects are challenging to detect due to their low luminosity. The wide coverage and deep sensitivity of the Euclid survey will increase the number of confirmed and well characterised UCDs by several orders of magnitude. In this study, we take advantage of the Euclid Quick Data Release (Q1) and in particular we look in detail at the known and new UCDs in the Euclid Deep Field North (22.9 deg2 down to JE = 24.5 mag), to understand the advantages of using the slitless Euclid spectroscopy. We compile a comparison sample of known UCDs and use their spectra to demonstrate the capability of Euclid to derive spectral types using a template matching method. This method is then applied to the spectra of the newly identified candidates. We confirm that 33 of these candidates are new UCDs, with spectral types ranging from M7 to T1 and JE = 17 to 21 mag. We look at their locus in colour colour diagrams and compare them with the expected colours of QSOs. A machine readable catalogue is provided for further study, containing both the comparison sample and the newly identified UCDs, along with their spectral classifications where the Q1 spectra quality allows for confident determination

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A. Mohandasan, R. L. Smart, C. Reylé, V. Le Brun, A. Pérez-Garrido, E. Bañados, B. Goldman, S. L. Casewell, M. R. Zapatero Osorio, T. Dupuy, M. Rejkuba, E. L. Martín, C. Dominguez-Tagle, M. {Ž}erjal, N. Huélamo, N. Lodieu, P. Cruz, R. Rebolo, M. W. Phillips, J. -Y. Zhang, N. Aghanim, B. Altieri, A. Amara, S. Andreon, N. Auricchio, C. Baccigalupi, M. Baldi, A. Balestra, S. Bardelli, P. Battaglia, A. Biviano, A. Bonchi, E. Branchini, M. Brescia, J. Brinchmann, S. Camera, G. Cañas-Herrera, V. Capobianco, C. Carbone, J. Carretero, S. Casas, M. Castellano, G. Castignani, S. Cavuoti, K. C. Chambers, A. Cimatti, C. Colodro-Conde, G. Congedo, C. J. Conselice, L. Conversi, Y. Copin, A. Costille, F. Courbin, H. M. Courtois, M. Cropper, A. Da Silva, H. Degaudenzi, G. De Lucia, H. Dole, M. Douspis, F. Dubath, X. Dupac, S. Dusini, S. Escoffier, M. Farina, F. Faustini, S. Ferriol, S. Fotopoulou, M. Frailis, E. Franceschi, S. Galeotta, K. George, W. Gillard, B. Gillis, C. Giocoli, J. Gracia-Carpio, B. R. Granett, A. Grazian, F. Grupp, S. V. H. Haugan, J. Hoar, W. Holmes, I. M. Hook, F. Hormuth, A. Hornstrup, K. Jahnke, M. Jhabvala, E. Keihänen, S. Kermiche, A. Kiessling, B. Kubik, K. Kuijken, M. Kümmel, M. Kunz, H. Kurki-Suonio, Q. Le Boulc'h, A. M. C. Le Brun, D. Le Mignant, S. Ligori, P. B. Lilje. 2025-03-28. Euclid Quick Data Release (Q1) Ultracool dwarfs in the Euclid Deep Field North. https://arxiv.org/abs/2503.22559

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