Accès ouvert déclaré
2025
preprint
Euclid: Quick Data Release (Q1) -- A census of dwarf galaxies across a range of distances and environments
F. R. Marleau, Rebecca Habas, D. Carollo, C. Tortora, Pierre-Alain Duc, Elisabeth Sola, T. Saifollahi, M. Fügenschuh, M. Walmsley, Raphael Zöller, A. Ferré-Mateu, M. Cantiello, M Urbano, Elham Saremi, Rosalia Ragusa, R. Laureijs, M. Hilker, Oliver Müller, Mélina Poulain, R. F. Peletier, Stefan Sprenger, O. Marchal, B Altieri, A Amara, S. Andreon, N. Auricchio, H Aussel, C. Baccigalupi, M. Baldi, A. Balestra, S Bardelli, Alberto Basset, P Battaglia, R. Bender, A. Biviano, D. Bonino, E. Branchini, M Brescia, J Brinchmann, S. Camera, G Cañas-Herrera, V Capobianco, J. Carretero, S. Casas, M. Castellano, G Castignani, S Cavuoti, A. Cimatti, C. Colodro-Conde, G. Congedo, C. J. Conselice L. Conversi, L. Corcione, F Courbin, H. M. Courtois, M. Cropper, Jean‐Charles Cuillandre, A da Silva, H. Degaudenzi, G. De Lucia, A.M Di Giorgio, H. Dole, F. Dubath, X. Dupac, S. Dusini, M. Farina, F Faustini, S. Ferriol, P Fosalba, S. Fotopoulou, E. Franceschi, P. Franzetti, M. Fumana, B. Gillis, C. Giocoli, B. R. Granett, A. Grazian, F. Grupp, S Gwyn, S. V. H. Haugan, Harald J. Hoekstra, W. Holmes, F. Hormuth, P. Hudelot, K. Jahnkę, M. Jhabvala, B Joachimi, E Keihänen, S. Kermiche, A. Kiessling, B. Kubik, M. Kümmel, M Kunz, H Kurki-Suonio, O. Lahav, Q. Le Boulc'h, A.M.C Le Brun, D. Le Mignant, S Ligori, P. B. Lilje, V. Lindholm, I. Lloro, G. Mainetti, D. Maino, E. Maiorano, O Mansutti, S Marcin, O Marggraf, M. Martinelli, N. Martinet, R Massey, S. Maurogordato, E. Medinaceli, Sitao Mei, M. Melchior, Y. Mellier, E. Merlin, G. Meylan, Antonio M. Mora, M. Moresco, L. Moscardini, R. Nakajima, C. Neissner, S. -M. Niemi, J.W Nightingale, C. Padilla, S. Paltani, F. Pasian, K. Pedersen, V. Pettorino, S. Pires, G. Polenta, M Poncet, L. A. Popa, F. Raison, R Rebolo, A. Renzi, J. Rhodes, G. Riccio, E. Romelli, M. Roncarelli, E. Rossetti, B. Rusholme, R. Saglia, Z. Sakr, Ariel G. Sánchez, D. Sapone, B. Sartoris, M. Sauvage, J.A Schewtschenko, M. Schirmer, Peter Schneider, M. Scodeggio, G. Seidel, M. D. Seiffert, S. Serrano, Paul Simon, G. Sirri, J. Skottfelt, L. Stanco, P. Tallada-Crespí, D. Tavagnacco, A. N. Taylor, Harry I. Teplitz, I Tereno, F. Torradeflot, I. Tutusaus, L. Valenziano, J. Valiviita, A Veropalumbo, Y. Wang, A Zacchei, F. M. Zerbi, E. Zucca, M. Bolzonella, C. Burigana, R. Cabanac, L. Gabarra, V. Scottez, D Scott
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Le résumé fourni par la source
The Euclid Q1 fields were selected for calibration purposes in cosmology and are therefore relatively devoid of nearby galaxies. However, this is precisely what makes them interesting fields in which to search for dwarf galaxies in local density environments. We take advantage of the unprecedented depth, spatial resolution, and field of view of the Euclid Quick Release (Q1) to build a census of dwarf galaxies in these regions. We have identified dwarfs in a representative sample of 25 contiguous tiles in the Euclid Deep Field North (EDF-N), covering an area of 14.25 sq. deg. The dwarf candidates were identified using a semi-automatic detection method, based on properties measured by the Euclid pipeline and listed in the MER catalogue. A selection cut in surface brightness and magnitude was used to produce an initial dwarf candidate catalogue, followed by a cut in morphology and colour. This catalogue was visually classified to produce a final sample of dwarf candidates, including their morphology, number of nuclei, globular cluster (GC) richness, and presence of a blue compact centre. We identified 2674 dwarf candidates, corresponding to 188 dwarfs per sq. deg. The visual classification of the dwarfs reveals a slightly uneven morphological mix of 58% ellipticals and 42% irregulars, with very few potentially GC-rich (1.0%) and nucleated (4.0%) candidates but a noticeable fraction (6.9%) of dwarfs with blue compact centres. The distance distribution of 388 (15%) of the dwarfs with spectroscopic redshifts peaks at about 400 Mpc. Their stellar mass distribution confirms that our selection effectively identifies dwarfs while minimising contamination. The most prominent dwarf overdensities are dominated by dEs, while dIs are more evenly distributed. This work highlights Euclid's remarkable ability to detect and characterise dwarf galaxies across diverse masses, distances, and environments.
Ce résumé expose les affirmations des auteurs. BNTIC ne l’interprète pas comme une validation indépendante des résultats.
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Les sujets associés
Astronomy and Astrophysical ResearchAstronomical Observations and Instrumentation