A catalog of polychromatic bulge-disk decompositions of ~ 17.600 galaxies in CANDELS

Understanding how bulges grow in galaxies is critical step towards unveiling the link between galaxy morphology and star-formation. To do so, it is necessary to decompose large sample of galaxies at different epochs into their main components (bulges and disks). This is particularly challenging, esp...

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Veröffentlicht in:	arXiv.org 2018-03
Hauptverfasser:	Dimauro, Paola, Huertas-Company, Marc, Daddi, Emanuele, Pérez-González, Pablo G, Bernardi, Mariangela, Barro, Guillermo, Buitrago, Fernando, Caro, Fernando, Cattaneo, Andrea, Dominguez-Sánchez, Helena, Faber, Sandra M, Häußler, Boris, Kocevski, Dale D, Koekemoer, Anton M, Koo, David C, Lee, Christoph T, Mei, Simona, Margalef-Bentabol, Berta, Primack, Joel, Rodriguez-Puebla, Aldo, Salvato, Mara, Shankar, Francesco, Tuccillo, Diego
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomical models Decomposition Galactic bulge Galactic evolution Galaxies Morphology Physics - Astrophysics of Galaxies Spectral energy distribution Star formation Stellar mass Surface brightness Websites
Online-Zugang:	Volltext
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Zusammenfassung:	Understanding how bulges grow in galaxies is critical step towards unveiling the link between galaxy morphology and star-formation. To do so, it is necessary to decompose large sample of galaxies at different epochs into their main components (bulges and disks). This is particularly challenging, especially at high redshifts, where galaxies are poorly resolved. This work presents a catalog of bulge-disk decompositions of the surface brightness profiles of ~17.600 H-band selected galaxies in the CANDELS fields (F160W
ISSN:	2331-8422
DOI:	10.48550/arxiv.1803.10234