Deep Near-Infrared Imaginmg of Galaxies at z > 2 with Subaru: Color and Magnitude Distribution in HDF-N and the 53W002 Field

dc.creatorYamada, Toru
dc.creatorKajisawa, Masaru
dc.date2002-02-22
dc.date.accessioned2026-07-07T02:02:53Z
dc.date.available2026-07-07T02:02:53Z
dc.descriptionWe present the results of the deep NIR imaging observations using the Subaru telescope. At the Hubble Deep Field North, we obtained the new and deepest K'-band image (10 hours) to study the rest-frame optical morphology of galaxies at z > 3 and the stellar mass distribution of galaxies at 2 < z < 4.5. We also study the rest-frame optical properties of the 'building blocks' in the field of 53W002 and overall color distribution there. We then combined these data to compare the color and magnitude distribution in these two fields. The opt-NIR color-magnitude distributions in the two fields looks very similar and we report the conspicuous color change below K_AB =22 and discuss the cause of the feature.
dc.description4 pages text, 5 jpg figures, for Proceedings, Mass of Galaxies at Low and High Redshift, Venice, October 2001, eds. R. Bender and A. Renzini (ESO Astrophysics Symposia, Springer-Verlag
dc.identifierhttps://arxiv.org/abs/astro-ph/0202413
dc.identifierhttp://arxiv.org/abs/astro-ph/0202413
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4199
dc.subjectAstrophysics
dc.titleDeep Near-Infrared Imaginmg of Galaxies at z > 2 with Subaru: Color and Magnitude Distribution in HDF-N and the 53W002 Field
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