Morphological analysis of HDF-N and HDF-S (Trujillo+, 2004)

Details Morphological analysis of HDF-N and HDF-S (Trujillo+, 2004) Morphological analysis of HDF-N and HDF-S (Trujillo+, 2004)

Feb 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ycat..73550082t&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/355/82. Originally published in: 2004MNRAS.355...82T

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Galaxies: Optical, Morphology, Redshifts

Scientific paper

Each HDF image consists of a 2.5x2.5arcmin2 Wide Field Pla Camera 2 (WFPC2) pointing. The images were acquired through the broad-band F300W, F450W, F606W and F814W filters. For the present work we have used the publicly available reduced F606W and F814W Version 2 drizzled images with a sampling of 0.04arcsec/pix and a total exposure time of 109050s (F606W; HDF-N), 123600s (F814W; HDF-N), 97200s (F606W; HDF-S) and 112200s (F814W; HDF-S). The high sampling of these images avoids the undersampling problems affecting other Hubble Space Telescope (HST) images.
(1 data file).

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