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Deep H-Band Galaxy Counts and Half-Light Radii from Hubble Space Telescope/NICMOS Parallel Observations

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Published 1998 July 17 Copyright is not claimed for this article. Printed in U.S.A.
, , Citation Lin Yan et al 1998 ApJ 503 L19 DOI 10.1086/311521

1538-4357/503/1/L19

Abstract

We present deep galaxy counts and half-light radii from F160W (λc=1.6 μm) images obtained with the Near-Infrared Camera and Multiobject Spectrograph on the Hubble Space Telescope. Nearly 9 arcmin2 have been imaged with camera 3, with 3 σ depths ranging from H=24.3 to 25.5 in a 0farcs6 diameter aperture. The slope of the counts fainter than H=20 is 0.31, and the integrated surface density to H≤24.75 is 4×105 galaxies deg-2. The half-light radii of the galaxies decline steeply with apparent magnitude. At H=24, we are limited by both the delivered FWHM and the detection threshold of the images.

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10.1086/311521