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arXiv · astro-ph/9912167

The Hubble Deep Field South - STIS Imaging

J. P. Gardner·S. A. Baum·T. M. Brown·C. M. Carollo·J. Christensen·I. Dashevsky·M. E. Dickinson·B. R. Espey·H. C. Ferguson·A. S. Fruchter·A. M. Gonnella·R. A. Gonzalez-Lopezlira·R. N. Hook·M. E. Kaiser·C. L. Martin·K. C. Sahu·S. Savaglio·T. E. Smith·H. I. Teplitz·R. E. Williams·J. Wilson
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Abstract

We present the imaging observations made with the Space Telescope Imaging Spectrograph of the Hubble Deep Field - South. The field was imaged in 4 bandpasses: a clear CCD bandpass for 156 ksec, a long-pass filter for 22-25 ksec per pixel typical exposure, a near-UV bandpass for 23 ksec, and a far-UV bandpass for 52 ksec. The clear visible image is the deepest observation ever made in the UV-optical wavelength region, reaching a 10 sigma AB magnitude of 29.4 for an object of area 0.2 square arcseconds. The field contains QSO J2233-606, the target of the STIS spectroscopy, and extends 50"x50" for the visible images, and 25"x25" for the ultraviolet images. We present the images, catalog of objects, and galaxy counts obtained in the field.

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J. P. Gardner, S. A. Baum, T. M. Brown, C. M. Carollo, J. Christensen, I. Dashevsky, M. E. Dickinson, B. R. Espey, H. C. Ferguson, A. S. Fruchter, A. M. Gonnella, R. A. Gonzalez-Lopezlira, R. N. Hook, M. E. Kaiser, C. L. Martin, K. C. Sahu, S. Savaglio, T. E. Smith, H. I. Teplitz, R. E. Williams, J. Wilson. 1999-12-08. The Hubble Deep Field South - STIS Imaging. https://doi.org/10.1086/301215

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