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Radio Observations of the Hubble Deep Field South Region IV: Optical Properties of the Faint Radio Population
M. T. Huynh, C. A. Jackson, R. P. Norris +1
The Australia Telescope Hubble Deep Field-South (ATHDFS) survey of the Hubble Deep Field South reaches sensitivities of ~10 miceoJyJy at 1.4, 2.5, 5.2 and 8.7 GHz, making the ATHDF…
High Resolution Spectra of Novae and the Quadratic Zeeman Effect
Robert Williams, Elena Mason
High resolution spectra of novae after outburst reveal distinctive characteristics in the line profiles and intensities. The higher Balmer lines are often broader than the lower me…
The Hubble Deep Field South Flanking Fields
Ray A. Lucas, Stefi A. Baum, Thomas M. Brown +22
As part of the Hubble Deep Field South program, a set of shorter 2-orbit observations were obtained of the area adjacent to the deep fields. The WFPC2 flanking fields cover a conti…
The Internal Extinction Curve of NGC 6302 and its Extraordinary Spectrum
Brent A. Groves, Michael A. Dopita, Robert E. Williams +1
In this paper we present a new method for obtaining the optical wavelength-dependent reddening function of planetary nebulae, using the nebular and stellar continuum. The data used…
Emission-Line Galaxies from the NICMOS/HST GRISM Parallel Survey
P. J. McCarthy, L. Yan, W. Freudling +10
We present the first results of a survey of random fields with the slitless G141 () grism on NICMOS. Approximately 64 square arcminutes have been observed at i…
The Hubble Deep Field: Observations, Data Reduction, and Galaxy Photometry
Robert E. Williams, the HDF team
The Hubble Deep Field (HDF) is a Director's Discretionary program on HST in Cycle 5 to image an undistinguished field at high Galactic latitude in four passbands as deeply as reaso…