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Keck Spectroscopy and NICMOS Photometry of a Redshift z = 5.60 Galaxy

Weymann, Ray J. and Stern, Daniel and Bunker, Andrew and Spinrad, Hyron and Chaffee, Frederic H. and Thompson, Rodger I. and Storrie-Lombardi, Lisa J. (1998) Keck Spectroscopy and NICMOS Photometry of a Redshift z = 5.60 Galaxy. Astrophysical Journal, 505 (2). L95-L98. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20170323-101239876

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Abstract

We present Keck Low Resolution Imaging Spectrometer spectroscopy along with Near-Infrared Camera and Multiobject Spectrometer (NICMOS) F110W (~J) and F160W (~H) images of the galaxy HDF 4-473.0 in the Hubble Deep Field (HDF), with a detection of an emission line consistent with Lyα at a redshift of z=5.60. Attention to this object as a high-redshift galaxy was first drawn by Lanzetta, Yahil, & Fernandez-Soto and appeared in their initial list of galaxies with redshifts estimated from the Wide Field Planetary Camera 2 (WFPC2) HDF photometry. It was selected by us for spectroscopic observation, along with others in the HDF, on the basis of the NICMOS F110W and F160W and WFPC2 photometry. For H_0=65 km s^(-1) Mpc^(-1) and q_0=0.125, the use of simple evolutionary models along with the F814W (~I), F110W, and F160W magnitudes allow us to estimate the star formation rate (~13 M_☉ yr^(-1)). The colors suggest a reddening of E(B-V)~0.06. The measured flux in the Lyα line is approximately 1.0×10^(−17) ergs cm^(-2) s^(-1), and the rest-frame equivalent width, correcting for the absorption caused by intervening H I, is ~90 Å. The galaxy is compact and regular, but resolved, with an observed FWHM of ~0."44. Simple evolutionary models can accurately reproduce the colors, and these models predict the Lyα flux to within a factor of 2. Using this object as a template shifted to higher redshifts, we calculate the magnitudes through the F814W and two NICMOS passbands for galaxies at redshifts 6<z<10.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1086/311625DOIArticle
http://iopscience.iop.org/article/10.1086/311625PublisherArticle
https://arxiv.org/abs/astro-ph/9807208arXivDiscussion Paper
ORCID:
AuthorORCID
Stern, Daniel0000-0003-2686-9241
Storrie-Lombardi, Lisa J.0000-0002-5987-5210
Additional Information:© 1998 American Astronomical Society. Received 17 July 1998. Accepted 6 August 1998. Published 31 August 1998. The near-infrared observations are supported by NASA grant NAG5-3042 to the NICMOS instrument definition team. R. J. W. thanks the W. M. Keck Observatory and the Lick Observatory for their hospitality during the period when this work was carried out and P. McCarthy and D. Koo for useful discussions. A. B. and L. J. S. L. gratefully acknowledge financial support from NICMOS postdoctoral positions.
Group:Infrared Processing and Analysis Center (IPAC)
Funders:
Funding AgencyGrant Number
NASANAG5-3042
Subject Keywords:early universe; galaxies: distances and redshifts; galaxies: evolution; galaxies: formation
Issue or Number:2
Record Number:CaltechAUTHORS:20170323-101239876
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20170323-101239876
Official Citation:Ray J. Weymann et al 1998 ApJ 505 L95
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:75351
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:23 Mar 2017 19:04
Last Modified:03 Oct 2019 16:49

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