Thompson, D. J. and Djorgovski, S. (1990) Spectroscopy of quasar candidates from the University of Michigan low-dispersion survey. Publications of the Astronomical Society of the Pacific, 102 (655). pp. 959-965. ISSN 0004-6280. https://resolver.caltech.edu/CaltechAUTHORS:20190827-082632491
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Abstract
We present the results of long-slit CCD spectroscopy on 39 objects and four close companions from the University of Michigan objective-prism survey lists. Twelve of them are quasars with redshifts ranging from 0.326 to 2.852, and an additional 12 objects (including companions) are Seyferts or active galaxies ranging in redshift from 0.0365 to 0.227. UM 443 may be a broad absorption-line quasar. UM 565 is a star with a puzzling spectrum. Spectra are presented for a total of 25 objects.
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| Additional Information: | © 1990 The Astronomical Society of the Pacific. Received 1990 June 8. We are indebted to the staffs of Las Campanas Observatory (especially Oscar Duahalde, Angel Guerra, Fernando Peralta, and Alberto Zuniga); Cerro Tololo Observatory (especially M. Hernandez, H. Tirado, R. Venegas, and M. Navarete); and Palomar Observatory (especially J. Carrasco, J. Henning, and D. Tennant), for their help during the observations. This work was supported in part by a Kingsley Foundaton Fellowship (D. J.T.), the Alfred P. Sloan Foundation, and the California Institute of Technology (S.G.D.). | ||||||||
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| Subject Keywords: | galaxies: redshifts-quasars-redshifts-spectroscopy | ||||||||
| Issue or Number: | 655 | ||||||||
| Record Number: | CaltechAUTHORS:20190827-082632491 | ||||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20190827-082632491 | ||||||||
| Official Citation: | D. J. Thompson and S. Djorgovski 1990 PASP 102 959 | ||||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | ||||||||
| ID Code: | 98257 | ||||||||
| Collection: | CaltechAUTHORS | ||||||||
| Deposited By: | Tony Diaz | ||||||||
| Deposited On: | 27 Aug 2019 16:15 | ||||||||
| Last Modified: | 03 Oct 2019 21:39 |
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