Hostname: page-component-78c5997874-ndw9j Total loading time: 0 Render date: 2024-11-19T07:12:54.971Z Has data issue: false hasContentIssue false
  • English
  • Français

Kiss: A New Digital Survey for Emission-Line Objects

Published online by Cambridge University Press:  25 May 2016

A. Kniazev ,
J. Salzer ,
V. Lipovetsky ,
T. Boroson ,
J. Moody ,
T. Thuan ,
Yu. Izotov ,
J. Herrero  and
L. Frattare
A. Kniazev
Affiliation:
Special Astrophysical Observatory, Russia
J. Salzer
Affiliation:
Wesleyan University, USA
V. Lipovetsky
Affiliation:
Special Astrophysical Observatory, Russia
T. Boroson
Affiliation:
NOAO, Gemini Project, USA
J. Moody
Affiliation:
Brigham Young University, USA
T. Thuan
Affiliation:
University of Virginia, USA
Yu. Izotov
Affiliation:
Main Astronomical Observatory, Ukraine
J. Herrero
Affiliation:
Wesleyan University, USA Center for Astrophysics, USA
L. Frattare
Affiliation:
Wesleyan University, USA Space Telescope Science Institute, USA

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We have initiated a major new survey for emission-line galaxies (ELGs) which we call the KPNO International Spectroscopic Survey (KISS). Survey observations began in March 1994 with the 0.61-m Burrell Schmidt telescope. The technique we employ combines the benefits of a traditional photographic objective-prism survey with the advantages of using a CCD detector. The field of view of our CCD is 1.1° square, and the prism employed provides a dispersion of 19 Å/pixel at 5000 Å. The spectral range covered (4800-5500 Å) is restricted by a specially designed filter that transmits from rest-frame Hβ to just shortward of the strong night-sky line at 5577 Å; this greatly reduces the sky background. We expect KISS to be sensitive to galaxies with magnitudes as faint as B = 20m –21m , much deeper than existing photographic surveys. Our initial pilot project covers 100 square degrees (Salzer et al. 1994) and overlaps the CfA/Dartmouth Century Redshift Survey (α = 8h 30m –16h 45m and δ = 29°–30°) in the North Galactic cap.

Type
Part 5. Extra-Galactic Astronomy
Information
Symposium - International Astronomical Union , Volume 179: New Horizons from Multi-Wavelength Sky Surveys , 1998 , pp. 302 - 304
Copyright
Copyright © Kluwer 1998 

References

Moreau, O. and Reboul, H., 1995. Astron. Astrophys. Suppl., 111, 169.Google Scholar
Salzer, J., et al. B.A.A.S., 26, 916.Google Scholar
Shergin, V.S., Kniazev, A.Y. and Lipovetsky, V.A. 1996. Astr. Nachrichten, 2, 95.CrossRefGoogle Scholar
Willmer, C.N.A., et al. Astrophys. J. Suppl., 104, 199.CrossRefGoogle Scholar