Autor: |
A. Kniazev, J. Salzer, V. Lipovetsky, T. Boroson, J. Moody, T. Thuan, Yu. Izotov, J. Herrero, L. Frattare |
Rok vydání: |
1998 |
Zdroj: |
Symposium - International Astronomical Union. 179:302-304 |
ISSN: |
0074-1809 |
DOI: |
10.1017/s0074180900128852 |
Popis: |
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 = 8h30m–16h45m and δ = 29°–30°) in the North Galactic cap. |
Databáze: |
OpenAIRE |
Externí odkaz: |
|