Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993egte.conf...74s&link_type=abstract
In NASA. Ames Research Center, The Evolution of Galaxies and Their Environment p 74-75 (SEE N93-26706 10-90)
Astronomy and Astrophysics
Astronomy
Astronomical Models, Astronomical Photometry, Astronomical Spectroscopy, Galactic Clusters, Infrared Imagery, Near Infrared Radiation, Optical Measurement, Red Shift, Stellar Color, Stellar Spectra, Cameras, Stellar Magnitude
Scientific paper
We have obtained near-IR imaging of 3 moderate-z clusters on the 1.3 m at KPNO with SQIID, a new camera offering wide-field (5.5 arcmin) simultaneous JHK band imaging. Our photometry on a sample of approximately 100 likely member galaxies in one of the clusters, Abell 370 at z = 0.37, shows that we can obtain magnitudes good to 20 percent down to K = 18, considerably below the estimated K* = 16.5 at this redshift. These data indicate that there are no systematic problems in obtaining photometry at faint levels with SQIID. With the development of larger arrays, the field is open to progress. The resulting J, H, and K data for three clusters are combined with previously obtained multiband optical photometry. We present an investigation of the spectral properties and evolution of the dominant cold stellar populations by comparing optical-to-IR colors and color-magnitude diagrams to predictions from population synthesis models and galaxy spectral evolution codes.
Dickinson Mark Everett
Eisenhardt Peter R. M.
Stanford Spencer A.
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