Deep galaxy counts in the K band with the Kech telescope

• 1 January 1995
• journal article
• Published by American Astronomical Society in The Astrophysical Journal
• Vol. 438, L13-L16
• https://doi.org/10.1086/187703

Abstract

Keywords

• MONTE CARLO METHOD
• CORRELATION FUNCTION
• NEAR INFRARED
• STAR FORMATION
• STELLAR MAGNITUDE
• GALAXY CLUSTERS
• INFRARED ASTRONOMY
• COSMIC DUST
• GALAXIES
• RED SHIFT
• COSMOLOGY
• CUMULANT