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The z ~ 1.2 Galaxy Luminosity Function from The LCIR Survey

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 نشر من قبل Hsiao-Wen Chen
 تاريخ النشر 2001
  مجال البحث فيزياء
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 تأليف H.-W. Chen




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We present results from the Las Campanas Infrared Survey, designed to identify a statistically significant sample of z>=1 galaxies using photometric redshift techniques. Here we summarize the design and strategies of the survey and present the first estimate of the galaxy luminosity function at z>=1 based on H-band selected galaxies identified in our survey. Results of number count studies and luminosity function measurements indicate that most early-type galaxies were already in place by z~1.2 with a modest space density evolution and a mild luminosity evolution over that expected from passive evolution.



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