1-m Byurakan Schmidt Reconstruction

Details 1-m Byurakan Schmidt Reconstruction 1-m Byurakan Schmidt Reconstruction

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007jena.confe..90d&link_type=abstract

"JENAM-2007, "Our non-stable Universe", held 20-25 August 2007 in Yerevan, Armenia. Abstract book, p. 90-90"

Physics

Scientific paper

Basic concept of 1-m reconstruction - to continue Markarian's method of SED AGN classification extrapolating it on deeper magnitude limits and wider redshift range with modern CCD detector and classification software. To realize this concept we plan to install a 4k x 4k CCD detector in telescope focus and equip it with 18 medium-band filters ~ 300 A FWHM. Filters will homogeneously cover entire optical spectral range from 3300 - 10000 AA. Methodically we plan to reach ABmag=23m with S/N~10 in 30 - 40 min in medium-band filters in UV and near the peak of detector quantum efficiency and in 160 - 180 min for near infrared filters.

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