Power of imaging surveys: Scientific goals of the reconstruction of 1-m Byurakan Schmidt Telescope

Details Power of imaging surveys: Scientific goals of the reconstruction of 1-m Byurakan Schmidt Telescope Power of imaging surveys: Scientific goals of the reconstruction of 1-m Byurakan Schmidt Telescope

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010vaoa.conf..350d&link_type=abstract

"Evolution of Cosmic Objects through their Physical Activity, Proceedings of the Conference dedicated to Viktor Ambartsumian's 1

Astronomy and Astrophysics

Astronomy

Scientific paper

Surveys performed with Schmidt telescopes had a great impact on the development of astronomy. Basic idea of 1m reconstruction - to continue Markarian's method of SED AGN classification, extrapolating it on deeper magnitude limits and wider redshift range using modern CCD detector and classification software. To realize this 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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