Мақола

Preliminary results of the alignment and Hartmann tests of the AZT-22 telescope

Z. AslanTUBITAK National Observatory, Antalia, TurkeyI. BikmaevKazan State University, Kremlevskaya ul. 18, Kazan, 420008, Tatarstan, RussiaÉ. A. VitrichenkoSpace Research Institute, Russian Academy of Sciences, Profsoyuznaya ul. 84/32, Moscow, 117810, RussiaR. I. GumerovKazan State University, Kremlevskaya ul. 18, Kazan, 420008, Tatarstan, RussiaL. A. DemboS. F. KamusV. KeskínAegean University, Izmir, TurkeyÜ. KızıloğluMiddle East Technical University, Ankara, 06531, TurkeyM. PavlinskySpace Research Institute, Russian Academy of Sciences, Profsoyuznaya ul. 84/32, Moscow, 117810, RussiaL. N. PanteleevН. А. СахибуллинKazan State University, Kremlevskaya ul. 18, Kazan, 420008, Tatarstan, RussiaS. O. SelamAnkara University, Ankara, TurkeyR. SunyaevSpace Research Institute, Russian Academy of Sciences, Profsoyuznaya ul. 84/32, Moscow, 117810, RussiaI. KhamitovAstronomical Institute, Academy of Sciences of Uzbekistan, Astronomicheskaya ul. 33, Tashkent, 700052, UzbekistanA. YaskovichSpace Research Institute, Russian Academy of Sciences, Profsoyuznaya ul. 84/32, Moscow, 117810, Russia

Astronomy Lettersjournal2001en

ABI

Аннотация

The AZT-22 telescope installed in Turkey (Antalia) was aligned and tested on stars by the Hartmann method. The rms normal deviation of an equivalent optical system is 0.040±0.016 µm. The circle of confusion is 0.40±0.04 arcsec in diameter at a 50% energy level.

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Historical Astronomy and Related Studies History and Developments in Astronomy Historical and Architectural Studies

Идентификаторлар

DOI: 10.1134/1.1374679

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