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dc.contributor.author | Aslan Z. | |
dc.contributor.author | Bikmaev I. | |
dc.contributor.author | Vitrichenko E. | |
dc.contributor.author | Gumerov R. | |
dc.contributor.author | Dembo L. | |
dc.contributor.author | Kamus S. | |
dc.contributor.author | Keskin V. | |
dc.contributor.author | Kiziloglu U. | |
dc.contributor.author | Pavlinsky M. | |
dc.contributor.author | Panteleev L. | |
dc.contributor.author | Sakhibullin N. | |
dc.contributor.author | Selam S. | |
dc.contributor.author | Sunyaev R. | |
dc.contributor.author | Khamitov I. | |
dc.contributor.author | Yaskovich A. | |
dc.date.accessioned | 2018-09-17T21:11:23Z | |
dc.date.available | 2018-09-17T21:11:23Z | |
dc.date.issued | 2001 | |
dc.identifier.issn | 1063-7737 | |
dc.identifier.uri | https://dspace.kpfu.ru/xmlui/handle/net/134645 | |
dc.description.abstract | 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. © 2001 MAIK "Nauka/Interperiodica". | |
dc.relation.ispartofseries | Astronomy Letters | |
dc.subject | Astronomical observing techniques | |
dc.subject | Instrumentation | |
dc.title | Preliminary results of the alignment and Hartmann tests of the AZT-22 telescope | |
dc.type | Article | |
dc.relation.ispartofseries-issue | 6 | |
dc.relation.ispartofseries-volume | 27 | |
dc.collection | Публикации сотрудников КФУ | |
dc.relation.startpage | 398 | |
dc.source.id | SCOPUS10637737-2001-27-6-SID0007172257 |