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 |
|