Hostname: page-component-848d4c4894-2xdlg Total loading time: 0 Render date: 2024-06-16T19:17:43.779Z Has data issue: false hasContentIssue false
  • English
  • Français

Photometric Facilities of the AIST Space Project

Published online by Cambridge University Press:  07 August 2017

I.M. Kopylov ,
D.L. Gorshanov  and
M.S. Chubey
I.M. Kopylov
Affiliation:
Pulkovo Observatory, 196140 St Petersburg, Russia e-mail: mchubey@gaoran.spb.su
D.L. Gorshanov
Affiliation:
Pulkovo Observatory, 196140 St Petersburg, Russia e-mail: mchubey@gaoran.spb.su
M.S. Chubey
Affiliation:
Pulkovo Observatory, 196140 St Petersburg, Russia e-mail: mchubey@gaoran.spb.su

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The arguments are given of the choice for the Vilnius seven color medium band photometric system as the most effective one for the AIST space project. A prediction is made of the limiting stellar magnitudes V for every Vilnius passband and the integral band T at σΣ ≤ 30mmag from a 3 year AIST mission.

Type
3. Expected Developments in High Precision Astrometry
Information
Symposium - International Astronomical Union , Volume 166: Astronomical and Astrophysical Objectives of Sub-Milliarcsecond Optical Astrometry , 1995 , pp. 327 - 330
Copyright
Copyright © Kluwer 1995 

References

Jaschek, C., Frankel, S., 1986, A&Ap, 158, 174.Google Scholar
Straižys, V., 1977, Multicolor Stellar Photometry, Mokslas, Vilnius.Google Scholar
Straižys, V., 1992, Baltic Astronomy, 1, 107.Google Scholar
Straižys, V., Boyle, R.P., Kuriliene, G., 1992, Baltic Astronomy, 1, 95.Google Scholar