© Special Astrophysical Observatory of the Russian Academy of
Sciences
Gallery
The Team
Valyavin, G. G. - head of the project (in the alphabetical order) Arkhypova L.N., Bakholdin A. V., Burlakova T. E., Bychkov V. D., Drabek S. V., Fabrika S. N., Galazutdinov G.A., Kravchenko V. M., Kryukov P. G., Kudryavtsev D. O., Kukushkin D. E., Larionov S., Perkov A. V., Sarkisyan A. N., Sazonenko D. A., Semenko E. A., Semjonov S. L., Shergin V. S., Starkov N.A., Pritychenko A. M., Musaev F. A., Valeev A.F., Yushkin M. V.
© Special Astrophysical Observatory of the Russian Academy of Sciences
Gallery
The Team
Valyavin, G. G. - head of the project (in the alphabetical order) Arkhypova L.N., Bakholdin A. V., Burlakova T. E., Bychkov V. D., Drabek S. V., Fabrika S. N., Galazutdinov G.A., Kravchenko V. M., Kryukov P. G., Kudryavtsev D. O., Kukushkin D. E., Larionov S., Perkov A. V., Sarkisyan A. N., Sazonenko D. A., Semenko E. A., Semjonov S. L., Shergin V. S., Starkov N.A., Pritychenko A. M., Musaev F. A., Valeev A.F., Yushkin M. V.
Kaleidoscope
Early
experimental
studies
of
the
mechanical
stability
of
the
instrument
based
on
ThAr
spectra:
what
happens
after
filling
the
CCD
cryostat
with
the
liquid
nitrogen
and
the effect of its evaporation.
The
adjustment
process
for
the
spectrograph's
camera is in progress.
Radial velocity curve of iota Pegasi.
