Program Mar 2025

Culmination is for 15.III.

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Spectroscopy:
abbrev. Target     obs     Vmag   culm[UT] interval  exp[s]  PI
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Normal mode:
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kelt7,  HD33643         SP     8.54   18:15    -/+3h      x900   Orikhovskyi, time critical
fmcma,  FMCMa           SP     8.73   18:15    -/+1h     3x900   Pribulla
jar10,  TYC1931-01040-1 SP     9.65   19:00    +/-2h     3x900   Vanko/Pribulla
bof01,  TOI-1157        SP    10.17   20:30    +/-3h     3x900   Vanko
bof03,  TOI-1786        SP     9.99   20:30    +/-3h     3x900   Vanko
jar05,  TYC0870-00084-1 SP    10.22   22:30    +/-1h     3x900   Vanko/Pribulla
tuuma,  TUUMa,         SP      9.26    22:50     +/-2h  3x900   Garai-Derekas
jar06,  TYC0870-00937-1 SP     9.83   00:30    +/-1h     3x900   Vanko/Pribulla
invir,  INVir           SP     9.13   00:30    +/-1h     3x900   Pribulla
alfcr,  AlphaCrB        SP     2.24   02:20      -2h     3x300   Pribulla

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Time-series spectroscopy. 15- minute exposures.
Calibration ThAr spectra between three consecutive object spectra.
Requires excellent seeing

14.3.2025, kelt7 SP  17:30 - 21:00  Orikhovskyi
25.3.2025, kelt7 SP  17:30 - 20:30  Orikhovskyi

Note:

Vzdy treba co najlepsie zaostrit ! Objekty slabsie ako V=9 merat len pri
dobrom seeingu <2-3".

Kazdu noc je treba ziskat aspon jedno spektrum RV standartu a
spektrofotometrickeho standartu (najlepsie su HD192907, HD21389 a
HD47839). V katalogu su oznacene ako RVstand a SPstand. Idealne cim
blizsie k meridianu.



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Photometry:
every night:
obj        time[UT]       obs  filter_exposure[s]  PI    Note
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time-critical:
date_evening    obj  obs  time[UT]      filter_exposure[s]  PI
yyyy mm dd                              one cycle 
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Time critical:
Observations not given in this list are planed based on the requirements 
of projects via direct message to the observers.