Program Apr 2025

Culmination is for 15.IV.

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Spectroscopy:
abbrev. Target     obs     Vmag   culm[UT] interval  exp[s]  PI
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Normal mode:
------------------------------------------------------------------
mad01 TIC14400891    SP     8.60   17:30   +3h        3x900   Vanko
mad02 TIC302581695   SP     6.10   18:00   +3h        3x600   Vanko
bof03 TOI-1786       SP     9.99   19:00   +4h        3x900   Vanko
jar09 TYC1439-1487-1 SP     7.45   20:30   +1h        3x900   Vanko
tuuma,  TUUMa,        SP     9.26   20:45    +/-1h     3x900   Garai-Derekas
jar06 TYC0870-0937-1  SP     9.83   21:00   +1h        3x900   Vanko
invir   INVir         SP     9.13   22:20    -/+1h    3x900  Pribulla
gkboo   GKBoo         SP    10.93   23:40    -/+2h     x900  Pribulla
alfcr   AlphaCrB      SP     2.24   00:20    -/+1h    3x300  Pribulla
bor27   TIC233684019  SP    10.14   02:20    -/+1h    3x900  Pribulla

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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.

Flaty treba kazdu noc. Darky minimalne kazde 2 tyzdne ! Zvecera 2x po sebe ThAr.


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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.