Program May 2025

Culmination is for 15.V.

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Spectroscopy:
abbrev. Target     obs     Vmag   culm[UT] interval  exp[s]  PI
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Normal mode:
------------------------------------------------------------------
bof03 TOI-1786       SP      9.99   17:00   evening   3x900   Vanko
tuuma,  TUUMa,       SP      9.26   evening            3x900   Garai-Derekas
invir   INVir         SP     9.13   20:20    -/+1h     3x900    Pribulla
jar20 TYC3852-0142-1 SP      8.14   21:00    +3h      3x900   Vanko/Pribulla
gkboo   GKBoo         SP    10.93   21:40    -/+2h      x900    Pribulla
alfcr   AlphaCrB      SP     2.24   22:40    -/+1h     3x300    Pribulla
jar16 TYC0363-0775-1 SP      8.13   23:00    +/-1h    3x900   Vanko/Pribulla
bor27   TIC233684019  SP    10.14   00:20    -/+1h     3x900    Pribulla
h1821   HD182144      SP     9.08   02:30     -1h      3x900    Pribulla
h1902   HD190257      SP     7.86   03:10     -1h      3x900    Pribulla
bor10   TIC278352276  SP    10.40   03:30     zrana    3x900    Pribulla
------------------------------------------------------------------

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 
-----------------------------------------------------------------

Time critical:
Observations not given in this list are planed based on the requirements 
of projects via direct message to the observers.