RA Range: 16.5 - 23.3h

Constraint set (Typical seeing, Transparency,Airmass, FLI, Moon distance): 0.8, THN, 2.0-2.5, 1.0, 30

Pre-imaging run?	No!	Chilean run?	No!	Special calibrations?	No!
Time critical?	No!	ToO?	No!	Carry-over run?	No!

 

 DDT program (consisting of 2 runs A and B of different OPC priority 
class) for radial-velocity follow-up of three extra-solar planet 
candidates recently detected during their planet transit search (June 
2001). Each star needs to be observed in different epochs (3 or 4 during 
this part of the program, i.e. run A), each one ideally separated by one 
day. Please, cf README file for more details. 

 Objects are setting fast: observations can start up to 15 minutes 
before astronomical twilight. Each object should be observed once per 
night, on consecutive nights whenever possible. All OBs have an attached 
wavelength calibration (the exp.time of these may need to be adjusted). 
One radial velocity standard star provided. 

 Two requirements: 1. it is essential that the stars are perfectly centered 
in the slit throughout each observation. 2. PI requests immediate release 
of the data after each night in order to re-assess priorities for run B 
(these depend on whether these candidates show early evidence of having 
M-dwarfs, brown dwarfs, or planets as companions). 

 
 

Run status page 267.C-5723A

README of this run:

267.C-5723A.README