71.C-0580(B)

PI:Littlefair/ Naylor/ Jeffries/ Burningham

Rank Class: A

RA Range: 16.5h - one field

Constraint set (Typical seeing, Transparency,Airmass, FLI, Moon distance):
2.0 3THN 2.0 1.0 60

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

 
 
This program intends to measure the rotation rates of young stars
in the Rho Ophiuchus dark cloud. The rotation rates are measured
by searching for PERIODIC photometric variability (caused by
starspots) in these stars. As such, the timing of OB execution
is the critical parameter for the success of this program.

Please read the Time Critical Aspects of README section for more
information.

Because of the need to detect and measure rotational periods for these
stars, THE TIMING OF OB EXECUTION IS CRITICAL. The OBs in this run are
all identical. Once the first OB is executed, the remaining OBs should
be executed, one a night, each night (if possible) until exhausted.
ONLY ONE OB IS TO BE OBSERVED ON A GIVEN NIGHT.

PI included one Cal OB for the observation of dark frames for this run.
 
 

Run status page 71.C-0580B

README of this run:

71.C-0580B.README

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