073.C-0138(A)

PI:Harries/ Bate/ Naylor/ Kurosawa/ Symington/ Littlefair

Rank Class: B

RA Range: 14:29-16:55

Constraint set (Typical seeing, Transparency,Airmass, FLI, Moon distance):
2.0 3THN 2.0 1.0 30

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

 
 
This is a UVES programme aimed at detecting brown dwarfs binaries 
from two-epochs observations.

For each target the PI has submitted 2 OBs, which should be executed
at least one day apart. Do not execute two OBs for the same target
on the same night. 

NOTE: some targets are rather faint. For them the acquisition must be
done using a blind offset from a field reference star (indicated in the
f.charts). For one target, namely GY141, no reference star could be found.
The PI asks to attempt the acquisition using a long integration time.
This is a a challenging one: this target has been observed with HIRES
at Keck, in the Halpha region. 


 

Run status page 073.C-0138A

README of this run:

073.C-0138A.README

Check if ftp directory/ies exist/s for this run:
P72 Directory does not exist for 073.C-0138A
P73 Directory exists for 073.C-0138A
P74 Directory does not exist for 073.C-0138A

P73 run ...search for JPEG finding charts in database:
Finding charts, click on them to display:

OB_ID	OB_name	Finding chart
OB:153959	USCO_109_second_obs	usco109.jpg
OB:153956	USCO_104_second_obs	usco104.jpg
OB:153938	USCO_056_second_obs	usco56.jpg
OB:153953	USCO_101_second_obs	usco101.jpg
OB:153950	USCO_100_second_obs	usco100.jpg
OB:153947	USCO_075_second_obs	usco75.jpg
OB:153944	USCO_067_second_obs	usco67.jpg
OB:153941	USCO_066_second_obs	usco66.jpg
OB:153957	USCO_109_first_obs	usco109.jpg
OB:153954	USCO_104_first_obs	usco104.jpg
OB:153951	USCO_101_first_obs	usco101.jpg
OB:153935	USCO_055_second_obs	usco55.jpg
OB:153932	USCO_053_second_obs	usco53.jpg
OB:153929	USCO_040_second_obs	usco40.jpg
OB:153926	GY_310_second_obs	gy310_finder.jpg
OB:153926	GY_310_second_obs	gy310.jpg
OB:153923	GY_141_second_obs	gy141.jpg
OB:153920	GY_037_second_obs	gy37_finder.jpg
OB:153920	GY_037_second_obs	gy37.jpg
OB:153948	USCO_100_first_obs	usco100.jpg
OB:153945	USCO_075_first_obs	usco75.jpg
OB:153942	USCO_067_first_obs	usco67.jpg
OB:153921	GY_141_first_obs	gy141.jpg
OB:153918	GY_037_first_obs	gy37_finder.jpg
OB:153918	GY_037_first_obs	gy37.jpg
OB:153915	GY_005_first_obs	gy5.jpg
OB:153917	GY_005_second_obs	gy5.jpg
OB:153939	USCO_066_first_obs	usco66.jpg
OB:153936	USCO_056_first_obs	usco56.jpg
OB:153933	USCO_055_first_obs	usco55.jpg
OB:153930	USCO_053_first_obs	usco53.jpg
OB:153927	USCO_040_first_obs	usco40.jpg
OB:153924	GY_310_first_obs	gy310_finder.jpg
OB:153924	GY_310_first_obs	gy310.jpg
OB:153965	USCO_121_second_obs	usco121_finder.jpg
OB:153965	USCO_121_second_obs	usco121.jpg
OB:153962	USCO_112_second_obs	usco112.jpg
OB:153974	USCO_132_second_obs	usco132_i.jpg
OB:153974	USCO_132_second_obs	usco132_r.jpg
OB:153969	USCO_130_first_obs	usco130_finder.jpg
OB:153969	USCO_130_first_obs	usco130.jpg
OB:153902	CAL_HD140538_rv_std	hd140538.jpg
OB:153904	CAL_HD145482_telluric_std	hd145482.jpg
OB:153909	CAL_LHS_3003_xcorr_template	lhs3003_i.jpg
OB:153909	CAL_LHS_3003_xcorr_template	lhs3003_j.jpg
OB:153912	CAL_LHS_429_xcorr_template	lhs429_i.jpg
OB:153912	CAL_LHS_429_xcorr_template	lhs429_j.jpg
OB:153906	CAL_LHS_049_xcorr_template	lhs49_i.jpg
OB:153906	CAL_LHS_049_xcorr_template	lhs49_j.jpg
OB:153963	USCO_121_first_obs	usco121_finder.jpg
OB:153963	USCO_121_first_obs	usco121.jpg
OB:153960	USCO_112_first_obs	usco112.jpg
OB:153968	USCO_128_second_obs	usco128_i.jpg
OB:153968	USCO_128_second_obs	usco128_r.jpg
OB:153972	USCO_132_first_obs	usco132_i.jpg
OB:153972	USCO_132_first_obs	usco132_r.jpg
OB:153971	USCO_130_second_obs	usco130_finder.jpg
OB:153971	USCO_130_second_obs	usco130.jpg
OB:153966	USCO_128_first_obs	usco128_i.jpg
OB:153966	USCO_128_first_obs	usco128_r.jpg