README web version of /home/usg/OPS/MTS/readme_xml/readme_81049301
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
We want to observe an eclipsing binary system in NGC 6822 having K ~ 18.5
mag
outside eclipses (e.g. close to both quadratures). For this reason two sets
of OBs (N6822-Q1-N* and N6822-Q2-N* to observe our system close to the
orbital phase of 0.75 and 0.25 respectively). Each OB should be executed on one
of the
nights listed in the ephemeris file appended to a given OB. In order to calibrate
our observations onto the standard system 5 standards from UKIRT list
were selected. One of our N6822* OBs should be executed on the photometric night
together
with those standards. We have specified N6822-Q1-N1 to observed under photometric
conditions.
However if during executing of N6822-Q2 OBs (e.g. on different nights) the conditions
are photometric and N6822-Q1-N1 is still not observed, please observe our set of
standard stars
together with a given N6822-Q2 OB. In such a case NGC6822-Q1-N1 OB could be executed
under not
photometric condition later on. (e.g. we do need just one N6822-* OB to be observed
under
photometric conditions together with the selected standard star OBs. It does not
matter
if this is N6822-Q1* or N6822-Q2). Since both sets of N6822 OBs will be observed
on different
nights this information should improve the chances to calibrate our observations.
We would appreciate very much if some additional standards
could be observed during twilights on the photometric night
(both NICMOS and UKIRT standard are usefull).
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
Our science N6822* OBs should be executed on different nights from the
appended lists, which are also given below. One of the OBs shoudl be executed togehter
with
selected standard stars (STD_FS*) - see general description.
OBs N6822-Q2-N* should be executed on some of the
following nights
jd date phase
4573.8 2008-04-16 0.23
4580.8 2008-04-23 0.28
4586.8 2008-04-29 0.18
4593.8 2008-05-06 0.23
4600.8 2008-05-13 0.28
4606.8 2008-05-19 0.19
4613.8 2008-05-26 0.24
4620.8 2008-06-02 0.29
4626.8 2008-06-08 0.19
4633.8 2008-06-15 0.24
4640.8 2008-06-22 0.30
4646.8 2008-06-28 0.20
4660.8 2008-07-12 0.30
4666.8 2008-07-18 0.20
4673.8 2008-07-25 0.26
4680.8 2008-08-01 0.31
4686.8 2008-08-07 0.21
4693.8 2008-08-14 0.26
4700.8 2008-08-21 0.31
4706.8 2008-08-27 0.21
4713.8 2008-09-03 0.27
4720.8 2008-09-10 0.32
4733.8 2008-09-23 0.27
4740.8 2008-09-30 0.32
4746.8 2008-10-06 0.23
4753.8 2008-10-13 0.28
4759.8 2008-10-19 0.18
OBs NGC6822-Q1-N* should be executed on some of these
nights
jd date phase
4570.8 2008-04-13 0.78
4576.8 2008-04-19 0.68
4583.8 2008-04-26 0.73
4590.8 2008-05-03 0.78
4596.8 2008-05-09 0.68
4603.8 2008-05-16 0.73
4610.8 2008-05-23 0.79
4616.8 2008-05-29 0.69
4623.8 2008-06-05 0.74
4630.8 2008-06-12 0.79
4636.8 2008-06-18 0.69
4643.8 2008-06-25 0.75
4650.8 2008-07-02 0.80
4656.8 2008-07-08 0.70
4663.8 2008-07-15 0.75
4670.8 2008-07-22 0.80
4676.8 2008-07-28 0.71
4683.8 2008-08-04 0.76
4690.8 2008-08-11 0.81
4696.8 2008-08-17 0.71
4703.8 2008-08-24 0.76
4710.8 2008-08-31 0.82
4716.8 2008-09-06 0.72
4723.8 2008-09-13 0.77
4730.8 2008-09-20 0.82
4736.8 2008-09-26 0.72
4743.8 2008-10-03 0.78
4749.8 2008-10-09 0.68
4756.8 2008-10-16 0.73
4763.8 2008-10-23 0.78
4769.8 2008-10-29 0.68
4766.8 2008-10-26 0.23
Special Calibration Information
ToO Information
ToO Activators List
Is this a Pre-imaging run ?
Pre-imaging Requirements
Source(s) of Pre-imaging
Pre-imaging sources not listed above
Do all your OBs comply with the instrument-specific requirements listed
on the instrument-specific Phase 2 web page ?
If this is a pre-imaging run, did you select PRE-IMAGING for the Observing
Category for each Observing Template ?
Do all your finding charts comply with both the general and instrument-specific
Phase 2 Web Pages ?
If you submitted OBs for standard stars, did you specify the magnitude
and spectral type of all standard stars in the OBs ?
Have you included OBs for any calibrations that you need but which are
not part of the Calibration Plan ?
If you are observing Moving Targets, have you attached suitable ephemeris
files to your OBs?
If you have preferences which OBs should be executed first, did you make
use of the User Priority field in the OBs ?
If this is a run that requires coordinated observations with other facilities,
did you give proper instructions in the Time-Critical Aspects Section ?
If you submitted OBs for standard stars, did you use the provided StandardStar
templates ?
If you are using a specific offset pattern or position angle, did you
check carefully the definition in the manual ?
If you are doing spectroscopy, did you draw the slit on the Finding Charts
?
Did you enter the magnitude of the brightest star in the field-of-view
in the 'Instrument Comments' field of each OB ?
If you use the MoveToPixel acquisition, have you given clear instructions
on the FC and in the OB comment section as to how the field should be centered ?
Last creation of page: Tue Oct 6 15:40:24 2009
If you have comments, please contact usd-help@eso.org