README web version of /home/usg/OPS/MTS/readme_xml/readme_77085300
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This is an imaging observing run with 1 science target: ESO338-IG04. Allocated
14 hours.
We will obtain images in Ks, IB_2.12 and IB_2.18 filters.
We will use the S27 and S54 cameras, always in FowlerNsamp mode.
There are 15 OBs, all in imaging mode. 12 for CLEAR condition, 3 for PHOT. As required
the PHOTOMETRIC observations comprise less than 20% of the allocated observing time
(2 hours of 14).
CLEAR Observations:
4 x IB_2.12
4 x IB_2.18
4 x Ks
PHOTOMETRIC Observations:
1 x Ks
1 x IB_2.12 & IB_2.18
1 x NICMOS standard star in IB_2.12 & IB_2.18
The IB Science and Standard OBs must be executed consecutively.
The brightest star in the field is the NGS with magnitude of K=12.6
None of the chopping patterns will observe objects brighter than the NGS.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
Special Calibration Information
There is one Ks-band OB to be carried out under photometric conditions.
This will be used to calibrate the remaining (4) Ks-band observations of the science
target. This calibration falls within the NACO calibration plan.
The Ks-band PHOT OB is E338_Ks_Cal
There are 2 Intermediate band calibration OBs to be carried out under photometric
conditions. Calibration of IB filters falls outside of the NACO calibration plan
and therefore requires separate OBs. One OB to observe the science target in both
intermediate band filters, the other to observe a NICMOS standard with both IB filters.
The two Intermediate Band PHOT OBs are CAL_Std_S234E_IB and E338_IB_Cal
The Ks-band apparent magnitude of the Calibrtion star is 12.070
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 have PSF reference star OBs, do the names of those OBs begin with
PSF_ ?
If there are Finding Charts attached to your OBs, is the field-of-view
of at least one of these charts 2' x 2' (with clearly labelled field orientation)
?
Have you clearly marked and labelled your wavefront reference objects
R1, R2, R3, ... (as specified in the NAOS Preparation Software) on your Finding
Charts ?
Have you specified the magnitude of the brightest object in the field-of-view
for each OB ?
Are there objects in any of your fields (including standard stars) which
are brighter than the limits specified in the User Manual and on NACO web Pages
?
If the previous answer is yes, have you given a list of OBs and a justification
for the brightness limit violation in the general description field ?
Last creation of page: Tue Oct 6 15:40:14 2009
If you have comments, please contact usd-help@eso.org