README web version of /home/usg/OPS/MTS/readme_xml/readme_82025500
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This is a FORS2 MXU observation of the outer halo of NGC 4696, in two
fields EAST and SOUTH. We use a mask of parallel slits, plus the narrow band filter
[OIII]/3000+51 and Grism-600B+22 to detect the [OIII]lambda 5007 AA emission line
from Planetary Nebulae associated with the light.
This is a blind search technique. The mask has 5 to 7 holes at the field star positions
so that the mask can be aligned correctly during service mode observations. Once
the mask is aligned with these positions a sequence of offsets in Right Ascesion
can be performed. This is detailed in the Special Execution Requirements.
Please execute all the OBs for one field before going to the next.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
Please execute all the OBs for the EAST field before moving to the SOUTH
field.
Each OB of the EAST field has the same acquisition and through-slit templates. Once
the through-slit image has been succesfully executed, please execute the offset
in Right Ascension, according to the OB name, as listed in the table below:
OB name offset in arcsecond in the R.A. direction
sciMXU_N4696_E0 0".0
" " _E01 1".3
" " _E02 2".6
" " _E03 3".9
" " _E04 5".2
" " _E05 6".5
" " _E06 7".8
" " _E07 9".1
" " _E08 10".4
" " _E09 11".7
" " _E10 13".0
" " _E11 14".3
Each OB has one finding chart showing the whole instrument field of view. We also
added two zoomed images of the field where are shown the positions of the stars
that have to be used for a correct alignent of the mask during the through-slit
image.
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Each OB of the SOUTH field has the same acquisition and through-slit templates.
Once the through-slit image has been succesfully executed, please execute the offset
in Right Ascention, according to the OB name, as listed in the table below:
OB name offset in arcsecond in the R.A. direction
sciMXU_N4696_S0 0".0
" " _S01 1".3
" " _S02 2".6
" " _S03 3".9
" " _S04 5".2
" " _S05 6".5
" " _S06 7".8
" " _S07 9".1
" " _S08 10".4
" " _S09 11".7
" " _S10 13".0
" " _S11 14".3
Each OB has one finding chart showing the whole instrument field of view. We also
added two zoomed images of the field where are shown the positions of the stars
that must be used for a correct alignent of the mask during the through-slit image.
Special Calibration Information
We need standard calibration. Please be aware that we are using the [OIII]/3000+51
narrow band filter, so the arclamp exposures and the flat fields need longer exposure
time to reach enough counts.
For the arclamp we need at least two bright emission lines for wavelength calibration.
The specto-photometric standard star calibration forseen in the ESO standard calibration
plan are adequate for our needs.
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 prepared your finding charts with tools other than FIMS,
do they comply with the specifications on the FORS1 Phase 2 web page ?
Last creation of page: Tue Oct 6 15:40:26 2009
If you have comments, please contact usd-help@eso.org