README web version of /home/usg/OPS/MTS/readme_xml/readme_84085300
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
Targets
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Prio Name OB-Naming K_vega mag H_beta calc wavelength
Offset Star K_vega mag
---------------------------------------------------------------------------------------------------------
1 ID7 SINS-ID7_H -* 19.61 1.5677 micron
14.8
2 ZC-782941 SINS-782941_H -* 19.65 1.5470 micron
13.11
3 D3a-12556 SINS-12556_J -* 19.29 1.2613 micron
15.3
4 D3a-6004 SINS-6004_H -* 19.10 1.6468 micron
14.1
Program description
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The program aims at detecting faint emission lines in high redshift galaxies.
The dither pattern is chosen to fit the object as well as sky for the next pointing
on the detector. Therefore an alternating pattern is used.
From dither-pair to dither-pair as well as between the OBs this dither
patter varies with small offsets of 0.5 arcsec in RA and DEC around the target.
Main characteristics of the observations
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- OBs are named after the target, with \"-0\", \"-1\", \"-2\", etc. appended for
different OBs.
- The DITs for our exposures of our faint targets are 600s.
- We are using the 250mas scale, with a FOV of 8\"x8\".
Priority of the targets
-----------------------
The priority of the targets is reflected by the \"User priority\" flag.
The OBs of a specific target should be executed according to increasing suffix of
the OBs.
Finder Charts
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All OBs have two findercharts attached (the OBs for target D3a6004 have three),
showing
the required 2x2 arcmin field (chart 1) as well as a close up view indicating
the dither pattern with the SINFONI-FOV (chart 2).
For target D3a-6004 the blind offset star falls out of the mandatory
2x2arcmin field. It therefore has a third chart (chart 1a) attached which shows
the blind offset star (marked as R1).
Waiver Requests
Critical Observing Condition Constraints
Transparency constraints:
- For all OBs, CLEAR sky transparency conditions is acceptable, as specified
in the proposal.
Moon constraints:
- Conforming to our proposal, there is no constraint on lunar phase and so
the illumination is set to 1.0.
Seeing constraints:
- Seeing < 0.8\", as specified in the proposal.
Time-Critical Aspects
Special Execution Requirements
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 ?
Did you indicate the magnitude of the brightest object in the field in
each SINFONI OB?
If you are using the AO: Did you indicate for every OB the magnitude
of the guide star, and its distance to the target (if any)?
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?
Did you make really sure that none of your OBs ever saturates the detector?
If you are using the AO: did you enter the correct Strehl Ratio (on-axis,
K-band) AND the seeing value in the constraint set?
Last creation of page: Tue Oct 6 15:40:32 2009
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