README web version of /home/usg/OPS/MTS/readme_xml/readme_82061101
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
For this observing period we propose the observation of the nucleus of
the galaxy NGC4303 in three bands: J, H, K. The SINFONI configuration selected is
the non-AO FoV 8"x8" (slices size 0".25), spectral resolution R=2000 (J-band), R=3000
(H-band), R=4000 (K-band).
We have divided the proposal in 11 OBs: 6 for NGC4303 (2 per band) and 5 for the
standard stars (3 in H-band, 2 in K-band).
NOTE: In order to secure the needed S/N with SINFONI, each galaxy band has to be
observed for the 2 requested OBs of 1 hour each. The observations will not be completed
for a given band until the 2 corresponding OBs have been done succesfully. Note
however that the OBs have not to be back-to-back provided they are executed with
similar observing conditions (seeing, zenital distance, transparency). For example,
if the first OB executed is the pointing of NGC4303 in the H-band, we will need
to have the other NGC4303 H-band OB of NGC4303 completed.
Finally, for all OBs, we expect that both sides of the SINFONI's FoV are aligned
with the North-East axes.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
Two standard stars will be observed in K-band (HD113678, HD116535), and
three in H-band (HD113678, HD116535, HD103295).
The K-band star OB must be observed right before, after or between the NGC4303 K-band
OBs. For example:
Star1
NGC4303
NGC4303
Star2
The H-band star OB must be observed right before, after or between the NGC4303 H-band
OBs. For example:
Star1
NGC4303
Star2
NGC4303
Star3
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 15:40:27 2009
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