README web version of /home/usg/OPS/MTS/readme_xml/readme_78024700
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
IFU ARGUS mapping of weak optical recombination lines (ORLs) from CNONeMg
ions in 3 Orion proplyds with the aim to derive per spaxel abundances from the ORLs
and compare with the corresponding abundances derived from the stronger forbidden-lines
(in LR mode).
The HR settings will allow us to compare the widths of the ORLs vis. the forbidden
lines per spaxel. The ORLs are predicted to arise from cold (<1000K) plasma and
should display narrower thermal widths than the forbidden lines emitted from the
same ions.
Critical ORLs aimed to be mapped at S/N > 10 per spaxel per OB are the OII 4089,
CII 4267-A (LR02) and OII 4649-A (LR03) lines. The Balmer discontinuity at 3646-A
(LR01) is also needed at average S/N.
Coverage of all 3 proplyds should allow for a good comparative study. Formal priorities
however are 1, 1 for TD and LV target OBs and 2 for target P OBs.
Waiver Requests
Critical Observing Condition Constraints
For all LR OBs:
Sky transp = Clear, Seeing = 0.8, Airmass = 2.0, Illum = 1.0, Moon ang. dist. =
50
For all HR OBs:
Sky transp = Clear, Seeing = 0.8, Airmass = 2.5, Illum = 1.0, Moon ang. dist. =
50
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 specify in your OBs the hour angle range for which your Target
Setup files are valid ?
Did you specify in your OBs the magnitudes of FACBs and Guide Star for
all your fields ?
Are the FACBs and Guide Star in the brightness ranges specified in the
FLAMES manual ?
Did you enter the expected signal to noise in your OBs ?
Last creation of page: Tue Oct 6 15:40:15 2009
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