README web version of /home/usg/OPS/MTS/readme_xml/readme_77050900
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
APPLES1 is the smallest dwarf galaxy ever discovered, which is also isolated.
It is at a distance of about 9 Mpc and has an absolute magnitude of -9.6 in the
I band. Despite its spheroidal morphology (which is associated, in dwarf galaxies
in the Local Group, with old stellar populations), APPLES1 is characterised by an
intermediate-age (3 Gyr old) stellar content with a relatively on-going star formation,
as revealed by the presence of OB stars. Its available FORS2 spectrum seems to rule
out the existence of an old (10 Gyr) stellar population, which, on the contrary,
is always present in the best-studied dwarf galaxies in the Local Group. The present
observations are aimed to measure the integrated colours of APPLES1 over a larger
baseline than its optical spectrum, and thus to put firm constraints on the presence
(or absence) and the mass-fraction of an old stellar population, on the global star-formation
history and total mass of APPLES1.
Waiver Requests
Critical Observing Condition Constraints
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 ?
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 15:40:13 2009
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