Notes on ComaLS data in Astro-WISE
Below are some notes on formats and content of the ComaLS data present in the
Astro-WISE system. Any data in the Astro-WISE can be viewed with the
For the ComLS data convenient shortcuts are given
The notes below discuss mostly these shortcuts. If you have any further
questions please contact Gijs Verdoes or John Mcfarland (see
If you want to become more familiar with the Astro-WISE system: the
are a good starting point.
ReducedScienceFrames: Astro-WISE vs HST format
The ComaLS ACS Multi-Drizzled images coming out of the COMA LS dedicated calibration pipeline are stored in the Astro-WISE research
environment. The drizzled frames are constructing using effective exposure time weighting. (For COMA-LS team members: they are the '*W_drz_cl.fits' files.) In Astro-WISE speak they are in the form of
CoaddedRegriddedFrames, but are ingested at the ReducedScienceFrame level.
This is because the regridding done by the Multi-Drizzle software was not done
to the same grid as used by Astro-WISE. The ReducedScienceFrames of the
ingested data can be regridded to this grid to allow coadding with other data
in Astro-WISE. The format of ReducedScienceFrame is close to the format of the
original *drz*fits files. The pixel values in the ReducedScienceFrame are
identical to the [SCI] fits extension of the Multi-Drizzled images. The [WHT]
fits extension, i.e., the weight frame, is stored as a separate WeightFrame and
is linked to its RedudcedScienceFrame. The pixel values in this WeightFrame are
divided by the exposure time as given by the header keyword EXPTIME in the
*drz.fits file. By storing the data in these common Astro-WISE formats, one can
make use of the Astro-WISE system capabilities for the ACS ComaLS data. One
example Astro-WISE capability is that all analysis results (e.g., GALFIT and
GALPHOT fits) are linked to the pixel data from which they were derived. This
way one can easily inspect the goodness of fit of different runs of GALFIT and
GALPHOT and how that depends on the settings of the fitting algorithm.
NOTE: ACS data ingestion currently only supports the Multi-Drizzled
images. Raw data should be supported also, but its ingestion has not been
tested. When requesting data from MAST, choose calibrated data to
get only the Multi-Drizzle data.
SourceLists are made by SExtractor. Sextractor is run inside the Astro-WISE
system. Information on how the sourcelist was derived (e.g., the SExtractor
configuration used) can be viewed by clicking on the objectview link in the
last column on the query page. You can store a sourcelist locally by selecting
one (done by clicking on its number in the SLID column on the query form) and
then using the "export-options" at the bottom end of the webpage. Make sure you
set the "max number of rows" in the query form to "rownum" if you want to
store all rows, i.e., all sources, in the sourcelist.