Creating updated, scientifically-calibrated mosaics for the RC3 Catalogue
The Third Reference Catalogue of Bright Galaxies (RC3) is a reasonably complete listing of 23,010 large, bright galaxies. Using the latest Sloan Digital Sky Survey’s Data Release 10 (SDSS DR10) data, we provide color composite images and scientifically-calibrated FITS mosaics in all SDSS imaging bands, for all the RC3 galaxies that lie within the survey’s footprint. To get a larger sky coverage, we then conduct the procedures on photographic plates taken by the Digitized Palomar Observatory Sky Survey (DPOSS) for the B, R, IR bands. Due to the positional inaccuracy inherent in the RC3 catalog, the mosaicking program uses a recursive algorithm for positional update first, then conduct the mosaicking procedure using IPAC’s Montage.The program is generalized into a pipeline, which can be easily extended to future survey data or other source catalogs.
Montage : Stitches images togther
- AstroPy Montage wrapper
SExtractor: Source extraction inside the positional update algorithm
STIFF: Generating color images
Python v2.7: other versions is fine but minor changes to the code may be necessary
- AstroPy preferably v4 dev for the SkyCoord procedures in the source confusion algorithm, but other AstroPy v3.* is fine, I have included the patch as a comment inside rc3.py
- sqlite3 : generates the searchable database. Not necessary for the mosaicing program to run.
Here are some notes that I made on installing these dependencies software on MacOSx or on the [NERSC Machines] (https://github.com/ProfessorBrunner/rc3-pipeline/wiki/Installing-dependencies-on-NERSC-Machines) ##Documentation