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mugdhapolimera/SDSS_spectra
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Written by Ashley Bittner on August 3 2017 (1) coords/ - directory containing coordinates of various subsamples from RESOLVE in batches of 1000 so that they can be read into SDSS D12 Cross ID tool (2) SDSS_ECO_create.py - plots emission line diagrams from ECO SDSS data (2a) (2a) ECO_SDSS_raw.fits and ECO_SDSS_dext.fits - contains full ECO SDSS flux meausurements (raw and de-extincted, respectively) (3) SDSS_RESOLVE_create.py - plots emission line diagrams from RESOVLVE SDSS data (3a, 3b) (3a) RESOVE_SDSS_raw.fits and RESOLVE_SDSS_dext.fits - contains full RESOLVE SDSS flux meausurements (raw and de-extincted, respectively) (3b) RESOVE_SDSS_dwarf.fits and RESOLVE_SDSS_dext_dwarf.fits - contains RESOLVE SDSS flux meausurements (raw and de-extincted, respectively) of dwarf galaxies (Mstar < 9.5 solar masses) (4) SQLquery.txt and SQLquery_ECO.txt - query used to identify SDSS line flux measurements of interest from various catalogues (5) resolve_comp.py - creates various plots attempting to understand the differences between the SDSS line flux measurements and the RESOLVE line flux measurements (merged_bztre.fits) made by Eriks codes
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