Prioritize the S0 paper. Avishek will do it.
Write a report on the work done with our Nair et al. sample (~ 8000 galaxies).
Define a Green Valley - Use the bifurcation between star forming and passive galaxies made in Bluck et al. 2014. I was wondering that we can also use a more objective definition for the main sequence as defined in Renzini & Peng 2015.
Find the number of AGN in the Nair et al. sample and see it's role in quenching star formation. Leslie et al. 2016 is one of the recent paper which talks about it.
Cross match Meert et al. sample with our Nair et. al sample and pull out B/T, bulge scale length, disc scale length etc.
Pull out bar, ring etc., information from the Nair et al. sample.
Find massive spirals in the Nair et al. sample.
Make a cutout of half a dozen images of the largest galaxies in 4-5 bands (NUV, r, K, W1 and W3) from the S0 sample.
Quote the chi-square and scatter of the stellar mass comparison of MAGPHYS run with Kauffmann et al. 2003.
Plot Fig. 3 of Renzini & Peng 2015.
Compare Nair et al. SFR with FSPS SFR.
Make two data files for bulge and disc and run MAGPHYS on the Nair-Meert cross-matched sample.
Correlation of CAS GM parameters with SFR and stellar mass, morphology etc.
Comparison between the SFR estimated via SED & spectroscopic method. Search catalogues from SDSS to do that.
Plot different correlations for high mass & low mass classical bulge.