Description file for Sedgwick19ab.fits (binary table)

These data describe the core-collapse supernovae (CCSN) rate density as a function of galaxy stellar mass and the inferred galaxy stellar mass function (GSMF) of star-forming galaxies. 

The details are described in Sedgwick et al. (2019a) https://ui.adsabs.harvard.edu/abs/2019MNRAS.484.5278S/abstract
and updated in Sedgwick et al. (2019b) https://ui.adsabs.harvard.edu/abs/2019arXiv190904535S/abstract

In particular, the relationship between CCSN rate as a function of mass and the GSMF is given in Section 2 of the 2019a paper.
The plots that can be reproduced using these data are shown in the 2019b paper.

The CCSN-rate densities are corrected for the effects of SN detection efficiencies as in Figure 11 of 2019a, or Fig. 1a of 2019b with the SFM photo-z also.
To convert these values to a star-formation rate density (SFRD) as a function mass, you need to divide by the R-value that is the number of CCSNe per mass of stars formed.
We used log R = -1.9 in 2019a to produce Fig. 12. For a Salpeter IMF, Madau & Dickinson (2014) provide a value of 0.0068 (log R = -2.17) for comparison (their Section 5.2, k_cc value).

SFRD per bin in log mass is then given in units of M_sun yr^{-1} Mpc^{-3} dex^{-1}.

Column details: 

1	logMstar				Galaxy Stellar Mass. Bin mid-point.																															log ($\mathcal{M}$/M$_{\odot}$) + 2 log h$_{70}$
2	logrhoccsn_zMedIC		CCSN-rate density using zMedIC photometric redshifts. Used in Sedgwick+19a & b.																				dex$^{-1}$ yr$^{-1}$ Mpc$^{-3}$ h$_{70}^{3}$
3	dlogrhoccsn_zMedIC		CCSN-rate density error using zMedIC photometric redshifts. Used in Sedgwick+19a & b.																		dex$^{-1}$ yr$^{-1}$ Mpc$^{-3}$ h$_{70}^{3}$
4	logrhoccsn_SFM			CCSN-rate density using SFM photometric redshifts. Used in Sedgwick+19b.																					dex$^{-1}$ yr$^{-1}$ Mpc$^{-3}$ h$_{70}^{3}$
5	dlogrhoccsn_SFM			CCSN-rate density error using SFM photometric redshifts. Used in Sedgwick+19b.																				dex$^{-1}$ yr$^{-1}$ Mpc$^{-3}$ h$_{70}^{3}$
6	logrhoccsn_wSFM			CCSN-rate density using SFM photometric redshifts and SFM nominal error-weighted redshift PDF. Used in Sedgwick+19b.										dex$^{-1}$ yr$^{-1}$ Mpc$^{-3}$ h$_{70}^{3}$
7	dlogrhoccsn_wSFM		CCSN-rate density error using SFM photometric redshifts and SFM nominal error-weighted redshift PDF. Used in Sedgwick+19b.									dex$^{-1}$ yr$^{-1}$ Mpc$^{-3}$ h$_{70}^{3}$
8	logphi_zMedIC			Number density using zMedIC photo-z's. Used in Sedgwick+19a & b.																							dex$^{-1}$ Mpc$^{-3}$ h$_{70}^{3}$
9	dlogphi_zMedIC			Number density error using zMedIC photo-z's, assuming constant SSFR with mass. Used in Sedgwick+19a & b.													dex$^{-1}$ Mpc$^{-3}$ h$_{70}^{3}$
10	dlogphi_zMedIC_ssfr_hi	Number density positive error using zMedIC photo-z's and accounting for uncertainty in SSFR. Used in Sedgwick+19a & b.										dex$^{-1}$ Mpc$^{-3}$ h$_{70}^{3}$
11	dlogphi_zMedIC_ssfr_lo	Number density negative error using zMedIC photo-z's and accounting for uncertainty in SSFR. Used in Sedgwick+19a & b.										dex$^{-1}$ Mpc$^{-3}$ h$_{70}^{3}$
12	logphi_SFM				Number density using SFM photo-z's. Used in Sedgwick+19b.																									dex$^{-1}$ Mpc$^{-3}$ h$_{70}^{3}$
13	dlogphi_SFM				Number density error using SFM photo-z's, assuming constant SSFR with mass. Used in Sedgwick+19b.															dex$^{-1}$ Mpc$^{-3}$ h$_{70}^{3}$
14	dlogphi_SFM_ssfr_hi		Number density positive error using SFM photo-z's and accounting for uncertainty in SSFR. Used in Sedgwick+19b.												dex$^{-1}$ Mpc$^{-3}$ h$_{70}^{3}$
15	dlogphi_SFM_ssfr_lo		Number density negative error using SFM photo-z's and accounting for uncertainty in SSFR. Used in Sedgwick+19b.												dex$^{-1}$ Mpc$^{-3}$ h$_{70}^{3}$
16	logphi_wSFM				Number density using SFM photo-z's and SFM nominal error-weighted redshift PDF. Used in Sedgwick+19b.														dex$^{-1}$ Mpc$^{-3}$ h$_{70}^{3}$
17	dlogphi_wSFM			Number density error using SFM photo-z's and SFM nominal error-weighted redshift PDF, assuming constant SSFR with mass. Used in Sedgwick+19b.				dex$^{-1}$ Mpc$^{-3}$ h$_{70}^{3}$
18	dlogphi_wSFM_ssfr_hi	Number density positive error using SFM photo-z's, SFM nominal error-weighted redshift PDF and accounting for uncertainty in SSFR. Used in Sedgwick+19b.	dex$^{-1}$ Mpc$^{-3}$ h$_{70}^{3}$
19	dlogphi_wSFM_ssfr_lo	Number density negative error using SFM photo-z's, SFM nominal error-weighted redshift PDF and accounting for uncertainty in SSFR. Used in Sedgwick+19b.	dex$^{-1}$ Mpc$^{-3}$ h$_{70}^{3}$