All Tables
- Table 1:
Hierarchy of galaxies extracted from the original SDSS
DR5 spectroscopic galaxy sample within z=0.04
- Table 2:
The table shows the expected CCSN rates within the SDSS DR5
spectroscopic survey area (14% of the entire sky) out to a distance of
.
- Table 3:
Relative CCSRs taken from
Smartt et al. (2007).
- Table 4:
Peak magnitude distributions from Richardson et al. (2002).
- Table 5:
Estimated intrinsic and detectable CCSRs within the
SDSS DR5 survey area and z<0.04. Also shown are the rates extended to the PS1 survey area.
- Table 6:
Estimated intrinsic and detectable CCSRs within the SDSS
DR5 survey area and z<0.056. Also shown are the rates extended to the PS4 survey area.
- Table 7:
The 25
AB limiting magnitudes for PS1, PS4 and LSST.
- Table 8:
Predicted CCSRs for PS1, PS4 and LSST.
- Table 9:
Comparison between the relative magnitudes of CCSNe we predict with a volume-limited (z<0.04) search with PS1 and those discovered within the same volume by the Nearby Supernova Factory.