SNfactory Selection of SN candidates & Definition of SN Samples


Generic Flags:    Avoid bright stars
                  Must have guide stars
                  Avoid exposure time hit due to moon



Unbiased: variable stars (flag if POSS star) AGN (flag if known AGN/radio/x-ray source) gamma-ray burster (HETI/SWIFT, etc., X-check) SN derived software requirements: links to APS, APM, USNO catalogs of POSS links to FIRST and NVSS catalogs derived observing requirements: single screening spectrum
Rates sub-sample derived software requirements: insertion & recovery of fake SNe derived observing requirements single screening spectrum
Peculiar velocity sub-sample derived software requirements: weight assigned based on being nearby and in coverage gap derived observing requirements screening spectrum lightcurve in B & V (minimum)
Calibration sub-sample derived software requirements: weight according to likelihood of having Cepheids, masers etc. using link to appropriate catalogs derived observing requirements single screening spectrum
Host-galaxy luminosity function sub-sample derived software requirements: software for galaxy photometry derived observing requirements: good final reference *image* of host single screening spectrum
SN Host properties correlation sub-sample derived software requirements: software to assess type of host (high-luminosity, low-luminosity, spiral, elliptical, LSB, dusty, IRAS, size of 4000A break, strength of OII3727, H-alpha, etc.) weight according need for given type of host derived observing requirements: full spectral/lightcurve follow-up
SN properties sub-sample derived software requirements: software to measure stretch, expansion velocity, colors, early phase, and other SN properties weight assigned by uniqueness of SN properties derived observing requirements: full spectral/lightcurve follow-up
Volume-limited sub-sample derived software requirements: definition of volumes covered by deep (z > 0.1), filled redshift surveys determination of SN redshift and sky position assign weight according to volume-limit and coverage by deep, filled redshift survey derived observing requirements: full spectral/lightcurve follow-up