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