pynrc.simul.dms.populate_group_table

pynrc.simul.dms.populate_group_table(starttime, grouptime, ramptime, numint, numgroup, ny, nx)

Create some reasonable values to fill the GROUP extension table. These will not be completely correct because access to other ssb scripts and more importantly, databases, is necessary. But they should be close.

Parameters

• starttime (astropy.time.Time) – Starting time of exposure

• grouptime (float) – Exposure time of a single group (seconds)

• ramptime (float) – Exposure time of the entire exposure (seconds)

• numint (int) – Number of integrations in data

• numgroup (int) – Number of groups per integration

• ny (int) – Number of pixels in the y dimension

• nx (int) – Number of pixels in the x dimension

Returns

grouptable (numpy.ndarray) – Group extension data for all groups in the exposure