DARKDECAYSIGNAL reference file
- REFTYPE:
DARKDECAYSIGNAL
- Data model:
DarkdecaysignalRefModel
The DARKDECAYSIGNAL reference file contains amplitudes and time constants for the exponential model for dark decay for each of the 18 WFI detectors. Time zero is referenced to the middle of the first science read, so the typical amplitude of the signal in the first read should correspond to the value of the amplitude given in the reference file. Decay times are in seconds and amplitudes are in DN.
Reference Selection Keywords for DARKDECAYSIGNAL
CRDS selects appropriate DARKDECAYSIGNAL references based on the following keywords. DARKDECAYSIGNAL is not applicable for instruments not in the table. All keywords used for file selection are required.
Instrument |
Keywords |
|---|---|
WFI |
instrument, date, time |
Standard ASDF metadata
The following table lists the attributes that are required to be present in all reference files. The first column shows the attribute in the ASDF reference file headers, which is the same as the name within the data model meta tree (second column). The second column gives the roman data model name for each attribute, which is useful when using data models in creating and populating a new reference file.
Attribute |
Fully Qualified Path |
|---|---|
author |
model.meta.author |
model_type |
model.meta.model_type |
date |
model.meta.date |
description |
model.meta.description |
instrument |
model.meta.instrument.name |
reftype |
model.meta.reftype |
telescope |
model.meta.telescope |
useafter |
model.meta.useafter |
NOTE: More information on standard required attributes can be found here: Standard ASDF metadata
Reference File Format
DARKDECAYSIGNAL reference files are asdf files with a
decay_table dictionary. This dictionary contains entries for
each WFI detector, WFI01–WFI18. Each entry in the dictionary
in turn contains a dictionary with two keywords,
amplitude and time_constant, both floats. These are
the amplitudes (in DN) and time constants (in seconds) of the
exponentially decaying dark decay model that needs to be
subtracted from uncalibrated Roman exposures.