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Observatory Support
STScI Exposure Time Calculators Oversight

Detector Count Rate Restrictions

The ETC uses the current count rate screening restrictions, which are taken from Section 11.5 of the COS Instrument Handbook. If the observation will exceed any of the count rate restrictions, a warning message will be given in the output page. The count rate restrictions for the detectors are as follows:

COS Count Rate Screening Limits

Detector Source type1 Type of limit Limiting count rate2
FUV Predictable Global 15,000 per segment
Local 40 per resel3
Irregular Global 6,000 per segment
Local 40 per resel3
NUV Predictable Global 30,000 per stripe
Local 70 per pixel
Irregular Global 12,000 per stripe
Local 70 per pixel
Imaging Global 170,000 (over entire detector)
Local 70 per pixel

1"Predictable" means the brightness of the source can be reliably predicted for the time of observation to within 0.5 magnitude.

2Entries are counts per second.

3An FUV resel is 6 pixels wide by 10 high.

Detector Dark Background

The following table lists the dark count rate and read noise characteristics of the COS detectors as measured in ground tests.

Detector background count rates (per second) for COS.

Detector: FUV XDL NUV MAMA
Dark rate (counts sec-1) 1.5 per cm2
7.2 x 10-7 per pixel
4.3 x 10-5 per resel
11 per cm2
2.1 x 10-4 per pixel
1.9 x 10-3 per resel
Read noise 0 0