APT ETC

 


User's Guide
Contents
Return to ETC
Welcome
SYNPHOT
SNR and Exposure Time
SNR
Time
Optimal SNR
Spectroscopy
Target Acquisition
Basic Use
Page Heirarchy
Reference
Extraction Regions
Spectral Distribution
User Spectra
Other Spectra
Extinction
Normalization
Background
CCD Parameters
ID Number
Calculations
SYNPHOT Calls
Call Descriptions
Call Parameters
NICMOS Spectroscopic Extraction Regions
Tables
Spectral Elements
NICMOS Filters
NICMOS Dispersers
ACS Filters and Dispersers
COS Dispersers
WFC3 Filters and Dispersers
STIS Filters and Dispersers
NICMOS Tables
COS Tables
STIS Tables and Topical Help

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 type 1

Type of limit

Limiting count rate 2

 

FUV

Predictable

Global

15,000 per segment

Local

40 per resel 3

Irregular

Global

6,000 per segment

Local

40 per resel 3

     

          NUV

Predictable

Global

30,000 per stripe

Local

80 per pixel

Irregular

Global

12,000 per stripe

Local

80 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)

0.5 per cm2
7.2 × 10-7 per pixel
4.3 × 10-5 per resel

34 per cm2
2.1 × 10-4 per pixel
1.9 × 10-3 per resel

Read noise

0

0