ETC Request ID: STIS.sp.733962

Exposure time (seconds) = 3,000.0000 at wavelength 1400.00 Å

gives: SNR = 38.1373 (per resolution element)


Table of Source and Noise Counts per Pixel


Plots


Detailed Information Count rate Total counts Associated noise
(counts/s) (counts) (counts)
Counts (box 7 pixels high) (1 pix x pix) (2.0 pix resel x pix)
    Source 0.243 1,460.73 38.22
    Background 0.001 6.30 2.51
        Sky 2.425e-12 1.45e-08 1.21e-04
        Dark Current 0.001 6.30 2.51
Total in selected region 0.245 1,467.03 38.30
Brightest Pixel (single exposure) (at 1241.10 Å) 0.281 843.21
Count rate entire detector 514.305

Buffer Time (sec)
For APT purposes, the recommended buffer time should be 4/5 of the buffer time calculated above. Please refer to the STIS Instrument Handbook for more details.

Global Count Rates
    Source only 242.178 726,533.559
    Background (sky+dark) 272.128 816,382.58

Encircled energy fraction 0.82


Instrument name: STIS
Mode: spectroscopic
Detector: FUVMAMA
Central Wavelength:
Grating: [G140L] R ~ 1000
Aperture: 52X0.2
Glow region:


Target: [point source]
Spectrum: Non-stellar Objects QSO (SDSS based) [800, 8554.5 Å z=0]
Extinction E(B-V): Milky Way Diffuse (Rv=3.1) = 0.06 applied before normalization
Normalization: Flux 1e-14 flam at 1400.0 Å
Redshift: z=0.0206
Emission Lines: None


Selected background:
  Sky Background:
    Level:

Table of Source and Noise Counts per Pixel


Plots

These results were computed using: ETC version 23.2