ETC Request ID: STIS.sp.181107

Exposure time (seconds) = 2,423.0000 at wavelength 2376.00 Å

gives: SNR = 16.9011 (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 0.078 375.88 19.39
    Background 0.025 118.73 10.90
        Sky 6.139e-07 2.98e-03 0.05
        Dark Current 0.025 118.73 10.90
Total in selected region 0.102 494.61 22.24
Brightest Pixel (single exposure) (at 2500.80 Å) 0.038 91.20
Count rate entire detector 3,733.396

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 63.372 153,549.906
    Background (sky+dark) 3,670.024 8,892,467.71

Encircled energy fraction 0.85


Instrument name: STIS
Mode: spectroscopic
Detector: NUVMAMA
Central Wavelength:
Grating: [G230L] R ~ 500
Aperture: 0.2X0.2


Target: [point source]
Spectrum: Bruzual Synthetic Stellar Spectra O9.5 I
Extinction E(B-V): Milky Way Diffuse (Rv=3.1) = 0.1 applied before normalization
Normalization: Renormalized to Johnson V = 18.87 in magnitudes relative to Vega
Redshift: None
Emission Lines: None


Selected background:
  Sky Background:
    Level:

Table of Source and Noise Counts per Pixel


Plots

These results were computed using: ETC version 19.2