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2p2 WFI Exposure Time Calculator

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Optical Imaging Mode Version 5.0.0
Description.
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Input Flux Distribution

 Uniform (constant with wavelength)
 Blackbody: T =		 Kelvin
 Template Spectra:	  Redshift Z = 

Object Magnitude (Vega System):    Band:
Magnitudes are given per square arcsec for extended sources. Note that some template spectra are 
defined over a limited wavelength range and may not allow calculations for all instrument configurations.
The object magnitude is not taken into account for the following single line source. Single line Wavelength: nm Flux: 10E-16 ergs/s/cm2 (per arcsec2 for extended sources) FWHM: nm (Minimum value: 0.50) Spatial Distribution: Point Source Extended Source

Sky Conditions

Days From New Moon: Airmass: Seeing: arcsec The sky brightness is determined by the moon phase according to this table

Instrumental Setup

Telescope throughput (2 aluminium coated mirrors): 75.00% at 670 nm
Filter: 	 			
Detector (CCD ESO#50-57): Readout mode:	  Binning:  pixels

Results

 S/N: Value    Plotting range  %
 Exposure Time (s): Value    Plotting range  %
Plots: Toggle All / No Plots
 Input spectrum in physical units
 Total Efficiency
 CCD Illumination
 S/N as a function of Seeing
 S/N as a function of Exposure Time
   

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