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2p2 WFI Exposure Time Calculator

Optical Imaging Mode Version 6.0.0
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Input Flux Distribution

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

Object Magnitude:    Band: Vega  AB

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: 10-16 ergs/s/cm2 (per arcsec2 for extended sources) FWHM: nm (Minimum value: 0.50) Spatial Distribution: Point Source Extended Source

Sky Conditions

Moon phase: days from new Moon
Seeing: arcsec FWHM in V-band at zenith (use this value in the proposal). The seeing is irrelevant for extended sources.
Probability 60% for a seeing smaller or equal to the requested value
For point sources, the resulting Image Quality FWHM is modeled by the ETC considering the transfer functions of the atmosphere, telescope and instrument. See the helpfile for details.

Instrumental Setup

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


 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
 Details of Image Quality Calculations (only for pointsources) 

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