VIRCAM Exposure Time Calculator

Infrared Imaging Mode Version 6.2.0
Description
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Target Input Flux Distribution

Template Spectrum Redshift
z =
Target Magnitude and Mag.System:   
= Vega
AB
Magnitudes are given per arcsec2 for extended sources
MARCS Stellar Model
Upload Spectrum
Blackbody Temperature: K
Power Law Index:           F(λ) ∝ λindex
Emission Line
Lambda: nm
Flux: 10-16 ergs/s/cm2 (per arcsec2 for extended sources)
FWHM: nm

Spatial Distribution:

Point Source
Extended Source diameter: arcsec
Extended Source (per pixel)

Instrument Setup

Filter:

Sky Conditions

Airmass:
Seeing/Image Quality:
For point sources, the resulting Image Quality FWHM is approximated by a gaussian in the ETC considering the transfer functions of the atmosphere, telescope and instrument. See the helpfile for details.
Seeing: arcsec FWHM in V-band at zenith (use this value in the proposal)
              Probability ---% of realising the seeing ≤ 0.80 arcsec
IQ: arcsec FWHM at the airmass and wavelength of observation (to be used for the OB constraint set)
              The corresponding seeing and probability will be indicated in the ETC output page
Image Quality is not a parameter in AO modes

Observing Setup

Detector on-chip integration time DIT = s (minimum DIT is 1.0 s)
Exposure Time: s
S/N ratio:
Observation Strategy:
       Exposure coadds (Ndit):
       Exposure loops (Nexp):
       Microstepping pattern (NxM):
       Jitter pattern (Njitter):
       Number of pawprints (Npaw):


Plots: Toggle All / No Plots

Input spectrum in physical units
CCD Illumination, Object only
Sky Radiance Spectrum in physical units (ph/s/m2/micron/arcsec2)
Total Background Emission Spectrum
Sky Transmission Spectrum
System Efficiency
S/N as a function of Exposure Time