MISTRAL ETC spectro
MISTRAL ETC Spectro
We give in the following the parameter ranges we tested. Values outside of these ranges will give a predicted exposure time (except for unphysical airmasses), but we suggest to carefully look at the 3D plots, as this exposure time may be affected by model divergences.
Moon conditions
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Choose a moon condition
45deg from moon + 25% illumination
45deg from moon + 50% illumination
45deg from moon + 75% illumination
45deg from moon + 100% illumination
90deg from moon + 25% illumination
90deg from moon + 50% illumination
90deg from moon + 75% illumination
90deg from moon + 100% illumination
135deg from moon + 25% illumination
135deg from moon + 50% illumination
135deg from moon + 75% illumination
135deg from moon + 100% illumination
180deg from moon + 25% illumination
180deg from moon + 50% illumination
180deg from moon + 75% illumination
180deg from moon + 100% illumination
OHP seeing is typically varying between 1arcsec (not very often), and 5arcsec, with a median value close to 2.5arcsec.
Seeing
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Object type
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Choose an object type
Punctual objects (stars)
Extended objects (distant galaxies not surface brightness dominated)
Object (modeled by a gaussian) apparent fwhm (arcsec). Only used if extended object
Object apparent fwhm
Targetted magnitude (V band, Vega system). Values below 0 are too bright for T193/MISTRAL. Values below 2 are difficult because camera shutter may have difficulties to follow such bright objects without saturation (minimal exposure time is ~0.5sec). Values above 21 are in unexplored domains, exposure times may be wrong. Such values are anyway too faint for T193/MISTRAL.
Magnitude you want to reach?
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Gives the Air Mass (>1). Values above 2 are in unexplored domains, exposure times may be wrong (and telescope broken...).
Air Mass
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Do you want an additionnal extinction? Give a magnitude (>0.)
Gives the required S/N (between 3 and 25). Values below 3 and upper 25 are in unexplored domains, exposure times may be wrong.
S/N
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Spectrum type (absorption or emission)
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Choose an spectrum type
Absorption lines
Emission lines
Dispersor (blue or red)
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Choose an dispersor
Blue
Red