Low Resolution Spectrum of M42
In order to understand which kind of objects can be observed, I try to find out what is the limiting magnetudes for the LHiRes III. To improve the sensitivity I ordered a 150 lines / mm grid which has been used with a 100m slit. Attached please find a spectra of M42 (together with one star of the central Trapez -Region)
The spectra has been taking using the telescopes of the Hans Ludwig Neuman Sternwarte. This observatory is operated by the Physikalischer Verein
A wavelength calibration has not been performed and is in this particular case not required. H-Alpha is the dominating line located as pixel 585. As well O [iii][ is located at pixel 318. A flux-calibration has also not yet been performed. This has a direct impact on the lineratios.
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RAW Spectra of Orion Nebula (M42)
November 28th, 2020 LHiRes III @ 60cm Cassegrain / |
Furthermore lines can be found:
Pixel
311 O[iii]
293 H-Beta
204 Hg (?)
467 He I
542 O I & S[III]
605 He I
614 S [ii]
671 H I
683 Ar [III]
715 O [ii]
Other spectra meanwhile obtained are stored on: Pandora Spectra