Własnie wyczytałem, że za uzyskane przeze mnie "dodatkowe" linie w paśmie 6300 -6500 i więcej może odpowiadać nasza ziemska atmosfera.
Zacytuję z książki "Analysis of astronomical spectra":
"It usually makes little sense to record the area on
the red side of Hα, except the emission lines of P Cygni and Be stars. Between approximately
6,200 – 7,700Å (see picture below), it literally swarms of atmospheric related (telluric)
H2O and O2 absorption bands.
Apart from their undeniable aesthetics they are interesting only for atmospheric physicist."
Słabo znam j.angielski, ale od czego mamy translatory?
Frugoslaw