Dear all,
I am from Reunion Island and following the mira 's spectrum variation with a star analyser. I dont understand the 7600A spike. Is it a process error or a real variation of the star ?
Thanks,
Emmanuel
Dear all,
I am from Reunion Island and following the mira 's spectrum variation with a star analyser. I dont understand the 7600A spike. Is it a process error or a real variation of the star ?
Thanks,
Emmanuel
Hi Emmanuel,
It is close to the very strong O2 telluric band.
http://www.astrosurf.com/buil/us/vatlas/vega4.gif
Could it be some sort of problem with the telluric line correction in that region ?
Cheers
Robin
Hi Robin,
You're right, i didn't remove the differents telluric spikes from my instrumental response.... and i think i have a calibration issue with the Hydrogen Balmer...
I will restart the process
Thanks,
Emmanuel
Dear All,
I removed the telluric lines from my differents instrumental response, the result seems better even if i have a calibration issue with the Hdelta and gamma. I hope the graph shows the real variation of Mira and not another problem in the process...
Thanks,
Emmanuel
To: Emmanuel,
Nice Mira spectrum! When you feel proficient, youmay want to invest in higher resolution spectroscope(s) like the Alpy600 or LISA. Here is a composite spectrum I took of Mira approximately the same time as yours with my Alpy600 working btw 3700-7400A and my LISA in IR mode working at 6200-9600A, stiched together. Looks like we agree on H-delta & H-gamma, but Alpy600 has 4-6x the resolution of the SA200 grating so the emission lines look more intense in mine, but definetly shows in yours. Note that Mira's spectrum (like most cool M stars) gets stronger well into the IR.
James