SPECTROSCOPY
Spectroscopy is definitely the "last frontier" for amateur astronomers and the spectrograph makes the difference between astronomy and astrophysics!
La espectroscopia es posiblemente la última y más atrevida frontera para los astronomos amateurs y el uso del espectrógrafo marca la diferencia entre Astronomia y Astrofisica!
The first spectroscope, just for visual usage
My first reference spectra lamps
Star Analyser, a good starting point for spectroscopy
NGC 1647 star cluster spectra throw a Star Analyzer diffraction grating
Basic optical layout of Tacande Observatory spectrograph
The first spectrograph prototype
The new spectrograph build and designed at Tacande Observatory
Sun spectra around H-alpha line
Sun spectra profile normalized to continuum
Antares (Alpha Scorpius) spectra + Neon reference spectra lines
Spectra of gamma Velorum, the most brighter Wolf Rayet star
Old reference lamps system, Ne, Kr and Glow starter lamps
Emission spectra lines from Neon reference lamp
Inside the new Tacande spectrograph
The spectrograph attached to a T400 telescope, Tacande Observatory
Sigma Aquila a spectroscopic double
Spectrum of sigma Aquila around the H-beta line
sigma Aquila spectrum along 5 observing nights. Please note the "notch" on some H-beta lines due to secondary start Doppler shift
Adapting fiber optics to the spectrograph
Neon and Krypton calibrations lamps adapter to Fiber Optics 1/2
Neon and Krypton calibrations lamps adapter to Fiber Optics 2/2
Complete Fiber Optics Astropriorat spectrograph layout
New DADOS spectrograph layout 1/2
New DADOS spectrograph layout 2/2
Fiber Optics Astropriorat spectrograph 1/2
Fiber Optics Astropriorat spectrograph 2/2
For more details on the
equipment and techniques used, see the page: Astronomical
Observatory Handbook on this blog
Para más información de
las técnicas y el equipo empleado, ver la página: Manual
del Observatorio Astronómico en este blog
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