 
mgavin at ntlworld dot com
2008 April 7
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Spectroscopy - general
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'players'
in spectroscopy
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spectro
for beginners
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lo-res
stellar spectra
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session
spectra
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hi-res
stellar spectra
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refraction
& spectra
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full
colour spectra [sun]
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planetary
spectra
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PNe
spectra
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cometary
spectra
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Papers published
papers
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Atmospheric phenomena
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rainbows
& arcs
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Equipment designs & reviews
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SBIG
spectrometer
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Rainbow
Optics grating
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WPO
spectrograph
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WPO
prism spectrograph
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Sivo
spectrograph
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spectra
without optics!
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lo-res
lunar spectrograph
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Ebert
solar spectrograph
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digicam
lo-res grism
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digicam
filter tester
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Observations
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main
session spectra
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Cool stars
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T
Cep series
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M-Type
spectra
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Rho
Cas 2003
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Hot stars
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Wolf-Rayet
stars
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Cygnus
Wolf-Rayets
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more WR
in colour
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emission
line stars
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mid-res
emission stars
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PNe
spectra
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WZ
Sge rare outburst
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SS433
- 'lawn sprinkler'
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Explosive events -novae
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Nova
1917=CI Aql
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Nova
Aql 1999 #1
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Nova
Aql 1999 #2
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Nova
Aql 2001
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Nova
Cyg 2001 #2
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Nova
Cyg 2001 #1
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Nova
Sgr 2001 #3
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Nova
Sgr 2001 #2
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Nova
Sco 2001
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Nova?
Mon 2002
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Nova
Oph 2002
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Nova
Sgr 2002 # 2
Nova
Sgr 2002 # 3
V838
Mon [nova]
Nova
Cen 2002
Nova
Sgr 2003#2
Nova
Sct 2003
Nova
Oph 2003
Nova
Oph 2004
Nova
Sco 2004 #1
Nova
Sco 2004 #2
Nova V1663 Aql05
Nova V2362 Cyg06
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Extra-galactic
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Supernovae
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SN
2001bg in NGC 2608
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Hypernova
SN2002ap
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SN2004dj
in NGC2403
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SN2005cf NCG-3-39-1 Lib
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SN2005cs M51 CVn
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Quasars
+ their redshifts
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BL
Lac outburst
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I
have a long-standing interest in spectroscopy and it thus dominates my
website. Most of the equipment, other than prisms and gratings, has
been home-made and building the various devices was great fun. It
is very rewarding to capture spectrograms of stars and planets showing
the gases and various elements in their atmospheres.
An
early Vega spectrogram below taken on Kodak 2475 [my favourite spectro
film in pre CCDs days] via OG prism. Print 'snapped' with Kodak DC40 camera
and image reworked via Paintshop Pro. Film has better penetration than
CCDs into UV [recording the hydrogen Balmer series to ~370nm] but only
just beyond Ha
at 656.3nm in red. The Balmer 'head' converges [H# = infinity] at 364.56nm
in UV.
Partial
colour spectrum of variable star XY Lyrae [north of Vega] via MX5c one-shot
colour CCD and WPO spectrograph.coupled to 0.3m Meade LX200
visitors via www.digits.com
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