 
mgavin at ntlworld dot com
2008 April 7/ 2010 Nov 2
- Spectroscopy - general
- 'players' in spectroscopy
- spectro for beginners
- lo-res stellar spectra
-
session spectra
- hi-res stellar spectra
-
refraction & spectra
-
full colour spectra [sun]
- planetary spectra
- PNe spectra
- cometary spectra
- Papers published papers
- Atmospheric phenomena
- rainbows
& arcs
- Equipment designs & reviews
- SBIG spectrometer
- Rainbow Optics grating
-
WPO spectrograph
- WPO
prism spectrograph
- Sivo spectrograph
- spectra
without optics!
- lo-res
lunar spectrograph
-
Ebert solar spectrograph
-
digicam lo-res grism
-
digicam filter tester
-
- Observations
- main
session spectra
- Cool stars
- T Cep series
- M-Type spectra
-
Rho Cas 2003
- Hot stars
- Wolf-Rayet stars
- Cygnus Wolf-Rayets
-
more WR in colour
- emission line stars
- mid-res emission stars
- PNe spectra
-
WZ Sge rare outburst
-
SS433
- 'lawn sprinkler'
- Explosive events -novae
- Nova 1917=CI Aql
- Nova Aql 1999 #1
- Nova Aql 1999 #2
- Nova
Aql 2001
- Nova
Cyg 2001 #2
- Nova
Cyg 2001 #1
- Nova
Sgr 2001 #3
- Nova
Sgr 2001 #2
- Nova
Sco 2001
- Nova?
Mon 2002
- Nova
Oph 2002
- 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
- Extra-galactic
- Supernovae
-
SN 2001bg in NGC 2608
-
Hypernova SN2002ap
-
SN2004dj in NGC2403
-
SN2005cf NCG-3-39-1
-
SN2005cs M51 CVn
- Quasars + their redshifts
-
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 |