M13 du 01-05-2009

Ma première M13 avec l’Equinox 120 et le Canon EOS 40D défiltré juste avant les RAP en 2009 (01-05-2009)

10 poses de 300s unitaires, 7 darks, 14 flats et 15 offsets

M13
M13 – RAP 2009

M106 (NGC4248) Galaxie spirale

M106 (NGC4248) Galaxie spirale dans la constellation des chiens de chasse réalisée le 01-05-2014 dans le Quercy lors d’une sortie astro d’une semaine où nous n’avons eu qu’une nuit de potable !

1 pose unitaire de 600s avec ma caméra Atik 383L+ à -20°C et filtre Luminance Astrodon au foyer de la Takahashi TSA 120 + .

M106 (NGC4248) Galaxie spirale
M106 (NGC4248) Galaxie spirale

NGC 6992 et 6995 – Les dentelles du Cygne

J’ai repris un peu l’astro et j’ai fait un petit traitement de les dentelles du Cygne : NGC 6995 et NGC 6992 avec la FSQ106 et un filtre H-alpha 5nm devant ma caméra CCD Atik 383L+.

Voici donc le résultat : 6 x 1200s à -20°C en BIN 2.
NGC6995 Nébuleuse des Dentelles du Cygne
NGC6992 et NGC 6995 Nébuleuse des dentelles du Cygne

CCDT67 AP

CCDT67

CCDT67
CCDT67

The CCD Telecompressor (CCDT67)
The focal length of the CCDT67 CCD Telecompressor is 305 mm or 12.0” Again, using the formula introduced above, a distance of 101 mm or 4.0 inches gives the stated 0.67X compression. (305 – 101) / 305 = 0.67 Because the CCDT67’s focal length is much shorter than the 27TVPH’s, an equal change in distance will have a greater effect on the compression. If we shorten the distance by 35 mm as we did above for the 27TVPH, the compression factor becomes 0.78X. (305 – 66) / 305 = 0.78 Changing from 0.67X to 0.78X is certainly more drastic than changing from 0.75X to 0.80X as was the case for the 27TVPH. Please note also that the CCDT67’s more aggressive compression makes it less suitable for faster instruments.
We strongly recommend using the CCDT67 only on instruments with focal ratios of f/9 and higher.
The CCDT67 takes up 16 mm of the distance in your calculations. The rest of the distance is in the nosepiece, filter wheel, CCD camera and any extensions you may use. Note also that, unlike the above example with the 27TVPH, the entire nosepiece length is a part of the light path with the CCDT67 since the nosepiece does not get buried inside another adapter relative to the telecompressor.
The CCDT67 has a clear aperture of 44 mm or 1.75”. At 0.67X compression, it will fully illuminate a 29 mm circle – 44 mm x 0.67 = 29 mm.
To give a real world example, let’s assume the following: We will set up a system with the CCDT67 @ 16 mm; our AP16T – 2”/T2 nosepiece @ 29 mm; a color filter wheel @ 25 mm; and a CCD camera @ 25 mm. 16+29+25+25 = 95 mm. (305 – 95) / 305 = 0.69X 44 mm x 0.69 = 30 mm – the fully illuminated circle.

Camera de guidage StarLight Xpress Lodestar

Starlight Xpress Lodestar : http://www.sxccd.com/lodestar-autoguider

Starlight Lodestar - Alban BERNARD
Starlight Lodestar – Alban BERNARD
  •  CCD type: ICX429AL Sony Exview interline CCD with low dark current and vertical anti-blooming.
  •  CCD Full resolution Pixel data: Pixel size: 8.2uM x 8.4uM, Image format: 752 x 580 pixels
  •  CCD Image area: 6.4mm (Horizontal) x 4.75mm (Vertical).
  •  CCD quality: Grade 1
  •  Spectral Response: QE max at 620nM (~65%), 35% at 400nM and 770nM.
  •  Readout Noise: Less than 15 electrons RMS – typically only 10 electrons.
  •  Full-well capacity: Greater than 50,000 e- (unbinned)
  •  Anti-blooming: Overload margin greater than 1000x.
  •  Dark current: Dark frame saturation time greater than 1 hour. Less than 0.1 electrons/second @ + 10C ambient.
  •  Data format: 16 bits.
  •  System gain:  0.9 electrons per ADU
  •  Computer Interface: Built-in USB 2.0 compatible interface.
  •  Image download time: Typically 0.2 seconds at full resolution using USB 2.0.
  •  Power requirements: USB powered.
  •  Cooling system: Ambient air cooling.
  •  Size: diameter 32mm, length 72mm
  • Color : black anodised aluminium barrel
  • Mechanical Connection : 25 x 0.75mm ‘C mount’ thread at the CCD window end & 1.25″.
  • Backfocus: 13mm
  • Weight: approx. 50g.
  • Passive air cooling

 

Spectral Sensitivity Characteritics ICX249AL
Caractéristiques de la sensibilité spectrale du capteur ICX249AL

Monture Skywatcher EQ6 Custom made

(modèle noir de première génération) entièrement restauré par mes soins avec l’aide du collectif AVEX:

EQ6 custom - Alban BERNARD
EQ6 custom – Alban BERNARD

Voici les changements que j’ai effectué :

– changement des roulements des axes de DEC (déclinaison) et d’AD (Ascension Droite) y compris ceux des vis sans fin,
– changement de la graisse,
– ré-alésage de la cloche de DEC,
– rajout d’une butée sur l’axe d’altitude,
– changement de l’axe d’altitude,
– changement du pignon de sortie de moteur de DEC.

Elle fonctionne parfaitement bien.