Baader L-RGB CCD-Filterset 50×50 mm

 625,00

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Baader L-RGB CCD-Filterset 50×50 mm

Beschikbaar via nabestelling

Type:
L-RGB
Grote (mm):
50x50 mm
Aansluiting op telescoop:
Niet van toepassing
Geschikt voor visueel:
Slecht
Geschikt voor astrofotografie:
Uitstekend
Geschikt voor fullframe:
Uitstekend
Diameter (mm):
50
Dikte (mm):
3
 625,00
Niet op voorraad (kan nabesteld worden)
Levertijd: vraag ons naar de levertijd + verzendtijd
Artikelnummer: B2458487 Categorieën: , , ,
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Beschrijving

Baader L-RGB CCD-Filterset 50×50 mm

Mechanical Properties

  • Parfocal and plane polished substrates. Each individual filter is optically fine-polished to 1/4 wave.
  • Baader L-RGB filters are hard coated individually.
  • Baader filters especially are not cut out of large size plate-glass, which is a typical manufacturing process for economy filters (cut-out filters exhibit micro-cracks around all edges. Capillary action between glass and coating layers will lead to premature ageing due to moisture deposition).
  • All Baader filters have individual coating sealed edges, impermeable against ageing because the the penetration of moisture impossible.
  • Baader filters are being tested repeatedly to comply with MIL-specifications. One common process is to boil the test specimen for one hour in salt water. Baader filters remained completely intact as opposed to filters drilled out of large glass plates.
  • All Baader filters sport scratch resistant hard coatings which can be cleaned repeatedly throughout their entire lifetime. As many times as needed – preferably with Baader Optical Wonder cleaning fluid.

Optische eigenschappen van de Baader L-RGB CCD-Filterset 50×50 mm zijn:

  • No reflections when compared to competing RGB-filter recipes.
  • Balanced RGB-design offer 1:1:1 exposure times for most telescope optical systems – an important benefit when imaging in automated mode.
  • Maximized colour contrast for each of the three RGB channels – achieved through steep slopes at all transmission curves combined with science approved placement of spectral window.
  • O III emission line double-weighted in the B and G channel as well, with maximum peak transmission for unparalleled deep sky S/N yield
  • R-Filter provides maximum transmission of H-alpha and S II emission but at the same time completely blocks all NIR and IR from 680 out to 1200 nm
  • Blocking of Mercury and Sodium vapour lamps at 580 nm in the G and R filters blackens the sky background and maximizes colour balance and colour separation.