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Chroma SII Filter Optimized for f/3 - 8nm

by Chroma
SKU CT-27011F3-1.25M
Original price CA$374.00 - Original price CA$1,129.00
Original price
CA$374.00
CA$374.00 - CA$1,129.00
Current price CA$374.00
Credit available from affirm logo

Description

Availability:
Backordered
Contact us to know when we will receive our next ones!
Availability:
Backordered
Contact us to know when we will receive our next ones!
Availability:
Backordered
Contact us to know when we will receive our next ones!
Availability:
Backordered
Contact us to know when we will receive our next ones!
Availability:
Backordered
Contact us to know when we will receive our next ones!
Availability:
Backordered
Contact us to know when we will receive our next ones!

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More information

SII filters isolate the spectral emission of singly ionized sulfur atoms, also common in nebulae. Emission is at two lines occurring as a doublet, at 671.6 and 673.1 nm. This filter also separates sulfur emission from H-alpha emission (656.3nm).

  • Filters designed for use with CCD and for f/3.0 telescopes
  • No reflections leading to image distortions or "back reflections"
  • Transmitted wavefront better than 0.25 waves/inch
  • Durable sputter coatings
  • Parallelism: < 30 arcsec
  • Thickness: 3.0 +/-0.05mm
  • Extremely durable coatings withstand humidity changes and extreme temperature fluxes and remain spectrally accurate
  • in CWL and band pass adherence
  • Capable of manufacturing large filters for large detectors: 50mm x 50mm, 65mm up to 76.2mm and 101.6mm square
  • All filters manufactured in Vermont

Chroma manufactures the highest quality astronomy filters with durable, sputtered hard coatings using single substrates of the best glass, eliminating the need for laminations. All primary filter coatings are applied on the front surface and anti-reflection coatings on the rear surface to prevent ghosting and to maximize transmission.

Highly precise and accurate, the passbands of these filters remain spectrally stable and do not drift in response to extreme temperature fluctuations or changes in humidity. They also can provide larger sizes and unique passbands upon request.