Filters

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A common system of filters is available for use with the CCD cameras at Moore and Mt. Kent Observatory. With some exceptions, noted below, all filters are mounted in wheels that may be changed on request.


Sloan Photometry

There are 4 sets of Sloan filters for use at the RC24, CDK20N, CDK20S, and CDK700 telescopes. Each set is in a wheel with 6 openings assigned serially With 4 separate sets it is possible for all telescopes to be used for photometry at any time.


  • (1) g' (400-530)
  • (2) r' (530-700)
  • (3) i' (700-825)
  • (4) z' (825-1100)
  • (5) blue block (500-1100)
  • (6) Open
Sloan griz ad.jpg

Transformation from Sloan to UBVRI Filter Bands

Transformation coefficients are discussed on the Sloan Digital Sky Survey Sloan Digital Sky Survey website

UBVRI Photometry

There will be one UBVRI filter wheel at each observatory. The filters are currently on order.

  • (1) U (340-390)
  • (2) B (375-490)
  • (3) V (490-580)
  • (4) R (570-690)
  • (5) I (725-1025)
  • (6) Open


Ubvric ad.jpg

BGRC Color Imaging

There is will be one color imaging wheel at each site. One is already available at Moore Observatory and a second one is on order.

  • (1) B (390-510)
  • (2) G (490-575)
  • (3) R (590-700)
  • (4) C (350-1100)
  • (5) Open
  • (6) Open
Lrgb ad.jpg

Narrowband

There are four narrowband imaging sets available. The standard wheels at Mt. Kent for CDK20S and CDK700 are

  • (1) [SII]
  • (2) H alpha (656)
  • (3) Red continuum
  • (4) Open
  • (5) [O III]
  • (6) Open

A wheel primarily use at the CDK20N is

  • (1) [SII]
  • (2) H alpha
  • (3) Red continuum
  • (4) He I (1083)
  • (5) [O III]
  • (6) Open

A wheel for use at the RC24 is

  • (1) [SII]
  • (2) H alpha
  • (3) Rec continuum
  • (4) Na D (590)
  • (5) [OIII]
Sii filter.jpg
Halpha 5nm ad.jpg
Red continuum ad.jpg
Oiii filter cs.jpg

SBIG STL Filters

The SBIG STL6303 cameras take 50 mm diameter filters in a 5-filter wheel. Moore and Mt. Kent observatories have the standard UBVIC set installed in the STL cameras:

  • (1) U (330-390)
  • (2) B (375-490)
  • (3) V (490-580)
  • (4) R (570-690)
  • (5) I (725-1025)

Additionally, at Mt. Kent there is a set of color imaging BGRC filters in a spare wheel. STL cameras require disassembly to change wheels.

The STL camera at Mt. Kent has been retired from Shared Skies and may be used on the APTA telescope there. The STL camera at Moore Observatory is in use on the FSQ roll roof telescope.