Difference between revisions of "Filters"
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A common system of filters is available for use with the CCD cameras at Moore and Mt. | A common system of filters is available for use with the CCD cameras at Moore, Mt. Kent and Mt. Lemmon observatories. With some exceptions, noted below, all filters are mounted in wheels that may be changed on request. | ||
== Sloan Photometry == | == Sloan Photometry == | ||
There | There is a set of Sloan filters for each of the ULMT, MORC24, CDK20N, CDK20S, and CDK700 telescopes. Each set excepton ULMT is in a wheel with 6 openings assigned serially. | ||
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*(3) i' (700-825) | *(3) i' (700-825) | ||
*(4) z' (825-1100) | *(4) z' (825-1100) | ||
*(5) | *(5) blue block (500-1100) | ||
*(6) Open | *(6) Open | ||
[[File: | Currently the ULMT wheel has 10 openings including the Sloan filters, color imaging filters, H-alpha and [OIII]. That wheel is scheduled to be replaced with a 7-filter wheel that has Sloan, plus others to be determined. | ||
[[File:astrodon_sloan.jpg|600px|center]] | |||
[[File:astrodon_cbb.jpg|600px|center]] | |||
== Transformation from Sloan to UBVRI Filter Bands == | |||
Transformation coefficients are discussed on the Sloan Digital Sky Survey | |||
[http://www.sdss.org/dr7/algorithms/sdssUBVRITransform.html Sloan Digital Sky Survey website] | |||
== UBVRI Photometry == | == UBVRI Photometry == | ||
There is one UBVRI filter wheel at each observatory to be used as needed an any telescope with an IFW3 filter wheel. | |||
*(1) B (375-490) | *(1) U (340-390) | ||
*( | *(2) B (375-490) | ||
*( | *(3) V (490-580) | ||
*( | *(4) R (570-690) | ||
*(5) I (725-1025) | |||
*(6) Open | *(6) Open | ||
[[File:Ubvric_ad.jpg|400px|center]] | |||
== BGRC Color Imaging == | == BGRC Color Imaging == | ||
There is one color imaging | There is one color imaging wheel at each site. | ||
*(1) | *(1) C (350-1100) | ||
*(2) | *(2) R (590-700) | ||
*(3) | *(3) G (490-575) | ||
*(4) | *(4) B (390-510) | ||
*(5) Open | *(5) Open | ||
*(6) Open | *(6) Open | ||
[[File: | [[File:Lrgb_ad.jpg|400px|center]] | ||
== Narrowband == | == Narrowband == | ||
There are | There are three narrowband filter sets available. The wheels at Mt. Kent for CDK20S and CDK700 use Astrodon filters: | ||
*(1) [SII] | *(1) [SII] (3/671.6) | ||
*(2) H alpha (656) | *(2) H alpha (3/656.3) | ||
*(3) Red continuum | *(3) Red continuum (5/645) | ||
*(4) | *(4) [O III] (3/500.7) | ||
*(5) | *(5) UV blocked clear | ||
*(6) Open | *(6) Open | ||
*(1) [SII] | A wheel for the CDK20N is | ||
*( | |||
*(1) He I (5/1083.0) (Custom Scientific) | |||
*(4) | *(2) [SII] (3/671.6) | ||
*(5) [O III] | *(3) H alpha (3/656.3) | ||
*(6) | *(4) Red continuum (5/645) | ||
*(5) [O III] (3/500.7) | |||
*(6) UV blocked clear | |||
A wheel for use at the RC24 is | A wheel for use at the RC24 is | ||
*(1) [SII] | *(1) [SII] (Custom Scientific) | ||
*(2) H alpha | *(2) H alpha (Custom Scientific) | ||
*(3) | *(3) Red continuum (Astrodon) | ||
*(4) Na D (590) | *(4) Na D (590) (Custom Scientific) | ||
*(5) [OIII] | *(5) [OIII] (Custom Scientific) | ||
*(6) UV blocked clear (Astrodon) | |||
[[File:Sii_filter.jpg|400px|center]] | [[File:Sii_filter.jpg|400px|center]] | ||
| Line 79: | Line 96: | ||
[[File:Red_continuum_ad.jpg|400px|center]] | [[File:Red_continuum_ad.jpg|400px|center]] | ||
[[File:Oiii_filter_cs.jpg|400px|center]] | [[File:Oiii_filter_cs.jpg|400px|center]] | ||
== SBIG STL Filters == | == 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 | The SBIG STL6303 cameras take 50 mm diameter filters in a 5-filter wheel. Moore and Mt. Kent observatories have the standard UBVRI set installed in the STL cameras used on the wide-field FSQ telescope for student projects: | ||
*(1) U (330-390) | *(1) U (330-390) | ||
| Line 92: | Line 107: | ||
*(5) I (725-1025) | *(5) I (725-1025) | ||
Additionally, at | Additionally, at both locations there is a set of color imaging RGBC filters in spare wheels. STL cameras require disassembly to change wheels. | ||
Latest revision as of 08:21, 1 January 2018
A common system of filters is available for use with the CCD cameras at Moore, Mt. Kent and Mt. Lemmon observatories. With some exceptions, noted below, all filters are mounted in wheels that may be changed on request.
Sloan Photometry
There is a set of Sloan filters for each of the ULMT, MORC24, CDK20N, CDK20S, and CDK700 telescopes. Each set excepton ULMT is in a wheel with 6 openings assigned serially.
- (1) g' (400-530)
- (2) r' (530-700)
- (3) i' (700-825)
- (4) z' (825-1100)
- (5) blue block (500-1100)
- (6) Open
Currently the ULMT wheel has 10 openings including the Sloan filters, color imaging filters, H-alpha and [OIII]. That wheel is scheduled to be replaced with a 7-filter wheel that has Sloan, plus others to be determined.
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 is one UBVRI filter wheel at each observatory to be used as needed an any telescope with an IFW3 filter wheel.
- (1) U (340-390)
- (2) B (375-490)
- (3) V (490-580)
- (4) R (570-690)
- (5) I (725-1025)
- (6) Open
BGRC Color Imaging
There is one color imaging wheel at each site.
- (1) C (350-1100)
- (2) R (590-700)
- (3) G (490-575)
- (4) B (390-510)
- (5) Open
- (6) Open
Narrowband
There are three narrowband filter sets available. The wheels at Mt. Kent for CDK20S and CDK700 use Astrodon filters:
- (1) [SII] (3/671.6)
- (2) H alpha (3/656.3)
- (3) Red continuum (5/645)
- (4) [O III] (3/500.7)
- (5) UV blocked clear
- (6) Open
A wheel for the CDK20N is
- (1) He I (5/1083.0) (Custom Scientific)
- (2) [SII] (3/671.6)
- (3) H alpha (3/656.3)
- (4) Red continuum (5/645)
- (5) [O III] (3/500.7)
- (6) UV blocked clear
A wheel for use at the RC24 is
- (1) [SII] (Custom Scientific)
- (2) H alpha (Custom Scientific)
- (3) Red continuum (Astrodon)
- (4) Na D (590) (Custom Scientific)
- (5) [OIII] (Custom Scientific)
- (6) UV blocked clear (Astrodon)
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 UBVRI set installed in the STL cameras used on the wide-field FSQ telescope for student projects:
- (1) U (330-390)
- (2) B (375-490)
- (3) V (490-580)
- (4) R (570-690)
- (5) I (725-1025)
Additionally, at both locations there is a set of color imaging RGBC filters in spare wheels. STL cameras require disassembly to change wheels.