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| Mar-18-2026 | 209166.99 руб. | 219624.52 руб. | 214395 руб. |
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Описание товара








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About this product
Chroma 5nm H-alpha filters are essential for imaging nebulae and other objects which are rich in ionised hydrogen. At 656.3nm, a narrow-band emission filter is required to separate H-alpha from the SII doublet (671.6nm and 673.1nm).
Chroma Technology is an employee-owned company based in Vermont, USA. Chroma manufacture 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 maximise transmission. Chroma astronomical filters are used worldwide in research and amateur applications.
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.
All filters may be used with focal ratios of f/4 or slower. For optics faster than f/4 then due to the spectral shift we recommend using the 5nm filters instead.
Manufacturer's number: 27002
FEATURES
CWL: 656nm, Bandwidth: 5nm
Durable sputter coatings
Parallelism: <30 arcsec
Thickness: 3.0 +/-0.05mm
Filters designed for use with CCD and for f/4.0 or slower
Transmitted wavefront better than 0.25 waves/inch
No reflections leading to image distortions or ‘back reflections’
36mm round unmounted
Transmission Chart

Chroma SII filters isolate the spectral emission of singly ionised 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).
Chroma Technology is an employee-owned company based in Vermont, USA. Chroma manufacture 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 maximise transmission. Chroma astronomical filters are used worldwide in research and amateur applications.
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.
All filters may be used with focal ratios of f/4 or slower. For optics faster than f/4 then due to the spectral shift we recommend using the 5nm filters instead.
Manufacturer's number: 27007
FEATURES
CWL: 672.4nm, Bandwidth: 5nm
Durable sputter coatings
Parallelism: <30 arcsec
Thickness: 3.0 +/-0.05mm
Filters designed for use with CCD and for f/4.0 or slower
Transmitted wavefront better than 0.25 waves/inch
No reflections leading to image distortions or ‘back reflections’
36mm round unmounted
Transmission Chart

Chroma’s OIII filters isolate the 500.7nm primary emission line of doubly ionized oxygen. After H-alpha, this is the next most common emission when imaging nebulaeChroma Technology is an employee-owned company based in Vermont, USA. Chroma manufacture 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 maximise transmission. Chroma astronomical filters are used worldwide in research and amateur applications.
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.
All filters may be used with focal ratios of f/4 or slower. For optics faster than f/4 then due to the spectral shift we recommend using the 5nm filters instead.
Manufacturer's number: 27010
FEATURES
CWL: 500.7nm, Bandwidth: 5nm
Durable sputter coatings
Parallelism: <30 arcsec
Thickness: 3.0 +/-0.05mm
Filters designed for use with CCD and for f/4.0 or slower
Transmitted wavefront better than 0.25 waves/inch
No reflections leading to image distortions or ‘back reflections’
36mm round unmounted
Transmission Chart

Handle coated pieces by the edges only. Clean gently only if necessary. Loose particles should be removed with a bulb puffer or filtered, pressurised air cleaner. If necessary, gently wipe surface using anhydrous alcohol and lint-free lab towels. Use new surface of towel with each wipe.
AVOID TOUCHING OR WIPING A/R COATED OR METAL MIRROR SURFACES
AVOID HANDLING EXPOSED COATINGS WITH BARE FINGERS
Proper orientation of the filter is necessary in order to minimise autofluorescence and maximise performance. There is a caret (arrow) located on the edge of each filter in order to aid orientation. Excitation (x) filters should be positioned with the arrow pointing toward the specimen, toward the inside of the cube, and away from the light source. Emission (m) filters should be placed with the arrow pointing toward the specimen, toward the inside of the cube, and away from the detector/eye. Dichroic mirrors should be mounted with the coated surface toward the light source, excitation filters, and the specimen. The dichroics either have an arrow on the side pointing to the coated side, or they are beveled on the coated side. The beveled side is the smaller surface.
Our shop is a Chroma certified authorized dealer



Andrea Ricciardi
Veil Nebula
Shot from the bad sky of the center of Rome, with some moon too...
200mm f/4 newton
Astrel Instruments AST8300B CCD camera
FILTERS
Chroma Technology 3nm spectral line filters: H-alpha, OIII and SII

Technical Details
Captured and processed by: Terry Hancock
Location: GrandMesaObservatory.com Purdy Mesa, Colorado
Dates of Capture July 30, August 6th, 8th, 11th and 13th 2020
HA 210 min 21 x 600 sec
OIII 140 min 14 x 600 sec
RGB 165 min 11 x 300 sec (per channel)
Narrowband Filters by Optolong
Camera: QHY600 Monochrome CMOS Photographic version
Camera Details and Specs
//www.qhyccd.com/index.php?m=content&c=index&a=show&catid=94&id=55
Gain 60, Offset 76 in Read Mode Photographic 16 bit
Calibrated with dark, Bias and Flat Frames
Optics: Walter Holloway's Takahashi FSQ 130 APO Refractor @ F5
Image Scale: 1.19 arcsec/pix
Field of View: 3d 7' 41.0" x 2d 3' 5.3 (127.3 x 190.1
arcmin)
EQ Mount: Paramount ME
Image Acquisition software Maxim DL6 Pre Processing in Pixinsight
Post Processed in Photoshop CC

Captured and processed by: Terry Hancock
Location: GrandMesaObservatory.com Purdy Mesa, Colorado
HA 210 min 21 x 600 sec
OIII 280 min 28 x 600 sec
SII 210 min 21 x 600 sec
Narrowband Filters by Chroma
Camera: QHY600 Monochrome CMOS Photographic version
Gain 60, Offset 76 in Read Mode Photographic 16 bit
Calibrated with Dark, Bias and Flat Frames
Optics: Walter Holloway's Takahashi FSQ 130 APO Refractor @ F5
Image Scale: 1.19 arcsec/pix
Field of View: 3d 7' 41.0" x 2d 3' 5.3 (127.3 x 190.1 arcmin)
EQ Mount: Paramount ME
Image Acquisition software Maxim DL6, Pre Processing and Starnet
in Pixinsight Post Processed in Photoshop CC
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Tax
The price list on our website is USD without tax
Please note that buyers are liable to pay tax involved, such as Import
tax, VAT , customs handling fee, etc. The additional fees may be collected at
time of delivery by courier.
Service
If you find any problem with the product,
please contact me as soon as possible and describe the problem in detail, we
will try our best to help you solve the problem.
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