Antlia
Antlia 4.5nm Narrowband Sulfur II (SII) EDGE Filter
Antlia 4.5nm Narrowband Sulfur II (SII) EDGE Filter
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Antlia SII EDGE narrowband filter optimizes the FWHM (full width half maximum) to 4.5nm bandpass. The suppression of optical density (OD)5 on unwanted wavelengths and the excellent transmittance characteristics found in the Antlia 3nm Pro series has been incorporated into the 4.5nm EDGE narrowband filters. The result is that these filters deliver superior SNR(signal to noise ratio) and better contrast in your images.
Antlia SII 4.5nm EGDE filters are designed to deliver high transmittance at the 672.4nm line that provides you with the maximum signal to reveal the faintest SII nebulae structures.
Conventional broader narrowband filters cause a heavy loss in transmission due to the strong Center Wavelength (CWL)-shift. We guarantee T>90% within 1nm range of the center bandwidth, which means that the SII 4.5nm EDGE narrowband filters can guarantee high transmittance for working with both long focal ratios and fast optical systems. Blue-shift data shows that Antlia 4.5nm EDGE filters can be used with nearly all systems as fast as f/3 with minimal loss in emission signal and meets the requirements of fast optics.
Application and Performance:
High transmittance and narrow bandwidth to maximize contrast
Steep spectral profile minimizes halos around bright stars
A single substrate to eliminate internal reflections
Narrowband Objects: SII Emission Nebulae, Planetary, Wolf-Rayet Nebulae and Supernova Remnants
Use in light polluted areas and dark sites
Extend imaging time when the moon is up
Antlia narrowband EDGE filters can be used down to f/3 systems with minimal loss of signal
All Antlia unmounted filters are edge blackened to eliminate internal reflections from stray light
Superior optical reliability reduces post image processing
This filter is only effective for deep sky objects that contain SII emissions
Technical Specifications:
Basic Substrate: Optical, Single / Non-glued substrate
Filter Thickness: 2mm+/-0.05mm for 1.25”, 2” mounted, Dia31mm and Dia36mm unmounted
3mm+/-0.05mm for Dia50mm unmounted
FWHM (Full width at half maximum): 4.5nm
CWL (Central Wavelength): 672.4nm
Peak Transmission: ＞90%
Blocking: > 5 OD(0.001% out of band blocking) @ 300-1000nm
Surface Quality: S/D (scratch/dig)= 60/40 (Refer to MIL-O-13830)
Transmitted Wavefront: Lambda/4 or better.
Parallelism: less than 30 arcsec
Warranty: 3-years against delamination
Spectrum Curve:
Filter Ring: 1.25'' (M28.5*0.6)
Not Recommended:
Solar imaging
Night visual observation
Not Permitted:
DO NOT LOOK AT THE SUN WITH THIS FILTER
Serious eye damage will result if you fail to observe the warning
Antlia SII EDGE narrowband filter optimizes the FWHM (full width half maximum) to 4.5nm bandpass. The suppression of optical density (OD)5 on unwanted wavelengths and the excellent transmittance characteristics found in the Antlia 3nm Pro series has been incorporated into the 4.5nm EDGE narrowband filters. The result is that these filters deliver superior SNR(signal to noise ratio) and better contrast in your images.
Antlia SII 4.5nm EGDE filters are designed to deliver high transmittance at the 672.4nm line that provides you with the maximum signal to reveal the faintest SII nebulae structures.
Conventional broader narrowband filters cause a heavy loss in transmission due to the strong Center Wavelength (CWL)-shift. We guarantee T>90% within 1nm range of the center bandwidth, which means that the SII 4.5nm EDGE narrowband filters can guarantee high transmittance for working with both long focal ratios and fast optical systems. Blue-shift data shows that Antlia 4.5nm EDGE filters can be used with nearly all systems as fast as f/3 with minimal loss in emission signal and meets the requirements of fast optics.
Application and Performance:
High transmittance and narrow bandwidth to maximize contrast
Steep spectral profile minimizes halos around bright stars
A single substrate to eliminate internal reflections
Narrowband Objects: SII Emission Nebulae, Planetary, Wolf-Rayet Nebulae and Supernova Remnants
Use in light polluted areas and dark sites
Extend imaging time when the moon is up
Antlia narrowband EDGE filters can be used down to f/3 systems with minimal loss of signal
All Antlia unmounted filters are edge blackened to eliminate internal reflections from stray light
Superior optical reliability reduces post image processing
This filter is only effective for deep sky objects that contain SII emissions
Technical Specifications:
Basic Substrate: Optical, Single / Non-glued substrate
Filter Thickness: 2mm+/-0.05mm for 1.25”, 2” mounted, Dia31mm and Dia36mm unmounted
3mm+/-0.05mm for Dia50mm unmounted
FWHM (Full width at half maximum): 4.5nm
CWL (Central Wavelength): 672.4nm
Peak Transmission: ＞90%
Blocking: > 5 OD(0.001% out of band blocking) @ 300-1000nm
Surface Quality: S/D (scratch/dig)= 60/40 (Refer to MIL-O-13830)
Transmitted Wavefront: Lambda/4 or better.
Parallelism: less than 30 arcsec
Warranty: 3-years against delamination
Spectrum Curve:
Filter Ring: 2'' (M48*0.75)
Not Recommended:
Solar imaging
Night visual observation
Not Permitted:
DO NOT LOOK AT THE SUN WITH THIS FILTER
Serious eye damage will result if you fail to observe the warning
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Antlia SII EDGE narrowband filter optimizes the FWHM (full width half maximum) to 4.5nm bandpass. The suppression of optical density (OD)5 on unwanted wavelengths and the excellent transmittance characteristics found in the Antlia 3nm Pro series has been incorporated into the 4.5nm EDGE narrowband filters. The result is that these filters deliver superior SNR(signal to noise ratio) and better contrast in your images. Antlia SII 4.5nm EGDE filters are designed to deliver high transmittance at the 672.4nm line that provides you with the maximum signal to reveal the faintest SII nebulae structures. Conventional broader narrowband filters cause a heavy loss in transmission due to the strong Center Wavelength (CWL)-shift. We guarantee T>90% within 1nm range of the center bandwidth, which means that the SII 4.5nm EDGE narrowband filters can guarantee high transmittance for working with both long focal ratios and fast optical systems. Blue-shift data shows that Antlia 4.5nm EDGE filters can be used with nearly all systems as fast as f/3 with minimal loss in emission signal and meets the requirements of fast optics. Application and Performance: High transmittance and narrow bandwidth to maximize contrast Steep spectral profile minimizes halos around bright stars A single substrate to eliminate internal reflections Narrowband Objects: SII Emission Nebulae, Planetary, Wolf-Rayet Nebulae and Supernova Remnants Use in light polluted areas and dark sites Extend imaging time when the moon is up Antlia narrowband EDGE filters can be used down to f/3 systems with minimal loss of signal All Antlia unmounted filters are edge blackened to eliminate internal reflections from stray light Superior optical reliability reduces post image processing This filter is only effective for deep sky objects that contain SII emissions Technical Specifications: Basic Substrate: Optical, Single / Non-glued substrate Filter Thickness: 2mm+/-0.05mm for 1.25”, 2” mounted, Dia31mm and Dia36mm unmounted 3mm+/-0.05mm for Dia50mm unmounted FWHM (Full width at half maximum): 4.5nm CWL (Central Wavelength): 672.4nm Peak Transmission: ＞90% Blocking: > 5 OD(0.001% out of band blocking) @ 300-1000nm Surface Quality: S/D (scratch/dig)= 60/40 (Refer to MIL-O-13830) Transmitted Wavefront: Lambda/4 or better. Parallelism: less than 30 arcsec Warranty: 3-years against delamination Spectrum Curve:
Filter Ring: 1.25''(M28.5*0.6)，2'' (M48*0.75) Ultra-thin filter cell to minimize vignetting, Black anodized finish, Laser engraving No fading Available Sizes： Mounted： 1.25''， 2'' Unmounted：Dia31mm，Dia36mm，Dia50mm Not Recommended: Solar imaging Night visual observation Not Permitted: DO NOT LOOK AT THE SUN WITH THIS FILTER. Serious eye damage will result if you fail to observe the warning.
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