Antlia SII 2.5nm Ultra Narrowband Filter
- Isolates Sulfur-II emission at 671.6nm and 673.1nm
- Ultra-narrow 2.5nm FWHM bandpass
- Peak transmission of >=95%
- Out-of-band blocking at OD5 (0.001%)
- Thermally stable quartz glass substrate
Check which filter and adapter sizes clear the sensor with the Antlia SII 2.5nm Ultra Narrowband Filter, and how much light the corners lose.
Check vignettingThe Antlia SII 2.5nm Ultra Narrowband Filter isolates the critical 671.6nm and 673.1nm sulfur-II emission lines with an exceptionally tight 2.5nm full width at half maximum (FWHM). It achieves a peak transmission of >=95% on its durable quartz glass substrate, while suppressing unwanted light to an optical density of OD5 (0.001%). Recommended for optics of f/3.5 or slower, it has a 2mm thickness identical to existing standards, made with utmost care for parfocality.
The defining feature of the Antlia 2.5nm Ultra series is its extremely narrow bandpass. At just 2.5nm, this filter passes the SII lines while blocking most background light from the Moon and artificial sources. Antlia states that this narrower FWHM gives an exceptionally high signal-to-noise ratio for deep sky imaging, revealing fainter nebulosity against a darker sky background.
The narrow bandpass is paired with a specified peak transmission of >=95% at the SII wavelengths. Compared with its 3nm Pro series, Antlia states the quartz-based Ultra series has higher transmittance for the emission lines and estimates it improves signal by 20-30% in your images.
Off-band rejection is as critical as in-band transmission. The Antlia SII 2.5nm Ultra filter provides blocking to an optical density of 5 (OD5), attenuating unwanted wavelengths by a factor of 100,000. Antlia designs this blocking to block interference from other wavelengths and minimize halos around bright stars.
The filter is engineered with a flat-top spectrum profile. This means it maintains its high transmission rate across its 2.5nm bandpass, rather than having a sharp peak that quickly falls off. Antlia states this minimizes the loss in transmission due to the central wavelength (CWL) shift.
Antlia builds the 2.5nm Ultra series on a quartz glass substrate, chosen for its ultra-low coefficient of thermal expansion and outstanding thermal and mechanical properties. Combined with Antlia's coating processes, this gives remarkable durability for imaging in the most challenging environmental conditions.
Compared with the Antlia 3nm Pro series, the 2.5nm Ultra series is coated on quartz glass and has higher transmittance for the emission lines and a narrower FWHM of 2.5nm +0.3/-0.1nm. Antlia estimates these filters improve signal by 20-30% in your images and says the narrower FWHM results in an exceptionally high signal-to-noise ratio for deep sky photography.
By rejecting more of the background sky glow, the 2.5nm filter helps pull out faint structural detail in emission nebulae.
The primary advantage is a higher signal-to-noise ratio. Compared with Antlia's 3nm Pro series, the Ultra has a tighter 2.5nm bandpass and, coated on quartz glass, higher transmittance at the SII lines (>=95%); Antlia estimates a 20-30% signal improvement. The tighter bandpass also rejects more background light, giving a darker sky background so fainter details in nebulae stand out more clearly.
Yes. f/4 is within Antlia's recommendation of f/3.5 or slower for best optical performance. Very narrow filters see their central wavelength (CWL) shift in steep light cones, so at f-ratios faster than f/3.5 you may see a reduction in transmission.
Quartz glass has an ultra-low thermal expansion coefficient with outstanding thermal and mechanical properties. Antlia states it also gives better fracture and scratch resistance and improved coating resilience to cleaning, for remarkable durability in challenging environmental conditions.
The Wizard Nebula is an emission nebula that emits Sulfur-II light along with H-alpha, so it is a suitable target. From a suburban location, the ultra-narrow 2.5nm FWHM blocks most broadband light pollution while passing the 671.6nm and 673.1nm lines, which helps separate the nebula from the bright sky background. SII is fainter than H-alpha, so plan for long total exposure time.
OD5 blocking means the filter reduces out-of-band light to just 0.001% of its original intensity. Antlia designs it to block interference from other wavelengths and minimize halos around bright stars.
Antlia makes the SII 2.5nm filter to a thickness of 2mm, identical to existing standards, with utmost care for parfocality; the H-alpha and OIII 2.5nm Ultra filters share the same 2mm thickness. Antlia does not state parfocality with its other series, so check focus when mixing filters of different series or thickness.
| Filter Type | SII Ultra Narrowband (SHO 2.5nm Ultra Series) |
| Central Wavelength (CWL) | 671.6nm / 673.1nm |
| Peak Transmission | >=95% at 671.6nm / 673.1nm |
| FWHM (Bandwidth) | 2.5nm (+0.3/-0.1nm) |
| Blocking | >=OD5 (0.001%) out-of-band |
| Spectrum Profile | Flat-Top |
| Recommended F-Ratio | f/3.5 or slower |
| Substrate | Quartz Glass |
| Filter Thickness | 2mm (+/-0.05mm on 2" mounted, +/-0.1mm on 36mm unmounted) |
| Surface Quality | Double-sided fine polishing |
| Edge Treatment | Coated to the edge; unmounted filters are edge blackened |
| Mounting (2" Version) | M48x0.75 threads, ultra-thin black anodized cell, laser engraved |
| Available Sizes | 36mm Round Unmounted, 2" Mounted |
| Quality Control | 100% of production scanned individually |
| Not Recommended For | Solar imaging, night visual observation |
Measured spectrum, transmission and blocking (OD) data
Actual measured data for your filter
This product is covered by Antlia's 3-year warranty against delamination.