ThaiExcite
88/41 Kanlapapruek Road, Bangkae, Bangkae, 10160, Bangkok, ประเทศไทย
ติดต่อสอบถาม: 081-239-3299
อีเมล์: info@thaiexcite.com
URL: http://www.thaiexcite.com/-PREORDER-Askar-SQA85-f-4.8-Quintuplet-Petzval-Refractor-Telescope.html
The Askar SQA85 is a premium quality quintuplet air-spaced SD glass Petzval Astrograph that can do something that is often claimed but rarely achieved: produce pinpoint stars to the corners on a full frame sensor.
Quintuplet air-spaced lens design, including 2 pieces of SD glass. The central star point has an RMS radius of less than 1.6 μm, and the star point at the corner is less than 2.5 μm, showing a super-fine star point. It also has excellent full-field illumination and MTF data.
Integrated self-flattened design, supporting a 44mm full-frame image circle, no need for additional flatteners, and no need for additional calculation of the back focus. Between 40mm and 70mm connection distance, users can directly use it for shooting after the OTA is in focus.
The dew shield is a retractable design that can be pulled out when used. It protects the lens from the impact of external and internal light and protects the lens itself.
Enlarged hand screws allow users to open and close the tube ring without additional tools.
There are 6 M4 and M6 threaded holes on both sides of the tube ring, which are convenient for installing the base or dovetail plate and connecting different accessories. You can even set up another set of OTA for shooting
Integrated pair of tube ring sets, with a hollow design in the middle to reduce overall weight.
The handle on the top of the tube ring is slotted with a multifunctional finder base, which can be used to install astronomical accessories.
On both sides of the focuser, there are two finder bases, which not only eliminate the need for disassembling when changing the position of the finder scope but also provide additional mounting positions for other astronomical accessories.
Standard Vixen-style 290mm dovetail plate, which is easy to dismantle and install.
In addition to connecting to the astronomical camera for astrophotography, the SQA85 can also be connected to a mirrorless camera or DSLR camera for shooting.
The rear of the focuser is equipped with a 360° high-precision rotator with a precision scale to allow the user to adjust and save the angle of ro-tation. It is also equipped with an enlarged locking screw for easy locking even under high loads.
Dual-speed rack-and-pinion large 2.8-inch rigid focuser, which can be compatible with most motorized focusers on the market. The focusing travel is 32 mm, and the focuser tube is engraved with high-precision scales. The entire focuser barrel is CNC machined with an anti-reflective internal design and matting paint, providing extra measures to eliminate stray light.
The end of the SQA85 is equipped with a variety of adapters, all of which are toothed and ribbed, making it easy to rotate manually without slipping. The adapters are available in sizes M68, M54, and M48 and can be used to attach various accessories, such as full-frame cameras.
85mm all-metallic handle can be purchased separately for easy use.
20mm all-metallic heightening section can be purchased separately and is available to further minimize the risk of telescope collision damage during equatorial mount operation and to create more space at the bottom of the OTA to accommodate different connecting devices.
The modulation transfer function (MTF) is a quantitative description of the clarity of the image (including resolution and contrast) of an optical lens. The vertical axis is the MTF value, and the horizontal axis is the distance from the center of the frame to the edge.
In the two sets of curves corresponding to low and high frequencies, even at the edge of the full frame the sagittal lines and sagittal lines distance of the SQA85 lens remain very small, and at the low frequency of 10LP/mm, it is higher than 0.9 overall, showing the high resolution and sharpness of the SQA85.
Relative Illumination (RI) represents the combined effect of light loss and attenuation at the corners of the lens, and the RI curve illustrates the change in illuminance (%) across the imaging range on the sensor. Illumination variations can adversely affect the image. The vertical axis means different percentages of example illumination intensities, and the horizontal axis is the distance from the center of the frame to the edge.
The SQA85 guarantees a high illumination of about 85% even at the edge of the full frame, minimizing vignettings.
The imaging quality of the optical system can be evaluated by analyzing the distribution of the spots on the spot diagram.
The SQA85 has a central star point with an RMS radius of less than 1.6 μm, and the star point at the corner is less than 2.5μm, showing very small star points.
The ZYGO interferometer is internationally recognized as a more authoritative instrument for testing optical lens quality, and the SQA85 test results show great star quality.