How does the Baader 2" ClickLock clamp work?
It has no clamping screws: a 20° turn of the rotary lever holds the accessory on three sides like a quick-action chuck, aligns it parallel to the optical axis even with diameter deviations, and the massive tension ring holds it without scratches.
What is the main advantage of the dielectric coating on the Baader 2" Mirror Diagonal?
The hard-coated surface allows safe cleaning and stays scratch-resistant even in extreme conditions, and the coating reflects only the visual part of the spectrum (400-700nm), so no UV or IR radiation reaches the eye.
Can I connect the diagonal directly to a Schmidt-Cassegrain?
Yes. Unscrewing the 2" nosepiece exposes a female 2" SC thread for direct connection, which reduces the overall length. The ClickLock usually has to be removed first so it does not hit the focusing knob, and the separately available 2" Locking Ring (#2458270) fixes the diagonal in any rotational position.
How do I achieve the shortest possible light path with this diagonal for my binoviewer?
Remove the ClickLock (six M2.5 screws), which reduces the required backfocus from 112mm to about 71.5mm, and fit the optional 2"/T-2 adapter (#1508035) for a low-profile male T-2 thread. Depending on the available backfocus, a binoviewer can then be attached directly, without an additional T-2 diagonal or a glasspath corrector.
What is the difference between this diagonal and the M68 version #2956100Z?
The #2956100Z version is the same diagonal with a male M68 (Zeiss) thread instead of the 2" Safety-Kerf nosepiece, giving a 51mm clear aperture and a 109mm optical length against 46.6mm and 112mm for this model. Filters cannot be mounted in front of the M68 version.
What is included?
The 2" ClickLock mirror diagonal. Baader ships its 2" diagonals without a 1.25" reducer; the ClickLock 2" to 1.25" reducer (#2956214) is available separately.
When should I choose this Baader dielectric mirror diagonal over a Baader prism diagonal?
There is no general recommendation, but light passing through a prism is refracted, which behind a fast telescope can lead to colour aberrations; for fast telescopes designed for use without a prism a mirror is the better choice, with the limit somewhere around f/6 to f/7. Refraction in a prism also produces less stray light than reflection on a mirror, which is why many planetary observers prefer a prism, and a prism must adapt to the ambient temperature like the rest of the optics. For binoviewers, the compact Baader T-2 prism diagonals are the better choice because of their much shorter optical length.
How do I integrate a 2" filter with the Baader ClickLock Diagonal?
The included 2" nosepiece has standard M48 filter threads on both ends. You can either screw a 2" filter onto the end that inserts into the telescope focuser, or into the second M48 female thread inside the nosepiece, where it stays permanently inside the body without adding to the length.
The ClickLock lever is in an awkward position on my telescope. Can I adjust it?
Yes. The position of the locking lever can be changed. It can be set for left- or right-hand use by six slotted screws or six Allen screws, depending on the model.
Can I attach T-2 accessories to the eyepiece side of the Baader 2" ClickLock Diagonal?
Yes. To do this, you must first remove the 2" ClickLock clamp by undoing the six screws holding it in place. Then, you can use the optional Baader 2"/T-2 Adapter (#1508035) which threads into the diagonal's body and provides a male T-2 thread for your accessories.
What is the S58 dovetail on the Baader Diagonal's housing for?
The S58 ring dovetail is designed for direct integration with Baader Diamond Steeltrack focusers. It allows you to replace the focuser's eyepiece clamp with the entire diagonal body, which extends the available backfocus for long accessories such as binoviewers; as the Diamond Steeltrack can be rotated, the eyepiece can always be brought into a comfortable viewing position.
What does Baader say about solar observation with this diagonal?
The dielectric mirror reflects only the visual part of the spectrum (400-700nm), so that no UV or IR radiation reaches the eye, and it provides high security for solar observation in white light and with H-alpha solar filters; however, it does not replace the diagonals of H-alpha telescopes with built-in blocking filters.