Differences

This shows you the differences between two versions of the page.

--- en:ost:telescope:ts-apo [2024/02/19 22:56] – [Reducer + QHY600M with Filter Wheel and Off-Axis Guider] rhainich
+++ en:ost:telescope:ts-apo [2024/07/08 10:32] (current) – rhainich
@@ Line 1: / Line 1: @@
-FIXME **This page is not fully translated, yet. Please help completing the translation.**\\ //(remove this paragraph once the translation is finished)//
 ====== 130mm Apochromat from Telescope-Service ======
@@ Line 75: / Line 73: @@
 It is important to note that before mounting the above adapter combination, the long M48 adapter, usually present on the reducer, must be unscrewed to expose the M76 thread.
+**Note:** If the off-axis guider is not used, a 20mm M68 extension must be used instead of the 10mm extension.
 </WRAP>
@@ Line 145: / Line 145: @@
 === Flattener + QHY600M with Filter Wheel and Off-Axis Guider ===
-[{{ ost:apo:apo_reducer_adapter_names.jpg?700 | **Placeholder image (must be replaced)** }}]
+[{{ ost:apo:apo_flattener_adapter_names.jpg?700 | APO with flattener, QHY600 with Filter Wheel and Off-Axis Guider, and all necessary adapters }}]
 The [[https://www.teleskop-express.de/en/astrophotography-and-photography-15/imaging-correctors-for-telescopes-138/ts-optics-refractor-1-0x-flattener-gen-2-for-apo-large-format-m92-connection-4047 | flattener]] is also from TS-Optics, keeps the focal length unchanged and has the following threads:
@@ Line 164: / Line 164: @@
 As mentioned earlier, the working distance from the M78 thread is 77.5mm, with the camera including filter wheel, filter, and off-axis guide having a back focus of 56mm. The remaining 21.5mm is bridged by the above adapter combination.
+**Note:** If the off-axis guide is not used, an additional 10mm M68 extension must be inserted between the fine adjustment rings.
 </WRAP>
@@ Line 199: / Line 201: @@
 </WRAP>
-Together, this results in an optical path length of approximately 58.8 mm depending on the tilter position and installed fine-tuning rings. Combined with the 17.5 mm back focus of the QHY600M and the installed filter, this leads to 77.5 mm from the M78 thread.
+Together, this results in an optical path length of approximately 58.8 mm, depending on the tilter position and fine-tuning rings installed. Combined with the 17.5 mm back focus of the QHY600M and the installed filter, this results in 77.5 mm from the M78 thread.
 \\
@@ Line 208: / Line 210: @@
 <WRAP group>
 <WRAP half column>
-A tension-free mounted solar filter for visual observations from [[https://www.baader-planetarium.com/en/solar/whitelight/astf-astrosolar-telescope-filter-od-5.0-(80mm---280mm).html | Baader Planetarium]] is used. This filter is simply mounted in front of the objective. Any eyepiece and camera can then be used. However, the Herschel prism described below usually allows for better imaging quality.
+For visual observations, a [[https://www.baader-planetarium.com/en/solar/whitelight/astf-astrosolar-telescope-filter-od-5.0-(80mm---280mm).html | Baader Planetarium tension-free solar filter]] can be used. This filter is simply mounted in front of the objective. Any eyepiece and camera can be used. However, the Herschel prism described below usually provides better image quality.
 </WRAP>
 <WRAP half column>
@@ Line 218: / Line 220: @@
 === Herschel Prism ===
-We also have a [[https://www.baader-planetarium.com/en/baader-cool-ceramic-safety-herschel-prism-markii.html | Herschel Prism Mark II from Baader Planetarium]], which allows us to observe the sun in white light with excellent quality. The Herschel prism can be equipped with different filters, allowing it to be configured for visual observations as well as camera observations with very short exposure times. Details about the Herschel prism and its operation can be found in the associated [[en:ost:telescope:herschel_prism | article]].
+We also have a [[https://www.baader-planetarium.com/en/baader-cool-ceramic-safety-herschel-prism-markii.html | Herschel Prism Mark II from Baader Planetarium]], which allows us to observe the Sun in white light with excellent quality. The Herschel prism can be equipped with different filters, so that it can be configured for visual observations as well as for camera observations with very short exposure times. Details about the Herschel prism and its operation can be found in the associated [[en:ost:telescope:herschel_prism | article]].
-The Herschel prism can be used in many different configurations, for example, with and without a Barlow lens. However, the standard procedure is to insert it directly into the 2" eyepiece clamp of the APO.
+The Herschel prism can be used in many different configurations, for example with or without a Barlow lens. However, the standard procedure is to insert it directly into the 2" eyepiece clamp of the APO.
 <WRAP group>
@@ Line 231: / Line 233: @@
 </WRAP>
-Different models can also be used on the camera side. The prism has a 2" eyepiece clamp for holding corresponding accessories.
+Different camera models can also be used here. The prism has a 2" eyepiece clamp for mounting accessories.