Differences
This shows you the differences between two versions of the page.
Both sides previous revision Previous revision Next revision | Previous revision | ||
en:ost:ccds:grunddaten [2022/10/18 08:42] – rhainich | en:ost:ccds:grunddaten [2024/03/27 13:09] (current) – rhainich | ||
---|---|---|---|
Line 6: | Line 6: | ||
Our newcomer, the QHY 600M is a CMOS camera that was developed especially for astrophotography. It is our new deep-sky camera and offers among other things a full format sensor, a very high quantum efficiency, a very low readout noise and a very low dark current. For this camera we also have an off-axis-guide and a filter wheel with 9 positions. | Our newcomer, the QHY 600M is a CMOS camera that was developed especially for astrophotography. It is our new deep-sky camera and offers among other things a full format sensor, a very high quantum efficiency, a very low readout noise and a very low dark current. For this camera we also have an off-axis-guide and a filter wheel with 9 positions. | ||
+ | |||
+ | As main camera for our two [[en: | ||
==== CCD Cameras ==== | ==== CCD Cameras ==== | ||
- | Furthermore, | + | Furthermore, |
- | The ST-7 and ST-8 are deep-sky cameras, but due to their relatively small field of view they are rarely used. The STF-8300M is used as main camera for our two [[de: | + | The ST-7, ST-8, and STF-8300M |
+ | \\ | ||
The ST-i, the QHY 485C, and the Skyris 445C are " | The ST-i, the QHY 485C, and the Skyris 445C are " | ||
- | \\ | + | All cameras can be controlled via [[de: |
- | \\ | + | |
- | All cameras can be controlled via [[de: | + | |
==== Basic data ==== | ==== Basic data ==== | ||
=== Main cameras === | === Main cameras === | ||
- | |< 100% 19%>| | + | [{{ : |
- | | | **QHY 600M** | + | |< 100% 27%>| |
- | | **Model number** | + | | | **QHY 600M (2x)** |
+ | | **Model number** | ||
| **pixel size** | | **pixel size** | ||
| **Number of pixels** | | **Number of pixels** | ||
Line 33: | Line 36: | ||
=== Planetary/ | === Planetary/ | ||
+ | [{{ : | ||
|< 100% 27%>| | |< 100% 27%>| | ||
- | | | **Skyris 445** | + | | | **Skyris 445** |
- | | **Model number** | + | | **Model number** |
- | | **pixel size** | + | | **pixel size** |
- | | **Number of pixels** | + | | **Number of pixels** |
- | | **Total size of the chip** | + | | **Total size of the chip** |
- | | **Field of view with the CDK20** | + | | **Field of view with the CDK20** |
- | | **Sampling** | + | | **Sampling** |
=== Cameras that are no longer in daily use === | === Cameras that are no longer in daily use === | ||
[{{ : | [{{ : | ||
- | |< 100% 19%>| | + | |< 100% 27%>| |
| | | | | | ||
| **Model number** | | **Model number** | ||
Line 73: | Line 77: | ||
| **Filter** | | **Filter** | ||
| **Comment** | narrow band | narrow band | narrow band | broad band | broad band | broad band | broad band | broad band | | | **Comment** | narrow band | narrow band | narrow band | broad band | broad band | broad band | broad band | broad band | | ||
+ | The transmission curves of the UBVRI filters can be found at the web page of //Baader Planetarium//: | ||
=== ST-7 & ST-8 === | === ST-7 & ST-8 === |