Astroblog

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Astrophotographic results with the ASI 1600 mono cooled:

October 23rd, 2017 by Wolfi


NGC 891 with ASI1600MMC & TS 16" f/8 RC

Image author: Michael Pagitz (AMOS Observatory)
Telescope: TS 16" f/8 Ritchey Chretien Astrograph
Camera: ASI1600MM-Cool - gain 200
Exposure: 20 x 120 sek / binning 2x





More Infos about the ASI 1600 cooled cameras

Customer comment:
Yesterday, we have installed everything and got it running and, quite frankly, I have NEVER made a quick and dirty photograph which was that good. We have snapshot "cross-country" just for fun and taken NGC 891 with 10x2 minutes. The image is unguided, no darks, no bias, just stacked and the contrast adjusted very slightly, nothing else.

The ASI1600MMC works like a DSLR, attach, pull the trigger, ready.




ASI 1600 cooled - a declaration of love
Unfortunately I have too little time for astrophotography and also not the desire anymore to work through the night during the week.

That is why, for me, astrophotography unfortunately was in "pause mode" - until I have worked with the ZWO AI 1600 cooled for the first time. For me, it is plain fun with this camera.

Just yesterday, I have taken a picture of NGC 7331 with my 12" TS RC (focal ratio f/5.4). Instead of using approximately 300 seconds per integration and to stay until 2 am as in the past, I have exposed only 40 seconds per integration with the ASI 1600 (Gain 300). I finished at 10 pm and made a beautiful picture - everything recorded - even the color information. Now I am looking forward to editing ... thus astrophotography is just fun ...

Wolfi Ransburg - Munich, 12.10.2017

Deep-sky photography with cooled ASI cameras with high resolution - without guiding - "lucky imaging" principle

The cooled cameras from ZWO offer new and extremely exciting opportunities in the field of deep-sky photography. Finally highly resolving, smooth deep-sky images without great effort!

With conventional CCDs, there is still a race taking place to the longest single exposure times (some of us know that from imaging with film). But long exposure times for each single frame place various demands and come with a few problems:
Perfect guiding / autoguiding
Calm air for fine details
Furthermore, airplane and satellite tracks on long exposure single frames are very annoying.


With the new CMOS sensors which are have been installed in the cooled ASI cameras from ZWO, you can tread indeed entirely new paths. It does not count anymore how long you expose, but how often!

Two of the biggest advantages of these new cameras are the extremely low readout noise, despite the high frame rates, and the enormous sensitivity of the sensors. In combination, these advantages are the key to impressive high-resolution images. The signal-to-noise ratio is excellent. The more frames are recorded, the more noiseless and deeper the summary image will become. Basically it is the same as with planetary imaging. Hundreds or even thousands frames are stacked.

The limit is set mainly by the capacity of the hard disk. The following should be kept in mind: while a conventional 16 megapixel CCD camera need up to 15 seconds for transfering a single frame to the PC, a CMOS camera like the ASI1600 can transfer up to 23 frames per second (of course depending on the exposure time). At an exposure time of 5 seconds, the CCD would achieve just under 3 images per minute, an ASI1600 approximately 12 images! So we can take 300% more exposures in the same time.

There are several free programs for imaging and editing (stacking) which can help us here, for example Firecapture. Many know this software already from planetary photography, but Firecapture can also be used for deep-sky images. It can control the cooling of the camera, create a dark and also a flat and subtract automatically, save in FITS format, and even do autoguiding. But we only need the latter for this type of deep-sky photography if the mount is not polar aligned properly or other extreme tracking errors are foreseeable.

Apart from that, we now just have to: set the exposure time to a value between 1 and 15 seconds. Set gain not too high but also not overcautiously low (approximately between 100 and 350), and take at least 200 single images.

A concrete example (Fig. 1):

We use a ZWO ASI1600MMC, a 300/1500 Newtonian telescope plus coma corrector on an EQ6. A fast(er) aperture ratio promotes short exposure times, of course.

Firecapture is started and the image is focused on a bright star with still short exposure times (<1s). Normally, a usable star can be found in the preset image field.

A check mark is set at 16Bit (top left) and the file type FITS is chosen. Exposure time is set to 5 seconds, gain set to 321 (without particular reason). Thereby the image noise still stays within acceptable limits. Cooling can be set at pleasure or matching the power supply. Gamma stays at 50. USB traffic is not relevant in this case.

Now set the mark at Dark Frame. Firecapture then takes the selescted number od dark frames (don´t forget to cover the telescope aperture) and subtracts their mean value from the single images. The few hot pixels disappear. Amplifier glow is no longer an issue.

Set as exposure number limit are, for example 1000 frames. However, it should be kept in mind that, in the case of the ASI1600, a single image has a size of 16 MB. A few hundred single images quickly result in a few gigabytes of data. It should always be ensured that a storage location is selected which is able to handle this amount of data.



Abb. 1


When the sleep-stealing part is over and the hard disk filled with raw images, it is recommended (for example with the program Fitswork) to classify them and to sort out possible "duds" with satellites, airplanes, wobbles, etc. One could also stack the frames with Fitswork, but with Autostakkert!, stars and details become finer. However, stacking with Fitswork makes sense if manual intervention is necessary, for example if much displacement between the single frames.

Attention - if you want to load the single images in Autostakkert!, the file type "Image files" has to be chosen. Then a bright star is selected as anchor point and clicked on "Surface" under "Image stabilisation" (just under the "open" button). "Planet (COG)" can also work with bright objects which have an obvious centre of brightness, but mostly, "Surface" is more succesfull. At this point, you click the button "Analyse". (Fig. 2)



Fig. 2


When this has been completed, a bright star is selected as "alignment point" again. You can set several ones, but it is not necessary (except with image rotation or similar problems).

Time to click on the "Stack" button. Now the single images are stacked.

The final result is saved by Autostakkert! in the chosen image file format (in any case, choose a 16-bit format like TIF or FITS).

The difference between a single frame and the summarized image becomes astonishing. (Fig. 3)



Fig. 3 histogram enhanced



At the beginning of the processing, the summary image will seem quite unremarkable and dark, but with the help of a histogramm adjustment, the object of desire emerges quickly. (Fig.4)



Fig. 4


Important! For further processing, a program should be used which can handle 16 bit and the corresponding formats! Once again, Fitswork is well suited for that. However, many amateur astronomers will use Photoshop for the final touches.

We suspect that one could intensely debate how long the maximal single exposure time should be. However this rule applies: the shorter, the crispier. Short exposures are less disturbed by seeing. Guiding errors carry no weight. Therefore, the attainable accuracy is accuracy is significantly better than with exposures of several minutes.

On the other hand, the (areal) brightness of the object must be taken into account, after all we need a bit of signal on the sensor.

Of course, you can also expose several minutes with the cooled cameras from ZWO. There is nothing to stop you from taking short focal length photographs, for example of nebula regions. One can definitely use the ASIs like a ctandard CCD camera. But this slightly different approach with short exposure times offers many amateurs astronomers the possibility for imaging nebulae and galaxies with additional details. Given the increasing light pollution in many places, this might possibly the long-awaited life belt for this wonderful hobby.

This photo technique is only just beginning and still offers many opportunities. We will continue, get involved!

Your Teleskop-Service Team





The experience of a customer might be helpful:

1. With the Starlight software, the Starlight filter wheel runs trouble-free under Win 7 (64 bit).

2. A USB stick from Intenso (64 GB) can be plugged at the same time and is recognised immediately in the laptop!




New Cameras from ZWO

September 7th, 2019 by Wolfi

Latest News from ZWO

ASI6200 - the camera is expected to be ready for delivery in December. The camera will be available in two versions (B/W and color). The most important specifications:
62 megapixel sensor.
3.76µm pixels.
16 bit ADC

... the last advantages of CCD cameras are no longer applicable.

GT Cameras - these cameras will be available in mid-November. ZWO now also offers cameras with integrated filter wheel. They´ll be black-and-white (mono) cameras. For example, the popular Panasonic 1600 sensor will be built into this camera.

We are happy to keep you informed about the new developments of ZWO




New Cameras from ZWO

November 2nd, 2019 by Wolfi

ZWO extends its lead with new Astro cameras.






While other manufacturers are still considering switching from CCD to CMOS, ZWO is already two steps ahead and underpins its dominant position in the market with new exciting models. Teleskop-Service, as a ZWO dealer, is of course one of the front runners.

The new cameras will be delivered in January, we gladly accept advance orders, we expect a very high demand and have therefore ordered in good quantity.

ZWO has four new cameras that equalize the last advantage of CCD cameras. The new cameras convince with 14Bit or 16Bit data depth. This means that stars no longer burn out so quickly and the images achieve a stronger dynamic. Due to the modern "Back-Illumination" technology the cameras are much more sensitive than conventional CCD cameras.

ASI 6200 Pro - Full Frame Cameras (Mono/Color)

With these two cameras ZWO offers two outstanding solutions for astrophotography with large sensors.
Sony IMX 455 Full Format Sensor
16 bit ADC - extreme dynamic range
High sensitivity
Powerful Peltier cooling
high resolution by 3.78µm pixel


Link to ASI6200 full size cameras


ASI 2600 Pro - APS-C Format Color Camera
This camera has a similar sensor format to a DSLR with 28.6mm sensor diameter. But in contrast to a DSLR, this camera has much better values.
Sony IMX 471 Back Illuminated Sensor
16 bit ADC - extreme dynamic range
High sensitivity
Powerful Peltier cooling
high resolution through 3.76µm pixel



Link zur Color APS-C Kamera


ASI 533 Pro - Color Camera with 16mm Sensor Diameter

This camera has a sensational price-performance ratio and is the entry into the semi-professional camera class. The square sensor (11.3 x 11.3mm) makes optimal use of the telescope´s correction. Many telescopes do not even require a corrector.
Sony IMX 533 Back Illuminated Sensor
14 bit ADC - extreme dynamic range
High sensitivity
Powerful Peltier cooling
high resolution through 3.76µm pixel


Link zur Color Astro Kamera







ASI 183GT and ASI 1600GT - MONO cameras with built-in 5-pos. filter wheel

With these two cameras ZWO turns to the astrophotographers, who like to work with SW cameras and want to take false color pictures or L-RGB pictures. ZWO has installed probably the most exciting MONO sensors on the market, the sensor of the ASI 1600 and the sensor of the ASI 183 in this new housing. Thus the camera is even more compact and lighter than the combination of camera and filter wheel.


Link zur ASI183GT MONO Astro Kamera

Link zur ASI1600GT MONO Astro Kamera

If you have any questions please do not hesitate to contact us

Your team of Teleskop-Service




Atik takes off with CMOS cameras

February 1st, 2020 by Wolfi

New exciting astro cameras from ATIK with CMOS technology.






Atik has recognized the signs of the times and offers the astrophotographer a good selection of modern CMOS peltier cooled cameras with high-quality sensors. Despite the new technology, the cameras can be operated with the proven ATIK software. The well-known reliability and ease of use that characterise ATIK cameras also applies to the new CMOS series. ATIK always offers the new cameras in a MONO and a COLOR version.

The sales launch of the new cameras is planned for mid-May.
ATKHORI2M und ATKHORI2C

The proven Horizon series with improved features. Entry into CMOS technology at a top Price, with the 21.9mm Panasonic Sensor.
ATK0192 und ATK0193

Sony Sensor IMX249 with 13,4mm Diameter and 5,86µm Pixel
ATK0190 und ATK0191

Sony Sensor IMX428 with 17,6mm Diameter and 4,5µm Pixel
ATK0194 und ATK0195

Sony Sensor IMX304 with 17,6mm Diameter and 3,45µm Pixel
ATikCosmos Full Sized Sensor

Big 24x36mm Sony Sensor IMX455 with 61,2 Megapixel

Link to the cooled ATIK Astro-Cameras

If you have any questions please do not hesitate to contact us

Your team of Teleskop-Service