MaxIm DL 6.20.0 can be downloaded from our software library for free. This PC software can manage the following extensions: ".raw", ".ccd" or ".cr2". The latest version of MaxIm DL can be installed on PCs running Windows XP/7/8/10/11, 32-bit.
The actual developer of the program is Diffraction Limited. The program lies within Multimedia Tools, more precisely Editors & Converters. The most frequent installation filename for the program is: MaxIm_DL.exe. The size of the latest downloadable installation package is 46.2 MB. The following versions: 6.1, 6.0 and 5.9 are the most frequently downloaded ones by the program users. This download was checked by our antivirus and was rated as virus free.
New Equipment Control Features1. Built-in Rotator control2. Built-in Dome control with slaving, shutter operation3. Support for second focuser and filter wheel for autoguider4. Built-in mini planetarium with All Sky view and Zoom view5. See all equipment status at a glance6. Autocenter now accepts PinPoint calibration7. Automatic pier flip tracking8. Autofocus V-curve display9. Improved camera setup10. Larger camera control window with most camera settings in one view11. Camera control presets let you quickly change between your favorite settings for find, focus, center, and acquisition sequences12. Instantly swap cameras13. Improved focus information displays with trend graphs14. User-configurable camera, guider, and focus status displays15. Virtual keyboard for number entry in the darkThe license of this software is Free Trial Software, the price is $199.00, you can free download and get a free trial.
The STX-16803 uses a 37 x 37 mm full frame antiblooming chip with microlenses. The quantum efficiency peaks at 550 nm with 60% and drops off to 46% at 656 nm (H-alpha). See also the angle depending quantum efficiency curve here. Even very fast systems at f/2.8 stay within the 10 degree light angle and so do not loose efficiency. The primary resolution of 4096 x 4096 pixel can be used in 1x1, 2x2, 3x3 and 4x4 binning mode to shorten readout time for previewing. However I always recommend the 1x1 binning mode for all frames. Readout is done without interrupting the guiding within 6 sec, the actual download takes 2 seconds in full resolution. The original power supply cable with extension from the AC adapter is quite flexible even in cold environment, I use a second custom cable set for direct 12 V field supply.
The power consumption of the camera is acceptable low without active cooling: approx. 1.8 A, peaking at 2.0 A during the STX filter wheel change. The dependance of the power consumption (current drain at 12V supply voltage) from cooling output and the cooling performance is shown in the graph at right. At 4 amps the cooling capacity is approx. 43 degree below ambient, at maximum cooling the current uptake is 8 amps. The cooling fan operates at fixed medium speed. At high cooling rates >80% the fan speeds up and gets quite noisy. A continuous regulation or setting of the cooling fan speed is missing so far. In comparison to the STL design the distance from the imaging chip to the chamber cover glass has been increased, this is a big advantage for avoiding icing on the cover glass. I never experienced ice on the chamber glass even at 100% humidity. Due to the effective camera design the cooling reaches 52 degree C below ambient at 100% output, at 80% output 50 degree C below ambient is possible. Lowest cooling setpoint is -35 degree C.
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When the file required to uninstall MaxIm DL 5.12 is corrupted or missing, it will not be able to uninstall the program. In such circumstance, reinstalling MaxIm DL 5.12 may do the trick. Run the installer either in the original disk or the download file to reinstall the program again. Sometimes, the installer may allow you to repair or uninstall the program as well.
The installer includes USB Drivers, User Guides and ASCOM support. You will be able to optionally install native plugins for AstroArt during installation. If you received a complimentary code for SGPro with your camera you can download it here.
QSI cameras are supported in PRiSM versions 7.2.9 or later. PRiSM is an integrated software package that incudes telescope control (telescope,filter wheel, focuser), CCD camera control, preprocessing, processing and analyzing astronomical images, and an efficient Skymap tool.Learn more and download a 60-day free trial directly from the PRiSM website
QSEye and QSEye Lite (free) provide support for image acquisition from QSI cameras. Both the free and paid versions can be downloaded from the Mac App Store. Additional details can be found on the QSEye website
QSI cameras are supported on Linux by GoQAT, a free Open Source Linux application designed to operate a QSI camera, autoguider and telescope. Read more about GoQAT and download the latest version directly from the GoQAT website
Used event hierarchy allowed us to maintain data consistency and completeness. Nevertheless, our method has some bottlenecks. Firstly, it is not common practice to combine events of different levels in one dataset. At the same time, each event level should be described in the dataset. This information requires a particular Darwin Core term, but it is currently absent. We used the general term dwc: dynamicProperties as a temporary solution in this work. Secondly, the event hierarchy includes 338 events (the soil sample level), which are not assigned to any occurrences. These events are empty not because no species were registered. We used this event level for the relationship between survey and sample layer event types. However, empty events are not shown on the GBIF dataset page. Moreover, complete data (with empty events) are available for download via the IPT installation page, not the GBIF interface. This fact restricts the reuse of our data.
Possibly, another data standardisation design could be more understandable. It would be simpler to use the soil sample as the event and bind samples from one sample plot via dwc: locationID and different surveys via dwc: parentEventID. This scheme avoids empty events not related to occurrences. However, its implementation is not possible due to technical IPT limitations. We cannot assign different depths for occurrences into one event because dwc: verbatimDepth, dwc: minimumDepthInMeters and dwc: maximumDepthInMeters are related to the Event Core. 2b1af7f3a8