nakbrooks

Happy to exchange thoughts if useful. I may be a bit ahead of you on Python in photometry but you’re streets ahead of me on most other aspects of astronomy as I’ve come to it late in life - and it appears we live only 30 mins or so away from each other. Feel free to private message me.

George, was your immediate objective to extract star locations from fits images? If so then you may want to look at astrometry.net. This is a free platesolving service that, as a byproduct, will give the xy coordinates of all stars in the image. There is an api which can be accessed using Python but you can also do it interactively here: http://nova.astrometry.net/ Note that the distortion coefficients generated (which seek to adjust for optical distortions, particularly away from the image centre) use the professional system, not the one used by most amateur tools such as Maxim and PinPoint, so if you use astrometry.net platesolve solutions for subsequent processing you’ll either need to use Astropy or platesolve again using PinPoint. If you do use Astropy then there are good tools in it to easily convert between image xy coords and RA/Dec in various epochs and coordinate frames.

If you do get into using Python then make sure you use the Anaconda Python framework - it is free and includes all the scientific/astronomy Python packages you’re likely to need so makes things easier. For program writing I strongly recommend Microsoft Visual Studio Code (NOT Visual Studio itself which is much more complex). VS Code is also free and has a Python extension which does syntax checking etc.

Yes it is far and away the most popular language for professional astronomers and is well supported by the Astropy and wider Python community.

Yes that’s why I use Astropy. It handles all that stuff.

Also, if you’ve not already located them: The formal FITS file standard: https://fits.gsfc.nasa.gov/standard40/fits_standard40aa-le.pdf The SBIG FITS extensions (an industry standard followed by Maxim and most camera drivers): http://www.company7.com/library/sbig/pdffiles/SBFITSEXT_1r0.pdf

Astropy does require a good working knowledge of Python programming (under either Windows, IOS or Linux). It isn’t a shrink-wrapped package - it is a library of astronomy-related Python modules. Core Astropy is documented here: http://docs.astropy.org/en/stable/ Astropy-affiliated packages are numerous. The most relevant include: ccdproc (FITS image processing) https://ccdproc.readthedocs.io/en/latest/ photutils (source detection and photometry) https://photutils.readthedocs.io/en/stable/ Astroquery (automated querying of Vizier, Simbad and dozens of other data sources): https://astroquery.readthedocs.io/en/latest/ astroplan (scheduling observations based on observability and other constraints) https://astroplan.readthedocs.io/en/latest/ Python isn’t a difficult language to learn (easier than C# in my view). I’m 67 years old and my previous programming experience has been Excel macros and VBA but I’ve picked it up well enough in just 9 months to write a full data reduction pipeline. Best of all it’s totally free. I’m keen to work with other amateur Python programmers as I’m looking to open source what I’m doing. Nigel

Catching up on this thread very late but if your friend is familiar with Python there are very extensive tools in the Astropy package and affiliated packages that would do pretty much everything you’d want. I’m sliwly building a web application, mostly using Astropy packages. This is primarily to support Photometry work.

Hi Daniel. You’ll have to ask ASA. I decided not to do the upgrade so I don’t have a price. Nigel

Does anyone know if Sequence has any undocumented command line parameters (eg to use a specific configuration)?

Thanks Mark. I’ll check that link out.

Sounds the same issue as this one last year. http://forum.astrosysteme.com/index.php?/topic/1045-strange-new-problem-with-sequence/?fromsearch=1

Did you install any other software (not ASA) around the time that Sequence stopped working? In particular any Microsoft .NET software? Was there a Windows 10 update about that time? Personally I use my observatory PC only for astronomy and I disable Windows updates on it.

Anyone else going to the IAU-100 event in Brussels on 13 April? https://www.iau-100.org/programme-amateur-day

Indeed. I’ll believe it when I see it.

V interesting if it actually materialises. If it is platform independent it is maybe Java based. Unclear whether this would control all ASA mounts or just the professional ones and whether it replaces Autoslew and Sequence.

Hi Christer. Did you get the dome working?

Development continues at E-Eye. https://www.facebook.com/1426801807576286/posts/2180125488910577/ Very happy to have my scope hosted there.

Title says it all. Does Astrooptik Server Telescope act as an ASCOM hub so I can connect using it from multiple apps or do I still need POTH?

Many thanks Mark. I think I’m clear now how to use MLPT on a sequence run - still not sure how or why the MLPT button on the main Sequence screen is used but seems to be superfluous to my needs!

I’m starting to use MLPT for the first time but am confused! Sequence (ver 2.2.1) has MLPT Exposure Distance in Minutes and MLPT Iterations boxes under Settings/Sequence. The Exposure Details panel under Sequence Run let’s me specify whether I want to use MLPT for a set of exposures. Question 1: If i specify that I want to use MLPT for a sequence does it calculate the duration from the sequence details (ignoring the Exposure Distance specified in Sequence Settings) or do I have to set that distance manually before running each sequence? There is a separate MLPT section under Sequence which asks for the Total Exposure Time, Number of Exposures and Number of Iterations; run an MLPT and upload the results to Autoslew. Question 2: If I specify that I want to use MLPT for a sequence (in the Exposure Details pane) will this happen automatically immediately prior to that sequence line being executed so there is no need for me to use the MLPT button on the main Sequence screen? Question 3: If I do have to use the MLPT procedure on the main Sequence screen how does it know what path to follow? Does it simply start from the current pointing location? Question 4: What are the appropriate values for Number of Exposures and Number of Iterations? I’ve read the Sequence and MLPT documentation but it doesn’t explain some of the fundamental points and also isn’t up to date with the latest software, so I’m hoping some kind soul can help me! Many thanks Nigel

I wanted to check the effect of different download speeds and RBI flash on bias and dark frames for my PL16803 camera. See the attached data and graphs. I would have expected RBI flash to increase counts somewhat but as the flash takes place before the exposure I wold have expected the effect to be the same for all exposure durations. However that does not seem to be the case. I'm probably not understanding the RBI flash process and its effect on the subsequent exposure. Can anyone explain this? (Forum wouldn't allow me to upload as a spreadsheet so had to convert to pdf). Nigel Data.pdf Charts.pdf

ASA may gave developed proprietary extensions to ACL, but if they haven’t and ASA mounts are compliant with the current ACL standard then that raises a lot of interesting ideas. Unfortunately I don’t have either the time or expertise to explore further.

I know little about usb/com port communications protocols but presumably there is a layered set of protocols: 1. FTDI (emulating com port) 2. Com port serial protocol (basic handshaking) 3. At least one layer of data protocols We would need to fully understand the protocol stack so the actual data can be extracted. Does Wireshark know about the stack being used so it can isolate only the application-level data?

I think Wireshark is primarily a LAN packet analyser. For FTDI-based serial over USB comms you would need something like https://www.eltima.com/products/serial-port-monitor/