We are excited to announce the launch of our new forums! You can access it forums.aavso.org. For questions, please see our blog post. The forums at aavso.org/forum have become read-only.
Announcement: New Applications
We are excited to announce the launch of our new applications! We're opening up early access to our new applications for searching, downloading, and submitting photometric observations. You can now access these applications through these links:
We ask for your feedback in order to help us improve these applications. Please send feedback for the applications above to feedback@aavso.org. Note: please avoid duplicating submissions across the two submit applications.
Re: 1), I use IRIS to create calibrated, stellar-registered images with color channels separated, saved as FITS files.
Until recently I was only doing photometry via IRIS too, i.e. extracting instrumental magnitudes then using the ensemble approach with spreadsheet created by Mark Blackford and others (originally Citizen Sky).
Re: 2), more recently I've been going on to use AstroImageJ to plate solve the images before upload to VPHOT.
I also wrote a script (on github; happy to share) to update the FITS header before upload. It also adjusts midpoint time etc, useful even for IRIS-only photometry.
I have not transitioned away from the ensemble/spreadsheet approach yet because for one thing I don't yet have a good quality set of transformation coefficents for my wide-field equipment (Canon 1100D). For another, it works quite well. I'm mostly trying to explore the possibility of reducing the amount of time it takes to get through the processing and improve efficiency.
So, my VPHOT DSLR photometry is still in the experimental stage.
Good to know you edited the FITS header okay. I mentioned a script above but never posted the link; did so in another forum topic recently. Here it is, for your interest:
Re: 1), I use IRIS to create calibrated, stellar-registered images with color channels separated, saved as FITS files.
Until recently I was only doing photometry via IRIS too, i.e. extracting instrumental magnitudes then using the ensemble approach with spreadsheet created by Mark Blackford and others (originally Citizen Sky).
Re: 2), more recently I've been going on to use AstroImageJ to plate solve the images before upload to VPHOT.
I also wrote a script (on github; happy to share) to update the FITS header before upload. It also adjusts midpoint time etc, useful even for IRIS-only photometry.
I have not transitioned away from the ensemble/spreadsheet approach yet because for one thing I don't yet have a good quality set of transformation coefficents for my wide-field equipment (Canon 1100D). For another, it works quite well. I'm mostly trying to explore the possibility of reducing the amount of time it takes to get through the processing and improve efficiency.
So, my VPHOT DSLR photometry is still in the experimental stage.
David
Succeeded last night upload a DSLR image to VPHOT...using Pin Point to Plate solve and editing the fits header. Been attempting this for months...
Mike
Hi Mike
Great!
Good to know you edited the FITS header okay. I mentioned a script above but never posted the link; did so in another forum topic recently. Here it is, for your interest:
https://github.com/dbenn/photometry_tools/blob/master/modify-fits-header.py
David