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Hmmm…that is very odd Max. Could it be the recent dip is a random fluctuation rather than an eclipse?
Definitely worth pursuing your lead about outburst amplitude relative to previous and successive brighter outbursts, Max. Correlations were found by Frank Bateson regarding normal outbursts between superoutbursts in the UGSU system, VW Hyi.
Latest reports on VSNet suggest that RY Sgr is fading rapidly. Latest obs by Jose Ripero on Sep 26.895 place it at mag 9.7
I see the dilemma, Max (also shows rage pitfalls CV observers can get into with less than ideal data). If you can confidently and consistently compensate that would be the way to go (sorry!). In any case, it would be important to identify those eclipses where there is some kind of uncertainty in assignment of type.
Interesting to see JWST papers already appearing: https://arxiv.org/abs/2208.01630
This one on flattened disc, reddened galaxies.
No doubt a trickle will soon become a torrent
They may even be a fraction deeper that’s the last pair, Max. Asymmetric, as before, as you noted, perhaps steeper entry…
