Our answser: we'll try pattern matching (like Gravity Spy) & image segmentation for spectra (like GZ Clump Scout).
Belatedly, here are a few key slides from the Dissemination, Engagement and Citizen Science talk. Besides showing our social media comms channels, we explained why we need & use crowdsourced data mining (citizen science)
Some beautiful logo options! Not yet proper to share in public, but excellent work by a graphic artist who will work up some final options for voting on. Finally our first formal ELSA General Assembly!
I'll put some summaries of my talk in here later, but first our next talk is Viola Allevato on some options for our ELSA logo (our current snowflake icon is just provisional)
First talk after lunch is me @stephenserjeant.bsky.social to talk about our Dissemination, Engagement and Citizen Science work package, so I won't live-skeet!
Our data(+code?) needs to be Findable, Accessible, Interoperable and Reusable (FAIR). GitHub is great for developing, testing & maintaining code, but connect to Zenodo (one button!) to publish FAIR code. Our first draft DMP is due in June 2024...
Giulia Caldoni, Data Steward in the Research Services Division in Bologna, now briefing us on the open science requirements and our Data Management Plan deliverable. Publication embargos are no longer allowed in Horizon. Peer-reviewed papers on arXiv are ok; APCs not funded in Horizon. A&A OA is ok.
Some catastrophic photo-z failures in template fitting but these are reduced with ML. Also tested on a COSMOS-like reference sample. Lots of multi-wavelength data for EDF from MeerKAT/LOFAR(2.0) to VISTA,HSC,Spitzer can help with deblending - could use GANs?
Next up is Andrea Enia, with a science talk on recovering of galaxy physical properties with template fitting and ML (Euclid paper in prep). They used MAMBO to simulate four Euclid surveys (Wide, Deep, calib16 and calib25), fitted with templateS, deep NN, CatBoost single+chained regressors, & NNPZ