astrocatalogs / supernovae

Astrocats module for the Open Supernova Catalog (OSC). Please use the issue tracker on this repo for all OSC issues.
https://sne.space
MIT License
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Unreasonably large negative/positive epochs for some events #50

Open jparrent opened 7 years ago

jparrent commented 7 years ago

Hey @guillochon, below is the list of objects with either highly negative or highly positive epochs that we looked over. I have loosely organized them by whether or not I think the problem is due to an inaccurate date of max (e.g., b/c of "C" photometry points), a problem of dates on WISeREP ("W"), and so on. There are some of these where the epoch will need to be estimated with something like SNID, in which case we might want to add a field/flag that highlights that the date of maximum has been determined by estimating the post/pre-max epoch of any available spectra and working backwards/forwards. I can jump to this if & when you feel it appropriate to do so.

Uncertain Max ("C")

W -- Questionable date for the spectra

Uncertain Max -- Other

The following list are simply events with questionable epochs given the limited photometry available; unclear how to address outside of SNID estimates.

guillochon commented 7 years ago

@jparrent I believe the C-band-related issues should be fixed now, I only checked a few but that should be corrected.

jparrent commented 7 years ago

@guillochon Awesome, I will check these out later this evening.

jparrent commented 7 years ago

@guillochon Alright, I've updated the list. We can check out the rest in the coming weeks and I think I'll start playing around with SNID on something these at home to see how accurate the estimates for epochs are going to be.

guillochon commented 7 years ago

Hey @jparrent, so the date of max is interesting. We have a separate "date of visual maximum" date now being computed that is based on either B or V (or similar), but currently we just use "date of maximum" for plotting on the page. It's not clear to me what the best selection is.

Really what we need to do is some basic LC fitting to determine a better date of max, or SNID, or both. Using individual photometric observations clearly isn't cutting it for some of the events.