SIMPLE-AstroDB / SIMPLE-db

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JWST spectra ingest, spectra utils improvements #458

Closed kelle closed 5 months ago

kelle commented 6 months ago

Ingesting one JWST T dwarf spectrum. Also working on improving spectra ingest scripts and modifying given new astrodb_scripts package.

For data ingests:

kelle commented 5 months ago

Apologies, this is really two different things.

kelle commented 5 months ago

I guess I could add some tests for ingest_spectrum function...

SherelynA commented 5 months ago

@kelle do you also plan to ingest the MIRI JWST photometry?

kelle commented 5 months ago

I do not have those data. If you want to post here, I'll give it a go at ingesting.

SherelynA commented 5 months ago

I do not have those data. If you want to post here, I'll give it a go at ingesting.

@kelle This is the data: We used the following filters and the magnitudes/uncertainties (aper_total_vegamag) used :MIRI.F1000W - (13.740374118847015, 0.00509224851727859) & MIRI.F1280W - (13.125575556995827, 0.00711303904668107) & MIRI.F1800W - (12.108791667404923, 0.01817644357837899)

kelle commented 5 months ago

I assume those are JY, right? And any reason to maintain all those significant figures?

kelle commented 5 months ago
kelle commented 5 months ago

This could be reviewed and merged at any point. I'm just gonna keep polishing the new scripts and tests until it's merged. :)

SherelynA commented 5 months ago

I assume those are JY, right? And any reason to maintain all those significant figures?

@kelle I don't know if I understand this well. I gave the magnitudes, not the fluxes which like you mentioned are in Janskys.

kelle commented 5 months ago

Yes, I reminded myself about magnitudes being flux ratios after posting that comment. I rounded the numbers based on the uncertainties. What numbers are reported in the paper?

SherelynA commented 5 months ago

Yes, I reminded myself about magnitudes being flux ratios after posting that comment. I rounded the numbers based on the uncertainties. What numbers are reported in the paper?

@kelle The numbers reported in the paper are the following F1000W: (13.740±0.005) & F1280W: (13.126±0.007) & F1800W: (12.107±0.017).