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I found there is an obvious difference in W3 transmit curves between pyphot and SVO. This difference affects the conversion from spectrum to synthetic photometry. I don't know which curve is correct. …
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reported by: peter
Synthetic photometry is done now in a pretty crude way using tophat approximations for the filter transmission curves of e.g. the Spitzer IRAC and MIPS filters. This can be done m…
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Are the HST + JWST filter throughput curves you used for the synthetic photometry available somewhere in the JADES data release?
Thanks!
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We have been looking in detail at the photometry from our Oculus Pro Camera (Starlight Xpress) with 150 deg FOV.
For exposure times greater than 1 sec the light entering the camera from an apparent m…
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When computing synthetic photometry with Filter().obj_counts, need to catch and better treat the case where the source spectrum is significantly lower resolution than the transmission curve.
In thi…
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@robelgeda mentioned that it would be useful for `synphot.units` to be separated out from this package, so others can take advantage of the flux unit conversion even if they are not interested in synt…
pllim updated
4 years ago
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- [ ] Update example notebooks to use `catalogs.for_proposal`, including synthetic photometry to match the right filters.
- [ ] Make more notebooks for various OTE programs (could be in a separate…
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Try adding a boring elliptical galaxy to the tutorial to see if its synthetic photometry is also biased in the same direction as the emission line galaxy example. This will be diagnostic: if the borin…
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I use `simCluster` to create synthetic clusters with the $Gaia$ magnitudes using the following lines in the `.yaml` file but I only get the $u, g, r, i, z, J, H,$ and $K$ data.
```
main_sequ…
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- [x] KRC find spectral models, send to JRAD
(The R~10,000 model grid at http://phoenix.astro.physik.uni-goettingen.de/?page_id=16 would be my recommended starting point)
## Pre NYC HW
- [ ] KRC fi…