-
For sources with a counterpart, the lightcurve of the flux with the reference magnitude added is more relevant
**Feature Summary**
On the source page; the difference magnitude of the alerts is sho…
-
Photometry done using Photutils from Jupyter Notebook (image attached), does not include a column in the output table indicating "FILTER" or "BAND", which is required by SNCosmo.
-
Sharing data with Hermes requires either Instrument or Telescope for each data point.
In these cases (Getting data from a broker, or forced photometry) we SHOULD know the instrument and telescope u…
-
A few Formatting improvements are possible:
- [ ] Better ascii table alignment. (not space delimited)
- [ ] Horizontal Lines to break up sections
- [ ] Currently includes only Photometry table an…
-
> Software which processes counterpart-less sources from our match lists. It will identify possible data quality
problems which have orphaned the source. It will also test for possible proper motion …
-
Hello,
Is Bagpipes able to handle an upper limit on the flux in a filter? If so, how should I load in the photometry for Bagpipes so the code knows to treat a flux value as an upper limit?
Best,…
-
dataproduct_extras.photometry_for_target
[code link](https://github.com/BHTOM-Team/bhtom2/blob/5f8cbfd5c9ab2d0d4fb51cb3dddc8dd4c2124ba6/bhtom2/templatetags/dataproduct_extras.py
)
handle limits …
-
_From @jparrent on May 5, 2016 18:19_
Spectra will need to be scaled to the photometry.
_Copied from original issue: astrocatalogs/astrocats#29_
-
hi when i execute this:
`python disk_sim.py -s 33000. -r 54220.65.try9.33kms.fits -d 54220.65.try9.33kms.fits -o 54220.65.try10.33kms.fits`
I got the following error:
```
Traceback (most rec…
-
Are the HST + JWST filter throughput curves you used for the synthetic photometry available somewhere in the JADES data release?
Thanks!