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Hi Adam,
I'm currently using BAGPIPES to fit an SED to some photometric data. I've followed the instructions in the Guthub example tutorial notebooks to get my flux and flux errors in the way BAGPI…
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I realised that I never really documented this enhancement.
Currently sets of annular spectra have 'normal' ARFs generated for each spectrum of each annulus, without regard for PSF effects that can…
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I noted that [`2007ApJ...662..145H`](http://labs.adsabs.harvard.edu/ui/abs/2007ApJ...662..145H) is showing an abstract of:
```
Abstract: Using Chandra and HST archival data, we have studied the indiv…
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At the moment we have the method `calculate_los_tau_v` on galaxy; this calculates the column density of metals, converts to a dust mass, and then calculates an optical depth (`tau_v`).
In addition…
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Hi,
I am excited to use Bagpipes - thank you for making this code accessible!
I am new to using Bagpipes, and trying to perform a fit on NIRCam observations of a redshift ~ 7 galaxy. I am using fi…
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Stargen Fake accretion process.
The other day I was looking at some of the Stargen code. I was looking for the file(s) that refer to the elements that are used in the accretion process, because the o…
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The molnet loader functions are currently divided into two groups with inconsistent APIs for specifying featurizers and splitters.
Most of them have arguments `featurizer` and `split` to specify th…
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### Instrument
Light curve fitting (Stages 4-6)
### What happened?
I'm using the WASP-39b ERS NIRSpec dataset, and I'm trying to fit a polynomial and step to it. I put values into the S5 fit_…
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See https://github.com/LSSTDESC/DC2_Repo/issues/31 for detail.
- [x] code to reduce mock data
- [ ] code that works within DESCQA framework
- [ ] validation data
- [ ] validation criteria
yymao updated
6 years ago
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**Describe the bug**
At Z = 0.001, for fiducial pythonSubmit, stars with MZAMS [15-30] have WR winds as their dominant Mass loss rate when they pass the VINK_MASS_LOSS_MINIMUM_TEMP on their way to b…