-
We should make a tutorial showing how to apply the interactive dashboards to low resolution spectra. We had previously focused on high-resolution applications, but many practitioners think at low res…
gully updated
2 years ago
-
Please list any corrections you noticed `typos` doesn't fix and we'll roll these up into a single PR, making it lighter weight for adding new corrections.
Preferred format (for easy copy/pasting):
…
-
### Data Owner Name
National Astronomical Observatories, Chinese Academy of Sciences
### Data Owner Country/Region
China
### Data Owner Industry
Environment
### Website
http://dr5.lamost.org/
…
-
Related to #230 which is about multiple systems where all of the components are UCDs. But this issue is about multiple systems where the companion is NOT a UCD and where we care more about some parame…
kelle updated
8 months ago
-
Take the simple case of four FITS files under template A3_-05_Dwarf.
Run PyHammer against them. Notice they are not reported as A3_-05.
Visually tune each file to A3_-05 and notice the smaller Templ…
-
**Describe the bug**
When running a binary star with the SeBa code via AMUSE, the order of the stars (primary or secondary) that is printed in the output file "starev.data" changes depending on the m…
-
From @mpgalleg comment on the Population Analysis Framework:
> I tried to follow the tutorial and ran into an error when trying to calculate the observable population of BBH mergers using a populat…
-
## Is your tweak request related to a problem? Please describe.
Confusion regarding users setting up PBR materials manually, especially in regards to the field for the Metallic/Specular and Smoothnes…
H3BO3 updated
3 years ago
-
First, thanks for making this code open source and available.
I am curious about adding support for the Baraffe et al. (e.g. BCAH 2002, BHAC 2015) pre-main sequence evolutionary models:
http://perso.e…
gully updated
4 years ago
-
Found by Oliver:
In the main Chempy() function (in wrapper.py) when SSPs are created, they are initialized with the ISM metallicity at time-step i (i.e. cube.cube['Z'][i]) but the element fractions o…