-
# Your Hack Title
A sampler class for sampling multiple sources according to some user-defined metric.
Contacts: @MilesCranmer @henrysky @maja-jablonska
Participants: @MilesCranmer @henrysky @m…
-
对于如下内容:
```python
Massive ($\gtrsim9$ M$_\odot$) and very massive ($\gtrsim100$ M$_\odot$) stars are expected to release large amounts of energy and metal-enriched material throughout their relative…
-
**Describe the bug**
When i run COMPAS using single lines like
./compas --initial-mass-1 6 --initial-mass-2 4 --emit-gravitational-radiation True --evolve-double-white-dwarfs True,
the Run_Detai…
-
I configured the script paths according to my system, and I am using the following model:
`set MODEL = p5777_g+4.4_m0.0_t01_st_z+0.00_a+0.00_c+0.00_n+0.00_o+0.00_r+0.00_s+0.00.mod`
I also create…
-
### Data Owner Name
SXX Future Data
### What is your role related to the dataset
Data Preparer
### Data Owner Country/Region
China
### Data Owner Industry
Not-for-Profit
### We…
-
When using the Two Stage Common Envelope formalism, and plotting BBH yields as a function of metallicity, we are finding two strange pileups:
![image](https://github.com/user-attachments/assets/36c…
-
Now that we have the Padova/Colibri models incorporated into the downloadable data #357 , we need some criteria for when to use the models for a given star. At the moment we are not assuming any dust …
-
The output mass on the prospector is the ever-formed stellar mass, right?
How can this be changed? so that the output is the surviving stellar mass? I think I should pass add_stellar_remnants = Fal…
-
The IDL Hammer version returned a table of equivalent widths and band measurements, especially Balmer series and TiO values (particularly useful for low-mass star work, and computing *zeta*). Any hope…
-
When running the following binary, it crashes due to the "separation" not being available for the RLO calculation.
Even though the orbital_period and masses are given, it feels counterintuitive that …