Skip to main content

# brutus #### _**Et tu, Brute?**_

brutus is a Pure Python package whose core modules involve using “brute force” Bayesian inference to derive distances, reddenings, and stellar properties from photometry using a grid of stellar models.

The package is designed to be highly modular, with current modules including utilities for modeling individual stars, star clusters, and stellar-based 3-D dust mapping.

### Documentation Currently nonexistent.

### Data

Various files needed to run different `brutus` modules can be downloaded [here](https://www.dropbox.com/sh/ozq9tk8iyy8fhte/AAC_G0wA9eQ8shHbZzAKwLe-a?dl=0). Various components of these are described below.

#### Stellar Models Note that while brutus can (in theory) be run over an arbitrary set of stellar models, it is configured for two by default: [MIST](http://waps.cfa.harvard.edu/MIST/) and [Bayestar](https://arxiv.org/abs/1401.1508).

#### Zero-points Zero-point offsets in several bands have been estimated using Gaia data and can be included during runtime. These are currently not thoroughly vetted, so use at your own risk.

#### Dust Map brutus is able to incorporate a 3-D dust prior. The current prior is based on the “Bayestar19” dust map from [Green et al. (2019)](https://arxiv.org/abs/1905.02734).

#### Generating SEDs brutus contains built-in SED generation utilities based on the MIST stellar models, modeled off of [minesweeper](https://github.com/pacargile/MINESweeper). These are optimized for either generating photometry from stellar mass tracks or for a single-age stellar isochrone based on artificial neural networks trained on bolometric correction tables.

Empirical corrections to the MIST models derived using several clusters are implemented by default, which improves main sequence behavior down to ~0.5 solar masses. These can be easily disabled by users using the appropriate flag. These are currently not thoroughly vetted.

Please contact Phil Cargile (pcargile@cfa.harvard.edu) and Josh Speagle (jspeagle@cfa.harvard.edu) for more information on the provided data files.

### Installation brutus can be installed by running ` python setup.py install ` from inside the repository.

### Demos Several Jupyter notebooks currently outline very basic usage of the code. Please contact Josh Speagle (jspeagle@cfa.harvard.edu) with any questions.

Metadata

Release files for astro-brutus 0.8.2

For a detailed explanation of source distributions (sdists) and built distributions (wheels), please see the package formats documentation.

Built distribution (wheel)

Table of built distributions (wheels) for astro-brutus 0.8.2
File Interpreter ABI Platform
astro_brutus-0.8.2-py3-none-any.whl Python 3 none any Details

Release files / astro_brutus-0.8.2-py3-none-any.whl

Download URL astro_brutus-0.8.2-py3-none-any.whl
Size 81.2 kB
Tags Python 3
SHA-256 checksum
How to use checksums
9ff39b96d0a9c22c6dbfb6e3677de2eeb2d22e9f428d38943445eee3109d18d1
BLAKE2b-256 checksum
How to use checksums
2f3f9e59aba583cd6a9044f9be2a31805abfd210a7e120a94abcb5dd0d99df19
Upload date
Uploaded using Trusted Publishing?
What is trusted publishing?
No
Uploaded via twine/3.1.1 pkginfo/1.5.0.1 requests/2.22.0 setuptools/46.4.0 requests-toolbelt/0.9.1 tqdm/4.42.0 CPython/3.7.6

Release history Release notifications | RSS feed

1.2.0

2 release files

1.1.0

2 release files

This release

0.8.2 This release

1 release file

Anthropic, PBC Visionary sponsor Bloomberg Visionary sponsor Hudson River Trading Visionary sponsor Meta Visionary sponsor NVIDIA Visionary sponsor Microsoft Sustainability sponsor Depot Continuous Integration AWS Cloud computing and Security Sponsor Datadog Monitoring Fastly CDN Google Download Analytics Sentry Error logging StatusPage Status page