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MeanStars-3.1.0
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مشاهده بیشترتوضیحات
Automated property interpolation and color calculations for main sequence stars
| ویژگی | مقدار |
|---|---|
| سیستم عامل | OS Independent |
| نام فایل | MeanStars-3.1.0 |
| نام | MeanStars |
| نسخه کتابخانه | 3.1.0 |
| نگهدارنده | [] |
| ایمیل نگهدارنده | [] |
| نویسنده | Dmitry Savransky |
| ایمیل نویسنده | ds264@cornell.edu |
| آدرس صفحه اصلی | https://github.com/dsavransky/MeanStars |
| آدرس اینترنتی | https://pypi.org/project/MeanStars/ |
| مجوز | - |
[](https://coveralls.io/github/dsavransky/MeanStars?branch=main)
[](http://www.astropy.org/)
[](https://badge.fury.io/py/MeanStars)
[](https://requires.io/github/dsavransky/MeanStars/requirements/?branch=main)
# MeanStars
This code provides functionality for automating calculations based on Eric Mamajek's "A Modern Mean Dwarf Stellar Color and Effective Temperature Sequence" (http://www.pas.rochester.edu/~emamajek/EEM_dwarf_UBVIJHK_colors_Teff.txt).
The purpose of the code is to allow users to automatically interpolate the property columns of the table, and to calcualte colors based on any combination of the photometry columns.
## Installation and Requirements
MeanStars requires the following python modules:
* numpy
* scipy
* astropy
To install, simply run:
pip install MeanStars
Alternatively, grab a copy of the repository and run:
python setup.py install
## Usage
To use MeanStars, you must first create a MeanStars object:
```python
from MeanStars import MeanStars
ms = MeanStars()
```
This object contains a number of useful attributes, including:
* `ms.data`: The full dataset in astropy table format
* `ms.bands`: The names of all unique bands from the dataset (in a string array)
* `ms.colors`: All of the original colors from the dataset (in an nx2 string array, where n is the length of `ms.bands` and the color is the first column minus the second). The same information is also encoded in `ms.colorstr`, which is the original color name from the dataset
* `ms.noncolors`: All data attributes not related to color (these include stellar masses, radii, etc.)
* `ms.SpecTypes`: All of the major spectral types from the dataset (in a string array - nominally this will always be O,B,A,F,G,K,M,L,T,Y)
* `ms.colorgraph`: A directed graph (encoded as a dictionary) mapping all relationships between bands established by the colors in the original dataset
### Interpolating Colors
MeanStars provides two methods for interpolating colors: `TeffColor` and `SpTColor`, where the former interpolates by effective temperature, and the latter by spectral type. In general, it is unlikely that you will want to query the data by any spectral type not explicilty listed, so the `SpTColor` most frequently acts as a simple lookup table of the data. In each case, the methods are called by providing the two bands defining the color (called `start` and `end` in the code such that the color is `start` - `end`), and the temperature or spectral type.
So, to find the 'U-B' color of a 29000 K star, you would execute:
```python
ms.TeffColor('U','B',29000)
```
This particular instance corresponds to an exact entry in the data table, and the value returned should exactly match the entry. A more interesting case is the 'U-H' color of a 6000 K star:
```python
ms.TeffColor('U','H',6000)
```
Here, you are requesting a color not found in the table at a temperature not found in the table (but bracketed by other temperature values). You can query to find the specific sets of color combined to give this result by running:
```python
ms.searchgraph('U','H')
```
which will return `['U', 'B', 'V', 'Ks', 'H']`, meaning that the 'U-B','B-V','V-Ks', and 'Ks-H' colors were added to get the result.
Interpolating by spectral type works exactly the same way, excpet that the type is defined by two input variables representing the major and minor subtype. So, to find the 'U-H' color of a G2V dwarf, you would execute:
```python
ms.SpTColor('U','H','G',2)
```
Each time one of these routines is called on a new color (for a given object instance), the generated interpolant is saved in `ms.Teffinterps` and `ms.SpTinterps` (as appropriate to the method call). This means that the interpolant is generated just once per object instance, speeding up subsequent computations.
### Interpolating Other Properties
Just as with colors, any other property in the original data set can be interpolated as a function of effective temperature or spectral type, via methods `TeffOther` and `SpTOther`, respectively. The methods use the same syntax as their color counterparts, save that the property is defined by a single string input.
So, to find the mean solar mass of a 5500 K star, you would run:
```python
ms.TeffOther('Msun',5500)
```
and to find the mean radius of a K9V star, you would run:
```python
ms.SpTOther('R_Rsun','K',9)
```
نیازمندی
| مقدار | نام |
|---|---|
| - | scipy |
| - | numpy |
| - | astropy |
نحوه نصب
نصب پکیج whl MeanStars-3.1.0:
pip install MeanStars-3.1.0.whl
نصب پکیج tar.gz MeanStars-3.1.0:
pip install MeanStars-3.1.0.tar.gz