-
Notifications
You must be signed in to change notification settings - Fork 10
Commit
This commit does not belong to any branch on this repository, and may belong to a fork outside of the repository.
- Loading branch information
Showing
1 changed file
with
25 additions
and
1 deletion.
There are no files selected for viewing
This file contains bidirectional Unicode text that may be interpreted or compiled differently than what appears below. To review, open the file in an editor that reveals hidden Unicode characters.
Learn more about bidirectional Unicode characters
Original file line number | Diff line number | Diff line change |
---|---|---|
@@ -1,4 +1,28 @@ | ||
Tutorials | ||
========= | ||
|
||
You can find the Jupyter notebooks on various applications of MiraPy for problem-solving in Astronomy in our `Github repository <https://github.com/mirapy-org/tutorials>`_. | ||
We have a set of MiraPy tutorials for problem-solving in Astronomy using Deep Learning. You can find the Jupyter notebooks in our `Github repository <https://github.com/mirapy-org/tutorials>`_. Following are the short description of MiraPy applications: | ||
|
||
- **Astronomical Image Reconstruction using Autoencoder** | ||
|
||
Encoder-decoder networks can be trained for noise removal from blurry image. We can use MiraPy for astronomical image reconstruction by training a simple denoising autoencoder using some images of galaxies and nebulae in Missier catalog. | ||
|
||
- **ATLAS variable star Classification** | ||
|
||
We demonstrate how to use MiraPy to classify variable stars using features extracted from light curves. These features are available in ATLAS catalog. We use deep neural network for the same. | ||
|
||
- **OGLE variable star Classification** | ||
|
||
We demonstrate how to use MiraPy to classify variable stars using light-curves available in OGLE variable star catalogs. We use Recurrent Neural Network (RNN) in the classification model. | ||
|
||
- **HTRU1 Batched Dataset Classification** | ||
|
||
MiraPy can be used for the classification of pulsars and non-pulsars in dataset released by HTRU1 survey. The dataset contains 60000 images which are classified using Convolutional Neural Network (CNN). | ||
|
||
- **X-Ray Binary Classification** | ||
|
||
Tutorial demonstrates how to use Fully-Connected Neural (FCN) network to classify features of pulsar, non-pulsar and black hole systems. | ||
|
||
- **2D and 3D visualisation** | ||
|
||
We demonstrate how to use MiraPy to visualize a feature dataset using 2D and 3D graphs. For this purpose, we use Pricipal Component Analysis (PCA) for feature reduction. |