Metadata-Version: 2.4
Name: sausero
Version: 0.2.4
Summary: This software is designed to reduce Broad Band Imaging observations obtained with OSIRIS+.
Home-page: https://github.com/Kennicutt/SAUSERO
Author: Fabricio M. Pérez-Toledo
Author-email: fabricio.telescope@gmail.com
Classifier: Programming Language :: Python :: 3
Classifier: License :: OSI Approved :: GNU General Public License v3 (GPLv3)
Classifier: Operating System :: OS Independent
Requires-Python: >=3.9
Description-Content-Type: text/markdown
License-File: LICENSE
Requires-Dist: astroalign
Requires-Dist: astrometry_net_client
Requires-Dist: astropy
Requires-Dist: astroquery
Requires-Dist: ccdproc
Requires-Dist: lacosmic
Requires-Dist: loguru
Requires-Dist: matplotlib
Requires-Dist: numpy
Requires-Dist: PyYAML
Requires-Dist: sep
Dynamic: author
Dynamic: author-email
Dynamic: classifier
Dynamic: description
Dynamic: description-content-type
Dynamic: home-page
Dynamic: license-file
Dynamic: requires-dist
Dynamic: requires-python
Dynamic: summary

# SAUSERO

__SAUSERO__ is a reduction software for the Broad Band Imaging mode of OSIRIS+ at GTC.

Developed by __Fabricio M. Pérez-Toledo__

## General Description

**S**oftware to **AU**omatize in a **S**imple **E**nvironment the **R**eduction of **O**siris+ data (**SAUSERO**) processes raw science frames to address noise, cosmetic defects, and pixel heterogeneity, preparing them for photometric studies. These corrections are essential before any analysis can be performed. The operations applied to the images depend on the type of observation. This software has been specifically designed to reduce and prepare science frames for photometric studies.

### Key Reduction Steps:

1. Application of a __Bad Pixel Mask (BPM)__ to all frames.
2. Creation of the __Master Bias__.
3. Creation of the __Master Flat__.
4. Application of master calibration frames to both __standard star__ and __science frames__.
5. Removal of __cosmic rays__.
6. __Sky subtraction__.
7. Alignment of __science frames__.
8. __Astrometric calibration__.
9. __Flux calibration__.

### Input Requirements:

The software requires the following frames as input:

- __Bias frames__
- __Sky flat frames__
- __Photometric standard star frames__
- __Science frames__

## Outputs

The generated results consist of one image per observed band. For each image, the following corrections and calibrations will have been applied:

- __Bias subtraction__
- __Flat-field correction__ (including fringing correction for the Sloan z band, if applicable)
- __Image alignment and stacking__
- __Astrometric calibration__
- __Photometric calibration__ (estimation of the zero-point, ZP ± error)

To address cosmetic defects, a __Bad Pixel Mask (BPM)__ is applied, and the __LACosmic algorithm__ is used to handle cosmic ray removal.

## Requirements

### Operative System
- __Any__: The software is designed to run within a __Conda environment__, ensuring compatibility across platforms.

### Dependencies
The following Python packages are required (minimum versions specified), however, they will be installed
automatically together the :

    astroalign>=2.4.1
    astrometry_net_client>=0.3.0
    astropy>=5.3.4
    astroquery>=0.4.6
    ccdproc>=2.4.1
    lacosmic>=1.1.0
    loguru>=0.7.2
    matplotlib>=3.8.0
    numpy>=1.25.2
    PyYAML>=6.0.2
    sep>=1.2.1`

### Hardware Requirements
- __RAM__: Minimum 4GB (higher is recommended for large datasets).

## Installation

Installing SAUSERO is straightforward. Follow these steps:

1. __Activate your Conda environment__ (or create a new one if needed (see below)):
    ```
    conda activate <your_env>

2. __Install SAUSERO__ using `pip`:
    ```
    pip install sausero

That's it! SAUSERO is now almost ready to use ;)

### Optional: Creating a New Conda Environment

If you don’t have an existing Conda environment, you can create one specifically for SAUSERO with the following commands:

    conda create -n sausero_env python=3.9 -y
    conda activate sausero_env
    pip install sausero

## First-Time Setup

Once Conda is set up, you should run __SAUSERO__ for the first time to create the file `configuration.json` that has to be configured.

    sausero -pr <your_program> -bl <your_ob>

- `-pr`: Your GTC program indicator.
- `-bl`: The observed block number.

**ATTENTION**: The first time, the code will 'fail' because the configuration file does not know the root 
directory where the images are stored and your astrometry-api-key. To fix this, follow the instructions below.

You must edit the configuration file, which is located in your home directory inside 
a folder named `sausero/`.

You need to set the following parameters in the configuration file:

1. `PATH_DATA`: Set this to the root directory containing your frames. Example:

    ```
    "PATH_DATA": "/path/to/your/frames/"

The directory structure must follow the format `<Your_Program>_<Your_OB>/`. Inside this directory, you should have 
a `raw/` folder where the original frames are stored. During execution, __SAUSERO__ will create a new folder named 
`reduced/`, where the reduced frames will be saved.

2. `No_Session`: This is your Astrometry.net API key. Example:

    ```
    "No_Session":"astrometry-api-key"

To obtain this key, create an account on [Astrometry.net](https://nova.astrometry.net/). Copy your API key and paste it into the configuration file.

## Running SAUSERO

After updating and saving the configuration file, you can run the command again. This time, the software will execute successfully.

    sausero -pr <your_program> -bl <your_ob>

### Outputs and Results

Once the process is complete, you will find a collection of reduced frames in the `reduced/` folder inside your frame 
directory. The output includes:

A. __Reduced science frames__:
- One version with the sky included.
- One version with the sky subtracted.

B. __Aligned frames__:
- Both sky-included and sky-subtracted versions.

C. __Astrometrized frames__:
- Frames with astrometric calibration applied.

D. __Visualization PNG files__:
- A PNG showing the detected sources in the Field of View (FoV).
- A PNG showing the photometric standard star.

E. __Final reduced science frames__:
- Both sky-included and sky-subtracted versions.


### Important Notes

- By default, __SAUSERO__ ensures your data remains private when using Astrometry.net. The software's internal configuration avoids sharing any data with the Astrometry.net community, ensuring your data's security.

## Project Structure

    SAUSERO/
        BPM/
            BPM_OSIRIS_PLUS.fits -> BAD PIXEL MASK
        config/
            configuration.json   -> Configuration file.
        aligning_osirisplus.py   -> Aligns the science frames. 
        astrometry_osirisplus.py -> Astrometrization of the science frames.
        Color_Codes.py           -> Gives color to the comments
        OsirisDRP.py             -> Handles all the sofware and manages the frames. 
        photometry_osirisplus.py -> Carries out the photometric calibration.
        reduction_osirisplus.py  -> Carries out the clean process.

## Note about the frames

The code is designed to work with __OSIRIS+__ frames. They must be in __FITS__ format.

## LICENSE

This software is under __GPL v3.0__ license. More information is available in the
repository.

## CONTACT

- __Email__: [fabricio.perez@gtc.iac.es](fabricio.perez@gtc.iac.es)

- __Repository__: [https://github.com/Kennicutt/SAUSERO](https://github.com/Kennicutt/SAUSERO)
