diff --git a/README.md b/README.md
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--- a/README.md
+++ b/README.md
@@ -1,3 +1,9 @@
+[**Main documentation**](https://aboucaud.github.io/galcheat/) | [**Getting started**](#getting-started) | [**CLI**](#cli) | [**API**](#api) | [**Contributing**](#contributing) | [**License**](#license)
+
+
+
+
+
[![Python package][gh-workflow-badge]][gh-workflow]
[![License][license-badge]](LICENSE)
![Python supported versions][pyversion-badge]
@@ -12,16 +18,11 @@
[pypi-badge]: https://badge.fury.io/py/galcheat.svg
[pypi]: https://pypi.org/project/galcheat/
-Galaxy Surveys cheatsheet
-=========================
-
Tiny package containing useful parameters from main galaxy surveys (**with units**).
The goal of this project is to provide a Python library with minimal dependencies that centralises galaxy survey properties with adequate reference. Such information tends to be scattered in many places or is often copy/pasted without all of the relevant information like units or sources.
-The current parameters and the corresponding units are specified in the [data README](galcheat/data/README.md)
-
-[**Getting started**](#getting-started) | [**CLI**](#cli) | [**API**](#api) | [**Contributing**](#contributing) | [**License**](#license)
+The current parameters and the corresponding units are specified in the [documentation](https://aboucaud.github.io/galcheat/parameters.html)
Getting started
---------------
@@ -44,7 +45,7 @@ galcheat
- **`--refs`**: print the source for each parameter
- **`-h, --help`**: get help
-### Exemples
+### Examples
```sh
galcheat -s LSST # LSST info
galcheat --refs # all surveys info with refs
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diff --git a/galcheat/data/README.md b/galcheat/data/README.md
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-`galcheat` data files
-=====================
-
-The following document describes the parameters expected for the photometric surveys and their filters: how they should be computed, their units, etc.
-
-[**Survey parameters**](#survey-parameters) | [**Filter parameters**](#filter-parameters) | [**References**](#references) | [**Data file layout**](#yaml-file-layout)
-
-Survey parameters
------------------
-
-### Units and types
-
-| parameter name | type | units |
-| ----------------- | ----- | -------------- |
-| name | str | – |
-| pixel_scale | float | arcsec / pixel |
-| gain | float | e- / ADU |
-| mirror_diameter | float | m |
-| obscuration | float | dimensionless |
-| zeropoint_airmass | float | dimensionless |
-
-### Parameter description
-
-#### `name`
-
-The classical name or abbreviation for the survey. Most often this is how the survey is referred to.
-In case of an ambiguity, for instance when a survey has several instruments, the name of the instrument should be added as a suffix (e.g. `Euclid_VIS`).
-
-#### `description`
-
-A bit of context around the survey: on which telescope, with which instrument, wide survey or a specific deep field.
-
-#### `pixel_scale`
-
-Size of a square pixel on the sky.
-
-#### `gain`
-
-Conversion factor between the photo-electrons received by the camera and the digital counts after the amplification of the electronics.
-
-#### `mirror_diameter`
-
-Primary mirror diameter, in meters.
-
-#### `obscuration`
-
-Proportion of the total area of the telescope that is obscured by the position of secondary mirrors, lenses, camera, etc.
-
-This parameter is used to compute the effective area of the telescope.
-
-#### `zeropoint_airmass`
-
-Airmass value at which the zeropoint is computed.
-The airmass is commonly defined as the optical path length through the atmosphere relative to the zenith path length.
-For space surveys, this value is set to 0.0.
-
-Filter parameters
------------------
-### Units and types
-
-| parameter name | type | units |
-| -------------------- | --------- | -------------- |
-| name | str | – |
-| sky_brightness | float | mag / arcsec^2 |
-| full_exposure_time | int/float | s |
-| zeropoint | float | mag |
-| psf_fwhm | float | arcsec |
-| effective_wavelength | float | nm |
-
-### Description
-#### `name`
-
-Name of the filter
-
-#### `sky_brightness`
-
-Average sky brightness computed for the survey and this filter.
-The moon conditions under which this number was computed will be given as a comment in the yaml file.
-
-#### `full_exposure_time`
-
-Average exposure time of the filter on the same spot in the sky over the course of the survey.
-
-#### `zeropoint`
-
-The zeropoint is the magnitude of an object that produces 1 e- per second on the detector. It is computed for a given filter, using the [`speclite`][speclite] library with a classical atmosphere, at the airmass indicated in the survey parameters: `zeropoint_airmass`.
-
-
-[speclite]: https://github.com/desihub/speclite
-
-#### `psf_fwhm`
-
-Average full width at half-maximum (FWHM) of the point spread function (PSF) over the filter.
-
-#### `effective_wavelength` – ***optional***
-
-Wavelength computed as a weighted average of the full passband throughput over the wavelength range.
-The throughput takes into account the transmission of the filter, the transmittance of the optics, the CCD efficiency as well as a standard atmospheric extinction model.
-
-References
-----------
-
-The parameters written in `galcheat` have all been sourced and referenced.
-
-These references can be specified for each parameter as a link and a comment string.
-
-YAML file layout
-----------------
-
-The information for a given survey should be written in an individual YAML file, with a specific layout.
-
-The survey information should appear first, with one parameter per line.
-
-After these parameters, the list of filters should appear. YAML uses new lines and indentation to create lists.
-
-An example for a survey called `Survey42` with two filters `a` and `b` is shown below.
-
-```yaml
-# Content of Survey42.yaml
-name: "Survey42"
-description: "The Survey42 was done on the XXX telescope with the YYY instrument"
-pixel_scale: 0.2
-gain: 2.0
-mirror_diameter: 4.2
-obscuration: 0.2
-zeropoint_airmass: 1.2
-filters:
- a:
- name: "a"
- sky_brightness: 19.4
- full_exposure_time: 500
- zeropoint: 26.90
- psf_fwhm: 1.1
- effective_wavelength: 500.00
- b:
- name: "b"
- sky_brightness: 18.6
- full_exposure_time: 500
- zeropoint: 27.36
- psf_fwhm: 1.2
- effective_wavelength: 600.00
-references:
- pixel_scale:
- link: "https://link-to-the-pixelscale-ref.com"
- comment: "See section 2.4"
- gain:
- link: "https://link-to-the-gain-info.org"
- comment: ""
- psf_fwhm:
- link: "https://link-to-filters-refs.org"
- comment: ""
-# goal is to have a reference per parameter, survey or filter-wise...
-```