Fitting
*******

Jupyter notebooks with fitting examples can be found `here
<https://github.com/Q3D/q3dfit/tree/main/jnb>`_. You can download and
run these examples on your own computer, either directly or by cloning
the ``q3dfit`` repository. Or, you can test the notebooks in binder:

.. image:: https://mybinder.org/badge_logo.svg
 :target: https://mybinder.org/v2/gh/Q3D/q3dfit/main

Six example notebooks are currently available.
	  
1. **Single Ground-based spectrum, rest-frame optical, single
   emission-line component, stellar population fit**

   Data cube is from Gemini/GMOS observations of ORC2/3C, as published in `Rupke et al. 2024a <https://ui.adsabs.harvard.edu/abs/2024ApJ...967...51R/abstract>`_.

   Jupyter notebook: `q3dfit_example_restframeopt_ground_ppxf.ipynb <https://github.com/Q3D/q3dfit/blob/main/jnb/q3dfit_example_restframeopt_ground_ppxf.ipynb>`_
	  
2. **Ground-based data, rest-frame optical, single emission-line
   component, quasar**

   Data cube is from Gemini/GMOS observations of `PG1411+442 <https://ned.ipac.caltech.edu/byname?objname=PG1411%2B442&hconst=67.8&omegam=0.308&omegav=0.692&wmap=4&corr_z=1>`_, as published in `Rupke et al. 2017 <https://ui.adsabs.harvard.edu/abs/2017ApJ...850...40R/abstract>`_.

   Jupyter notebook: `q3dfit_example_restframeopt_ground.ipynb <https://github.com/Q3D/q3dfit/blob/main/jnb/q3dfit_example_restframeopt_ground.ipynb>`_
	  
3. **JWST/NIRSpec-IFU data, rest-frame optical, multiple components,
   quasar**

   Data cube is from observations of `SDSSJ165202.64+172852.3 <https://ned.ipac.caltech.edu/byname?objname=SDSSJ165202.64%2B172852.3&hconst=67.8&omegam=0.308&omegav=0.692&wmap=4&corr_z=1>`_, as published in `Wylezalek et al. 2022 <https://ui.adsabs.harvard.edu/abs/2022arXiv221010074W/abstract>`_.

   Jupyter notebook: `q3dfit_example_restframeopt_nirspec.ipynb <https://github.com/Q3D/q3dfit/blob/main/jnb/q3dfit_example_restframeopt_nirspec.ipynb>`_

4. **Spitzer data, rest-frame mid-IR, single emission-line component, single spectrum, galaxy**
   
   Spectrum is a `low-resolution Spitzer IRS observation <https://cassis.sirtf.com/atlas/cgi/onespectrum.py?aorkey=22128896&ptg=0>`_ of `2MASX J15561599+3951374 <http://ned.ipac.caltech.edu/cgi-bin/objsearch?objname=2MASX%20J15561599%2B3951374&extend=no&hconst=73&omegam=0.27&omegav=0.73&corr_z=1&out_csys=Equatorial&out_equinox=J2000.0&obj_sort=RA+or+Longitude&of=pre_text&zv_breaker=30000.0&list_limit=5&img_stamp=YES#ObjNo1>`_.

   Jupyter notebook: `q3dfit_example_restframeMIR_Spitzer.ipynb <https://github.com/Q3D/q3dfit/blob/main/jnb/q3dfit_example_restframe
   MIR_Spitzer.ipynb>`_

5. **JWST/MIRI-MRS data, rest-frame mid-IR, single band, one emission line**

   Data cube is from observations of `F2M110648.35+480712.3 <http://ned.ipac.caltech.edu/byname?objname=SDSS+J110648.32%2B480712.3&hconst=67.8&omegam=0.308&omegav=0.692&wmap=4&corr_z=1>`_, as published in `Rupke et al. 2024b <https://ui.adsabs.harvard.edu/abs/2023ApJ...953L..26R/abstract>`_.

   Jupyter notebook: `q3dfit_example_restframeMIR_miri_ch3b.ipynb <https://github.com/Q3D/q3dfit/blob/main/jnb/q3dfit_example_restframeMIR_miri_ch3b.ipynb>`_
   
6. **JWST/MIRI-MRS data, rest-frame mid-IR, all bands, multiple emission-line components, continuum dust + silicate emission**
   
   Data cube is from observations of `PDS 466 <https://ned.ipac.caltech.edu/byname?objname=pds+456&hconst=67.8&omegam=0.308&omegav=0.692&wmap=4&corr_z=1>`_, as published in `Seebeck et al. 2024 <https://ui.adsabs.harvard.edu/abs/2024ApJ...976..240S/abstract>`_.

   Jupyter notebook: `q3dfit_example_restframeMIR_miri_all.ipynb <https://github.com/Q3D/q3dfit/blob/main/jnb/q3dfit_example_restframeMIR_miri_all.ipynb>`_