Fitting

Jupyter notebooks with fitting examples can be found here. 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:

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.

   Jupyter notebook: 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, as published in Rupke et al. 2017.

   Jupyter notebook: 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, as published in Wylezalek et al. 2022.

   Jupyter notebook: 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 of 2MASX J15561599+3951374.

   Jupyter notebook: q3dfit_example_restframeMIR_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, as published in Rupke et al. 2024b.

   Jupyter notebook: 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, as published in Seebeck et al. 2024.

   Jupyter notebook: q3dfit_example_restframeMIR_miri_all.ipynb