| Notebook | Description | Notebook Stage |
|---|
| General |
| Baseline |
| asdf | - Use case: create ASDF (Advanced Scientific Data Format) file from FITS file
- Data: CANDELS image of the COSMOS field
- Tools: asdf, gwcs, astrocut
- Cross-instrument: all instruments
| Baseline |
| Background Estimation | - Use case: estimate the sky background in complex scenes and evaluate the quality of the sky estimation
- Data: images with pathological background pattern created in the notebook
- Tools: Photutils
- Cross-instrument: all instruments
| Baseline |
| Redshift Cross-Correlation | - Use case: reproduce the workflow of the IRAF task XCORFIT to measure redshift with a cross-correlation algorithm
- Data: LEGA-C spectra and galaxy template spectra; optical rest-frame
- Tools: Specutils
- Cross-instrument: all instruments
| Baseline |
| Composite Model Spectral Fitting | - Use case: Fitting the complex continuum around Lyman-alpha in the spectrum of an active galaxy NGC 5548.
- Data: 3-column ECSV file with units for each column.
- Tools: Specutils, numpy
- Cross-instrument: all spectra
| Baseline |
| Querying MAST | - Use case: How to submit a NIRSpec MAST query using Python, and how to perform checks for potential duplication issues with any given targets by comparing with pre-existing MAST data
- Data:
- Tools: MAST, Astroquery
- Cross-instrument: created for NIRSpec, but good for all instruments
| Baseline |
| Specviz GUI Interaction | - Use case: How to inspect spectra in Specviz, export spectra from the GUI in the notebook, select regions in the GUI and in the notebook, and measure the redshift of a source in the GUI
- Data: NIRISS simulation of a generic scene with extended sources generated with the code MIRAGE
- Tools: Specutils, Jdaviz
- Cross-instrument: created for NIRISS, but good for all instruments
| Baseline |
| NIRCam |
| Baseline |
| Point Source Aperture Photometry | - Use case: Crowded field imaging with aperture-fitting photometry
- Data: JWST simulated NIRCam images from MIRAGE, run through the JWST calibration pipeline; LMC astrometric calibration field
- Tools: jwst, photutils
- Cross-instrument: potentially MIRI
| Baseline |
| PSF Photometry | - Use case: PSF photometry of crowded star field
- Data: JWST simulated NIRCam images from MIRAGE, run through the JWST calibration pipeline; LMC astrometric calibration field
- Tools: photutils, webbpsf
- Cross-instrument:
| Baseline |
| Extended Aperture Photometry | | Baseline |
| PSF Matched Extended Aperture Photometry | - Use case: Similar to multi-band extended aperture photometry (above), but PSF-matching is used to correct photometry measured in the Long Wavelength images (redder than F200W).
- Data: JWST simulated NIRCam images from JADES JWST GTO extragalactic blank field.
- Tools: photutils, webbpsf
- Cross-instrument:
| Baseline |
| NIRISS |
| Baseline |
| WFSS Single Object Galaxy Extraction and Analysis | - Use case: optimal extraction of grism spectra; redshift measurement; emission-line maps
- Data: JWST simulated NIRISS data from MIRAGE, run through the JWST calibration pipeline; galaxy cluster
- Tools: Specutils
- Cross-instrument: NIRSpec
| Baseline |
| WFSS Multi-Object Spectroscopy | - Use case: emission-line measurements and template matching on 1D spectra
- Data: LEGA-C spectra and galaxy template spectra; optical rest-frame
- Tools: Specutils
- Cross-instrument: NIRSpec
| Baseline |
| SOSS Transiting Exoplanet | - Use case: primary transit of an exoplanet
- Data: JWST simulated SOSS data from
AWESIMSOSS simulator - Tools: jwst, Juliet
- Cross-instrument:
| Baseline |
| NIRISS AMI Binary Star | - Use case: Find the binary parameters of AB Dor
- Data: MIRAGE simulations for a binary point source AB Dor and calibrator HD37093 using the Aperture Masking Interferometry (AMI) mode on JWST NIRISS
- Tools: jwst, nrm_analysis
- Cross-instrument:
| Baseline |
| NIRSpec |
| Baseline |
| IFU Analysis (Continuum Fitting) | - Use case: continuum and emission-line modeling of AGN; 1.47–1.87 μm
- Data: NIFS on Gemini; NGC 4151
- Tools: Specutils, Cubeviz, Specviz
- Cross-instrument: potentially MIRI
| Advanced |
| IFU Cube Modeling | - Use case: Extracting spatial-spectral features of interest from the cube of data and measuring their attributes. Create line and PAH maps from the model parameters map
- Data: Spitzer IRS on Messier 58
- Tools: Specutils, custom functions
- Cross-instrument: MIRI, NIRSpec
| Baseline |
| MOS Optimal Extraction | - Use case: optimal spectral extraction, method by Horne (1986)
- Data: JWST simulated NIRSpec MOS data; point sources
- Tools: jwst, custom functions
- Cross-instrument: any spectrograph
| Baseline |
| MOS Pre-Imaging w/ NIRCam | - Use case: Simulation of NIRCam imaging that can be used for NIRSpec MOS
- Data: JWST simulated NIRCam data from MIRAGE; LMC
- Tools: MIRAGE, jwst
- Cross-instrument: NIRCam.
| Baseline |
| BOTS Transiting Exoplanet | - Use case: bright object time series; extracting exoplanet spectra
- Data: JWST simulated NIRSpec data from ground-based campaign; GJ436b spectra from the Goyal et al. (2018)
- Tools:
- Cross-instrument:
| Baseline |
| IFU Optimal Extraction | - Use case: optimal spectral extraction; method by Horne (1986)
- Data: faint (quasar) point source was simulated using the NIRSpec Instrument Performance Simulator (IPS), then run through the JWST Spec2 pipeline
- Tools: jwst, Scipy, Specutils, Jdaviz, photutils, astropy.io, stropy.wcs, stropy.stats, astropy.utils, regions
- Cross-instrument:
| Baseline |
| MIRI |
| Baseline |
| LRS Optimal Extraction | - Use case: extract spectra with different locations, extraction apertures, and techniques
- Data: JWST simulated MIRI data
- Tools: jwst, Specutils, Specviz, specreduce, gwcs
- Cross-instrument: any spectrograph
| Baseline |
| MRS IFU Cube Analysis 1 | - Use case: Run the jwst pipeline on MIRI MRS data
- Data: JWST simulated MIRI MRS spectrum of AGB star.
- Tools: Specutils, Specviz, photutils
- Cross-instrument: any IFU
| Advanced |
| MRS IFU Cube Analysis 2 | - Use case: Optimal extraction of a MIRI MRS spectrum using a detector based extraction algorithm
- Data: JWST simulated MIRI MRS spectrum of AGB star.
- Tools: Specutils, Specviz, photutils
- Cross-instrument: any IFU
| Advance |
| MRS IFU Cube Analysis 3 | - Use case: Extract spatial-spectral features from IFU cube and measure their attributes
- Data: JWST simulated MIRI MRS spectrum of AGB star.
- Tools: Specutils, Specviz, photutils
- Cross-instrument: any IFU
| Advanced |
| IFUs of YSOs in LMC | - Use case: Detect point sources and extract photometry in a 3D cube. Analyze spectral lines.
- Data: ALMA 13CO data cubes.
- Tools: Specutils, Photutils, custom functions
- Cross-instrument: MIRI, NIRSpec
| Baseline |