Learning JWST Data Analysis With the JWebbinars
STScI hosts JWebbinars to teach the JWST community about tools and methods to analyze data from the James Webb Space Telescope. The JWebbinars are led by experts from STScI and the JWST Observer community. Participants are given hands-on experience with the data analysis tools. A virtual programming environment is provided so that participants will not be required to install software prior to attending the event. Each event lasts 2-3 hours.
The JWST data analysis ecosystem is based on Python and it is recommend that participants be familiar with basic Python coding and the Jupyter notebook interface to get the most out of the JWebbinars.
JWebbinar Registration
To register for a JWebbinar, please click on the links in the Information & Registration section below. After registration closes, you will receive an email with instructions pertaining to your particular JWebbinar. NOTE: This email and others from the organizer will come from from jwebbinars AT stsci DOT edu. Please make sure your spam filter does not block emails from this address. You will also receive an email with a Slack invitation, as there will be a Slack channel for the JWebbinar. Lastly, you will receive an email from Webex with the link to connect to the meeting.
Recordings of the JWebbinars and the accompanying material will be made available shortly after the class meets. Even if you plan to only use the offline material, if you register you will receive an email when the materials are posted to this website. Materials and Videos are available below.
If you have questions about the JWebbinars, please refer to the Frequently Asked Questions or contact the JWST Help Desk.
JWebbinar Schedule and Materials
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JWebbinar Content Dates Registration 40 - NIRCam and MIRI Coronagraphy: An Update 3 Years into Operations Nearly 3 years into operations, we will briefly present an update on the performance and capabilities of NIRCam and MIRI coronagraphs. We will review recommended observing strategies and the products provided by the automated calibration pipeline. We will also walk users through spaceKLIP, an STScI-supported JWST high-contrast imaging PSF subtraction and analysis package that also allows you to run and adapt the pipeline to your coronagraphy program. April 3, 11 am-1 pm (US Eastern Time) Register now
Registration closes on March 31
Special JWebbinar -Key Requirements for Submitting a Compliant Cycle 4 Budget Proposal This JWebbinar will provide you with what you need to know to submit a compliant Cycle 4 budget proposal. The budget proposal process has undergone significant changes for Cycle 4. Join us to learn about preparing a successful budget, allowable and unallowable costs, and how to avoid common pitfalls. A question and answer session will follow. The webinar is open to everyone involved in the budget proposal process including PIs, Co-Is, personnel in Sponsored Research, Budgeting, or P&A Department, etc. If you are unable to attend, the session will be recorded and added to the Material & Videos section. April 2, 3-4:30 pm (US Eastern Time) No registration required.
Webinar number: 2820 837 3094
Webinar password: XHmqDPn6W6
39 - Pipeline 101: An Introduction to the JWST Science Calibration Pipeline This JWebbinar will provide an introduction to the JWST Calibration Pipeline, giving an overview of the pipeline architecture and workflow along with its interaction with calibration reference files. We will walk through some example pipeline notebooks, demonstrate how to configure the pipeline for specific science cases, and discuss where to find answers to common questions. While most of the webinar will be focused on new users, we will touch briefly on a few advanced techniques. March 6, 11 am-1 pm (US Eastern Time) Registration is now closed
38 - Photometry with JWST: An Introduction to Photutils and Imviz This JWebbinar will focus on performing photometry on JWST NIRCam images using the Photutils package. Photutils is a Python library that provides commonly-used tools and key functionality for detecting and performing photometry of astronomical sources. We will also explore how to use Imviz to visualize images, load catalogs, and perform quick-look aperture photometry on a few objects. February 26, 11 am-1 pm (US Eastern Time)
Registration is now closed
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JWebbinar Materials Videos 39 - Pipeline 101: An Introduction to the JWST Science Calibration Pipeline Link to presentation:
Link to notebooks in PDF:
Github for the notebooks:
38 - Photometry with JWST: An Introduction to Photutils and Imviz Link to notebooks in PDF:
Github for the notebooks:
Other materials:
37 - Planning Solar System Observations with JWST Link to presentation:
Link to tutorial:
36 - What’s New in JWST Cycle 4 Links to presentations:
35 - NIRCam Short-wavelength Grisms: A Primer for TSOs Link to presentation:
The example APT file is available to retrieve within APT: File>Retrieve from STScI>Retrieve using Program ID 38.
The example ETC workbook is publicly accessible as a Sample Workbook titled "NIRCam Short Wavelength Grism Time-Series (Enabled by DHS)", workbook number 214650.34 - Introduction to WebbPSF: Modeling the Inflight PSF for JWST Link to presentation:
Link to notebook in PDF:
Github for the notebook:
33 - JWST NIRSpec MOS Data Reduction Link to presentation:
Links to notebooks in PDF:
Github for the notebooks:
32 - JWST Data Analysis with Jdaviz Link to presentation:
Links to notebooks in PDF:
- Imviz with associated screenshot #1 and screenshot #2
- Cubeviz with associated screenshot
- Specviz2d with associated screenshot
Github for the notebooks:
31 - Pipeline Reprocessing of JWST Imaging Data Link to presentation:
Links to notebooks in PDF:
Github for the notebooks:
30 - MOS Planning with MPT using an Example Science Case Link to presentation:
29 - JWST NIRSpec Time-Series Observations: From Uncalibrated Data to Transit Light Curves using CalWebb Links to presentations:
Links to notebooks in PDF:
Github for the notebooks
28 - Pipeline Reprocessing of Integral Field Unit Spectroscopy Link to presentation:
Links to notebooks in PDF:
Github for the MRS and NIRSpec notebooks (refer to the README in the repository for instructions)
27 - Introduction to the Astronomer's Proposal Tool for JWST for Cycle 3 Link to presentation:
26 - Introduction to the JWST Exposure Time Calculator for Cycle 3 Link to presentation:
25 - MAST: The JWST Data Archive Link to presentation:
Links to notebooks in PDF:
Github for the notebooks
24 - Jdaviz, the Visualization Tool for JWST
Link to presentation:
Links to notebooks in PDF (note the tool does not render in PDF):
- Specviz and screenshot
- Mosviz and screenshot
- Specviz2d and screenshot
- Imviz and screenshot
- Cubeviz and screenshot
Download all presentations and notebooks in PDF
Github (refer to the README in the repository for instructions)
23 - PDRs4ALL: Community Telecons in Support of JWST Cycle 2 Proposals
Materials and recordings are posted on https://pdrs4all.org/meeting-announcements/ 22 - NIRSpec and MIRI: Lessons Learned from Commissioning (December 2022)
Links to presentations:
21 - NIRISS and NIRCam: Lessons Learned from Commissioning (November 2022)
Links to presentatons:
20 - JWST Science Use Cases (November 2022) Link to presentation:
Github (refer to the README in the repository for instructions)
19 - ERS: Reducing & Analyzing JWST Coronagraphic Data with spaceKLIP (October 2022) Link to presentation:
18 - JWST Pipeline Refresher (October 2022) Links to presentations:
Links to notebooks in PDF:
- Pipeline products part 1
- Pipeline products part 2
- Pipeline products part 3
- Imagine pipeline stage 1
- Imagine pipeline stage 2
- Imagine pipeline stage 3
- Spectroscopy pipeline stage 2
- Spectroscopy pipeline stage 3
Download all presentations and notebooks in PDF
Github (refer to the README in the repository for instructions)
17 - MAST: Retrieving and Downloading Data (September 2022) Link to presentation:
Links to notebooks in PDF:
Download all presentations and notebooks in PDF
Github (refer to the README in the repository for instructions)
16 - JWST Time Series Observations: Performance and Caveats (July 2022) Download the presentation in PDF 15 - PDRs4all - Simulate NIRCam Observations of an Extended Source (June 2022) Links to presentations:
Links to notebooks in PDF:
Download all presentations and notebooks in PDF
Github (refer to the README in the repository for instructions)
14 - Q3D: Fitting Spectra and Data Cubes of Galaxies and Quasars (April 2022) Links to presentations:
Links to notebooks in PDF:
- Q3Dfit Baseline Example
- Q3Dfit with ETC NIRSpec Data
- Q3Dfit with MIR Spitzer Data
- Q3Dfit with MIR ETC Data
Download all presentations and notebooks in PDF
Github (refer to the README in the repository for instructions) and installation instructions
13 - CEERS NIRCam and MIRI Imaging (February 2022) Links to presentations:
Links to notebooks in PDF:
Download all presentations and notebooks in PDF
Github (refer to the README in the repository for instructions)
12 - JWST Pipeline 101 This webinar was a condensed version of JWebbinar 1, 3, and 4. Check out the materials and videos from those sessions provided above. 11 - Time-Series Observations (November 2021)
Links to presentations:
Links to notebooks in PDF format:
Download all presentations and notebooks in PDF
Github (refer to the README in the repository for instructions)
10 - Simulations with MIRAGE and MIRISim (November 2021)
Links to presentations:
Links to notebooks in PDF format:
Download all presentations and notebooks in PDF
Github (refer to the README in the repository for instructions)
9 - JWST Science Use Cases (October 2021)
Link to presentation: Introduction and workflow
Github (refer to the README in the repository for instructions)
8 - Spectral Analysis for JWST (September 2021)
Links to notebooks in PDF format:
- Overview of specutils for spectral data analysis
- IFU Spectral Extraction
- Redshift and Template Fitting
Github (refer to the README in the repository for instructions)
7 - NIRSpec MSA (August 2021)
Link to presentations:
Links to notebooks in PDF format will be provided when the dataset needed to run them can be made publicly available.
Github (refer to the README in the repository for instructions)
6 - NIRCam and MIRI Point-Source Imaging (July 2021) Link to presentation:
Links to notebooks in PDF format:
Download all presentations and notebooks in PDF
Github (refer to the README in the repository for instructions)
5 - MIRI and NIRSpec IFU (June 2021) Link to presentation:
Links to notebooks in PDF format:
- NIRSpec IFU pipeline processing
- MIRI MRS pipeline processing
- IFU analysis with Cubeviz (note that the GUI does not render in the PDF)
Download all presentations and notebooks in PDF
Github (refer to the README in the repository for instructions)
4 - Pipeline: Spectroscopic Mode (June 2021) Links to presentations:
Links to notebooks in PDF format:
Download all presentations and notebooks in PDF
Github (refer to the README in the repository for instructions)
- Calibration Pipeline Resources
- Overview of the Pipeline in Spectroscopic Mode
- Walkthrough of the Steps in Stage2 of the Various Spectroscopic Modes
- Walkthrough of the Steps in Stage3 of the Various Spectroscopic Modes
- Example Pipeline Run in Fixed Slit Mode (NIRSpec)
- Example Pipeline Run in IFU Mode (MIRI)
3 - Pipeline: Imaging Mode (May 2021) Links to presentations:
Links to notebooks in PDF format:
Download all presentations and notebooks in PDF
Github (refer to the README in the repository for instructions)
2 - Introduction to the JWST Data Analysis Tools (May 2021)
NOTE: The materials presented here for JWebbinar #2 regarding Jdaviz are out-of-date. For an updated JWebbinar presentation on Jdaviz, please view the materials for JWebbinar #24 (from February 2023) below.
Links to presentations:
Links to notebooks in PDF format (note that GUIs do not render in PDF):
Download all presentations and notebooks in PDF
Github (refer to the README in the repository for instructions)
1 - Pipeline Information and Data Products (April 2021) Links to presentations:
Links to notebooks in PDF format:
Download all presentations and notebooks in PDF
Github (refer to the README in the repository for instructions)
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JWebbinar Content Dates Held 37 - Planning Solar System Observations with JWST JWST is capable of observing the majority of solar system objects found beyond the Earth's orbit, such as asteroids, giant planets and their satellites, comets, and trans-Neptunian objects. Solar system targets may present additional challenges when planning observations, such as their apparent rates of motion, proximity to bright sources, or ephemeris uncertainties. This JWebbinar will focus on how to use available tools to determine valid observing windows for solar system targets, estimate signal-to-noise ratios for extended sources in the ETC, as well as create solar system targets, visualize target ephemerides, and specify constraints in APT. September 17, 11 am-1 pm (US Eastern Time) 36 - What’s New in JWST Cycle 4 This JWebbinar will cover updates in Cycle 4 to JWST proposal preparation tools and policies of which JWST proposers should be aware. We will discuss updates to the Astronomer’s Proposal Tool (APT), the Exposure Time Calculator (ETC), and the duplicate observation checking tool. We will also cover changes in the Call for Proposals, including the reduction of page limits and revisions to size and science categories. September 10, 11 am-1 pm (US Eastern Time) 35 - NIRCam Short-wavelength Grisms: A Primer for TSOs This webinar will cover implementation of time series observations using NIRCam's Dispersed Hartmann Sensor (DHS) grisms in the short-wavelength channel, which are being introduced for JWST Cycle 4. The DHS enables 0.6 to 2.3 µm low resolution spectroscopy simultaneously with the long-wavelength grism (2.4 to 5.0 µm) for NIRCam Grism Time Series Observations. The capability improves the bright limit for such observations, and relies on rather novel new subarray operations. Technical aspects of proposal planning will be highlighted, and a few scientific use cases of relatively bright transiting exoplanets will be presented. August 29, 11 am-1 pm (US Eastern Time) 34 - Introduction to WebbPSF: Modeling the Inflight PSF for JWST In this JWebbinar, we will cover the basics about simulating Webb’s PSF by using the inflight measurements of the optical performance of the telescope via Optical Path Difference files. Then we will introduce different tools and functions that allow the user to setup their simulations directly from the observations, to understand how the optical performance of the telescope might affect PSFs in science data and, finally, to use WebbPSF simulations to perform basic operations in science observations like PSF subtraction. July 16, 10 am-12 pm (US Eastern Time) 33 - JWST NIRSpec MOS Data Reduction This webinar will cover NIRSpec MOS (multi-object spectroscopy) data reduction by the JWST pipeline with example notebooks. We will cover recent pipeline updates that deliver improved spectra with default settings. We will also discuss lingering caveats, workarounds, and techniques to reprocess data, including editing the MSA metafile and master background subtraction. June 27, 10 am-12 pm (US Eastern Time) 32 - JWST Data Analysis with Jdaviz Introduction to the Jdaviz visualization package. Presenters will provide examples of the latest developed features available in the various configurations (Specviz, Cubeviz, Mosviz, Imviz, and Specviz2d) and will guide attendees through basic and advanced workflows to analyze JWST spectra and images. May 22, 10 am-12 pm (US Eastern Time) 31 - Pipeline Reprocessing of JWST Imaging Data This webinar will give an overview of the JWST science calibration pipeline and demonstrate how to process JWST NIRCam and MIRI Imaging observations from uncalibrated images to drizzled mosaics. The webinar will include examples on running the pipeline with custom settings, and also show how to incorporate manual processing to address common imaging issues. February 15, 10 am-12 pm (US Eastern Time)
February 16, 2-4 pm (US Eastern Time)
30 - MOS Planning with MPT using an Example Science Case The MSA Planning Tool (MPT) can be used to create NIRSpec multi-object spectroscopy (MOS) observations that achieve desired science goals. Using a real science program as an example the presenter will demonstrate how instrument and observational constraints inform MOS planning strategies in MPT. January 23, 10 am-12 pm (US Eastern Time)
January 24, 3-5 pm (US Eastern Time)
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JWebbinar Content Dates Held 29 - JWST NIRSpec Time-Series Observations: From Uncalibrated Data to Transit Light Curves using CalWebb This JWebbinar covers:
- Introduction to transit spectroscopy with BOTS
- Download of uncalibrated data from the MAST
- Step-by-step pipeline processing using the 'Detector1Pipeline' and visualization of intermediate products
- Spectral and complementary fitting data extraction and production of white light curve
December 14, 9-11 am (US Eastern Time)
December 15, 2-4 pm (US Eastern Time)
28 - Pipeline Reprocessing of Integral Field Unit Spectroscopy This JWebbinar will focus on how to use the current JWST calibration pipeline to reprocess integral field unit (IFU) spectroscopic data from JWST. The JWebbinar will present the default processing of IFU spectroscopic data, followed by what is often done to reprocess the data. This JWebbinar will cover such topics as modifying parameters for a specific step, adding a non-default step, manipulating parameter files, and more. December 5, 9-11 am (US Eastern Time)
December 6, 2-4 pm (US Eastern Time)
27 - Introduction to the Astronomer's Proposal Tool for JWST for Cycle 3 The presenters will describe how to create a basic APT program and the tools available in APT. Topics included will be the form editor, mosaics, visit planner, timeline and Aladin. Moving targets, pure parallels, and the MSA Planning Tool will not be covered in this JWebbinar. September 27, 9-11 am (US Eastern Time)
September 28, 2-4pm (US Eastern Time)
26 - Introduction to the JWST Exposure Time Calculator for Cycle 3 This JWebbinar will focus on the Exposure Time Calculator (ETC), one of the possible entry points when constructing a JWST proposal. The ETC provides many options that contemporary calculators do not, which can be both helpful and daunting. The purpose of this JWebbinar is to first walk through ETC usage linearly to obtain results for a straightforward observation of a point source, followed by the inclusion of more advanced ETC features for more complex observations. These advanced features are "modular" in the sense that multiple, or only one, can be used for any given ETC calculation, so the various options will first be presented separately, then combined to represent real use cases. September 21, 2-4 pm (US Eastern Time)
September 22, 10 am-12 pm (US Eastern Time)
25 - MAST: The JWST Data Archive Investigators who intend to propose for JWST observations in Cycle 3 will benefit from learning about MAST tools to search for existing or anticipated data that may help their research programs, and to discover potential duplications with observations they would like to make. This JWebbinar will include presentations and notebooks for graphical and scripted queries of MAST holdings, and tips for evaluating potential duplications. We will also offer tips and advice for retrieving JWST data, and provide links to documents and other resources for visualizing advanced JWST data products. There will be ample time during the workshop for participant questions and answers. September 19, 9-11 am (US Eastern Time)
September 20, 2-4pm (US Eastern Time)
24 - Jdaviz, the Visualization Tool for JWST Introduction to the Jdaviz visualization package. The presenters will describe the newest features available in the various configurations (Specviz, Cubeviz, Mosviz, Imviz, and Specviz2d) and will guide the attendees through basic and advanced workflows to analyze JWST spectra and images. February 13, 2023 - 2 pm (EST)
February 14, 2023 - 11 am (EST)
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JWebbinar Content Dates Held 23 - PDRs4ALL: Community Telecons in Support of JWST Cycle 2 Proposals As part of ERS proposal 1288: “Radiative Feedback from Massive Stars as Traced by Multiband Imaging and Spectroscopic Mosaics,” we have obtained NIRCam, NIRSpec, and MIRI imaging of the Orion Bar, a bright, extended object that is a concern for saturation with a large number of strong emission lines and high-contrast regions. These community telecons are meant to provide an overview of the “lessons learned” about the data reduction, calibration and data analysis related to this program.
Webinar 1: Status of Our ERS Observations (December 1)
Design, JWST instrument capabilities, and current status of our ERS program and data products. This includes data processing, remaining issues, cross calibrations and stitching.
Webinar 2: Modeling Tools (December 6)
Using the power of PDR models to determine physical conditions.
Webinar 3: Tools To Quantify the Spectral Information (December 16)
From JWST data to line/feature strength maps using PAHFIT, PAHTAT and the NASA Ames PAHdb.December 1, 2022, 11 am (EST)
December 6, 2022, 11 am (EST)
December 16, 2022, 11 am (EST)
22 - NIRSpec and MIRI: Lessons Learned from Commissioning
Members of the NIRSpec and MIRI instrument teams describe the features and caveats learned during commissioning. This webinar consists of presentations and does not include work on the science platform. December 7, 2022 - 11 am (EST) 21 - NIRISS and NIRCam: Lessons Learned from Commissioning
Members of the NIRISS and NIRCam instrument teams describe the features and caveats learned during commissioning. This webinar consists of presentations and does not include work on the science platform. November 30, 2022 - 11 am (EST) 20 - JWST Science Use Cases This JWebbinar covers:
- Understanding the concept of the data analysis example science notebook environment
- Installing and running the notebooks
- Using the JWST Data Analysis Visualization Tool (Jdaviz) within a notebook
- Analyzing real JWST data of different types (i.e., imaging, spectroscopy, and IFU cubes)
November 3, 2022 - 2 pm (EDT)
November 4, 2022 - 10 am (EDT)19 - ERS: Reducing & Analyzing JWST Coronagraphic Data with spaceKLIP In coordination with the JWST Early Release Science team for high contrast observations of exoplanets and exoplanetary systems, we are providing a 2-hour presentation and live demonstration of JWST coronagraphic data reduction and analysis using the open-source spaceKLIP Python package. This JWebbinar draws heavily from our experience of working with true on-sky data, and covers:
- Converting raw JWST data cubes to calibrated images
- Subtraction of the residual stellar PSF
- Calculating measurements of contrast performance
- Companion PSF Fitting
- JWST-specific caveats to all of the above
NOTE: This webinar consists of presentations and does not include work on the science platform.October 28, 2022 - 11 am (EDT) 18 - JWST Pipeline Refresher This 2-hour JWebbinar covers the basics of the JWST calibration pipeline. Two presentations introduce the calibration pipeline and the calibration reference data system (CRDS). The Jupyter Notebooks from JWebbinar 1, 3, and 4 are available on the science platform for the attendees to practice on and ask questions to the experts on the call. These notebooks feature inflight data from the Early Release Observations. October 11, 2022 - 2 pm (EDT)
October 13, 2022 - 10 am (EDT)17 - MAST: Retrieving and Downloading Data This JWebbinar demonstrates how to search the MAST archive for JWST data. We cover the features of the Portal Interface, customizable programmatic searches through two Jupyter Notebooks, and talk about creating DOIs (as requested by the mission) to promote reproducibility and increase your citation count. We do this in three mini-sessions where you follow along. Each session is followed by dedicated time for Q&A:
- We start with a brief overview of the Archive itself, then explore the features of the MAST Portal user interface, including basic/advanced search and subscription notifications. (~30 mins.)
- Next, we look at two Jupyter Notebooks: one analyzing exoplanet spectra, and the other looking at sources in a crowded field to retrieve the products you need to extract your own spectra. (~40 mins.)
- We close the session by going over DOIs; MAST offers a convenient way to create custom DOIs that permanently link to the raw data you used in your analysis. (~20 mins.)
September 20, 2022 - 10 am (EDT)
September 22, 2022 - 3 pm (EDT)16 - JWST Time Series Observations: Performance and Caveats This JWebbinar covers:
- Initial performance assessment of the JWST Time Series Observations (TSO) modes using commissioning observations
- Tour through the JDox documentation, as well as results on transiting exoplanet observations
- The performance of the four instruments will be discussed
NOTE: This webinar consists of presentations and does not include work on Jupyter notebooks.
July 15, 2022 - 11 am (EDT) 15 - PDRs4all: Simulate NIRCam Observations of an Extended Source This JWebbinar covers:
- Presentation of the ERS PDRs4All (scientific objectives and observing strategy)
- Simulation of raw NIRCam images with MIRAGE on an extended source (the Orion Bar) from a “mosaic” input image
- Reduction of NIRCam SW and LW imaging, step by step, using the latest version of the pipeline
June 23, 2022 - 10 am (EDT)
June 24, 2022 - 10 am. (EDT)14 - Q3D: Fitting Spectra and Data Cubes of Galaxies and Quasars Presentation of the q3dfit tools: a Python data analysis package for continuum and emission-line fitting of IFS data cubes of galaxies and quasars. Participants will:
- Learn about the inputs and outputs of the tool
- Run q3dfit on a set of rest-frame optical, near-IR, and mid-IR test data
April 7, 2022 - 11 am (EDT)
April 8, 2022 - 11 am (EDT)
13 - CEERS NIRCam and MIRI Imaging This JWebbinar covers:
- Reduction of a single chip of NIRCam SW and LW imaging in 6 broadband filters
- Reduction of a single MIRI pointing in 5 broadband filters
- Science cases: detection and analysis of high-redshift galaxies; dust emission from z~1-3 galaxies
February 24, 2022 - 10 am (EST)
February 25, 2022 - 2 pm (EST)
Virtual AAS239 Workshop: Intro to Data Analysis This JWebbinar covers:
- An overview of the Jdaviz tools
- JWST Science Use Case notebooks
The full content can be found at https://github.com/spacetelescope/aas239-jwebbinar
January 11, 2022 - 1 pm (EST) -
JWebbinar Content Dates Held 12 - JWST Pipeline 101 This JWebbinar is a condensed version of JWebbinars 1, 3, and 4 and covers:
- Introduction to JWST data products
- JWST pipeline in imaging mode
- Introduction to “Ramps to Slopes”
- Walkthrough Image2 and Image3
- JWST pipeline in spectroscopic mode
- Introduction to the different spectroscopic modes
- Work through an IFU use case
December 1, 2021 - 4 pm (EST) 11 - Time-Series Observations This JWebbinar covers:
- Introduction to TSOs with JWST:
- Instrumental capabilities and peculiarities
- MIRI, NIRCam, NIRISS, and NIRSpec
- Calibrating TSO data:
- How it works and how to engage with the pipeline
- TSO data analysis:
- Strategies and what to expect
November 30, 2021 - 2:30 pm (EST)
December 3, 2021 - 9 am (EST)10 - Simulations with MIRAGE and MIRISim This JWebbinar covers:
- Introduction to the MIRI simulator MIRISim and practice
- Introduction to the NIRISS and NIRCam simulator MIRAGE and practice
November 15, 2021 - 1 pm (EST)
November 17, 2021 - 9 am (EST)9 - JWST Science Use Cases This JWebbinar covers:
- Introduction to the JWST Data Analysis Tools notebooks
- Learn the github workflow: Download a JDAT notebook, prepare the appropriate environment, and start up the notebook
- Learn about JWST Science Use Cases working through these notebooks
- Try it on your own science use case and data
October 27, 2021 - 3 pm (EDT)
October 28, 2021 - 9:30 am (EDT)8 - Spectral Analysis for JWST This JWebbinar covers:
- Introduction to Specutils
- IFU spectral extraction
- Redshift measurement/template fitting with 1D spectra
- Spectral visualization tools: The Jdaviz package
September 29, 2021 - 9:30 am (EDT)
September 30, 2021 - 3:30 pm (EDT)
7 - NIRSpec MSA This JWebbinar covers:
- Introduction to NIRSpec MOS
- Brief refresher on MOS program updates
- NIRSpec MOS pipeline processing
- MOS data analysis using MOSviz
August 3, 2021 - 3 pm (EDT)
August 4, 2021 - 9 am (EDT)
August 6, 2021 - 12 pm (EDT)
6 - NIRCam and MIRI Point-Source Imaging This JWebbinar covers:
- Introduction to MIRI and NIRCam Imager
- MIRI Aperture Photometry
- NIRCam PSF Photometry
July 12, 2021 - 11 am (EDT)
July 13, 2021 - 3 pm (EDT)
July 14, 2021 - 1 pm (EDT)
5 - MIRI and NIRSpec IFU This JWebbinar covers:
- Introduction to MRS and IFU
- MIRI MRS pipeline processing
- NIRSpec IFU pipeline processing
- IFU + MRS data analysis using Cubeviz and specutils
June 28, 2021 - 1 pm (EDT)
June 30, 2021 - 3 pm (EDT)
July 1, 2021 - 10 am (EDT)
4 - Pipeline: Spectroscopic Mode This JWebbinar covers:
- Introduction to data products
- Introduction to Detector1 step
- Highlights of the different spectroscopic modes
- Default pipeline run (Spec2 and Spec3)
- Fixed slit example case
- IFU example case
June 14, 2021 - 10 am (EDT)
June 16, 2021 - 4 pm (EDT)
June 17, 2021 - 1 pm (EDT)
3 - Pipeline: Imaging Mode This JWebbinar covers:
- Introduction to data products
- Introduction to imaging pipeline
- Running the pipeline for imaging (Detector1, Image2, Image3)
May 27, 2021 - 10 am (EDT)
June 1, 2021 - 1 pm (EDT)
June 2, 2021 - 4:30 pm (EDT)
2 - Introduction to the JWST Data Analysis Tools This JWebbinar covers:
- Introduction to resources (JWST User Documentation, the Jdaviz package, Data analysis notebooks)
- Introduction to specutils
- Specviz workflow
- Mosviz workflow
- Cubeviz workflow
- The JWST data analysis notebooks
May 12, 2021 - 1 pm (EDT)
May 13, 2021 - 4 pm (EDT)
May 14, 2021 - 10 am (EDT)
1 - Pipeline Information and Data Products This JWebbinar covers:
- Introduction to resources (MAST, JWST User Documentation, Read-the-docs)
- Pipeline stages overview
- Open and explore JWST pipeline products
- Working with jwst.datamodels
August 18, 2021 - 10:30 am (EDT)
August 19, 2021 - 2 pm (EDT)
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April 28, 2021 - 10 am (EDT)
April 29, 2021 - 4 pm (EDT)
May 3, 2021 - 1 pm (EDT)
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Q. Why do you limit attendance to JWebbinars?
A. To maximize the interaction between the lecturers and the audience.
Q. What happens if all events are fully booked?
A. You can still register and will be added to a waiting list. If people cancel, we will go down the list to fill their spots. We will also consider organizing additional events to reach as many people as possible.
Q. Who should I contact if I have problems downloading or running the material posted after the event?
A. You can reach out to the JWST Help Desk.
Q. What do I need to set up my computer to use the online material?
A. Instructions can be found in the README file that comes with every webinar.
Q. How do I get started with Python?
A. If you're new to Python a great place to start is the official Python getting started page: https://www.python.org/about/gettingstarted/
Below are several resources to get you started learning Python if you are not familiar with Python:
- https://docs.python.org/tutorial/
- https://realpython.com/
- https://docs.python-guide.org/intro/learning/
Or, if you are familiar with Python or similar programming languages, but not the scientific programming ecosystem in Python:
- https://learn.astropy.org/
- https://realpython.com/numpy-tutorial/
- https://github.com/rougier/numpy-100
- https://matplotlib.org/stable/gallery/index.html
Q. How do I use the material on Github?
A. To use the material on github, you will need to download the notebooks to your local directory. You will then need a Python environment set up that is capable of running Jupyter notebooks. If you are new to Python, you may want to review these instructions for some resources on how to install and learn the basics of Python. Depending on your preferences and system choices, you may find the install instructions there sufficient, but note that many scientists find it easier to use the Anaconda Python distribution and package manager.
Each webinar will require a certain set of packages. For detailed instruction, you can refer to the readme files of each JWebbinar branch in the github repository.
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The NASA James Webb Space Telescope, developed in partnership with ESA and CSA, is operated by AURA’s Space Telescope Science Institute.