Mission Overview

The JWST Advanced Deep Extragalactic Survey (JADES)

Primary Investigator: Daniel Eisenstein, Nora Luetzgendorf, Marcia Rieke, Emma Curtis-Lake

HLSP Authors: Marcia Rieke, Brant Robertson, Sandro Tacchella,  Christopher Willmer, Ben Johnson, Stefano Carniani, Andy Bunker, Chris Willott, Alex Cameron, Emma Curtis-Lake, Francesco D'Eugenio, Jan Scholtz

Released: 2023-06-06

Updated: 2026-10-12

Primary Reference(s): Bunker et al. 2023, Eisenstein et al. 2023, Hainline et al. 2024, Rieke, M. et al. 2023, Eisenstein et al. 2023b, D'Eugenio et al. 2024, Curtis-Lake, Cameron, Bunker et al. 2026, Scholtz, Carniani et al. 2026

DOI: 10.17909/8tdj-8n28

Citations: See ADS Metrics

Read Me, Photometric Catalog Extension Read Me

Source Data:

 

Slideshow

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JADES Second Data Release Area

JADES Second Data Release Area

Figure 1: JADES second data release area.  The first release area is outlined in yellow while the green line outlines the region with new JADES data. The brown shaded regions have coverage only in F182M, F210M, and F444W from PID 1895, PI Pascal Oesch, FRESCO.

JADES Third Data Release Area (GOODS-N)

JADES GOODS-N coverage map in false color, showing thousands of galaxies dotted across the rectangular-shaped field.

Figure 2: The JADES third data release provides mosaics for GOODS-N with coverage using F090W, F115W, F200W, F277W,  F335M, F356W, F410M, and F444W. It also includes additional data using F182M, F210M, and F444W from FRESCO, PID 1895, PI Pascal Oesch.

Example JADES galaxy

Example JADES galaxy, with comparison to HST

Figure 3: A heavily obscured spiral shown on the left in a JADES F090W, F200W, and F444W composite. The image on the right is the HST ACS F814W image.

Example Clear/Prism Spectra

Example Clear/Prism spectra with R~100

Figure 4: Sample R~100 Clear/Prism spectra from the first data release (Bunker et al. 2023).

Example preview image of JADES spectra

Example preview image of JADES spectra

Figure 5: Example preview image of JADE clear/prism spectra, included for all sources in the data release.

JADES survey logo

Logo for the JADES survey

Figure 6: Logo for the JADES survey.

Example high-quality emission-line spectra from DR4

False-color spectral map showing a selection of high-quality JADES DR4 emission-line galaxy spectra ordered by increasing redshift. The horizontal axis shows observed wavelength from about 0.6 to 5.7 microns. Bright emission features appear as luminous curved bands that sweep diagonally from the lower left to the upper right, tracing how spectral lines shift to longer wavelengths with increasing redshift. Several major features are labeled along these tracks, including the Lyman-alpha drop, Balmer break, Hβ and [O III], Hα and [N II]/[S II], Hγ, [S III], He I and Paγ, Paβ, and Paα. Fainter continuum structures and additional emission features are visible throughout the background. The figure illustrates the richness and wavelength coverage of the JADES DR4 spectroscopic dataset and the clear detection of numerous emission-line and continuum features across a wide range of galaxy redshifts.

Figure 7: A selection of high-quality emission-line spectra from DR4, sorted by redshift. Numerous emission line and continuum features are clearly visible, showcasing the richness of the dataset.

Overview

The JWST Advanced Deep Extragalactic Survey (JADES) was the largest deep survey program undertaken during the first few years of JWST operations. Three GTO teams (NIRCam, NIRSpec, and MIRI-U.S.) combined observing time to produce a survey that will ultimately cover more than 100 square arcminutes from 0.7 to 5 microns and 10 square arcminutes at 7.7 microns, as well as obtain thousands of galaxy spectra.

The imaging data include Data Release 2 (DR2), which covers a larger area of GOODS-S and combines all JADES imaging with publicly available data in the field. The DR2 mosaics supersede those from Data Release 1 (DR1). Data Release 3 (DR3) provides the first JADES imaging mosaics of GOODS-N, covering 56 square arcminutes.

DR1 included spectra for more than 250 sources in GOODS-S; these spectra were subsequently superseded by Data Release 4 (DR4). DR2 did not include spectroscopic data. DR3 added more than 4,000 spectra, with measured redshifts for 2,375 sources. DR4 provides a full and consistent re-reduction of the NIRSpec spectroscopic sample, including spectra for more than 1,700 new sources and yielding a final sample with robust redshifts for 3,297 galaxies. DR4 spectra supersede all DR1 spectra and the majority of DR3 spectra.

DR2 and DR3 include photometric catalogs, while DR1, DR3, and DR4 include catalogs of emission-line fluxes. Photometric measurements and photometric-redshift estimates in the latest catalogs were produced using the same methodology as in the first data release.

Additionally, "FITSMap" provides a multicolor images browser and links to the photometry.  FITSMap is also accessible directly for the GOODS-S and GOODS-N fields.

Updates

10/12/26:  JADES Data Release 4 (DR4)

Re-reduction of full spectroscopic sample as well as new spectra for sources in GOODS-S and GOODS-N.  Includes catalogs (v1.2) of emission line fluxes and redshifts. DR4 spectra (v2.0) supersede all DR1 spectra and and a majority of DR3 spectra (v1.0).

05/06/24:  JADES Data Release 3 (DR3)

Mosaics (v2.0), spectra (v1.0), photometric catalog (v1.0) and spectral catalogs (v1.1) for GOODS-N, and spectra (v1.0) and new spectral catalogs (v1.1) for GOODS-S.

10/20/23:  JADES Data Release 2 (DR2)

NIRCam mosaics (v2.0) with new filters included, as well as an update to segmentation/detection maps and deep photometric catalogs (v2.0) for GOODS-S.  

06/15/23:  JADES Data Release 1 (DR1)

NIRCam mosaics, detection, and segmentation images (v1.0) and spectra (v1.0) for GOODS-S.

 

Median Sensitivities in GOODS-N Third Release Mosaics 

Measured in 0.15” Diameter Apertures (D'Eugenio et al. 2024)

Filter

3rd Release 5-sigma (nJy) 

Filter

3rd Release 5-sigma (nJy)

Filter

3rd Release 5-sigma (nJy)

F090W

9.8

F200W

6.4

F356W 3.7

F115W

6.9

F210M

14.4

F410M 7.7

F150W

7.6

F277W 3.8 F444W 6.4
F182M 11.3 F335M 6.0    

 

 

Sensitivities in Deepest Areas of First Release Mosaics

Measured in 0.3” Diameter Apertures (Rieke et al. 2023)

Filter

1st Release 5-sigma (nJy) 

Filter

1st Release 5-sigma (nJy)

Filter

1st Release 5-sigma (nJy)

F090W

5.8

F200W

4.4

F356W 3.6

F115W

4.3

F277W

3.4

F410M 5.7

F150W

4.6

F335M 5.9 F444W 4.5


Figure 1 shows the footprint for this Data Release 2 while Figure 2 shows the footprint for GOODS-N, part of Data Release 3.

In addition to increasing the areal coverage, the production of mosaics was modified to permit co-addition of all images in a given filter covering an area. Photometric measurements and photo-z estimations were done in the same fashion as for the first data release.

Figure 3 shows an example of a galaxy with a photometric redshift of 1.78 that is nearly invisible to HST ACS but is seen as a well-resolved but obscured spiral to JWST. 

The NIRSpec spectra presented as part of this release comprise a sample selected largely from objects detected using HST imaging of the ultra deep field (UDF). Bunker et al. 2023 describes the process of prioritizing objects to be placed on slits. About 250 galaxies were targeted using the 0.6 to 5.3 micron prism with up to 28 hours of exposure. Most of these objects were also targeted using all three R~1000 gratings and the longest wavelength R~2700 grating with up to 7 hours of exposure.

Data Products

Images

NIRCam images are named according to the following convention:

hlsp_jades_jwst_nircam_<region>_<filter>_<version>_<exten>.fits

where:

  • <region> is the imaging target region ("goods-s-deep" or "goods-n")
  • <filter> is the filter used (see sensitivity table above for examples)
  • <version> is the data product version ("v2.0")
  • <exten> is the file extension, including:
    • drz : Image mosaics with a pixel scale of 0.030” 
    • detection: "Detection" image constructed from long wavelength data and used to find objects on all the other images (see Rieke et al. 2023, D'Eugenio et al. 2024).
    • segmentation: "Segmentation" image (based closely on Source Extractor) used to assign pixels to objects for the photometric measurements (see Rieke et al. 2023, D'Eugenio et al. 2024).

Data file types:

_drz.fits NIRCam images
_detection.fits NIRCam detection image
_segmentation.fits NIRCam segmentation image

  

Spectra

The spectra are organized into five collections with each collection containing the spectra from a particular NIRSpec filter/disperser combination, and are named according to the following convention:

hlsp_jades_jwst_nirspec_<id-no>_<disperser-filter>_<version>_<extraction-type>.fits

where:

  • <id-no> is a combination of the survey name (e.g. "goods-s-deephst", “goods-s-deepjwst”, "goods-s-mediumhst", "goods-s-mediumjwst", "goods-s-ultradeep", "goods-n-mediumhst", or "goods-n-mediumjwst") and the identification number in the input catalog. Please note that “goods-s-mediumjwst1180” was also used in DR1 and DR3 but re-labelled “goods-s-mediumjwst” in DR4.
  • <disperser-filter> is the combination of disperser and filter used (e.g. "clear-prism", "f070lp-g140m", "f170lp-g235m", "f290lp-g395h", or "f290lp-g395m")
  • <version> is the data product version ("v1.0" for DR1 and DR3, “v2.0” for DR4)
  • <extraction-type> is the type of spectral extraction, one of "s2d" (2D spectra) or "x1d" (1D spectra)

An example spectrum file name is: hlsp_jades_jwst_nirspec_goods-s-deephst-10105275_clear-prism_v2.0_s2d.fits

Preview png files of the clear-prism spectra (1D and 2D on the same plot) are included, and named according to the following convention:

hlsp_jades_jwst_nirspec_<id-no>_<disperser-filter>_<version>_preview.png

Data file types:

_x1d.fits NIRSpec 1D spectra
_s2d.fits NIRSpec 2D spectra
_preview.png Preview image of NIRSpec spectra (1D and 2D)

Catalogs

The photometric catalog contains photometry for over 45,000 sources.  Photometry is given in both PSF-matched (denoted by conv) and non-convolved formats.  Kron photometry (denoted by "kron")  is presented as well as photometry in seven circular apertures (denoted by "circ").  See the Photometric Catalog Extension Readme for more details, including detailed descriptions of table extensions. The catalog includes photometry from the JEMS program.

The spectroscopic catalogs provide target information, redshifts and line fluxes as measured from the low-resolution prism and medium-resolution gratings. See the ReadMe above for more details.

hlsp_jades_jwst_<instrument>_<region>_<type>_<version>_catalog.fits

where:

  • <instrument> is the instrument used (one of "nircam" or "nirspec")
  • <region> is the imaging target region (one of "goods-s-deephst", "goods-s-deep", "goods-s", or "goods-n")
  • <type> is the type of catalog (one of "photometry", "clear-prism-line-fluxes", "gratings-line-fluxes" or “clear-prism-gratings-line-fluxes” where the grating and prism line fluxes are included in the same table for DR4)
  • <version> is the data product version (one of "v1.0", "v1.1", or "v1.2")

Data file types:

_catalog.fits Photometric or Line Flux catalogs

Data Access

JADES images and spectra are available in the MAST Portal (web-based, cross-mission search interface) and Astroquery (Python package to search for and download files from Python scripts you write), and via the direct download table below.

  • In the MAST Search Portal, set the Provenance Name filter to JADES in an Advanced Search to find these data. A direct Portal link to JADES data is provided here as well.
  • The user guide for how to search and download products using the MAST Portal is available here.
  • For Astroquery, the following example code demonstrates how to search for and download these products. This code assumes that you want to download all products from this HLSP, so you may want to consider narrowing down your search for large HLSPs (> 10 GB) or those with many individual files (> 10k). You can find more astroquery.mast tutorials here.

Clear-prism spectra contain preview images. To retrieve the preview spectral images, select the observations of interest, add them to the download basket, and uncheck (Minimum Recommended Products) MRP in the Download Manager.

Catalogs are only available via the direct download links below.

from astroquery.mast import Observations
f115w_obs = Observations.query_criteria(provenance_name="jades",instrument_name='NIRCAM/IMAGE',filters='F115W')
data_products = Observations.get_product_list(f115w_obs)
Observations.download_products(data_products)
  • A web-based interface for cross-mission searches of data at MAST or the Virtual Observatory
  • Search for and retrieve JADES data products programmatically.

Direct Download

Spectra files (all, including 1D, 2D, and preview images) can be downloaded using MAST interfaces as detailed above.

Image files can also be downloaded directly from the table below based on the filter used.

  Images
Field Mosaics by Filter
GOODS-S F090W | F115W | F150W |F182M| F200W |F210M| F277W | F335M | F356W | F410M |F430M| F444W|F460M|F480M (11 GB each)
  Detection Image | Segmentation Image (2.6 GB each)
GOODS-N F090W | F115W | F150W |F182M| F200W |F210M| F277W | F335M | F356W | F410M | F444W (14 GB each)
  Detection Image | Segmentation Image (3.4 GB each)

 

Catalog files can be downloaded directly from the table below. The file sizes are all <0.8 GB.

Catalogs
GOODS-S GOODS-N
NIRCam Photometry (GOODS-S-Deep v2.0) NIRCam Photometry (GOODS-N v1.0)
NIRSpec Clear-Prism Line Fluxes (GOODS-S-DeepHST v1.0) NIRSpec Clear-Prism Line Fluxes (GOODS-N v1.1)
NIRSpec Gratings Line Fluxes (GOODS-S-DeepHST v1.0) NIRSpec Gratings Line Fluxes (GOODS-N v1.1)
NIRSpec Gratings Line Fluxes (GOODS-S v1.1) NIRSpec Clear-Prism-Gratings Line Fluxes (GOODS-N v1.2)
NIRSpec Clear-Prism Line Fluxes (GOODS-S v1.1)  
NIRSpec Clear-Prism-Gratings Line Fluxes (GOODS-S v1.2)  

Citations

Please remember to cite the appropriate paper(s) below and the DOI. if you use these data in a published work. If you use any of the photometric catalogs please also reference the JEMS DOI .

Note: These HLSP data products are licensed for use under CC BY 4.0.

References