Mission Overview

The GLASS JWST Early Release Science Program

(GLASS-JWST)

 

Primary Investigator: Tommaso Treu

HLSP Authors: GLASS-JWST Team

Released: 2023-07-07

Updated: 2024-10-25

Primary Reference(s): Treu, T. et al. 2022, Paris, D., et al. 2023, Mascia et al. 2024

DOI: 10.17909/kw3c-n857

Citations: See ADS metrics

Readme.md (see also: author README)

Source Data:

 
Abell 2744 Cluster
Color composite (RGB) image of the Hubble Frontier Field cluster Abell 2744, derived by combining the F090W+F115W+F150W as blue, F200W+F277W as green and F356W+F410M+F444W as red. Colored borders show the position of the three different JWST data sets used here: GLASS (green), UNCOVER (GO-2561, blue) and DD-2756 (red). The entire image (including the empty space) is approximately 12.7 × 5.9 arcmin on the sky.

 

Overview

The GLASS-JWST Early Release Science Program (hereafter GLASS-JWST ERS) has obtained the deepest observations of galaxies obtained of all Early Release Science Programs by targeting the Hubble Frontier Field, and in particular the lensing cluster Abell 2744. This high-level science product collection combines the GLASS-JWST NIRCam imaging data (ERS-1324) with NIRCam data from two other JWST programs targeting the same field: UNCOVER (GO-2561; PI: I. Labbé and R. Bezanson) and Program DD-2756 (PI: W. Chen). The observed area in the wide-band filters - covering the central and extended regions of the cluster, as well as new parallel fields - is 46.5 arcmin2 in total.

The spectra are from NIRSpec observations in the Abell 2744 field, and were obtained in this program, and from the program DDT-2758 (PI: Chen). Please refer to Mascia et al. (2024) for more details on the GLASS-JWST Spectroscopic Data.

Data Products

The first release of this collection includes JWST NIRCam mosaics plus root-mean-square (RMS) maps for 8 IR filters. The mosaics were produced by the JWST calibration pipeline, as supplemented by several custom procedures developed by the GLASS-JWST team to correct for residual defects that were not addressed in standard processing. All mosaics are in FITS format with brightness in μJy/sr and a zero-point of ZP_AB = 23.9.

The first release also includes a mult-wavelength catalog consisting of photometry from these mosaics, and is combined with publicly available HST photometry in the F435W, F606W, F775W and F814W ACS bands, and in the F105W, F125W, F140W and F160W WFC3 bands. The photometric catalog was derived by detecting objects in the NIRCam F444W image and computing PSF-matched forced photometry on the remaining bands, using various apertures. The apertures sizes were 0.28′′, 0.56′′, 1.12′′ and 2.24′′ (corresponding to 2×, 3×, 8× and 16× the point-spread function (PSF) of the F444W image, respectively), and also the isophotal (segmentation) aperture. The resulting catalog contains 24,389 sources.

The second release consists of 263 spectral images and extracted spectra of 245 unique sources obtained with NIRSpec in the Abell 2744 field. The Level-1 products were produced by the JWST calibration pipeline, and the higher level products were produced with msaexp. The spectral coverage depends upon the redshift of the sources. The products also include a spectral template of high-redshift galaxies, which was constructed by stacking the 74 highest-quality spectra that span redshifts from 0.3 to 9.3.

The second release also includes a spectral line detection catalog, which indicates for each spectral source which of more than 60 emission lines were detected with a signal-to-noise ratio of at least 5.

Data file naming convention:

hlsp_glass-jwst_jwst_<instrument>_abell2744_<optElem>_v1_<prodType>.fits

where:

  • <instrument> is either nircam or nirspec
  • <optElem> is the optical element name:
    • one of f090w, f115w, f150w, f200w, f277w, f356w, f410m, f444w for images
    • one of f100lp-g140h, f170lp-g235h, f290lp-g395h, clear-prism for spectra
  • <prodType> is the product semantic type, shown below:
_sci

Science image

_rms RMS image
_spec Source spectrum (incl. 2-D and 1-D extractions)
_spec-template Stacked spectrum template
_cat Catalog

Data Access

GLASS-JWST images and spectra are available in the MAST Portal (the web-based, cross-mission search interface) and Astroquery (a Python package to search for and download files from Python scripts you write), and via the direct download table below. Set the Provenance Name filter to GLASS-JWST in the Portal Advanced Search to find the data products.

from astroquery.mast import Observations
all_obs = Observations.query_criteria(provenance_name="glass-jwst")
data_products = Observations.get_product_list(all_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 GLASS-JWST data products programmatically.

Direct Download

Access the JWST special products from the table below. The catalog sizes are small, but the spectral template is approximately 2.4 MB.

Content Type File Link
Photometric catalog

hlsp_glass-jwst_jwst-hst_multi_abell2744_multiband_v1.0_cat.fits.gz

Composite spectral template hlsp_glass-jwst_jwst_nirspec_abell2744_v1_spec-template.fits
Emission line detection catalog hlsp_glass-jwst_jwst_nirspec_abell2744_v1_cat.fits

 

The photometric source catalog consists of a FITS file with multiple BINTABLE extensions, named corresponding to the photometric aperture on which the photometry was performed. The emission line detection catalog consists of a FITS file with two BINTABLE extensions.

Citations

Be sure to cite the appropriate paper(s) below and the DOI if you use these data in a published work. 

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

References