"Gas outflows in two recently quenched galaxies at z = 4 and 7" (Valentino+2025): photometry and spectra

We release the photometric and spectroscopic dataset analyzed and presented in the article "Gas outflows in two recently quenched galaxies at z = 4 and 7" by Valentino, Heintz, Brammer et al., Astronomy & Astrophysics (2025). This work is based in part on observations made with the JWST and HST telescopes and are associated with the programs # 1176, 1837, 3567, 4233, and 4446. The data were retrieved from the Dawn JWST Archive (DJA). The reduction made use of the grizli (Brammer+2023) and msaexp (Brammer+2023) pipelines. Details of the general data reduction and release are described in Valentino+2023 (photometry), de Graaff+2024, and Heintz+2025 (spectroscopy, v3). The files are organized as follows: 0) README.txtThis file is a copy of this description. It presents the content of the file "supplementary_material.tar" containing tables for the manuscript "Gas outflows in two recently quenched galaxies at z=4 and 7" by Valentino, Heintz, Brammer et al. (2025, A&A). 1) Photometry:The "[name of the target]_photometry.cat.release" files contain the HST and JWST photometry of NS_274 at RUBIES-UDS-QG-Z7. The filters names follow the convention established in the Dawn JWST Archive (DJA). We report the pivot wavelength in angstrom for convenience. The flux densities and their uncertainties are expressed per unit frequency and in microJanskies (uJy). 2) Spectra:The "[name of the target]_[prism|g140m|g235m|g395m].spec_central.release" files contain the JWST/NIRSpec spectra of NS_274 at RUBIES-UDS-QG-Z7. Each file contains an observed wavelength column in angstrom, flux densities, and their uncertainties are expressed per unit wavelength and in units of 1e-20 erg/cm^2/s/angstrom. We include the wavelength mask generated by msaexp as a column of "True/False" values in string format.