J/other/PASA/42.158           GLEAM-300                      (Duchesne+, 2025)

GLEAM-300: The GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey at 300 MHz. Duchesne S., Cook J.H., Hurley-Walker N., Thomson A.J.M., Paterson S., Riseley C.J., McSweeney S.J., Mantovanini S., Heald G., Franzen T.M.O., Ross K., Seymour N., Wayth R.B., Galvin T.J. <Publ. Astron. Soc. Australia, 42, 158 (2025)> =2025PASA...42..158D 2025PASA...42..158D (SIMBAD/NED BibCode)
ADC_Keywords: Surveys ; Radio sources ; Galaxy catalogs ; Morphology Keywords: techniques: interferometric - galaxies: general - radio continuum: general - surveys Abstract: We present a wide-field radio survey at 300MHz covering the sky from -90 degrees to +40 degrees in declination using the Murchison Widefield Array (MWA). This 300-MHz survey follows the Galactic and Extragalactic All-sky MWA (GLEAM) survey, and provides an additional comparatively high-frequency data point to existing multi-frequency (72-231MHz) data. With this data release we provide mosaic images and a catalogue of compact source components. We use two-minute snapshot observations covering 2015 to 2016, combining overlapping two-minute snapshot images to provide full-sensitivity mosaic images with a median root-mean-square noise of 9.1+5.5-2.8mJy/beam and median angular resolution of 128.8"x112.5", with some position-dependent variation. We find a total of 338080 unique Gaussian components across the mosaic images. The survey is the first at 300MHz from the MWA covering the whole Southern Hemisphere. It provides a unique spectral data point that complements the existing GLEAM survey and the ongoing GLEAM-eXtended survey, and points toward results from the upcoming SKA-Low surveys. Description: The GLEAM-300 catalogue is constructed by running the Aegean source finder (2012ascl.soft12009H) on individual mosaics and merging the resultant source lists.The merging process removes duplicate measurements in overlap regions to return a final catalogue of unique radio components. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file gleam300.dat 203 338080 GLEAM-300 catalogue -------------------------------------------------------------------------------- See also: VIII/100 : GaLactic and Extragalactic All-sky MWA survey (Hurley-Walker+, 2016) VIII/102 : GLEAM II. Galactic plane (Hurley-Walker+, 2019) VIII/105 : The GLEAM 4-Jy (G4Jy) Sample (White+, 2020) VIII/109 : GLEAM III. South Galactic Pole (Franzen+, 2021) VIII/110 : GLEAM-X Data Release 1 (Hurley-Walker+, 2022) VIII/113 : GLEAM-X Data Release 2 (Ross+, 2024) J/other/PASA/38.41 : GLEAM 200MHz local radio luminosity function (Franzen+, 2021) J/other/PASA/42.137 : GLEAM-X. Galactic plane (Mantovanini+, 2026) https://doi.org/10.25919/z80f-5t62 : catalogue and mosaic images Byte-by-byte Description of file: gleam300.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 24 A24 --- Name Component name following IAU convention, GLEAM-300 JHHMMSS±DDMMSS (name) 26- 35 F10.6 deg RAdeg Right ascension (J2000) of the component (RAJ2000) 37- 44 F8.6 deg e_RAdeg Uncertainty on right ascension from fitting the component (err_RAJ2000) 46- 55 F10.6 deg DEdeg Declination (J2000) of the component (DEJ2000) 57- 64 F8.6 deg e_DEdeg Uncertainty on declination from fitting the component (err_DEJ2000) 66- 72 F7.4 Jy/beam localrms Local estimate of the root- mean-square noise (local_rms) 74- 80 F7.4 Jy/beam background Local estimate of the background (background) 82- 95 F14.9 Jy/beam Fpeak Peak flux density at 300MHz of the component (peak_flux) 97-103 F7.5 Jy/beam e_Fpeak Uncertainty in the peak flux density (errpeakflux) 105-118 F14.9 Jy Fint Integrated flux density at 300MHz of the component (int_flux) 120-127 F8.5 Jy e_Fint Uncertainty in the integrated flux density of the component (errintflux) 129-135 F7.2 arcsec amaj FWHM of the major axis of the component (a) 137-143 F7.2 arcsec e_amaj Uncertainty in the FWHM of the major axis (err_a) 145-151 F7.2 arcsec bmin FWHM of the minor axis of the component (b) 153-159 F7.2 arcsec e_bmin Uncertainty in the FWHM of the minor axis (err_b) 161-167 F7.3 deg PA [] Position angle of the component (pa) 169-175 F7.3 deg e_PA Uncertainty in the position angle (err_pa) 177-183 F7.3 arcsec bamaj Local major axis of the beam (bmaj) 185-189 F5.1 arcsec bbmin Local minor axis of the beam (bmin) 191-196 F6.2 deg bPA Local position angle of the beam (bpa) 198 I1 --- Flags Aegean fitting flags (flags) 200-203 F4.2 --- FluxScaleErr Flux density scale uncertainty (fluxscaleerr) -------------------------------------------------------------------------------- Acknowledgements: Stefan Duchesne, stefan.duchesne(at)csiro.au References: Wayth et al., 2015PASA...32...25W 2015PASA...32...25W Hurley-Walker et al., 2017MNRAS.464.1146H 2017MNRAS.464.1146H, Cat. VIII/100
(End) Patricia Vannier [CDS] 19-Feb-2026
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line