GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey II: Galactic Plane ,
arXiv:1911.08127 · doi:10.1017/pasa.2019.37
Abstract
This work makes available a further 2,860deg of the GLEAM survey, covering half of the accessible Galactic Plane, across twenty frequency bands sampling MHz, with resolution . Unlike previous GLEAM data releases, we used multi-scale clean to better deconvolve large-scale Galactic structure. For the Galactic longitude ranges , , we provide a compact source catalogue of 22,037 components selected from a 60-MHz bandwidth image centred at 200-MHz, with RMS noise mJy beam and position accuracy better than . The catalogue has a completeness of 50% at mJy, and a reliability of 99.86%. It covers Galactic latitudes toward the Galactic Centre and for other regions, and is available from Vizier; images covering for all longitudes are made available on the GLEAM VO server and SkyView.
14 pages, 9 figures, 2 tables, accepted to PASA
References in corpus (6)
- The NumPy array: a structure for efficient numerical computation
- WSClean: an implementation of a fast, generic wide-field imager for radio astronomy
- GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey I: A low-frequency extragalactic catalogue
- The Very Large Array Low-frequency Sky Survey Redux (VLSSr)
- A radio spectral index map and catalogue at 147-1400 MHz covering 80 per cent of the sky
- Calibration and Stokes Imaging with Full Embedded Element Primary Beam Model for the Murchison Widefield Array
Cited by in corpus (9)
- The Galactic center chimneys: The base of the multiphase outflow of the Milky Way
- Radio Observations of Supernova Remnant G1.9+0.3
- Hoinga: A supernova remnant discovered in the SRG/eROSITA All-Sky Survey eRASS1
- Thermal radio absorption as a tracer of the interaction of SNRs with their environments
- Observing the Reionization : Effect of Calibration and Position Errors on Realistic Observation Conditions
- Determination of Planetary Nebulae angular diameters from radio continuum Spectral Energy Distribution modeling
- Evolutionary Map of the Universe (EMU):Compact radio sources in the SCORPIO field towards the Galactic plane
- Where is the Western Part of the Galactic Center Lobe Located really?
- Low X-ray Efficiency of a Young High-B Pulsar PSR J1208-6238 Observed with Chandra