The Parkes Catalogue of Radio Sources, also known as the Parkes Southern Radio Source Catalog, consists of 8264 astronomical radio sources, mostly south of declination +27. The catalogue was mostly compiled by John Bolton and his colleagues for 20 years. Both the Molonglo 408-MHz survey and the 80-MHz Culgoora measurements of Slee et al have contributed to the usefulness of the catalogue. For now, the catalogue only contains sources originally found in the Parkes 2700-MHz survey. The catalogue contains radio sources that have a frequency range of 80 - 22,000 MHz.[1][2]
Objects
editSee also
editReferences
edit- ^ "PKSCAT90 - Parkes Southern Radio Source Catalog, Version 1.01". heasarc.gsfc.nasa.gov.
- ^ "PKSCAT90 - The Southern RadioSource Database". www.parkes.atnf.csiro.au.
- ^ "PKS 0637-752: NASA Unveils First Images From Chandra X-Ray Observatory". harvard.edu.
- ^ "SNR PKS1209". nasa.gov.
- ^ Jackson, C. A.; Wall, J. V.; Shaver, P. A.; Kellermann, K. I.; Hook, I. M.; Hawkins, M. R. S. (2002). "The Parkes quarter-Jansky flat-spectrum sample: I. Sample selection and source identifications". Astronomy & Astrophysics. 386 (1): 97–113. doi:10.1051/0004-6361:20020119. ISSN 0004-6361.
- ^ Liuzzo, E.; Falomo, R.; Treves, A.; Donato, D.; Sambruna, M.; Arcidiacono, C.; Giovannini, G.; Farinato, J.; Moretti, A.; Ragazzoni, R.; Diolaiti, E.; Lombini, M.; Brast, R.; Donaldson, R.; Kolb, J.; Marchetti, E.; Tordo, S. (April 1, 2011). "The jet of the BL Lacertae object PKS 2201+044: MAD near-IR adaptive optics observations and comparison with optical, radio and X-ray data". Astronomy & Astrophysics. 528: A34. arXiv:1012.3620. Bibcode:2011A&A...528A..34L. doi:10.1051/0004-6361/201015570 – via www.aanda.org.
- ^ Bahcall, John N.; Kirhakos, Sofia; Schneider, Donald P.; Schneider, D. P. (1995). "PKS 2349–014: A Luminous Quasar with Thin Wisps, a Large Off-Center Nebulosity, and a Close Companion Galaxy". The Astrophysical Journal. 447: L1–L4. arXiv:astro-ph/9504076. Bibcode:1995ApJ...447L...1B. doi:10.1086/309548. S2CID 119342203.