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Volumn 10, Issue 4, 2000, Pages 419-437

What will the next generation radio telescope detect at 1.4 GHZ?

Author keywords

Galaxies: Evolution; Galaxies: General; Galaxies: Luminosity function

Indexed keywords


EID: 0034360127     PISSN: 09226435     EISSN: None     Source Type: Journal    
DOI: 10.1023/A:1008171310884     Document Type: Article
Times cited : (34)

References (52)
  • 11
    • 0042225334 scopus 로고    scopus 로고
    • N. Jackson and R. J. Davis (eds.) Cambridge: Cambridge University Press
    • de Bruyn A. G.: 1996, in: N. Jackson and R. J. Davis (eds.) High Sensitivity Radio Astronomy (Cambridge: Cambridge University Press), p. 233.
    • (1996) High Sensitivity Radio Astronomy , pp. 233
    • De Bruyn, A.G.1
  • 31
    • 0042225332 scopus 로고    scopus 로고
    • D. Breitschwerdt, M. J. Freyberg, J. Truemper (eds.), IAU Colloquium Springer Verlag
    • Mac Low M.-M. and Ferrara A.: 1998, in: D. Breitschwerdt, M. J. Freyberg, J. Truemper (eds.), The Local Bubble and Beyond (IAU Colloquium 166, Springer Verlag), p. 559
    • (1998) The Local Bubble and Beyond , vol.166 , pp. 559
    • Mac Low, M.-M.1    Ferrara, A.2
  • 52
    • 0041725014 scopus 로고    scopus 로고
    • H. J. A. Röttgering, P. N. Best, M. D. Lehnert (eds.), Kluwer Academic Publishers, Dordrecht
    • Windhorst R. A.: 1999, in: H. J. A. Röttgering, P. N. Best, M. D. Lehnert (eds.), The Most Distant Galaxies (Kluwer Academic Publishers, Dordrecht).
    • (1999) The Most Distant Galaxies
    • Windhorst, R.A.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.