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Titlebook: Reviews of Physiology, Biochemistry and Pharmacology; Volume: 73 R. H. Adrian,E. Helmreich,A. Weber Book 1975 The Editor(s) (if applicable)

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nt both about the source population in the Universe and the sensitivity of detectors employed in astronomical observations). To observe large number densities of sources, one needs deep observations to probe the faint (and thus more numerous) population of galaxies. Faint galaxies, however, are smal
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Reviews of Physiology, Biochemistry and Pharmacologyhttp://image.papertrans.cn/r/image/829725.jpg
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https://doi.org/10.1007/BFb0034656biochemistry; pharmacology; physiology; research
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Reviews of Physiology, Biochemistry and Pharmacology978-3-540-37572-2Series ISSN 0303-4240 Series E-ISSN 1617-5786
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W. HasselbachO-galaxy association to be explained by gravitational lensing ? We can reexamine observations and theories (minding, however, Roger Blandford‘s warning to ponder the fate of Albigensians). In particular, we may wonder how much the background QSO counts are affected by lensing. Microlensing on Δθ ≲ 1
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E. De RobertisO-galaxy association to be explained by gravitational lensing ? We can reexamine observations and theories (minding, however, Roger Blandford‘s warning to ponder the fate of Albigensians). In particular, we may wonder how much the background QSO counts are affected by lensing. Microlensing on Δθ ≲ 1
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