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- W4244550008 abstract "The Hubble (magnitude-redshift) diagram for brightest cluster galaxies (BCGs) is a classic cosmological tool, widely studied because of the remarkably small dispersion (∼ 0.3 mag) in the absolute optical magnitudes of low redshift BCGs (Postman and Lauer 1995). Extending the BCG Hubble diagram to higher redshifts would greatly enhance its role as a cosmological probe, but this has been frustrated by several technical problems: – the conventional means of cluster selection in the optical become increasingly compromised by projection effects at z > 0.1 – at higher redshifts the interpretation of optical magnitudes becomes increasingly complicated by the effects of possible star formation." @default.
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- W4244550008 date "1998-01-01" @default.
- W4244550008 modified "2023-09-27" @default.
- W4244550008 title "The K-Band Hubble Diagram for X-Ray Selected Brightest Cluster Galaxies" @default.
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- W4244550008 doi "https://doi.org/10.1017/s0074180900128955" @default.
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