The New Era of Wide‐Field Astronomy

By R. Clowes. 2001

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Evidence for Quasar Activity Triggered by Galaxy Mergers in HST Observations of Dust-reddened Quasars (2007, background): “Optical quasar surveys tend to miss dust-reddened quasars which have been found either with infrared surveys (Cutri et al. 2001; Lacy et al. 2004), radio surveys (White et al. 2003), hard X-ray surveys (Norman et al. 2002), or surveys for high-ionization narrow-line objects (Zakamska et al. 2006).”
A synthetic view on structure and evolution of the Milky Way (2003, methodology): “…observed star counts can be found in Goldman et al. (2002), Ojha (2001), Robin et al. (2000), Reylé & Robin (2001a) and Castellani (2001) in visible bands; Krause (2003) in the I band; Ruphy et al. (1996), Persi et al. (1999), Persi et al. (2001) and Reylé & Robin (2001a) in the near infrared.”
Power Spectrum Covariance of Weak Gravitational Lensing (2000, background): “The numerical values here are appropriate for surveys that reach a limiting magnitude in R ∼ 25 (e.g., Smail et al 1995).”
The WFCAM Science Archive (2006, background): “The WSA is the prototype science archive for the VISTA surveys, and the design of the VISTA Science Archive will follow closely that described here.”