... 15 fields[*]
Based on observations collected at the European Southern Observatory, Chile, as part of large programme 166.A-0162 (the ESO Distant Cluster Survey).
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...[*]
Full Table 4 is only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/482/419
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...hyperz[*]
http://webast.ast.obs-mip.fr/hyperz
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... spectrograph[*]
http://www.eso.org/instruments/fors
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... IRAF[*]
IRAF is distributed by the National Optical Astronomy Observatories, which are operated by the Association of Universities for Research in Astronomy, Inc., under cooperative agreement with the National Science Foundation.
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... Tables[*]
Tables is a product of the Space Telescope Science Institute, which is operated by AURA for NASA.
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...fceval[*]
The task fceval was kindly written for us by Frank Valdes from the IRAF project. The task is now included in the IRAF distribution.
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... fit[*]
When we discuss the numerical values of $\Delta x_{\rm r}$, we are referring to the situation where the size in Å of the pixels in x and in $x_{\rm r}$ is approximately the same. This is a natural choice, but not the only one possible. The $x_{\rm r}$ coordinate in some sense is arbitrary: it is only defined as soon as the 2D wavelength calibration (the slightly nonlinear mapping $(x,y_{\rm t}) \mapsto \lambda$) is used to construct an interpolated image pixelised in $(x_{\rm r},y_{\rm t})$, where $x_{\rm r}$ is linearly-related to $\lambda$, as $\lambda = a + bx_{\rm r}$.
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... library[*]
The idlutils library is developed by Doug Finkbeiner, Scott Burles, David Schlegel, Michael Blanton, David Hogg and others. See the Princeton/MIT SDSS Spectroscopy Home Page at http://spectro.princeton.edu/
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... list[*]
http://www.eso.org/observing/standards/spectra/
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...(ESA 1997)[*]
http://cadcwww.dao.nrc.ca/astrocat/hipparcos/
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...)[*]
Also available at http://www.ls.eso.org/lasilla/sciops/observing/Extinction.html
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Copyright ESO 2008