Abstract.
All observations were made using the Double-Beam Spectrograph on the 2.3m telescope at Siding Spring. See Table 1 for a log of observations. Both the red and blue sides were utilised together with the D1 dichroic mirror. All spectra were reduced using the standard reduction techniques in IRAF.
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Buxton, M., Vennes, S. Optical Spectroscopic Observations of Black-Hole Candidates. In: Kaper, L., Heuvel, E.P.J.v.d., Woudt, P.A. (eds) Black Holes in Binaries and Galactic Nuclei: Diagnostics, Demography and Formation. ESO ASTROPHYSICS SYMPOSIA. Springer, Berlin, Heidelberg. https://doi.org/10.1007/10720995_9
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DOI: https://doi.org/10.1007/10720995_9
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