...¹

Visiting Astronomer, German-Spanish Astronomical Center, Calar Alto, operated by the Max-Planck-Institut für Astronomie jointly with the Spanish National Commission for Astronomy.

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...luminosity

The R band data from the 2.2 m telescope yielded very similar results: The profile is detected out to about 55$^{\prime\prime}$, is flat in the center, and shows an exponential distribution law with a scale length of 16 $\pm$ 1.2$^{\prime\prime}$.

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...HREF="/articles/aas/full/1999/02/ds1591/node3.html#tab3">3

An upper flux limit had been set when running DAOPHOT to avoid saturated stars. Therefore, the brightest stars visible in Fig. 1 cannot be found in Table 3, but they are Milky Way objects anyway.

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...0.1

A formation time of $z_{\rm f} = 4$, h = 0.6, and q₀ = 0.1 are assumed; B-J is not used because of some uncertainties of the NIR model colors.

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