All Tables

Table 1: Comparison of coordinates, and number of positional matches, before and after a correction was applied.
Table 2: First entries in the electronically available table, which lists: OGLE-field, OGLE-name, the three fitted periods with errors and amplitude (0.00 means no fit), mean $I_{\rm ogle}$ , and associated DENIS IJK photometry with errors, and associated 2MASS JHK photometry with errors (99.9 and 9.99 means no association, or no value).
Table 3: First entries in the electronically available table, which list: OGLE-field, OGLE-name, other names, spectral type and references and comments.
Table 4: Definition of the boundary lines of the sequences in the K-band PL-diagram in Fig. 3. Relations are of the form $K_{\rm min,max}= {\rm slope_{min,max}} \log P + {\rm zp_{min,max}}$ , with K the dereddened magnitude on the 2MASS system.
Table 5: Theoretical colours of M- and C-stars of solar metallicity. For some models, the second line indicates the colours when the star is obscured by circumstellar dust equivalent to a dimming in K by 0.05 mag.
Table 6: First entries in the electronically available table, which list: OGLE-field, OGLE-name, other names, periods (respectively the historical period-in the majority of cases from the Hughes list or WBP-then the present-day period from OGLE and finally other available periods with reference between parentheses), spectral type and references and comments on period changes.
Table 7: The infrared selected sample. As Table 2.
Table 8: The infrared selected sample. As Table 3.
Table 9: K-band PL-relations in box "C'', of the form $m_{\rm K}= a \log P + b$ .