All Tables

• Table 1: Number of images taken during the AGAPE observations.
• Table 2: Variable stars with period estimate. Shortest period objects are population II Cepheid-like objects; longest period objects are LPVs.
• Table 3: Extraction of the catalogue of the AGAPE variable stars showing the first and last star for each field and the 12 novae candidates (more information are given in the text). L is the likelihood function. The nova number is added (with respect to CDS catalog) in the last column; more information on the columns is given in Sect. 4.1.
• Table 4: Characteristics of the 12 novae candidates named as NOVn (first column) where n goes from 01 to 12.