Table 2
Lists of the analysed nights per season from the 11-year WeCAPP campaign.
Season | R-band | I-band | ||||||
F1 | F2 | F3 | F4 | F1 | F2 | F3 | F4 | |
|
||||||||
1997–1998 | 36 | 7 | 1 | 4 | 33 | 7 | 0 | 3 |
1998–1999 | 33 | 1 | 1 | 1 | 28 | 1 | 1 | 1 |
1999–2000 | 154 | 0 | 0 | 0 | 145 | 0 | 0 | 0 |
2000–2001 | 184 | 108 | 124 | 108 | 159 | 89 | 104 | 89 |
2001–2002 | 240 | 136 | 159 | 136 | 212 | 119 | 140 | 119 |
2002–2003 | 34 | 18 | 24 | 18 | 30 | 16 | 24 | 18 |
2003–2004 | 35 | 24 | 29 | 31 | 33 | 21 | 26 | 29 |
2004–2005 | 25 | 23 | 26 | 25 | 19 | 16 | 19 | 19 |
2005–2006 | 30 | 26 | 28 | 29 | 26 | 20 | 22 | 23 |
2006–2007 | 107 | 106 | 103 | 103 | 48 | 45 | 46 | 47 |
2007–2008 | 62 | 56 | 52 | 58 | 36 | 35 | 35 | 38 |
|
||||||||
Total | 940 | 505 | 547 | 513 | 769 | 369 | 417 | 386 |
Notes. Each season starts from the 1 May until the 30 April in the next year. The WeCAPP campaigns began in 1997 focusing on F1 with the Wendelstein Observatory. From 1999 until 2002 we extended our observations by including the Calar Alto Observatory, which boosted the number of images taken in these seasons. From 2002 on, we use the Wendelstein Observatory solely and mosaic the full Calar Alto FOV with four pointings.
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