Table 2
Photometry of Nova Del 2013 from other sources.
| Magnitude | Filter | JD |
|
|
||
| 17.58 | POSS-I E | 2 433 835.923 |
| 17.2 | Asiago B | 2 444 016.506 |
| 17.2 | Asiago B | 2 444 436.502 |
| 17.8 | Asiago B | 2 444 526.399 |
| 17.4 | Asiago V | 2 444 812.455 |
| 17.2 | Asiago B | 2 444 840.491 |
| 17.2 | Asiago B | 2 444 854.431 |
| 17.2 | Asiago B | 2 444 901.382 |
| 17.1 | Asiago B | 2 444 925.258 |
| 17.4 | Asiago B | 2 444 931.316 |
| 17.5 | Asiago B | 2 445 148.554 |
| 16.9 | Asiago B | 2 445 166.542 |
| 17.8 | Asiago V | 2 445 263.365 |
| 18.26 | POSS-II BJ | 2 448 091.863 |
| 17.77 | POSS-II RF | 2 448 150.706 |
| 18.49 | POSS-II IN | 2 449 917.867 |
| 16.76† | CMC r′ | 2 452 102 |
| 17.33 ± 0.09 ‡ | APASS B | 2 456 040.833 |
| 17.06 ± 0.10 ‡ | APASS V | 2 456 040.833 |
Notes. The POSS plate photometry is on the Vega scale and comes from the SuperCOSMOS Sky Survey (Hambly et al. 2001b). The Carlsberg Meridian (CMC 2006) point is on the AB scale and the Asiago and APASS measurements are on the Vega scale.
The Carlsberg Meridian catalogue lists the two datapoints for the object as being non-photometric. Additionally the epoch and magnitude are means of the two observations.
The APASS measurements result from Munari & Henden (2013) stacking three observations from the nights of the 21st, 24th and 25th of April 2012. Here we assign APASS observations the mean epoch of these three dates.
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