Table 3
Flux ratios of the HE0435-1223 components measured at several epochs (compiled from the literature).
| Date | HJDa range | Band | A / B | C / B | D / B | References |
|
|
||||||
| 2003 Aug. | 2870 | V | 1.70 ± 0.22 | 0.93 ± 0.08 | 0.88 ± 0.12 | 1 |
| 2003 Aug. | 2870 | I | 1.67 ± 0.11 | 0.99 ± 0.04 | 0.81 ± 0.06 | 1 |
| 2004 Jan. | 3013-3036 | R | 1.73 ± 0.05 | 1.02 ± 0.02 | 0.88 ± 0.02 | 2 |
| 2004 Jan. | 3015 | H | 1.57 ± 0.10 | 1.00 ± 0.03 | 0.79 ± 0.05 | 1 |
| 2007 Sep. | 4366 | J | 1.58 ± 0.09 | 1.01 ± 0.08 | 0.84 ± 0.06 | 3 |
| 2007 Sep. | 4366 | H | 1.54 ± 0.08 | 1.03 ± 0.08 | 0.83 ± 0.06 | 3 |
| 2007 Sep. | 4366 | K | 1.42 ± 0.03 | 1.02 ± 0.04 | 0.79 ± 0.03 | 3 |
| 2007 Oct. | 4316-4340 | R | 2.16 ± 0.04 | 1.10 ± 0.02 | 0.91 ± 0.02 | 2 |
| 2008 Jul.-Oct. | 4675-4744 | V | 1.58 ± 0.08 | 1.06 ± 0.06 | 0.85 ± 0.05 | 4 |
| 2008 Jul.-Oct. | 4675-4744 | R | 1.56 ± 0.05 | 1.06 ± 0.05 | 0.84 ± 0.04 | 4 |
| 2008 Jul.-Oct. | 4674-4766 | R | 1.66 ± 0.04 | 1.10 ± 0.03 | 0.86 ± 0.02 | 2 |
| 2008 Jul.-Oct. | 4675-4744 | I | 1.51 ± 0.08 | 1.06 ± 0.06 | 0.82 ± 0.04 | 4 |
| 2008 Aug.-Dec. | 4682-4829 | R | 1.63 ± 0.05 | 1.09 ± 0.03 | 0.86 ± 0.02 | 2 |
| 2008 Aug. | 4709 | K | 1.45 ± 0.18 | 0.79 ± 0.04 | 0.67 ± 0.07 | 5 |
| 2008 Dec. | 4822 | L ′ | 1.72 ± 0.23 | 1.01 ± 0.08 | 0.82 ± 0.16 | 5 |
| 2009 Aug.-Sep. | 5064-5094 | V | 1.41 ± 0.04 | 1.03 ± 0.02 | 0.82 ± 0.02 | 4 |
| 2009 Aug.-Sep. | 5064-5094 | R | 1.43 ± 0.05 | 1.05 ± 0.03 | 0.81 ± 0.03 | 4 |
| 2009 Aug.-Sep. | 5047-5099 | R | 1.53 ± 0.03 | 1.08 ± 0.03 | 0.82 ± 0.02 | 2 |
| 2009 Aug.-Sep. | 5064-5094 | I | 1.45 ± 0.05 | 1.05 ± 0.03 | 0.79 ± 0.03 | 4 |
| 2009 Oct.-Dec. | 5111-5176 | R | 1.53 ± 0.05 | 1.07 ± 0.04 | 0.80 ± 0.03 | 2 |
| 2009 Oct.-Dec. | 5123,5174,5175,5180 | H | 1.43 ± 0.03 | 1.02 ± 0.03 | 0.72 ± 0.02 | 6 |
Notes.
Reference. (1) Kochanek et al. (2006); (2) Courbin et al. (2011); (3) Blackburne et al. (2011); (4) Ricci et al. (2011); (5) Fadely & Keeton (2011); (6) This work: the photometric flux ratios were computed by multiplying the spectrum of each quasar image by the transmission of the H-band filter and then integrating the flux.
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