Table 5
Results of the parametric modeling of the 11 newly deconvolved quads.
Object | Model | R Ein | e, θ e | R eff | γ, θ γ | Flux ratios | d.o.f. | χ 2 | Time delays |
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(a) JVAS B0218+357† | SIS+γ | 0.151 | / | / | 0.096, –28.87 | fB/fA = 1.707 | 0 | 0.0 | ΔtAB= 4.9 |
SIE+γ | 0.152 | (0.04, –73.56) | / | 0.093, –25.26 | fB/fA= 1.702 | 0 | 0.0 | ΔtAB= 4.8 | |
DV+ㆆ | 0.150 | (0.04, –73.60) | (0.31) | 0.125, –26.28 | fB/fA= 1.707 | 0 | 0.0 | ΔtAB= 6.0 | |
ExpD+γ | 0.182 | (0.04, –73.60) | (0.31) | 0.011, 21.86 | fB/fA= 1.707 | 0 | 0.0 | ΔtAB= 1.9 | |
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(b) SBS 0909+532 | SIS+γ | 0.557 | / | / | 0.066, 54.72 | fB/fA= 0.885 | 0 | 0.0 | ΔtAB= –29.2 |
SIE+γ | 0.548 | (0.11, –48.05) | / | 0.101, 49.96 | fB/fA= 0.885 | 0 | 0.0 | ΔtAB= –27.2 | |
DV+γ | 0.543 | (0.11, –48.12) | (0.54) | 0.125, 50.18 | fB/fA= 0.885 | 0 | 0.0 | ΔtAB = –39.2 | |
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(c) RX J0911.4+0551 | SIE+γ | 1.086 | 0.24, (-72.00) | / | 0.327, 9.39 | fA2/fA1= 1.872 | 1 | 0.4 | ΔtA1B= –148.9 |
0.225 | / | / | / | fA3/fA1= 0.881 |
![]() |
ΔtA2B= –147.9 | |||
/ | / | / | fB/fA1 = 0.341 | ![]() |
ΔtA3B= –149.5 | ||||
DV+γ | 1.085 | (0.16, –65.47) | (1.03) | 0.380, 8.06 | fA2/fA1= 1.921 | 2 | 112.7 | ΔtA1B = –213.2 | |
0.255 | / | / | / | fA3/fA1= 0.888 | ![]() |
ΔtA2B= –211.9 | |||
/ | / | / | fB/fA1= 0.476 |
![]() |
ΔtA3B= –214.2 | ||||
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(d) FBQS J0951+2635 | SIS+γ | 0.541 | / | / | 0.098, 0.18 | fB/fA= 0.283 | 0 | 0.0 | ΔtAB = 13.8 |
SIE+γ | 0.583 | (0.47, 12.80) | / | 0.133, –66.57 | fB/fA= 0.283 | 0 | 0.0 | ΔtAB = 16.5 | |
DV+γ | 0.526 | (0.47, 12.81) | (0.78) | 0.017, –33.02 | fB/fA= 0.283 | 0 | 0.0 | ΔtAB = 20.8 | |
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(e) HE 1104-1805 | SIS+γ | 1.382 | / | / | 0.136, 22.44 | fB/fA= 0.259 | 0 | 0.0 | ΔtAB= –185.2 |
SIE+γ | 1.405 | (0.14, 54.71) | / | 0.120, 12.96 | fB/fA= 0.259 | 0 | 0.0 | ΔtAB= –189.9 | |
DV+γ | 1.359 | (0.14, 54.70) | (0.98) | 0.201, 19.50 | fB/fA= 0.259 | 0 | 0.0 | ΔtAB= –268.9 | |
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(f) PG 1115+080 | SIE+γ | 1.141 | 0.14, (–67.59) | / | 0.125, 53.80 | fC/fA1= 0.271 | 2 | 29.9 | ΔtCA1= 10.4 |
/ | / | / | fA2/fA1= 0.926 |
![]() |
ΔtCA2= 10.5 | ||||
/ | / | / | fB/fA1= 0.218 |
![]() |
ΔtCB= 17.0 | ||||
DV+γ | 1.137 | (0.14, –67.59) | (0.92) | 0.178, 59.91 | fC/fA1= 0.294 | 3 | 152.7 | ΔtCA1= 15.7 | |
/ | / | / | fA2/fA1= 0.908 |
![]() |
ΔtCA2= 15.9 | ||||
/ | / | / | fB/fA1= 0.203 |
![]() |
ΔtCB= 26.1 | ||||
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(g) JVAS B1422+231 | SIE+γ | 0.771 | 0.27, (–57.45) | / | 0.177, –52.25 | fB/fA= 1.270 | 2 | 10.0 | ΔtAC= –0.7 |
/ | / | / | fC/fA= 0.641 |
![]() |
ΔtBC= –0.9 | ||||
/ | / | / | fD/fA= 0.048 |
![]() |
ΔtDC= –24.6 | ||||
DV+γ | 0.722 | (0.47, –55.80) | (0.49) | 0.375, –53.63 | fB/fA= 1.045 | 3 | 110.5 | ΔtAC= –1.3 | |
/ | / | / | fC/fA= 0.674 |
![]() |
ΔtBC= –1.7 | ||||
/ | / | / | fD/fA= 0.029 |
![]() |
ΔtDC= –39.7 | ||||
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(h) SBS 1520+530 | SIS+γ | 0.745 | / | / | 0.128, –1.56 | fB/fA= 0.471 | 0 | 0.0 | ΔtAB= 93.6 |
SIE+γ | 0.732 | (0.49, –26.50) | / | 0.144, 43.33 | fB/fA= 0.471 | 0 | 0.0 | ΔtAB= 95.9 | |
DV+γ | 0.644 | (0.49, –26.50) | (0.76) | 0.229, 21.80 | fB/fA= 0.471 | 0 | 0.0 | ΔtAB= 122.3 | |
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(i) CLASS B1600+434 | SIS+γ | 0.613 | / | / | 0.143, 46.80 | fB/fA= 0.897 | 0 | 0.0 | ΔtAB = 27.6 |
SIE+γ | 0.721 | (0.75, 36.90) | / | 0.265, –54.85 | fB/fA= 0.897 | 0 | 0.0 | Δt = 39.5 | |
DV+ㆆ | 0.579 | (0.75, 36.90) | (0.29) | 0.175, 58.36 | fB/fA= 0.897 | 0 | 0.0 | ΔtAB= 44.6 | |
ExpD+γ | 0.673 | (0.75, 36.90) | (0.29) | 0.086, –78.89 | fB/fA= 0.897 | 0 | 0.0 | ΔtAB= 44.6 | |
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(j) CLASS B1608+656 | SIE+γ | 1.124 | 0.80, (72.89) | / | 0.195, –7.76 | fA/fB = 2.009 | 1 | 7.4 | ΔtAB= –48.1 |
0.113 | / | / | / | fC/fB= 0.974 |
![]() |
ΔtCB= –53.9 | |||
/ | / | / | fD/fB= 0.190 | ![]() |
ΔtDB= –115.8 | ||||
DV+γ | 1.072 | (0.59, 78.73) | (1.51) | 0.102, 48.51 | fA/fB= 1.768 | 2 | 595.0 | ΔtAB= –27.7 | |
0.357 | / | / | / | fC/fB= 1.389 |
![]() |
ΔtCB= –32.1 | |||
/ | / | / | fC/fB= 0.213 |
![]() |
ΔtDB= –102.0 | ||||
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(k) HE2149-2745 | SIS+γ | 0.858 | / | / | 0.016, 8.30 | fB/fA= 0.234 | 0 | 0.0 | ΔtAB= 93.7 |
SIE+γ | 0.834 | (0.21, 9.80) | / | 0.063, –80.35 | fB/fA= 0.234 | 0 | 0.0 | ΔtAB= 88.6 | |
DV+γ | 0.784 | (0.21, 9.79) | (1.10) | 0.076, –69.73 | fB/fA= 0.234 | 0 | 0.0 | ΔtAB= 116.8 |
Notes. Quantities which are results of the modeling (i.e. not explicit model parameters) are displayed in italic and parameters which are fitted to their observed values are displayed into parentheses. Note that flux ratios are used to constrain the lens model only for doubles.
The models of this lensed quasar might be affected by strong systematic errors owing to the large uncertainty on the exact location of the lens from the NICMOS data.
An exponential profile better reproduces the light distribution of the spiral lens galaxy and therefore the ExpD mass model should be prefered to the DV mass model. The Reff used for our DV mass model is the effective radius derived in Table 3 using exponential light distribution.
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