Free Access

Table 6

Median value of the model parameters and 68% confidence interval of the 11 newly deconvolved quads.

Object Model R Ein e θ e R eff γ θ γ

(a) JVAS B0218+357 SIS+γ / / /
SIE+γ /
DV+ㆆ
ExpD + γ 0.182

(b) SBS 0909+532 SIS+γ / / /
SIE+γ /
DV+γ

(c) RX J0911.4+0551 SIE+γ /
DV+γ

(d) FBQS J0951+2635 SIS+γ / / /
SIE+γ /
DV+γ

(e) HE 1104-1805 SIS+γ / / /
SIE+γ /
DV+γ

(f) PG 1115+080 SIE+γ /
DV+γ

(g) B1422+231 SIE+γ /
DV+γ

(h) SBS 1520+530 SIS+γ / / /
SIE+γ /
DV+γ

(i) CLASS B1600+434 SIS+γ / / /
SIE+γ /
DV+ㆆ
ExpD + γ 0.673

(j) CLASS B1608+656 SIE+γ /
DV+γ

(k) HE 2149-2745 SIS+γ / / /
SIE+γ /
DV+γ

Notes.

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 Tab. 3 using exponential light distribution.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.