Issue |
A&A
Volume 593, September 2016
|
|
---|---|---|
Article Number | C2 | |
Number of page(s) | 2 | |
Section | Cosmology (including clusters of galaxies) | |
DOI | https://doi.org/10.1051/0004-6361/201526773e | |
Published online | 31 August 2016 |
The elliptical power law profile lens (Corrigendum)
1 Jodrell Bank Centre for Astrophysics,
University of Manchester, Alan Turing
Building, Oxford Road, Manchester, M13
9PL, UK
e-mail: nicolas.tessore@manchester.ac.uk
2 Department of Physics and Astronomy,
Università di Bologna, viale Berti
Pichat 6/2, 40127
Bologna,
Italy
e-mail: robertbenton.metcalf@unibo.it
Key words: gravitational lensing: strong / methods: analytical / errata, addenda
The authors would like to point out two errors in the article as it was originally published.
Due to a typographical error, Eq. (17) erroneously expresses the shear of the elliptical power law profile lens in the elliptic coordinates R and ϕ instead of the physical polar coordinates r and θ. The correct expression is
(17)
i.e. the same formula with the substitutions R → r and ϕ → θ. This result correctly recovers the singular isothermal ellipsoid result γ = − κ (z/z⋆) = − ei2θκ when t = 1. The preceding Eq. (16) is correct.
Furthermore, Fig. 2 incorrectly contains and refers to the pseudo-caustics for power law profile lenses with slope t> 1. Since the main result of the original paper shows that the elliptical lenses have the same (elliptical) radial profile as the circular ones, the degenerate critical line at the origin R = 0 is mapped to R = ∞ when t> 1, just as in the circular case. Hence only the isothermal case t = 1 has a pseudo-caustic at finite radius. The dashed lines in the plot are due to a numerical error. A corrected version of Fig. 2 is shown below.
![]() |
Fig. 2 Critical lines (black) and caustics (grey) of the elliptical power law profile lens. Also shown is an ellipse with semi-minor axis equal to the scale length b and axis ratio q (red, dotted). For the purpose of illustration, the scale length b decreases as q1/2. The slope of the power law profile varies from t = 0.25 (left) to t = 1.75 (right) in steps of 0.5. The axis ratio varies from q = 0.8 (top) to q = 0.2 (bottom) in steps of 0.2. |
Acknowledgments
The authors thank Yiping Shu and Massimo Meneghetti for their careful reading of the original article.
© ESO 2016
All Figures
![]() |
Fig. 2 Critical lines (black) and caustics (grey) of the elliptical power law profile lens. Also shown is an ellipse with semi-minor axis equal to the scale length b and axis ratio q (red, dotted). For the purpose of illustration, the scale length b decreases as q1/2. The slope of the power law profile varies from t = 0.25 (left) to t = 1.75 (right) in steps of 0.5. The axis ratio varies from q = 0.8 (top) to q = 0.2 (bottom) in steps of 0.2. |
In the text |
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