Zackrisson, E., T. Riehm, O. Möller, K. Wiik and P. Nurmi: Strong lensing by subhalos in the dwarf galaxy mass range - I. Image separations. In: The Astrophysical Journal 684, 2, 804-810 (2008).
doi: 10.1086/590541
Zackrisson, E., T. Riehm, H. Lietzen, O. Möller, K. Wiik and P. Nurmi: The detectability of dark galaxies through image-splitting effects. In: Dark Galaxies and Lost Baryons, (Eds.) J.I. Davies, M.J. Disney. IAU Symposium and Colloquium Proceedings Series IAU Symposium 244. Cambridge University Press, Cambridge, UK (2008) 397-398.
localid: Reihe: IAU...., 244 p.397-398
doi: 10.1017/S1743921307014457
Riehm, T., E. Zackrisson, K. Wiik and O. Möller: On the probability for sub-halo detection through quasar image splitting. In: Dark Galaxies and Lost Baryons, (Eds.) J.I. Davies, M.J. Disney. IAU Symposium and Colloquium Proceedings Series IAU Symposium 244. Cambridge University Press, Cambridge, UK (2008) 376-377.
localid: Reihe: IAU...., 244 p.376-377
doi: 10.1017/S1743921307014354
Nilsson, K. K., P. Møller, O. Möller, J. P. U. Fynbo, M. J. Michaloswski, D. Watson, C. Ledoux, P. Rosati, K. Pedersen and L. F. Grove: A multi-wavelength study of z = 3.15 Lyman-α emitters in the GOODS south field. In: Astronomy & Astrophysics 471, 1, 71-82 (2007).
doi: 10.1051/0004-6361:20066949
Elíasdóttir, Á. and O. Möller: A comparison of the strong lensing properties of the Sérsic and the Navarro, Frenk and White profiles. In: Journal of Cosmology and Astroparticle Physics, 7, Seq. No.: 006 (2007).
doi: 10.1088/1475-7516/2007/07/006
localid: 322227
Sandvik, H. B., O. Moeller, J. Lee and S. D. M. White: Why does the clustering of haloes depend on their formation history?. In: Monthly Notices of the Royal Astronomical Society 377, 1, 234-244 (2007).
doi: 10.1111/j.1365-2966.2007.11595.x
Möller, O., M. Kitzbichler, V. R. Eke and P. Natarajan: Lensing by groups. In: Groups of Galaxies in the Nearby Universe, (Eds.) I. Saviane, V.D. Ivanov, J. Borissova. ESO Astrophysics Symposia. Springer, Berlin [u.a.] (2007) 233-237.
localid: AS 80/220, p.233-237
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