scholarly journals Dust and Extinction Curves in Galaxies with \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $z> 0$ \end{document} : The Interstellar Medium of Gravitational Lens Galaxies

1999 ◽  
Vol 523 (2) ◽  
pp. 617-632 ◽  
Author(s):  
E. E. Falco ◽  
C. D. Impey ◽  
C. S. Kochanek ◽  
J. Lehar ◽  
B. A. McLeod ◽  
...  
2006 ◽  
Vol 20 ◽  
pp. 289-290
Author(s):  
I. Momcheva ◽  
K. Williams ◽  
C. Keeton ◽  
A. Zabludoff

2018 ◽  
Vol 867 (2) ◽  
pp. 107 ◽  
Author(s):  
Kenneth C. Wong ◽  
Alessandro Sonnenfeld ◽  
James H. H. Chan ◽  
Cristian E. Rusu ◽  
Masayuki Tanaka ◽  
...  

2006 ◽  
Vol 642 (1) ◽  
pp. 22-29 ◽  
Author(s):  
Jaiyul Yoo ◽  
Christopher S. Kochanek ◽  
Emilio E. Falco ◽  
Brian A. McLeod

2009 ◽  
Vol 5 (H15) ◽  
pp. 77-77
Author(s):  
V. Motta ◽  
E. Mediavilla ◽  
E. E. Falco ◽  
J. A. Muñoz

Simple gravitational lens models usually suffice to reproduce the positions of lensed quasar images, but they have problems to reproduce their optical flux ratios. The so-called flux ratio anomalies are thought to be produced by small-scale structure in the lens galaxies (microlensing).


2006 ◽  
Vol 641 (1) ◽  
pp. 169-189 ◽  
Author(s):  
Ivelina Momcheva ◽  
Kurtis Williams ◽  
Charles Keeton ◽  
Ann Zabludoff

2013 ◽  
Vol 436 (3) ◽  
pp. 2120-2126 ◽  
Author(s):  
A. M. Nierenberg ◽  
D. Oldenburg ◽  
T. Treu

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