Pictures of gravitational lensing (p. 3) |
by Nityananda, R |
Determination of cosmological parameters by the gravitational lens effect (p. 13) |
by Refsdal, S |
Cosmic gravitational diagnostics (p. 16) |
by Kovner, I |
Gravitational redshifts and lensing by large scale structures (p. 29) |
by Nottale, L |
What the present observed lens systems tells about the lensing agent (p. 39) |
by Narasimha, D |
Gravitational lens models with elliptical geometry (p. 46) |
by Schramm, T |
Amplification near a gravitational lens macro-caustic (p. 49) |
by Kunze, W D |
Statistics of lensing on extended sources (p. 51) |
by Marchandon, S |
Observational aspects of gravitational lensing (p. 57) |
by Surdej, J |
A search for gravitational lensing among highly luminous quasars: observationsl strategy and survey (p. 83) |
by Swings, J P |
A search for gravitational lensing among highly luminous quasars: new results (p. 88) |
by Magain, P |
Gravitational magnification effects on distant 3CR galaxies (p. 93) |
by Lefèvre, O |
0957+561: the time delay revisited (p. 96) |
by Falco, E E |
The time delay of Q0957+561 A, B from 10 years of optical monitoring (p. 102) |
by Schild, R |
Application of image processing techniques in a search for gravitational lenses and quasar pairs (p. 108) |
by Djorgovski, S |
A search for gravitational lenses and quasar pairs and the discovery of a new multiple QSO system (p. 111) |
by Meylan, G |
Evolution and gravitational lensing in quasar absorption line systems (p. 117) |
by Thomas, P A |
Preliminary analysis of high-resolution spectra for UM 673 A&B (p. 122) |
by Smette, A |
Bidimensional spectrography of the âワClover leafâ H1413+117 at sub-arcsec: Spatial resolution (p. 124) |
by Angonin, M C |
The MIT search program for gravitational lenses (p. 127) |
by Burke, Bernard F |
First epoch VLBI observations of the gravitational lens system 2016+112 (p. 136) |
by Heflin, M B |
X-ray observations of gravitational lenses (p. 141) |
by Kellog, E |
Consequences of gravitational lensing for gamma radiation from 3C273 (p. 163) |
by Metcalfe, L |
Searching for cosmic strings (A la recherché des cordes perdues) (p. 166) |
by Hindmarsh, M |
Microlensing (p. 175) |
by Schneider, P |
Microlensing calculations with hierarchical tree code: new results (p. 186) |
by Wambsganss, J |
Statistical investigations of the amplification near gravitational lens caustics (p. 192) |
by Witt, H J |
The deconvolution of the quasar structure from the lightcurve of a high amplification event with the regularization method (p. 198) |
by Grieger, B |
The Hamburg quasar monitoring program at Calar Alto: analyses of micro-lensing variability (p. 203) |
by Borgeest, U |
Photometric monitoring of 2237+0305 (p. 206) |
by Corrigan, R T |
Spectrophotometry of 0957+561 and the micro-lensing effect (p. 210) |
by Vanderriest, C |
IR imaging and the light curve of 2237+030 (p. 216) |
by Nadeau, D |
Clusters of galaxies: A new observable class of gravitational lenses (p. 221) |
by Fort, B |
Lensing the background population of galaxies (p. 230) |
by Tyson, J A |
The redshift distribution of faint galaxies - implications for gravitational lensing (p. 236) |
by Ellis, Richard S |
The theory and practice of radio ring lenses (p. 244) |
by Kochanek, C S |
Lens and source models for arcs in cluster Abell 370 and CL 2244 (p. 254) |
by Petrosyan, V |
Modeling the giant arcs in A370 and A2390 (p. 261) |
by Mellier, Y |
New results from the gravitational telescope (p. 271) |
by Hammer, F |
Probing rich galaxy clusters with mini-arcs (p. 275) |
by Grossman, S A |
Gravitationally lensed arcs as galaxy redshift indicators (p. 280) |
by Nemiroff, R J |
Spatial correlation in gravitationally lensed images (p. 284) |
by Deguchi, S |
Optical-infrared studies of arcs in Abell 370 (p. 288) |
by Aragón-Salamanca, A |
Spectroscopy of arcs in CI 2244-02 and A370 (A5) (p. 291) |
by Soucail, G |
First results on the spectroscopy of the arc-like object in Abell 2390 (p. 293) |
by Pellò, R |
Deep photometry of CI.2244-02 in U colour with an electronographic camera (p. 295) |
by Wlerik, G |
Concluding remarks (p. 301) |
by Blandford, R D |