Beware the Nonuniqueness of Einstein Rings
Author(s) -
Prasenjit Saha,
Liliya L. R. Williams
Publication year - 2001
Publication title -
the astronomical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.61
H-Index - 271
eISSN - 1538-3881
pISSN - 0004-6256
DOI - 10.1086/321151
Subject(s) - einstein ring , qsos , galaxy , einstein , simple (philosophy) , plot (graphics) , ring (chemistry) , physics , graphics , lens (geology) , contour line , astrophysics , computer graphics (images) , gravitational lens , computer science , mathematics , mathematical physics , optics , philosophy , quasar , redshift , statistics , chemistry , epistemology , organic chemistry , meteorology
We explain how an approximation to the rings formed by the host galaxies inlensed QSOs can be inferred from the QSO data alone. A simple ring image can bemade from any lens model by a simple piece of computer graphics: just plot acontour map of the arrival-time surface with closely-spaced contours. We go onto explain that rings should be (a) sensitive to time-delay ratios betweendifferent pairs of images, but (b) very insensitive to H_0. We illustrate thisfor the well-known quads 1115+080 and 1608+656.Comment: To appear in AJ (circa Aug 2001
Accelerating Research
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom
Address
John Eccles HouseRobert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom