Separating intrinsic and microlensing variability using parallax measurements
| dc.creator | Haugan, S. V. H. | |
| dc.date | 1995-08-24 | |
| dc.date.accessioned | 2026-07-07T02:20:03Z | |
| dc.date.available | 2026-07-07T02:20:03Z | |
| dc.description | In gravitational lens systems with 3 or more resolved images of a quasar, the intrinsic variability may be unambiguously separated from the microlensing variability through parallax measurements from 3 observers when there is no relative motion of the lens masses (Refsdal 1993). In systems with fewer than 3 resolved images, however, this separation is not straightforward. A general approach that may be used for this purpose is presented. For simplicity, only the one-dimensional case is considered in detail: Given a well-sampled time series of the observed flux at two points in space with a known separation, choosing a velocity $v_{\perp}$ of the observers perpendicular to the line of sight determines the microlensing magnification history, and thereby also the intrinsic variability. The velocity is chosen by minimizing some measure ($χ^2$) of the residual intrinsic variability. In many cases this gives a close approximation to the true magnification. In cases where the relative motion of the lensing point masses is important, only a partial separation will be possible. | |
| dc.description | 2 pages LaTeX, no figures. Uses crckapb.sty. To appear in the Proceedings of the IAU Symposium 173: ``Astrophysical Applications of Gravitational Lensing'', Kluwer Academic Publishers, Eds.: C. S. Kochanek and J. N. Hewitt. Also available, with additional information, through http://www.uio.no/~steinhh/index.html | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9508112 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9508112 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/10097 | |
| dc.subject | Astrophysics | |
| dc.title | Separating intrinsic and microlensing variability using parallax measurements | |
| dc.type | text |