Cultural advice

The Australian National University acknowledges, celebrates and pays our respects to the Ngunnawal and Ngambri people of the Canberra region and to all First Nations Australians on whose traditional lands we meet and work, and whose cultures are among the oldest continuing cultures in human history.

Aboriginal and Torres Strait Islander peoples are advised that ANU Library collections may include images, names, voices, and other representations of deceased persons.

Material in the collection may contain terms, language or views that reflect the period in which the item was created and may be considered inappropriate today.

A complete set of solutions for caustic crossing binary microlensing events

dc.contributor.authorAlbrow, M. D.en
dc.contributor.authorBeaulieu, J. P.en
dc.contributor.authorCaldwell, J. A.R.en
dc.contributor.authorDepoy, D. L.en
dc.contributor.authorDominik, M.en
dc.contributor.authorGaudi, B. S.en
dc.contributor.authorGould, A.en
dc.contributor.authorGreenhill, J.en
dc.contributor.authorHill, K.en
dc.contributor.authorKane, S.en
dc.contributor.authorMartin, R.en
dc.contributor.authorMenzies, J.en
dc.contributor.authorNaber, R. M.en
dc.contributor.authorPogge, R. W.en
dc.contributor.authorPollard, K. R.en
dc.contributor.authorSackett, P. D.en
dc.contributor.authorSahu, K. C.en
dc.contributor.authorVermaak, P.en
dc.contributor.authorWatson, R.en
dc.contributor.authorWilliams, A.en
dc.date.accessioned2025-12-23T07:40:27Z
dc.date.available2025-12-23T07:40:27Z
dc.date.issued1999-09-10en
dc.description.abstractWe present a method to analyze binary lens microlensing light curves with one well-sampled fold caustic crossing. In general, the surface of χ2 shows extremely complicated behavior over the nine-parameter space that characterizes binary lenses. This makes it difficult to systematically search the space and verify that a given local minimum is a global minimum. We show that for events with well-monitored caustics, the caustic crossing region can be isolated from the rest of the light curve and easily fitted to a five-parameter function. Four of these caustic crossing parameters can then be used to constrain the search in the larger nine-parameter space. This allows a systematic search for all solutions and thus identification of all local minima. We illustrate this technique using the PLANET data for MACHO 98-SMC-1, an excellent and publicly available caustic crossing data set. We show that a very broad range of parameter combinations are compatible with the PLANET data set, demonstrating that observations of binary lens light curves with a sampling of only one caustic crossing do not yield unique solutions. The corollary to this is that the time of the second caustic crossing cannot be reliably predicted on the basis of early data including the first caustic crossing alone. We investigate the requirements for determination of a unique solution and find that occasional observations of the first caustic crossing may be sufficient to derive a complete solution.en
dc.description.statusPeer-revieweden
dc.format.extent15en
dc.identifier.issn0004-637Xen
dc.identifier.otherORCID:/0009-0008-9259-5123/work/190080487en
dc.identifier.scopus0033543433en
dc.identifier.urihttps://hdl.handle.net/1885/733796912
dc.language.isoenen
dc.rights© 1999 The Author(s)en
dc.sourceAstrophysical Journalen
dc.subjectAstrometryen
dc.subjectDark matteren
dc.subjectGravitational lensingen
dc.titleA complete set of solutions for caustic crossing binary microlensing eventsen
dc.typeJournal articleen
dspace.entity.typePublicationen
local.bibliographicCitation.lastpage1036en
local.bibliographicCitation.startpage1022en
local.contributor.affiliationAlbrow, M. D.; University of Canterburyen
local.contributor.affiliationBeaulieu, J. P.; University of Groningenen
local.contributor.affiliationCaldwell, J. A.R.; South African Astronomical Observatoryen
local.contributor.affiliationDepoy, D. L.; Ohio State Universityen
local.contributor.affiliationDominik, M.; University of Groningenen
local.contributor.affiliationGaudi, B. S.; Ohio State Universityen
local.contributor.affiliationGould, A.; Ohio State Universityen
local.contributor.affiliationGreenhill, J.; University of Tasmaniaen
local.contributor.affiliationHill, K.; University of Tasmaniaen
local.contributor.affiliationKane, S.; University of Tasmaniaen
local.contributor.affiliationMartin, R.; Government of Western Australiaen
local.contributor.affiliationMenzies, J.; South African Astronomical Observatoryen
local.contributor.affiliationNaber, R. M.; University of Groningenen
local.contributor.affiliationPogge, R. W.; Ohio State Universityen
local.contributor.affiliationPollard, K. R.; University of Canterburyen
local.contributor.affiliationSackett, P. D.; University of Groningenen
local.contributor.affiliationSahu, K. C.; Space Telescope Science Instituteen
local.contributor.affiliationVermaak, P.; South African Astronomical Observatoryen
local.contributor.affiliationWatson, R.; University of Tasmaniaen
local.contributor.affiliationWilliams, A.; Government of Western Australiaen
local.identifier.citationvolume522en
local.identifier.doi10.1086/307699en
local.identifier.pured1802ad7-470c-4a4c-b3ac-bcc29018dea4en
local.identifier.urlhttps://www.scopus.com/pages/publications/0033543433en
local.type.statusPublisheden

Downloads