A Rapid Microlensing Event in the Q0957+561 A,B Gravitational Lens System
arXiv:astro-ph/0303170 · doi:10.1086/376832
Abstract
We re-analyze brightness data sampled intensively over 5 nights at two epochs separated by the quasar lens time delay, to examine the nature of the observed microlensing. We find strong evidence for a microlensing event with an amplitude of 1% and a time scale of twelve hours. The existence of such rapid microlensing, albeit at low amplitude, imposes constraints on the nature of the quasar and of the baryonic dark matter.
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Cited by in corpus (18)
- Microlensing of the Broad Emission Line Region in the Quadruple Lens SDSS J1004+4112
- Microlensing variability in the gravitationally lensed quasar Q2237+0305 = the Einstein Cross, I. Spectrophotometric monitoring with the VLT
- Observations Supporting the Existence of an Intrinsic Magnetic Moment Inside the Central Compact Object Within the Quasar Q0957+561
- Observational determination of the time delays in gravitational lens system Q2237+030
- A New Microlensing Event in the Doubly-Imaged Quasar Q0957+561
- Anomalous Fluctuations in Observations of Q0957+561 A,B: Smoking Gun of a Cosmic String?
- Microlensing of a Ring Model for Quasar Structure
- Quasar Microlensing: when compact masses mimic smooth matter
- Accretion Disc Structure and Orientation in the Lensed and Microlensed Q0957+561 Quasar
- Gravitational Nanolensing from Subsolar Mass Dark Matter Halos
- GLITP Optical Monitoring of QSO 0957+561: VR Light Curves and Variability
- Revealing the nonlinear behaviour of the lensed quasar Q0957+561
- High-redshift microlensing and the spatial distribution of dark matter in the form of MACHOs
- Q2237+0305 in X-rays: spectra and variability with XMM-Newton
- Do the Herschel cold clouds in the Galactic halo embody its dark matter?
- The Mass Function of Primordial Rogue Planet MACHOs in quasar nanolensing
- Primordial Planet Formation
- A partially occulting MACHO-microlensing event in the Twin Quasar Q0957+561