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相关论文: A Ubiquitous Unifying Degeneracy in Two-Body Micro…

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We inspect 4 microlensing events KMT-2021-BLG-1968, KMT-2021-BLG-2010, KMT-2022-BLG-0371, and KMT-2022-BLG-1013, for which the light curves exhibit partially covered short-term central anomalies. We conduct detailed analyses of the events…

By considering linear-order departures from general relativity, we compute a novel expression for the weak lensing convergence power spectrum under alternative theories of gravity. This comprises an integral over a 'kernel' of general…

宇宙学与河外天体物理 · 物理学 2015-04-22 C. Danielle Leonard , Tessa Baker , Pedro G. Ferreira

The light curve of the microlensing event KMT-2021-BLG-1898 exhibits a short-term central anomaly with double-bump features that cannot be explained by the usual binary-lens or binary-source interpretations. With the aim of interpreting the…

Gravitational lensing offers unique opportunities to learn about the astrophysical origin of distant sources, the abundance of intervening objects acting as lenses, and gravity and cosmology in general. However, all this information can…

宇宙学与河外天体物理 · 物理学 2024-11-20 Anson Chen , Paolo Cremonese , Jose María Ezquiaga , David Keitel

The light curve of the microlensing event KMT-2021-BLG-0240 exhibits a short-lasting anomaly with complex features near the peak at the 0.1~mag level from a single-lens single-source model. We conducted modeling of the lensing light curve…

The microlens parallax is a crucial observable for conclusively identifying the nature of lens systems in microlensing events containing or composed of faint (even dark) astronomical objects such as planets, neutron stars, brown dwarfs, and…

We investigate the properties of microlensing events caused by planetary systems where planets with a moon are widely separated from their host stars. From this investigation, we find that the moon feature generally appears as an very…

地球与行星天体物理 · 物理学 2016-08-03 Sun-Ju Chung , Yoon-Hyun Ryu

Weak gravitational lensing is considered to be one of the most powerful tools to study the mass and the mass distribution of galaxy clusters. However, the mass-sheet degeneracy transformation has limited its success. We present a novel…

天体物理学 · 物理学 2007-05-23 M. Bradac , P. Schneider , M. Lombardi , T. Erben

We study the local behavior of gravitational lensing near fold catastrophes. Using a generic form for the lensing map near a fold, we determine the observable properties of the lensed images, focusing on the case when the individual images…

天体物理学 · 物理学 2009-11-07 B. Scott Gaudi , A. O. Petters

Microlensing is able to reveal multiple body systems located several kilo-parsec away from the Earth. Since it does not require the measurement of light from the lens, microlensing is sensitive to a range of objects from free-floating…

地球与行星天体物理 · 物理学 2018-10-17 E. Bachelet , J. -P. Beaulieu , I. Boisse , A. Santerne , R. A. Street

Clusters of galaxies are the most recently assembled, massive, bound structures in the Universe. As predicted by General Relativity, given their masses, clusters strongly deform space-time in their vicinity. Clusters act as some of the most…

宇宙学与河外天体物理 · 物理学 2012-02-06 Jean-Paul Kneib , Priyamvada Natarajan

Gravitational lensing offers a competitive method to measure $H_0$ with the goal of 1% precision. A major obstacle comes in the form of lensing degeneracies, such as the mass sheet degeneracy (MSD), which make it possible for a family of…

宇宙学与河外天体物理 · 物理学 2020-12-01 Matthew R. Gomer , Liliya L. R. Williams

We reexamine the usefulness of fitting blended lightcurve models to microlensing photometric data. We find agreement with previous workers (e.g. Wozniak & Paczynski) that this is a difficult proposition because of the degeneracy of blend…

天体物理学 · 物理学 2009-11-13 Christian L. Thomas , Kim Griest

We investigate a driven particle system, a multilane asymmetric exclusion process, where the particle number in every lane is conserved, and stationary state is fully uncorrelated. The phase space has, starting from three lanes and more, an…

统计力学 · 物理学 2026-03-24 Johannes Schmidt , Žiga Krajnik , Vladislav Popkov

The two outer triangular caustics (regions of infinite magnification) of a close binary microlens move much faster than the components of the binary themselves, and can even exceed the speed of light. When $\epsilon > 1$, where $\epsilon c$…

天体物理学 · 物理学 2009-10-31 Zheng Zheng , Andrew Gould

We undertake the first study of two-planet microlensing models recovered from simulations of microlensing events generated by realistic multi-planet systems in which 292 planetary events including 16 two-planet events were detected from…

地球与行星天体物理 · 物理学 2015-06-22 Wei Zhu , Andrew Gould , Matthew Penny , Shude Mao , Rieul Gendron

The homogeneous spectral linewidth associated with light-matter interactions is a fundamental descriptor of the optical properties of materials, governed by the quantum dynamics of the condensed-matter system. We discuss here that the…

化学物理 · 物理学 2026-05-13 Simón Paiva-Ortega , Hao Li , Eric R. Bittner , Carlos Silva-Acuña

Cosmological parameter constraints from observations of time-delay lenses are becoming increasingly precise. However, there may be significant bias and scatter in these measurements due to, among other things, the so-called mass-sheet…

宇宙学与河外天体物理 · 物理学 2017-12-27 Amitpal S. Tagore , David J. Barnes , Neal Jackson , Scott T. Kay , Matthieu Schaller , Joop Schaye , Tom Theuns

MACHO-97-BLG-41 is a gravitational microlensing event produced by a lens composed of multiple masses detected by the first-generation lensing experiment. For the event, there exist two different interpretations of the lens from independent…

太阳与恒星天体物理 · 物理学 2015-06-15 Youn Kil Jung , Cheongho Han , Andrew Gould , Dan Maoz