Astrophysical Applications of Gravitational Microlensing

A special issue of Galaxies (ISSN 2075-4434).

Deadline for manuscript submissions: closed (31 March 2021) | Viewed by 2870

Special Issue Editor


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Guest Editor
Physics Department, Sharif University of Technology, Tehran 11155-9161, Iran
Interests: Gravitational lensing and Microlensing; Exoplanet Observations; Cosmology; Modified Gravity models; MOND

Special Issue Information

Dear Colleagues,

In recent years, gravitational microlensing has been used for the detection of compact astrophysical halo objects. This technique is then applied for the detection of extra-solar planets in the binary systems. The results of this observation were the discovery of tens of exoplanets through the method. The advantage of microlensing compared to conventional methods is that we can detect exoplanets that are as small as the Earth mass planets at a few kilo-parsec distances beyond the snowline of parent stars.

In recent years, microlensing observations have extended to space-based observations using Kepler and Spitzer Telescopes. The space-based telescope accompanying the ground-based telescope could break the degeneracy between the parameters of lensing to identify the mass of lenses. Gravitational microlensing as a natural telescope will enter a new phase of observations in other wavelengths, such as radio-waves, in the observations of self-lensing of binary compact objects for the discovery of the back holes and neutron stars, and in polarimetry observations.

With this Special Issue we aim to summarize where we stand today and our knowledge in different aspects of gravitational microlensing. Some of the key topics that will be covered in this Special issue of Galaxies are:

  • Gravitational microlensing and searching MACHOs in the galactic halo;
  • Investigating the structure of the Milky Way galaxy with microlensing observation;
  • Theory of binary lensing and observations of exoplanets;
  • Statistics of exoplanets from the microlensing observations;
  • Quasar microlensing;
  • Astrophysical applications of microlensing;
  • Polarization observations in microlensing;
  • Extending microlensing observations to the ratio wavelengths.

Dr. Sohrab Rahvar
Guest Editor

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Keywords

  • MACHOs
  • exoplanet detection and data analyzing
  • statistics of exoplanets
  • Quasar microlensing
  • astrophysical application of microlensing
  • polarimetry of microlensing events
  • microlensing in radio wavelengths

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Published Papers (1 paper)

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10 pages, 278 KiB  
Article
Exploiting the IRT-THESEUS Capability to Observe Lensed Quasars
by Lindita Hamolli, Mimoza Hafizi, Francesco De Paolis and Achille A. Nucita
Galaxies 2021, 9(2), 35; https://doi.org/10.3390/galaxies9020035 - 14 May 2021
Cited by 1 | Viewed by 2210
Abstract
THESEUS is an ESA space based project, which aims to explore the early universe by unveiling a complete census of Gamma-ray Burst (GRB) population in the first billion years. This goal is expected to be realized by the combined observations of its three [...] Read more.
THESEUS is an ESA space based project, which aims to explore the early universe by unveiling a complete census of Gamma-ray Burst (GRB) population in the first billion years. This goal is expected to be realized by the combined observations of its three instruments on board: the Soft X-ray Imager (SXI), the X and Gamma Imaging Spectrometer (XGIS), and the InfraRed Telescope (IRT). This last one will identify, localise, and study the afterglow of the GRBs detected by SXI and XGIS, and about 40% of its time will be devoted to an all-sky photometric survey, which will certainly detect a relevant number of extragalactic sources, including Quasars. In this paper, we focus on the capability of IRT-THESEUS Telescope to observe Quasars and, in particular, Quasars lensed by foreground galaxies. In our analysis we consider the recent results for the Quasar Luminosity Function (QLF) in the infrared band based on the Spitzer Space Telescope imaging survey. In order to estimate the number of lensed Quasars, we develop Monte Carlo simulations using the mass-luminosity distribution function of galaxies and the galaxy and Quasar redshift distributions. We predict about 2.14 × 105 Quasars to be observed during IRT-Theseus sky survey, and approximately 140 of them lensed by foreground galaxies. Detailed studies of these events would provide a powerful probe of the physical properties of Quasars and the mass distribution models of the galaxies. Full article
(This article belongs to the Special Issue Astrophysical Applications of Gravitational Microlensing)
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