A Second-order Moment of Microlensing Variability as a Novel Tool to Constrain Source Emission Size or Discrete Lens Demographics in Extragalactic Research-Reference-Cited by-同舟云学术

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A Second-order Moment of Microlensing Variability as a Novel Tool to Constrain Source Emission Size or Discrete Lens Demographics in Extragalactic Research

Published:2020-06-17 Issue:2 Volume:896 Page:111
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Guerras Eduardo^ORCID,Dai Xinyu^ORCID,Mediavilla Evencio^ORCID

Funder

NASA/SAO

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/1538-4357/ab76b9/pdf

Reference33 articles.

1. BLACK HOLE MASS ESTIMATES BASED ON C IV ARE CONSISTENT WITH THOSE BASED ON THE BALMER LINES

2. Confirmation of Planet-mass Objects in Extragalactic Systems

3. THE OPTICAL, ULTRAVIOLET, AND X-RAY STRUCTURE OF THE QUASAR HE 0435–1223

4. THE STRUCTURE OF HE 1104-1805 FROM INFRARED TO X-RAY

5. DISCOVERY OF ENERGY-DEPENDENT X-RAY MICROLENSING IN Q2237+0305

Cited by 3 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Microlensing of Strongly Lensed Quasars;Space Science Reviews;2024-02

2. Black hole masses for 14 gravitationally lensed quasars;Astronomy & Astrophysics;2023-12

3. NuSTAR Hard X-Ray Monitoring of Gravitationally Lensed Quasar RX J1131–1231;The Astrophysical Journal;2023-12-01

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