Prospects of observation of gravitationally lensed sources by space submillimeter telescopes
arXiv:1912.09342 · doi:10.1134/S106377371912003X
Abstract
In the current paper we consider the prospects of observation of gravitationally lensed sources in far-infrared and submillimeter wavelength ranges by the future space telescopes equipped with actively cooled main mirrors. We consider the possibility of solving some of the important cosmological and astrophysical scientific tasks by observation of gravitationally lensed sources. The number counts of lensed sources for wavelengths from 70 up to 2000 were calculated. We discuss the distribution of lensed sources at different redshifts and magnification coefficients and also mass distribution of lenses. Model sky maps that illustrate the contribution of lensed sources were created.
arXiv comment23 pages, 6 figures
References in corpus (43)
- The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
- Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM
- Submillimeter Galaxies
- The Carnegie-Chicago Hubble Program. VIII. An Independent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch
- Dusty Star-Forming Galaxies at High Redshift
- Direct Detection of CDM Substructure
- Evidence for substructure in lens galaxies?
- The Detection of a Population of Submillimeter-Bright, Strongly-Lensed Galaxies
- Probing the Coevolution of Supermassive Black Holes and Galaxies Using Gravitationally Lensed Quasar Hosts
- H0LiCOW I. Lenses in COSMOGRAIL's Wellspring: Program Overview
- Kiloparsec-scale dust disks in high-redshift luminous submillimeter galaxies
- Bayesian Strong Gravitational-Lens Modeling on Adaptive Grids: Objective Detection of Mass Substructure in Galaxies
- Astrophysical and Cosmological Information from Large-scale sub-mm Surveys of Extragalactic Sources
- Cosmology from gravitational lens time delays and Planck data
- Gravitational Lens Models Based on Submillimeter Array Imaging of Herschel-selected Strongly Lensed Sub-millimeter Galaxies at z>1.5
- Ultraviolet Emission Lines in Young Low Mass Galaxies at z~2: Physical Properties and Implications for Studies at z>7
- Submillimetre galaxies in a hierarchical universe: number counts, redshift distribution, and implications for the IMF
- Flux ratios as a probe of dark substructures in quadruple-image gravitational lenses
- Spectroscopic detections of CIII]1909 at z~6-7: A new probe of early star forming galaxies and cosmic reionisation
- The Star Formation Histories of Local Group Dwarf Galaxies II. Searching For Signatures of Reionization
- MoMaF : The Mock Map Facility
- Modeling the evolution of infrared galaxies: A Parametric backwards evolution model
- AzTEC millimeter survey of the COSMOS field - III. Source catalog over 0.72 sq. deg. and plausible boosting by large-scale structure
- SILVERRUSH. III. Deep Optical and Near-Infrared Spectroscopy for Lya and UV-Nebular Lines of Bright Lya Emitters at z=6-7
- ALMA Observations of SPT-Discovered, Strongly Lensed, Dusty, Star-Forming Galaxies
- The Megamaser Cosmology Project: IV. A Direct Measurement of the Hubble Constant from UGC 3789
- How well can cold-dark-matter substructures account for the observed radio flux-ratio anomalies?
- Gas-rich mergers and feedback are ubiqitous amongst starbursting radio galaxies, as revealed by JVLA, IRAM PdBI and Herschel
- Effects of Dark Matter Substructures on Gravitational Lensing: Results from the Aquarius Simulations
- The Megamaser Cosmology Project VIII. A Geometric Distance to NGC 5765b
- Resolved UV and [CII] structures of luminous galaxies within the epoch of reionisation
- Candidate Gravitationally Lensed Dusty Star-forming Galaxies in the Herschel Wide Area Surveys
- The Megamaser Cosmology Project. VI. Observations of NGC 6323
- A Submillimeter Perspective on the GOODS Fields (SUPER GOODS). III. A Large Sample of ALMA Sources in the GOODS-S
- The Absence of [CII] 158m Emission in Spectroscopically-Confirmed Galaxies at
- The Intrinsic Far-infrared Continua of Type-1 Quasars
- A search for CII-158m line emission in HCM\,6A, a Lyman- emitter at
- Lyman-Alpha Emitting Galaxies as a Probe of Reionization: Large-Scale Bubble Morphology and Small-Scale Absorbers
- A Deep Ly Survey in ECDF-S and COSMOS: I. General Properties of Lyman-alpha Emitters at
- Galaxy stellar mass assembly: the difficulty matching observations and semi-analytical predictions
- HerMES: A Deficit in the Surface Brightness of the Cosmic Infrared Background Due to Galaxy Cluster Gravitational Lensing
- Modeling the Images of Relativistic Jets Lensed by Galaxies with Different Mass Surface Density Distributions
- A Model of the Cosmic Infrared Background Produced by Distant Galaxies