Li, 2023 - Google Patents
Cosmic tomography with weak gravitational lensingLi, 2023
View PDF- Document ID
- 14227088247573805034
- Author
- Li S
- Publication year
External Links
Snippet
Approximately 13.8 billion years ago (Planck Collaboration et al. 2020), an event known as the 'Big Bang'marked the inception of the physical Universe. As the Universe continues to expand, its energy density decreases, leading to the separation of the four fundamental …
Classifications
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01N—INVESTIGATING OR ANALYSING MATERIALS BY DETERMINING THEIR CHEMICAL OR PHYSICAL PROPERTIES
- G01N21/00—Investigating or analysing materials by the use of optical means, i.e. using infra-red, visible or ultra-violet light
- G01N21/17—Systems in which incident light is modified in accordance with the properties of the material investigated
- G01N21/25—Colour; Spectral properties, i.e. comparison of effect of material on the light at two or more different wavelengths or wavelength bands
- G01N21/31—Investigating relative effect of material at wavelengths characteristic of specific elements or molecules, e.g. atomic absorption spectrometry
- G01N21/35—Investigating relative effect of material at wavelengths characteristic of specific elements or molecules, e.g. atomic absorption spectrometry using infra-red light
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01N—INVESTIGATING OR ANALYSING MATERIALS BY DETERMINING THEIR CHEMICAL OR PHYSICAL PROPERTIES
- G01N23/00—Investigating or analysing materials by the use of wave or particle radiation not covered by G01N21/00 or G01N22/00, e.g. X-rays or neutrons
- G01N23/02—Investigating or analysing materials by the use of wave or particle radiation not covered by G01N21/00 or G01N22/00, e.g. X-rays or neutrons by transmitting the radiation through the material
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01M—TESTING STATIC OR DYNAMIC BALANCE OF MACHINES OR STRUCTURES; TESTING STRUCTURES OR APPARATUS NOT OTHERWISE PROVIDED FOR
- G01M11/00—Testing of optical apparatus; Testing structures by optical methods not otherwise provided for
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01N—INVESTIGATING OR ANALYSING MATERIALS BY DETERMINING THEIR CHEMICAL OR PHYSICAL PROPERTIES
- G01N33/00—Investigating or analysing materials by specific methods not covered by the preceding groups
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01V—GEOPHYSICS; GRAVITATIONAL MEASUREMENTS; DETECTING MASSES OR OBJECTS
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01B—MEASURING LENGTH, THICKNESS OR SIMILAR LINEAR DIMENSIONS; MEASURING ANGLES; MEASURING AREAS; MEASURING IRREGULARITIES OF SURFACES OR CONTOURS
- G01B11/00—Measuring arrangements characterised by the use of optical means
-
- G—PHYSICS
- G06—COMPUTING; CALCULATING; COUNTING
- G06F—ELECTRICAL DIGITAL DATA PROCESSING
- G06F17/00—Digital computing or data processing equipment or methods, specially adapted for specific functions
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01J—MEASUREMENT OF INTENSITY, VELOCITY, SPECTRAL CONTENT, POLARISATION, PHASE OR PULSE CHARACTERISTICS OF INFRA-RED, VISIBLE OR ULTRA-VIOLET LIGHT; COLORIMETRY; RADIATION PYROMETRY
Similar Documents
Publication | Publication Date | Title |
---|---|---|
Ding et al. | Detection of stellar light from quasar host galaxies at redshifts above 6 | |
Treu et al. | Strong lensing time-delay cosmography in the 2020s | |
Birrer et al. | Line-of-sight effects in strong lensing: putting theory into practice | |
Qi et al. | Strongly gravitationally lensed type Ia supernovae: Direct test of the Friedman-Lemaître-Robertson-Walker metric | |
Martens et al. | A radial measurement of the galaxy tidal alignment magnitude with BOSS data | |
Monna et al. | Separating galaxies from the cluster dark matter halo in Abell 611 | |
Meng et al. | Precision cosmology with time delay lenses: high resolution imaging requirements | |
O’Riordan et al. | Galaxy mass profiles from strong lensing I: the circular power-law model | |
Everall et al. | The photo-astrometric vertical tracer density of the Milky Way–II. Results from Gaia | |
Cao et al. | Anisotropies of cosmic optical and near-IR background from the China space station telescope (CSST) | |
Quici et al. | Selecting and modelling remnant AGNs with limited spectral coverage | |
Kakiichi et al. | Photometric IGM tomography with Subaru/HSC: the large-scale structure of Ly α emitters and IGM transmission in the COSMOS field at z˜ 5 | |
Li | Cosmic tomography with weak gravitational lensing | |
Zhang et al. | A search for the third lensed image in JVAS B1030+ 074 | |
Wilson et al. | Imaging reionization's last phases with I-front Lyman-α emissions | |
Duboscq et al. | Weak lensing of strong lensing: beyond the tidal regime | |
Linder | Tailoring strong lensing cosmographic observations | |
Weinstein | Why Do You Think It is a Black Hole? | |
GHUGAL | Two-component modeling of Strong Gravitational Lenses | |
Broughton | Probing the Dark Universe at the Pixel-Level in Large-Scale Surveys | |
Li | Li, SS (2023, October 25).. Retrie ed from https://hdl. handle. net/1887/3645974 | |
Myles | Combining Spectroscopic and Imaging Galaxy Surveys for Improved Measurements of Large-Scale Structure | |
Sharma | High Resolution Source Reconstruction of Lensed High Redshift Galaxies | |
Garayar | Redshift Distribution Uncertainty in Weaklensing Cosmology | |
Mahony | Cosmoparticle constraints with large-scale structure |