Nothing Special   »   [go: up one dir, main page]

Fox et al., 2002 - Google Patents

The distance to clusters: correcting for asphericity

Fox et al., 2002

View PDF @Full View
Document ID
1077847473118783014
Author
Fox D
Pen U
Publication year
Publication venue
The Astrophysical Journal

External Links

Snippet

ABSTRACT X-ray and Sunyaev-Zeldovich (SZ) effect observations can be combined to measure the distance to clusters of galaxies. The Hubble constant, H 0, can be inferred from the distance to low-redshift clusters. With enough clusters to measure the redshift-distance …
Continue reading at iopscience.iop.org (PDF) (other versions)

Classifications

    • 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
    • G01J5/00—Radiation pyrometry
    • G01J2005/0048—Calibrating; Correcting
    • G—PHYSICS
    • G01—MEASURING; TESTING
    • G01R—MEASURING ELECTRIC VARIABLES; MEASURING MAGNETIC VARIABLES
    • G01R29/00—Arrangements for measuring or indicating electric quantities not covered by groups G01R19/00 - G01R27/00
    • G—PHYSICS
    • G01—MEASURING; TESTING
    • G01R—MEASURING ELECTRIC VARIABLES; MEASURING MAGNETIC VARIABLES
    • G01R31/00—Arrangements for testing electric properties; Arrangements for locating electric faults; Arrangements for electrical testing characterised by what is being tested not provided for elsewhere
    • G01R31/28—Testing of electronic circuits, e.g. by signal tracer
    • G—PHYSICS
    • G01—MEASURING; TESTING
    • G01T—MEASUREMENT OF NUCLEAR OR X-RADIATION
    • G01T1/00—Measuring X-radiation, gamma radiation, corpuscular radiation, or cosmic radiation
    • G—PHYSICS
    • G01—MEASURING; TESTING
    • G01T—MEASUREMENT OF NUCLEAR OR X-RADIATION
    • G01T7/00—Details of radiation-measuring instruments
    • 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
    • G01J1/00—Photometry, e.g. photographic exposure meter
    • G—PHYSICS
    • G01—MEASURING; TESTING
    • G01R—MEASURING ELECTRIC VARIABLES; MEASURING MAGNETIC VARIABLES
    • G01R33/00—Arrangements or instruments for measuring magnetic variables
    • G—PHYSICS
    • G01—MEASURING; TESTING
    • G01N—INVESTIGATING OR ANALYSING MATERIALS BY DETERMINING THEIR CHEMICAL OR PHYSICAL PROPERTIES
    • G01N15/00—Investigating characteristics of particles; Investigating permeability, pore-volume, or surface-area of porous materials
    • G01N15/02—Investigating particle size or size distribution
    • 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
    • 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

Similar Documents

Publication Publication Date Title
Bacon et al. Cosmology with Phase 1 of the Square Kilometre Array Red Book 2018: technical specifications and performance forecasts
LaRoque et al. X-ray and Sunyaev-Zel’dovich effect measurements of the gas mass fraction in galaxy clusters
Bartelmann et al. Weak gravitational lensing
Hirata et al. Correlation of CMB with large-scale structure. II. Weak lensing
Hoekstra et al. Properties of galaxy dark matter halos from weak lensing
Baxter et al. A measurement of gravitational lensing of the cosmic microwave background by galaxy clusters using data from the South Pole Telescope
Hogg et al. Cosmic homogeneity demonstrated with luminous red galaxies
Kettula et al. CFHTLenS: weak lensing calibrated scaling relations for low-mass clusters of galaxies
Mathiesen et al. The effects of clumping and substructure on intracluster medium mass measurements
Liu et al. Cosmological constraints from weak lensing peak statistics with Canada–France–Hawaii Telescope Stripe 82 Survey
Gralla et al. A measurement of the millimetre emission and the Sunyaev–Zel'dovich effect associated with low-frequency radio sources
Romero et al. Pressure Profiles and Mass Estimates Using High-resolution Sunyaev–Zel’dovich Effect Observations of Zwicky 3146 with MUSTANG-2
Sayers et al. A comparison and joint analysis of Sunyaev–Zel’dovich effect measurements from Planck and Bolocam for a set of 47 massive galaxy clusters
Ruppin et al. Non-parametric deprojection of NIKA SZ observations: Pressure distribution in the Planck-discovered cluster PSZ1 G045. 85+ 57.71
Fox et al. The distance to clusters: correcting for asphericity
Sereno et al. CLUMP-3D: three-dimensional lensing and multi-probe analysis of MACS J1206. 2− 0847, a remarkably regular cluster
Ameglio et al. Joint deprojection of Sunyaev–Zeldovich and X-ray images of galaxy clusters
Di Mascolo et al. A joint ALMA–Bolocam–Planck SZ study of the pressure distribution in RX J1347. 5− 1145
Cain et al. Measuring gravitational lensing flexion in a1689 using an analytic image model
Bard et al. Effect of Measurement errors on predicted cosmological constraints from shear peak statistics with large synoptic survey telescope
Saini et al. Eccentricity-induced systematic error on parametrized tests of general relativity: Hierarchical Bayesian inference applied to a binary black hole population
Draper et al. Sunyaev-Zel’dovich signal of the maxBCG SDSS galaxy clusters in WMAP
Sayers et al. A search for cosmic microwave background anisotropies on arcminute scales with Bolocam
Morandi et al. Non-parametric method for measuring gas inhomogeneities from X-ray observations of galaxy clusters
Bengaly et al. Testing the isotropy of cosmic acceleration with the Pantheon+ and SH0ES datasets: A cosmographic analysis