Inferences from Surface Brightness Fluctuations of Zwicky 3146 via the Sunyaev–Zel’dovich Effect and X-Ray Observations [PDF]
The galaxy cluster Zwicky 3146 is a sloshing cool-core cluster at z = 0.291 that in Sunyaev–Zel’dovich (SZ) imaging does not appear to exhibit significant pressure substructure in the intracluster medium.
Charles E. Romero+18 more
doaj +5 more sources
Forecasting Constraints from Surface Brightness Fluctuations in Galaxy Clusters [PDF]
Abstract Studies of surface brightness (SB) fluctuations in the intracluster medium present an indirect estimate of turbulent pressure support and associated Mach numbers. While high-resolution X-ray spectroscopy can directly constrain line-of-sight gas motions, including those due to turbulence, such observations are relatively ...
Charles E. Romero
doaj +5 more sources
A Database of Cepheid Distance Moduli and TRGB, GCLF, PNLF and SBF Data Useful for Distance Determinations [PDF]
We present a compilation of Cepheid distance moduli and data for four secondary distance indicators that employ stars in the old stellar populations: the planetary nebula luminosity function (PNLF), the globular cluster luminosity function (GCLF), the ...
Ferrarese, Laura+16 more
core +5 more sources
Power spectrum estimation methods on intracluster medium surface brightness fluctuations [PDF]
Accurate estimation of galaxy cluster masses is a central problem in cosmology. Turbulence is believed to introduce significant deviations from the hydrostatic mass estimates. Estimation of turbulence properties is complicated by projection of the 3D cluster onto the 2D plane of the sky, and is commonly done in the form of indirect probes from ...
Bishop M.+3 more
doaj +7 more sources
SBF Distances to Dwarf Elliptical Galaxies in the Sculptor Group [PDF]
As part of an ongoing search for dwarf elliptical galaxies (dE) in the vicinity of the Local Group, we acquired deep B and R-band images for five dE candidates identified in the Sculptor (Scl) group region. We carried out a surface brightness fluctuation
B. Binggeli+13 more
core +5 more sources
Studying the ICM in clusters of galaxies via surface brightness fluctuations of the cosmic X-ray background [PDF]
We study the surface brightness fluctuations of the cosmic X-ray background (CXB) using Chandra data of XBOOTES. After masking out resolved sources we compute the power spectrum of fluctuations of the unresolved CXB for angular scales from ~2 arcsec to ...
Gilfanov, Marat+3 more
core +7 more sources
The Infrared Surface Brightness Fluctuation Hubble Constant [PDF]
We measured infrared surface brightness fluctuation (SBF) distances to an isotropically-distributed sample of 16 distant galaxies with redshifts reaching 10,000 km/s using the near-IR camera and multi-object spectrometer (NICMOS) on the Hubble Space Telescope (HST).
Edward A. Ajhar+8 more
semanticscholar +6 more sources
Surface brightness fluctuation distances for nearby dwarf elliptical galaxies [PDF]
We obtained B and R-band CCD images for the dwarf elliptical (dE) galaxies DDO44, UGC4998, KK98_77, DDO71, DDO113, and UGC7356 at the NOT. Using Fourier analysis technique we measure stellar R-band surface brightness fluctuations (SBFs) and magnitudes in 29 different fields of the galaxies.
Jerjen, Helmut+4 more
semanticscholar +10 more sources
The Infrared Surface Brightness Fluctuation Distances to the Hydra and Coma Clusters [PDF]
24 pages, 4 PostScript figures, 2 JPEG images; accepted for publication in ...
Gerard A. Luppino+3 more
core +8 more sources
Cluster detection from surface-brightness fluctuations in SDSS data [PDF]
7 pages, submitted to Astronomy & ...
Matthias Bartelmann, S. N. White
core +7 more sources