Millimeter/Submillimeter Search for the Sunyaev‐Zeldovich Effect in the Coma Cluster
Author(s) -
R. F. Silverberg,
E. S. Cheng,
D. A. Cottingham,
D. J. Fixsen,
C. A. Inman,
M. S. Kowitt,
S. S. Meyer,
Lyman A. Page,
Jason Puchalla,
Yoel Rephaeli
Publication year - 1997
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/304427
Subject(s) - coma cluster , physics , astrophysics , millimeter , intensity (physics) , coma (optics) , radius , telescope , optics , galaxy cluster , galaxy , computer security , computer science
Observations from the first flight of the Medium Scale Anisotropy Measurement(MSAM1-92) are analyzed to search for the Sunyaev-Zel'dovich (SZ) effecttowards the Coma cluster. This balloon-borne instrument uses a $28\arcmin$ FWHMbeam and a three position chopping pattern with a throw of $\pm40\arcmin$. Withspectral channels at 5.7, 9.3, 16.5, and 22.6~\icm, the observationssimultaneously sample the frequency range where the SZ spectral distortion inthe intensity transitions from a decrement to an increment and where thefractional intensity change is substantially larger than in the Rayleigh-Jeansregion. We set limits on the Comptonization parameter integrated over ourantenna pattern, $\Delta y \leq 8.0 \times 10^{-5}$($2 \sigma$). For aspherically symmetric isothermal model, this implies a central Comptonizationparameter, $y_o \leq 2.0 \times 10^{-4}$, or a central electron density, $n_o\leq 5.8 \times10^{-3}$cm$^{-3}h_{50}$, a result consistent with centraldensities implied by X-ray brightness measurements and central Comptonizationestimates from lower frequency observations of the SZ effect.Comment: 11 pages, LaTeX+aasms4 package, 1 PostScript figure. Submitted to Ap.J Letter
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