J/MNRAS/376/1073  Sunyaev-Zel'dovich effect in galaxy clusters   (Zemcov+, 2007)

A study of the Sunyaev-Zel'dovich increment using archival SCUBA data. Zemcov M., Borys C., Halpern M., Mauskopf P., Scott D. <Mon. Not. R. Astron. Soc., 376, 1073-1098 (2007)> =2007MNRAS.376.1073Z 2007MNRAS.376.1073Z
ADC_Keywords: Clusters, galaxy ; Millimetric/submm sources Keywords: galaxies: clusters: general - cosmic microwave background - cosmology: observations - submillimetre Abstract: In a search for evidence of the short wavelength increment in the Sunyaev-Zel'dovich (SZ) effect, we have analysed archival galaxy cluster data from the Submillimetre Common User Bolometer Array (SCUBA) on the James Clerk Maxwell Telescope, resulting in the most complete pointed survey of clusters at 850µm to date. SCUBA's 850µm passband overlaps the peak of the SZ increment. The sample consists of 44 galaxy clusters in the range 0<z<1.3. Maps of each of the clusters have been made and sources have been extracted; as an ancillary product, we generate the most thorough galaxy cluster point source list yet from SCUBA. 17 of these clusters are free of obvious active galactic nuclei (AGN) and have data deep enough to provide interesting measurements of the expected SZ signal. Description: This work has made use of both JCMT archival data and new JCMT observations. For Cl 0152.7-1357, new JCMT data were obtained on 2003 Sept. 28, 29 and 2003 Oct. 17. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file cluster.dat 48 44 Cluster positions (from Simbad) tablea1.dat 119 130 Archival cluster data sets tableb1.dat 71 83 Positions, fluxes at 850 and 450um, errors and chi2 statistics for the candidate sources -------------------------------------------------------------------------------- See also: J/A+A/417/827 : Relativistic corr. to Sunyaev-Zeldovich effect (Itoh+, 2004) Byte-by-byte Description of file: cluster.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 13 A13 --- Cluster Cluster name 17- 18 I2 h RAh Simbad Right ascension (J2000) 20- 21 I2 min RAm Simbad Right ascension (J2000) 23- 24 I2 s RAs Simbad Right ascension (J2000) 26 A1 --- DE- Simbad Declination sign (J2000) 27- 28 I2 deg DEd Simbad Declination sign (J2000) 30- 33 F4.1 arcmin DEm Simbad Declination sign (J2000) 35- 48 A14 --- SName Simbad name -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 13 A13 --- Cluster Cluster 15- 24 A10 --- Project JCMT project IDs 26-101 A76 --- ObsDates Observation dates 104-108 F5.1 ks Time Integration time 110-114 F5.3 --- tau850 Mean scatter of the optical depth at 850um for the uncorrupted parts of the data sets 116-119 F4.2 --- e_tau850 ? Scatter of the optical depth for the uncorrupted parts of the data sets blank for sets with insufficient tau850 -------------------------------------------------------------------------------- Byte-by-byte Description of file: tableb1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 13 A13 --- Cluster Cluster 14 A1 --- --- [-] 15 I1 --- Galaxy Galaxy number within the Cluster 16 A1 --- n_Galaxy [a] Note (1) 18- 19 I2 h RAh Right ascension (J2000) 21- 22 I2 min RAm Right ascension (J2000) 24- 27 F4.1 s RAs Right ascension (J2000) 29 A1 --- DE- Declination sign (J2000) 30- 31 I2 deg DEd Declination sign (J2000) 33- 34 I2 arcmin DEm Declination sign (J2000) 36- 37 I2 arcsec DEs Declination sign (J2000) 39- 42 F4.1 mJy F850um Flux at 850um 44- 47 F4.1 mJy S/N850um Signal-to-noise ratio at 850um 49- 51 I3 --- chi2 chi2 statistic (2) 52 A1 --- --- (/) 53- 55 I3 --- DOF Degrees of freedom 57- 59 I3 mJy F450um ? Flux at 450um 61- 63 I3 mJy e_F450um ? rms uncertainty on F450um 64- 71 A8 --- n_F450um "Off Edge" for sources that not appear in the 450um maps -------------------------------------------------------------------------------- Note (1): The sources flagged with 'a' are possibly images of the SZ effect and we do not subtract them before doing the SZ effect fit. Because in a number of cases the apparent source is resolved, the chi2 in some of these sources is poor. Note (2): The chi2 values are determined by subtracting the fiducial JCMT PSF from the map centred on the nominal point source's position and then summing the squared residuals for the entire image. -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 28-Sep-2007
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