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2012MNRAS.423..529D - Mon. Not. R. Astron. Soc., 423, 529-542 (2012/June-2)
Calculating the transfer function of noise removal by principal component analysis and application to AzTEC deep-field observations.
DOWNES T.P., WELCH D., SCOTT K.S., AUSTERMANN J., WILSON G.W. and YUN M.S.
Abstract (from CDS):
Abstract Copyright: 2012 The Authors Monthly Notices of the Royal Astronomical Society2012 RAS
Journal keyword(s): atmospheric effects - methods: data analysis - galaxies: high-redshift - galaxies: starburst - submillimetre: galaxies
VizieR on-line data: <Available at CDS (J/MNRAS/423/529): table1.dat table2.dat table3.dat table4.dat table5.dat>
Nomenclature: Table 1, col(1): AzTEC JHHMMSS.ss+DDMMSS.s N=50 = Table 1, col(2): [DWS2012] AzTEC/COSMOS NN (Nos 1-50). Table 2, col(1): AzTEC JHHMMSS.ss+DDMMSS.s N=40 = Table 2, col(2): [DWS2012] AzTEC/GN NN (Nos 1-40). Table 3, col(1): AzTEC JHHMMSS.ss+DDMMSS.s N=95 = Table 3, col(2): [DWS2012] AzTEC/LH NN (Nos 1-95). Table 4, col(1): AzTEC JHHMMSS.ss+DDMMSS.s N=65 = Table 4, col(2): [DWS2012] AzTEC/SXDF NN (Nos 1-65). Table 5, col(1): AzTEC JHHMMSS.ss+DDMMSS.s N=57 = Table 5, col(2): [DWS2012] AzTEC/GS NN.N (Nos 1-2, 2.1-2.2, 3-55).
Status at CDS : All or part of tables of objects could be ingested in SIMBAD with priority 2.
Simbad objects: 5
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