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Volumn 75, Issue 4, 2007, Pages

Magnification-temperature correlation: The dark side of integrated Sachs-Wolfe measurements

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EID: 33847179429     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.75.043519     Document Type: Article
Times cited : (48)

References (49)
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    • To be precise: we make use of Table 4 of the former, and Table 9 (Case 3) of the latter, and linearly interpolate between adjacent rest bands. Our assumed observed I-band blueshifts (going back in time) beyond the bluest rest-frame band (centered at 1500Å) given in the above papers by a redshift of about 4.33. For redshifts higher than this, we simply use the luminosity function centered at rest-frame 1500Å to obtain dN/dz etc.-altering the extrapolation scheme should have only a mild impact on the highest z bin we consider.
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