On the abundance of gravitational arcs produced by submillimeter galaxies at radio and submm wavelengths

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Volume 508 / No 1 (December II 2009)

A&A, 508 1 (2009) 141-160

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Table 4:

Predicted number of submm ( $850~\mu$ m) arcs produced by SMGs for an all-sky survey, using all the synthetic cluster population to compute the optical depths (see Fig. 9).
$B_{850~\mu{\rm m}}^{~(1)}$	$\rm 5~mJy~arcsec^{-2}$		$\rm 1~mJy~arcsec^{-2}$		$\rm0.5~mJy~arcsec^{-2}$		$\rm0.1~mJy~arcsec^{-2}$
d₀⁽²⁾	7.5	10	7.5	10	7.5	10	7.5	10
SPZ DB⁽³⁾	575	250	3792	1650	8275	3600	50 767	22 075
PHZ DB⁽³⁾	550	233	3575	1533	7800	3342	47 892	20 517
CHM DB⁽³⁾	1142	517	7425	3325	16 200	7267	99 458	44 592
SPZ SM⁽³⁾	542	233	2208	958	3567	1550	9658	4200
PHZ SM⁽³⁾	508	217	2083	892	3367	1442	9117	3900
CHM SM⁽³⁾	1058	475	4317	1933	6992	3133	1058	475

⁽¹⁾ Surface brightness limit used to determine the number of arcs; ⁽²⁾ arc length-to-width ratio thresholds; ⁽³⁾ redshift distribution and number count function, as introduced in Figs. 3 and 6.

Source LaTeX | All tables | In the text

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