The imprint of cosmic voids from the DESI Legacy Survey DR9 Luminous Red Galaxies in the Planck 2018 lensing map through spectroscopically calibrated mocks

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Table 1.

Number of voids in each sample used.

Full sample

Void sample	Legacy north	Legacy south	Legacy full-sky	Buzzard north	Buzzard south	Buzzard full-sky
λ_v ∈ ( − ∞, ∞)	78 231	62 481	140 712	71 041	70 555	127 765
λ_v ∈ ( − ∞, −5)	17 687	14 035	31 722	14 560	14 516	26 449
λ_v ∈ [ − 5, 5)	30 603	24 018	54 621	28 112	27 741	50 394
λ_v ∈ [5, 1000)	29 941	24 428	54 369	28 369	28 298	50 922

0.35 ≤ z < 0.50

Void sample	Legacy north	Legacy south	Legacy full-sky	Buzzard north	Buzzard south	Buzzard full-sky

λ_v ∈ ( − ∞, ∞)	10 480	9343	19 823	9211	9676	17 008
λ_v ∈ ( − ∞, −5)	2338	2017	4355	2012	2086	3748
λ_v ∈ [ − 5, 5)	3973	3371	7344	3187	3330	5860
λ_v ∈ [5, 1000)	4169	3955	8124	4012	4260	7400

0.50 ≤ z < 0.65

Void sample	Legacy north	Legacy south	Legacy full-sky	Buzzard north	Buzzard south	Buzzard full-sky

λ_v ∈ ( − ∞, ∞)	15 868	12 937	28 805	14 560	14 861	26 498
λ_v ∈ ( − ∞, −5)	3770	3132	6902	3348	3425	6146
λ_v ∈ [ − 5, 5)	6120	4770	10 890	5215	5380	9540
λ_v ∈ [5, 1000)	5978	5035	11 013	5998	6055	10 811

0.65 ≤ z < 0.80

Void sample	Legacy north	Legacy south	Legacy full-sky	Buzzard north	Buzzard south	Buzzard full-sky

λ_v ∈ ( − ∞, ∞)	21 640	16 763	38 403	20 714	20 080	36 860
λ_v ∈ ( − ∞, −5)	5439	4234	9673	4743	4598	8500
λ_v ∈ [ − 5, 5)	8368	6321	14 689	8308	7940	14 691
λ_v ∈ [5, 1000)	7833	6208	14 041	7664	7542	13 669

0.80 ≤ z ≤ 0.95

Void sample	Legacy north	Legacy south	Legacy full-sky	Buzzard north	Buzzard south	Buzzard full-sky

λ_v ∈ ( − ∞, ∞)	29 853	23 118	52 971	26 170	25 565	46 710
λ_v ∈ ( − ∞, −5)	6045	4574	10 619	4381	4321	7907
λ_v ∈ [ − 5, 5)	12 008	9439	21 447	11 250	10 958	20 042
λ_v ∈ [5, 1000)	11 800	9105	20 905	10 539	10 286	18 760

Notes. The table above shows the number of voids in each sample used in this analysis, both observed and simulated, for the North and South regions as well as the full-sky. The table presents the number of voids for the entire data set and for each redshift bin, further differentiated by the three λ_v bins considered. For the Buzzard mocks, the number of voids is the average across the four realizations.

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