Table 1.

Summary of the [O ii] ELG data used in this paper.*

NB816 (1.178 < z < 1.208)NB921 (1.453 < z < 1.489)
FieldArea (deg2)Ngng (h3 Mpc−3)NsubArea (deg2)Ngng (h3 Mpc−3)Nsub
COSMOS1.375664.48 × 10−395.8031344.30 × 10−341
DEEP2-34.9824855.40 × 10−3354.9221073.41 × 10−335
ELAIS-N14.8129276.59 × 10−3344.8130985.13 × 10−334
SXDS+XMM-LSS5.1723244.86 × 10−3371.3312397.44 × 10−39
Total16.3383025.50 × 10−311516.8695784.53 × 10−3119
NB816 (1.178 < z < 1.208)NB921 (1.453 < z < 1.489)
FieldArea (deg2)Ngng (h3 Mpc−3)NsubArea (deg2)Ngng (h3 Mpc−3)Nsub
COSMOS1.375664.48 × 10−395.8031344.30 × 10−341
DEEP2-34.9824855.40 × 10−3354.9221073.41 × 10−335
ELAIS-N14.8129276.59 × 10−3344.8130985.13 × 10−334
SXDS+XMM-LSS5.1723244.86 × 10−3371.3312397.44 × 10−39
Total16.3383025.50 × 10−311516.8695784.53 × 10−3119
*

The area value is after masking with bright object masks, Ng is the number of galaxies used in this paper after making the magnitude and flux cuts, ng is the number densities of the galaxies, and Nsub is the number of sub-regions using jackknife resampling (see subsection 3.2). The last row shows the values for the sum of the four fields.

Table 1.

Summary of the [O ii] ELG data used in this paper.*

NB816 (1.178 < z < 1.208)NB921 (1.453 < z < 1.489)
FieldArea (deg2)Ngng (h3 Mpc−3)NsubArea (deg2)Ngng (h3 Mpc−3)Nsub
COSMOS1.375664.48 × 10−395.8031344.30 × 10−341
DEEP2-34.9824855.40 × 10−3354.9221073.41 × 10−335
ELAIS-N14.8129276.59 × 10−3344.8130985.13 × 10−334
SXDS+XMM-LSS5.1723244.86 × 10−3371.3312397.44 × 10−39
Total16.3383025.50 × 10−311516.8695784.53 × 10−3119
NB816 (1.178 < z < 1.208)NB921 (1.453 < z < 1.489)
FieldArea (deg2)Ngng (h3 Mpc−3)NsubArea (deg2)Ngng (h3 Mpc−3)Nsub
COSMOS1.375664.48 × 10−395.8031344.30 × 10−341
DEEP2-34.9824855.40 × 10−3354.9221073.41 × 10−335
ELAIS-N14.8129276.59 × 10−3344.8130985.13 × 10−334
SXDS+XMM-LSS5.1723244.86 × 10−3371.3312397.44 × 10−39
Total16.3383025.50 × 10−311516.8695784.53 × 10−3119
*

The area value is after masking with bright object masks, Ng is the number of galaxies used in this paper after making the magnitude and flux cuts, ng is the number densities of the galaxies, and Nsub is the number of sub-regions using jackknife resampling (see subsection 3.2). The last row shows the values for the sum of the four fields.

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