Miscellaneous


Stellar mass completeness in CANDELS/3D-HST
	Completeness in stellar mass of the 3D-HST/CANDELS catalogs was estimated by comparing source detection in the wide and deep components of the CANDELS survey. 25% of the CANDELS/deep data in the GOODS-S field were reduced and combined to match the depth of the wide component (visits 1 and 2 as defined by Grogin et al. 2011). These images were combined with direct imaging data from 3D-HST to create a noise equalized detection image. Source detection in the new "shallow" image was compared to source detection in CANDELS/deep in order to determine completeness in stellar mass (for full details see Tal et al. 2014). The catalogs are estimated to be 90% complete in stellar mass down to M_s = 1.1×10⁹M_⊙ at z < 1.8 and down to M_s = 2.6×10⁹M_⊙ at z < 2.5.

	Stellar mass completeness in the 3D-HST v3.0 catalog. Data	Stellar mass completeness in the 3D-HST v4.0 catalog. Data


Evolving quiescent fractions of group galaxies
	Quiescent fractions of central, satellite and background galaxies at different selection values of fixed cumulative number density.

	$Quiescent fractions at n=4e-4$ Quiescent fractions of central galaxies at n=4×10^-4 Mpc^-3 (red points), their satellites (blue points) and background galaxies at the same mass as the satellites (black points). Data	$Quiescent fraction of central galaxies$ Quiescent fractions of central galaxies at fixed cumulative number density values n=1,2,4,6×10^-4 Mpc^-3 Data