TL;DR
This study investigates galactic conformity in SDSS DR7, finding that previous signals are likely due to systematic errors, but identifies a potential new detection of 2-halo conformity in galaxy morphology at certain scales.
Contribution
It provides a comprehensive analysis of galactic conformity, highlighting the impact of systematic errors and presenting possibly the first robust detection of 2-halo conformity.
Findings
1-halo conformity signals are likely spurious due to systematics.
Radial segregation within massive groups is detected.
Potential first robust detection of 2-halo conformity in galaxy morphology.
Abstract
Galactic conformity is the phenomenon whereby galaxy properties exhibit excess correlations across distance than that expected if these properties only depended on halo mass. We perform a comprehensive study of conformity at low redshift using a galaxy group catalogue from the SDSS DR7 spectroscopic sample. We study correlations both between central galaxies and their satellites (1-halo), and between central galaxies in separate haloes (2-halo). We use the quenched fractions and the marked correlation function (MCF), to probe for conformity in three galaxy properties, colour, specific star formation rate (sSFR), and morphology. We assess the statistical significance of conformity signals with a suite of mock galaxy catalogues that have no built-in conformity, but contain the same group-finding and mass assignment errors as the real data. In the case of 1-halo conformity,…
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