# Halo Histories vs. Galaxy Properties at z=0 II: Large-Scale Galactic Conformity

## TL;DR

This study investigates large-scale galactic conformity at z=0 using SDSS data, finding minimal evidence for conformity and showing that some observed signals may arise from contamination or other mechanisms rather than halo assembly bias.

## Contribution

The paper provides a detailed analysis of galactic conformity signals at large scales, testing halo age-matching models and clarifying the impact of contamination and alternative explanations.

## Key findings

- Minimal statistical evidence for conformity at >1 Mpc scales.
- Strong halo age-matching models predict too large conformity signals.
- Contamination affects conformity measurements, reducing the observed signal.

## Abstract

Using group catalogs from the SDSS DR7, we attempt to measure galactic conformity in the local universe. We measure the quenched fraction of neighbor galaxies around isolated primary galaxies, dividing the isolated sample into star-forming and quiescent objects. We restrict our measurements to scales $>1$ Mpc to probe the correlations between the formation histories of distinct halos. Over the stellar mass range $10^{9.7} \le M_\ast/M_\odot \le 10^{10.9}$, we find minimal statistical evidence for conformity. We further compare these data to predictions of the halo age-matching model, in which the oldest galaxies are associated with the oldest halos at fixed $M_\ast$. For models with strong correlations between halo and stellar age, the conformity signal is too large to be consistent with the data. For weaker implementations of age-matching, galactic conformity is not a sensitive diagnostic of halo assembly bias, and would not produce a detectable signal in SDSS data. We reproduce the results of Kauffmann et al 2013, in which the star formation rates of neighbor galaxies are significantly reduced around primary galaxies when the primaries are themselves low star formers. However, we find this result is mainly driven by contamination in the isolation criterion, when using our group catalog to remove the small fraction of satellite galaxies in the sample, the conformity signal largely goes away. Lastly, we show that small conformity signals, i.e., 2-5% differences in the quenched fractions of neighbor galaxies, can be produced by mechanisms other than halo assembly bias. For example, if passive galaxies occupy more massive halos than star forming galaxies of the same stellar mass, a conformity signal that is consistent with recent measurements from PRIMUS (Berti et al 2016) can be produced.