%0 Generic %1 miller2015submillimetre %A Miller, Tim B. %A Hayward, Christopher C. %A Chapman, Scott C. %A Behroozi, Peter S. %D 2015 %K bias galaxies submm %T The bias of the submillimetre galaxy population: SMGs are poor tracers of the most massive structures in the z ~ 2 Universe %U http://arxiv.org/abs/1501.04105 %X It is often claimed that overdensities of (or even individual bright) submillimetre-selected galaxies (SMGs) trace the assembly of the most-massive dark matter structures in the Universe. We test this claim by performing a counts-in-cells analysis of mock SMG catalogues derived from the Bolshoi cosmological simulation to investigate how well SMG associations trace the underlying dark matter structure. We find that SMGs exhibit a relatively complex bias: some regions of high SMG overdensity are underdense in terms of dark matter mass, and some regions of high dark matter overdensity contain no SMGs. Because of their rarity, Poisson noise causes scatter in the SMG overdensity at fixed dark matter overdensity. Consequently, rich associations of less-luminous, more-abundant galaxies (i.e. Lyman-break galaxy analogues) trace the highest dark matter overdensities much better than SMGs. Even on average, SMG associations are relatively poor tracers of the most significant dark matter overdensities because of `downsizing': at z < ~2.5, the most-massive galaxies that reside in the highest dark matter overdensities have already had their star formation quenched and are thus no longer SMGs. Furthermore, because of Poisson noise and downsizing, some of the highest overdensities are not associated with any SMGs. Conversely, some bright SMGs are in underdense regions.

@misc{miller2015submillimetre, abstract = {It is often claimed that overdensities of (or even individual bright) submillimetre-selected galaxies (SMGs) trace the assembly of the most-massive dark matter structures in the Universe. We test this claim by performing a counts-in-cells analysis of mock SMG catalogues derived from the Bolshoi cosmological simulation to investigate how well SMG associations trace the underlying dark matter structure. We find that SMGs exhibit a relatively complex bias: some regions of high SMG overdensity are underdense in terms of dark matter mass, and some regions of high dark matter overdensity contain no SMGs. Because of their rarity, Poisson noise causes scatter in the SMG overdensity at fixed dark matter overdensity. Consequently, rich associations of less-luminous, more-abundant galaxies (i.e. Lyman-break galaxy analogues) trace the highest dark matter overdensities much better than SMGs. Even on average, SMG associations are relatively poor tracers of the most significant dark matter overdensities because of `downsizing': at z < ~2.5, the most-massive galaxies that reside in the highest dark matter overdensities have already had their star formation quenched and are thus no longer SMGs. Furthermore, because of Poisson noise and downsizing, some of the highest overdensities are not associated with any SMGs. Conversely, some bright SMGs are in underdense regions.}, added-at = {2015-01-20T10:10:35.000+0100}, author = {Miller, Tim B. and Hayward, Christopher C. and Chapman, Scott C. and Behroozi, Peter S.}, biburl = {https://www.bibsonomy.org/bibtex/225e6b4c0e3559bd67495d1bb8bbe679c/miki}, description = {[1501.04105] The bias of the submillimetre galaxy population: SMGs are poor tracers of the most massive structures in the z ~ 2 Universe}, interhash = {e049d15452f05121e141024d9dddfad0}, intrahash = {25e6b4c0e3559bd67495d1bb8bbe679c}, keywords = {bias galaxies submm}, note = {cite arxiv:1501.04105Comment: 5 pages, 3 figures; submitted to MNRAS Letters; comments welcome}, timestamp = {2015-01-20T10:10:35.000+0100}, title = {The bias of the submillimetre galaxy population: SMGs are poor tracers of the most massive structures in the z ~ 2 Universe}, url = {http://arxiv.org/abs/1501.04105}, year = 2015 }