M. Alpaslan
Galaxy And Mass Assembly (GAMA): the large-scale structure of galaxies and comparison to mock universes
Alpaslan, M.; Robotham, A.S.G.; Driver, S.; Norberg, P.; Baldry, I.; Bauer, A.E.; Bland-Hawthorn, J.; Brown, M.; Cluver, M.; Colless, M.; Foster, C.; Hopkins, A.; Van Kampen, E.; Kelvin, L.; Lara-Lopez, M.A.; Liske, J.; Lopez-Sanchez, A.R.; Loveday, J.; McNaught-Roberts, T.; Merson, A.; Pimbblet, K.
Authors
A.S.G. Robotham
S. Driver
Professor Peder Norberg peder.norberg@durham.ac.uk
Professor
I. Baldry
A.E. Bauer
J. Bland-Hawthorn
M. Brown
M. Cluver
M. Colless
C. Foster
A. Hopkins
E. Van Kampen
L. Kelvin
M.A. Lara-Lopez
J. Liske
A.R. Lopez-Sanchez
J. Loveday
T. McNaught-Roberts
A. Merson
K. Pimbblet
Abstract
From a volume-limited sample of 45 542 galaxies and 6000 groups with z ≤ 0.213, we use an adapted minimal spanning tree algorithm to identify and classify large-scale structures within the Galaxy And Mass Assembly (GAMA) survey. Using galaxy groups, we identify 643 filaments across the three equatorial GAMA fields that span up to 200 h−1 Mpc in length, each with an average of eight groups within them. By analysing galaxies not belonging to groups, we identify a secondary population of smaller coherent structures composed entirely of galaxies, dubbed ‘tendrils’ that appear to link filaments together, or penetrate into voids, generally measuring around 10 h−1 Mpc in length and containing on average six galaxies. Finally, we are also able to identify a population of isolated void galaxies. By running this algorithm on GAMA mock galaxy catalogues, we compare the characteristics of large-scale structure between observed and mock data, finding that mock filaments reproduce observed ones extremely well. This provides a probe of higher order distribution statistics not captured by the popularly used two-point correlation function.
Citation
Alpaslan, M., Robotham, A., Driver, S., Norberg, P., Baldry, I., Bauer, A., …Pimbblet, K. (2014). Galaxy And Mass Assembly (GAMA): the large-scale structure of galaxies and comparison to mock universes. Monthly Notices of the Royal Astronomical Society, 438(1), 177-194. https://doi.org/10.1093/mnras/stt2136
Journal Article Type | Article |
---|---|
Publication Date | Feb 11, 2014 |
Deposit Date | Jun 3, 2014 |
Publicly Available Date | Jun 5, 2014 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Royal Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 438 |
Issue | 1 |
Pages | 177-194 |
DOI | https://doi.org/10.1093/mnras/stt2136 |
Keywords | Methods: observational, Surveys, Large-scale structure of Universe. |
Public URL | https://durham-repository.worktribe.com/output/1460437 |
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Copyright Statement
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society. © 2013 The Authors
Published by Oxford University Press on behalf of the Royal Astronomical Society.
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