Galaxy And Mass Assembly (GAMA): the large-scale structure of galaxies and comparison to mock universes
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 equator...
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| Published in | Monthly notices of the Royal Astronomical Society Vol. 438; no. 1; pp. 177 - 194 |
|---|---|
| Main Authors | , , , , , , , , , , , , , , , , , , , , |
| Format | Journal Article |
| Language | English |
| Published |
London
Oxford University Press
11.02.2014
|
| Subjects | |
| Online Access | Get full text |
| ISSN | 0035-8711 1365-8711 1365-2966 1365-2966 |
| DOI | 10.1093/mnras/stt2136 |
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| 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. |
|---|---|
| AbstractList | 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. 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^sup -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^sup -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. |
| Author | Robotham, Aaron S. G. Loveday, Jon Norberg, Peder Bland-Hawthorn, Joss Pimbblet, Kevin Colless, Matthew Liske, Jochen Kelvin, Lee Alpaslan, Mehmet McNaught-Roberts, Tamsyn Cluver, Michelle Van Kampen, Eelco Lopez-Sanchez, Angel R. Baldry, Ivan Lara-Lopez, Maritza A. Bauer, Amanda E. Brown, Michael Foster, Caroline Merson, Alexander Driver, Simon Hopkins, Andrew |
| Author_xml | – sequence: 1 givenname: Mehmet surname: Alpaslan fullname: Alpaslan, Mehmet organization: 1SUPA, School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews, Fife KY16 9SS, UK – sequence: 2 givenname: Aaron S. G. surname: Robotham fullname: Robotham, Aaron S. G. organization: 1SUPA, School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews, Fife KY16 9SS, UK – sequence: 3 givenname: Simon surname: Driver fullname: Driver, Simon organization: 1SUPA, School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews, Fife KY16 9SS, UK – sequence: 4 givenname: Peder surname: Norberg fullname: Norberg, Peder organization: 1SUPA, School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews, Fife KY16 9SS, UK – sequence: 5 givenname: Ivan surname: Baldry fullname: Baldry, Ivan organization: 1SUPA, School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews, Fife KY16 9SS, UK – sequence: 6 givenname: Amanda E. surname: Bauer fullname: Bauer, Amanda E. organization: 1SUPA, School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews, Fife KY16 9SS, UK – sequence: 7 givenname: Joss surname: Bland-Hawthorn fullname: Bland-Hawthorn, Joss organization: 1SUPA, School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews, Fife KY16 9SS, UK – sequence: 8 givenname: Michael surname: Brown fullname: Brown, Michael organization: 1SUPA, School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews, Fife KY16 9SS, UK – sequence: 9 givenname: Michelle surname: Cluver fullname: Cluver, Michelle organization: 1SUPA, School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews, Fife KY16 9SS, UK – sequence: 10 givenname: Matthew surname: Colless fullname: Colless, Matthew organization: 1SUPA, School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews, Fife KY16 9SS, UK – sequence: 11 givenname: Caroline surname: Foster fullname: Foster, Caroline organization: 1SUPA, School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews, Fife KY16 9SS, UK – sequence: 12 givenname: Andrew surname: Hopkins fullname: Hopkins, Andrew organization: 1SUPA, School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews, Fife KY16 9SS, UK – sequence: 13 givenname: Eelco surname: Van Kampen fullname: Van Kampen, Eelco organization: 1SUPA, School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews, Fife KY16 9SS, UK – sequence: 14 givenname: Lee surname: Kelvin fullname: Kelvin, Lee organization: 1SUPA, School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews, Fife KY16 9SS, UK – sequence: 15 givenname: Maritza A. surname: Lara-Lopez fullname: Lara-Lopez, Maritza A. organization: 1SUPA, School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews, Fife KY16 9SS, UK – sequence: 16 givenname: Jochen surname: Liske fullname: Liske, Jochen organization: 1SUPA, School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews, Fife KY16 9SS, UK – sequence: 17 givenname: Angel R. surname: Lopez-Sanchez fullname: Lopez-Sanchez, Angel R. organization: 1SUPA, School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews, Fife KY16 9SS, UK – sequence: 18 givenname: Jon surname: Loveday fullname: Loveday, Jon organization: 1SUPA, School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews, Fife KY16 9SS, UK – sequence: 19 givenname: Tamsyn surname: McNaught-Roberts fullname: McNaught-Roberts, Tamsyn organization: 1SUPA, School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews, Fife KY16 9SS, UK – sequence: 20 givenname: Alexander surname: Merson fullname: Merson, Alexander organization: 1SUPA, School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews, Fife KY16 9SS, UK – sequence: 21 givenname: Kevin surname: Pimbblet fullname: Pimbblet, Kevin organization: 1SUPA, School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews, Fife KY16 9SS, UK |
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| Copyright | 2013 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society 2013 Copyright Oxford University Press, UK Feb 11, 2014 |
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| SubjectTerms | Cosmology Stars & galaxies Universe |
| Title | Galaxy And Mass Assembly (GAMA): the large-scale structure of galaxies and comparison to mock universes |
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