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GAMA plus KiDS: Alignment of galaxies in galaxy groups and its dependence on galaxy scale

Georgiou, C; Chisari, NE; Fortuna, MC; Hoekstra, H; Kuijken, K; Joachimi, B; Vakili, M; ... Shan, H; + view all (2019) GAMA plus KiDS: Alignment of galaxies in galaxy groups and its dependence on galaxy scale. Astronomy & Astrophysics , 628 , Article A31. 10.1051/0004-6361/201935810. Green open access

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Abstract

Intrinsic galaxy alignments are a source of bias for weak lensing measurements as well as a tool for understanding galaxy formation and evolution. In this work, we measure the alignment of shapes of satellite galaxies, in galaxy groups, with respect to the brightest group galaxy (BGG), as well as alignments of the BGG shape with the satellite positions, using the highly complete Galaxy And Mass Assembly (GAMA) spectroscopic survey and deep imaging from the Kilo Degree Survey. We control systematic errors with dedicated image simulations and measure accurate shapes using the DEIMOS shape measurement method. We find a significant satellite radial alignment signal, which vanishes at large separations from the BGG. We do not identify any strong trends of the signal with galaxy absolute magnitude or group mass. The alignment signal is dominated by red satellites. We also find that the outer regions of galaxies are aligned more strongly than their inner regions, by varying the radial weight employed during the shape measurement process. This behaviour is evident for both red and blue satellites. BGGs are also found to be aligned with satellite positions, with this alignment being stronger when considering the innermost satellites, using red BGGs and the shape of the outer region of the BGG. Lastly, we measure the global intrinsic alignment signal in the GAMA sample for two different radial weight functions and find no significant difference.

Type: Article
Title: GAMA plus KiDS: Alignment of galaxies in galaxy groups and its dependence on galaxy scale
Open access status: An open access version is available from UCL Discovery
DOI: 10.1051/0004-6361/201935810
Publisher version: https://doi.org/10.1051/0004-6361/201935810
Language: English
Additional information: This version is the version of record. For information on re-use, please refer to the publisher’s terms and conditions.
Keywords: Science & Technology, Physical Sciences, Astronomy & Astrophysics, galaxies: evolution, large-scale structure of Universe, gravitational lensing: weak, cosmology: observations, MASS ASSEMBLY GAMA, INTRINSIC ALIGNMENTS, DARK-MATTER, RADIAL ALIGNMENT, SHAPE MEASUREMENT, LENSING ANALYSIS, IMPACT, MODEL, SHEAR, CONSTRAINTS
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy
URI: https://discovery.ucl.ac.uk/id/eprint/10080141
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