Outputs (264)

Galaxy And Mass Assembly (GAMA): end of survey report and data release 2 (2015)
Journal Article
Vázquez-Mata, J. A., López-Sánchez, Á. R., Lara-López, M. A., Häußler, B., Liske, J., Baldry, I. K., Driver, S. P., Tuffs, R. J., Alpaslan, M., Andrae, E., Brough, S., Cluver, M. E., Grootes, M. W., Gunawardhana, M. L. P., Kelvin, L. S., Loveday, J., Robotham, A. S. G., Taylor, E. N., Bamford, S. P., Bland-Hawthorn, J., …Wright, A. H. (2015). Galaxy And Mass Assembly (GAMA): end of survey report and data release 2. Monthly notices of the Royal Astronomical Society, 452(2), 2087-2126. https://doi.org/10.1093/mnras/stv1436

The Galaxy And Mass Assembly (GAMA) survey is one of the largest contemporary spectroscopic surveys of low redshift galaxies. Covering an area of ∼286 deg² (split among five survey regions) down to a limiting magnitude of r < 19.8 mag, we have collec... Read More about Galaxy And Mass Assembly (GAMA): end of survey report and data release 2.

Galaxy And Mass Assembly (GAMA): trends in galaxy colours, morphology, and stellar populations with large-scale structure, group, and pair environments (2015)
Journal Article
Alpaslan, M., Driver, S., Robotham, A. S. G., Obreschkow, D., Andrae, E., Cluver, M., Kelvin, L. S., Lange, R., Owers, M., Taylor, E. N., Andrews, S. K., Bamford, S., Bland-Hawthorn, J., Brough, S., Brown, M. J. I., Colless, M., Davies, L. J. M., Eardley, E., Grootes, M. W., Hopkins, A. M., …Tuffs, R. (2015). Galaxy And Mass Assembly (GAMA): trends in galaxy colours, morphology, and stellar populations with large-scale structure, group, and pair environments. Monthly notices of the Royal Astronomical Society, 451(3), 3249-3268. https://doi.org/10.1093/mnras/stv1176

© 2015 The Authors. We explore trends in galaxy properties with Mpc-scale structures using catalogues of environment and large-scale structure from the Galaxy And Mass Assembly (GAMA) survey. Existing GAMA catalogues of large-scale structure, group,... Read More about Galaxy And Mass Assembly (GAMA): trends in galaxy colours, morphology, and stellar populations with large-scale structure, group, and pair environments.

The influence of red spiral galaxies on the shape of the local K-band luminosity function (2015)
Journal Article
Bonne, N. J., Brown, M. J. I., Jones, H., & Pimbblet, K. A. (2015). The influence of red spiral galaxies on the shape of the local K-band luminosity function. The Astrophysical journal, 799(2), Article ARTN 160. https://doi.org/10.1088/0004-637x/799/2/160

We have determined K-band luminosity functions for 13,325 local universe galaxies as a function of morphology and color (for Ktot ≤ 10.75). Our sample is drawn from the Two Micron All Sky Survey Extended Source Catalog, with all sample galaxies havin... Read More about The influence of red spiral galaxies on the shape of the local K-band luminosity function.

Erratum: The stellar masses of ~40 000 UV-selected galaxies from the WiggleZ survey at 0.3 < z < 1.0: Analogues of Lyman break galaxies? (2014)
Journal Article
Banerji, M., Glazebrook, K., Blake, C., Brough, S., Colless, M., Contreras, C., Couch, W., Croton, D. J., Croom, S., Davis, T. M., Drinkwater, M. J., Forster, K., Gilbank, D., Gladders, M., Jelliffe, B., Jurek, R. J., Li, I.-H., Madore, B., Christopher Martin, D., Pimbblet, K., …Yee, H. K. C. (2015). Erratum: The stellar masses of ~40 000 UV-selected galaxies from the WiggleZ survey at 0.3 < z < 1.0: Analogues of Lyman break galaxies?. Monthly notices of the Royal Astronomical Society, 447(1), 325-325. https://doi.org/10.1093/mnras/stu2478

The clustering and halo masses of star-forming galaxies at z<1 (2014)
Journal Article
Dolley, T., Brown, M. J. I., Weiner, B. J., Brodwin, M., Kochanek, C. S., Pimbblet, K. A., Palamara, D. P., Jannuzi, B. T., Dey, A., Atlee, D. W., & Beare, R. (2014). The clustering and halo masses of star-forming galaxies at z

We present clustering measurements and halo masses of star-forming galaxies at 0.2 < z < 1.0. After excluding active galactic nuclei (AGNs), we construct a sample of 22,553 24 μm sources selected from 8.42 deg2 of the Spitzer MIPS AGN and Galaxy Evol... Read More about The clustering and halo masses of star-forming galaxies at z<1.

An accurate new method of calculating absolute magnitudes and K-corrections applied to the Sloan filter set (2014)
Journal Article
Beare, R., Brown, M. J. I., & Pimbblet, K. (2014). An accurate new method of calculating absolute magnitudes and K-corrections applied to the Sloan filter set. The Astrophysical journal, 797(2), Article ARTN 104. https://doi.org/10.1088/0004-637x/797/2/104

We describe an accurate new method for determining absolute magnitudes, and hence also K-corrections, that is simpler than most previous methods, being based on a quadratic function of just one suitably chosen observed color. The method relies on the... Read More about An accurate new method of calculating absolute magnitudes and K-corrections applied to the Sloan filter set.

Shapley Supercluster Survey: Galaxy evolution from filaments to cluster cores (2014)
Journal Article
Merluzzi, P., Busarello, G., Haines, C. P., Mercurio, A., Okabe, N., Pimbblet, K. J., Dopita, M. A., Grado, A., Limatola, L., Bourdin, H., Mazzotta, P., Capaccioli, M., Napolitano, N. R., & Schipani, P. (2015). Shapley Supercluster Survey: Galaxy evolution from filaments to cluster cores. Monthly notices of the Royal Astronomical Society, 446(1), 803-822. https://doi.org/10.1093/mnras/stu2085

We present an overview of a multiwavelength survey of the Shapley Supercluster (SSC; z ∼ 0.05) covering a contiguous area of 260 h−2 70 Mpc² including the supercluster core. The project main aim is to quantify the influence of cluster-scale mass asse... Read More about Shapley Supercluster Survey: Galaxy evolution from filaments to cluster cores.

The frequency of anomalously red galaxies in SDSS clusters (2014)
Journal Article
Shearman, O., & Pimbblet, K. A. (2014). The frequency of anomalously red galaxies in SDSS clusters. Publications / Astronomical Society of Australia, 31, Article ARTN e038. https://doi.org/10.1017/pasa.2014.34

We present a systematic photometric search for spectroscopically confirmed anomalously red galaxies members of 748 low redshift clusters between 0.03 < z < 0.17 from the SDSS-C4 cluster catalogue (Miller et al. 2005). For each cluster we spectroscopi... Read More about The frequency of anomalously red galaxies in SDSS clusters.

Galaxy And Mass Assembly (GAMA): galaxy close pairs, mergers and the future fate of stellar mass (2014)
Journal Article
Robotham, A. S. G., Driver, S. P., Davies, L. J. M., Hopkins, A. M., Baldry, I. K., Agius, N. K., Bauer, A. E., Bland-Hawthorn, J., Brough, S., Brown, M. J. I., Cluver, M., De Propris, R., Drinkwater, M. J., Holwerda, B. W., Kelvin, L. S., Lara-Lopez, M. A., Liske, J., López-Sánchez, Á. R., Loveday, J., Mahajan, S., …Wilkins, S. M. (2014). Galaxy And Mass Assembly (GAMA): galaxy close pairs, mergers and the future fate of stellar mass. Monthly notices of the Royal Astronomical Society, 444(4), 3986-4008. https://doi.org/10.1093/mnras/stu1604

We use a highly complete subset of the Galaxy And Mass Assembly II (GAMA-II) redshift sample to fully describe the stellar mass dependence of close pairs and mergers between 10⁸ and 10¹² Mʘ. Using the analytic form of this fit we investigate the tota... Read More about Galaxy And Mass Assembly (GAMA): galaxy close pairs, mergers and the future fate of stellar mass.

The rarity of star formation in brightest cluster galaxies as measured by WISE (2014)
Journal Article
Fraser-McKelvie, A., Brown, M. J. I., & Pimbblet, K. A. (2014). The rarity of star formation in brightest cluster galaxies as measured by WISE. Monthly notices of the Royal Astronomical Society. Letters, 444(1), L63-L67. https://doi.org/10.1093/mnrasl/slu117

We present the mid-infrared star formation rates of 245 X-ray selected, nearby (z < 0.1) brightest cluster galaxies (BCGs). A homogeneous and volume limited sample of BCGs was created by X-ray selecting clusters with Lx > 1 × 1044 erg s⁻ ¹. The Wide-... Read More about The rarity of star formation in brightest cluster galaxies as measured by WISE.