Outputs (102)

Galaxy and mass assembly (GAMA): Panchromatic data release (far-UV-far-IR) and the low-z energy budget (2015)
Journal Article
Driver, S. P., Wright, A. H., Andrews, S. K., Davies, L. J., Kafle, P. R., Lange, R., Moffett, A. J., Mannering, E., Robotham, A. S. G., Vinsen, K., Alpaslan, M., Andrae, E., Baldry, I. K., Bauer, A. E., Bamford, S. P., Bland-Hawthorn, J., Bourne, N., Brough, S., Brown, M. J. I., Cluver, M. E., …Williams, R. (2016). Galaxy and mass assembly (GAMA): Panchromatic data release (far-UV-far-IR) and the low-z energy budget. Monthly notices of the Royal Astronomical Society, 455(4), 3911-3942. https://doi.org/10.1093/mnras/stv2505

We present the Galaxy And Mass Assembly (GAMA) Panchromatic Data Release (PDR) constituting over 230 deg2 of imaging with photometry in 21 bands extending from the far-UV to the far-IR. These data complement our spectroscopic campaign of over 300k ga... Read More about Galaxy and mass assembly (GAMA): Panchromatic data release (far-UV-far-IR) and the low-z energy budget.

Shapley Supercluster Survey: Construction of the photometric catalogues and i-band data release (2015)
Journal Article
Mercurio, A., Merluzzi, P., Busarello, G., Grado, A., Limatola, L., Haines, C. P., Brescia, M., Cavuoti, S., Dopita, M., Dall'Ora, M., Capaccioli, M., Napolitano, N., & Pimbblet, K. A. (2015). Shapley Supercluster Survey: Construction of the photometric catalogues and i-band data release. Monthly notices of the Royal Astronomical Society, 453(4), 3685-3698. https://doi.org/10.1093/mnras/stv1905

The Shapley Supercluster Survey is a multi-wavelength survey covering an area of ∼23 deg² (∼260 Mpc² at z = 0.048) around the supercluster core, including nine Abell and two poor clusters, having redshifts in the range 0.045–0.050. The survey aims to... Read More about Shapley Supercluster Survey: Construction of the photometric catalogues and i-band data release.

Galaxy And Mass Assembly (GAMA): the bright void galaxy population in the optical and mid-IR (2015)
Journal Article
Penny, S. J., Brown, M. J. I., Pimbblet, K. A., Cluver, M. E., Croton, D. J., Owers, M. S., Lange, R., Alpaslan, M., Baldry, I., Bland-Hawthorn, J., Brough, S., Driver, S. P., Holwerda, B. W., Hopkins, A. M., Jarrett, T. H., Heath Jones, D., Kelvin, L. S., Lara-López, M. A., Liske, J., López-Sánchez, A. R., …Rodrigues, M. (2015). Galaxy And Mass Assembly (GAMA): the bright void galaxy population in the optical and mid-IR. Monthly notices of the Royal Astronomical Society, 453(4), 3519-3539. https://doi.org/10.1093/mnras/stv1926

© 2015 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. We examine the properties of galaxies in the Galaxies and Mass Assembly (GAMA) survey located in voids with radii > 10 h -1 Mpc. Utilizing the GAM... Read More about Galaxy And Mass Assembly (GAMA): the bright void galaxy population in the optical and mid-IR.

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.