Galaxy And Mass Assembly (GAMA): the bright void galaxy population in the optical and mid-IR

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 GAMA equatorial survey, 592 void galaxies are identified out to z ≈ 0.1 brighter than M r  = −18.4, our magnitude completeness limit. Using the W Hα versus...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2015-11, Vol.453 (4), p.3519-3539
Hauptverfasser:	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., Jones, D. Heath, Kelvin, L. S., Lara-López, M. A., Liske, J., López-Sánchez, A. R., Loveday, J., Meyer, M., Norberg, P., Robotham, A. S. G., Rodrigues, M.
Format:	Artikel
Sprache:	eng
Schlagworte:	Assembly Astronomy Astrophysics Color Colour Diagnostic systems Infrared radiation Quenching Quenching (cooling) Sciences of the Universe Star & galaxy formation Star formation Star maps Stellar populations Voids
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