We present observations of 18 galaxies from the Galaxy And Mass Assembly (GAMA) survey made with the SPIRAL optical integral field unit (IFU) on the Anglo-Australian Telescope. The galaxies are selected to have a narrow range in stellar mass (6 × 109
Aims: We aim to investigate if the environment (characterised by the host dark matter halo mass) pla...
We present a detailed investigation into the effects of galaxy environment on their star formation r...
Aims: We aim to investigate if the environment (characterised by the host dark matter halo mass) pla...
We present observations of 18 galaxies from the Galaxy And Mass Assembly (GAMA) survey made with the...
We present observations of 18 galaxies from the Galaxy And Mass Assembly (GAMA) survey made with the...
We present observations of 18 galaxies from the Galaxy And Mass Assembly (GAMA) survey made with the...
We present observations of 18 galaxies from the Galaxy And Mass Assembly (GAMA) survey made with the...
We present observations of 18 galaxies from the Galaxy And Mass Assembly (GAMA) survey made with the...
We present observations of 18 galaxies from the Galaxy And Mass Assembly (GAMA) survey made with the...
We present observations of 18 galaxies from the Galaxy And Mass Assembly (GAMA) survey made with ...
We present observations of 18 galaxies from the Galaxy And Mass Assembly (GAMA) survey made with the...
We present observations of 18 galaxies from the Galaxy And Mass Assembly (GAMA) survey made with the...
We present observations of 18 galaxies from the Galaxy And Mass Assembly (GAMA) survey made with the...
Aims: We aim to investigate if the environment (characterised by the host dark matter halo mass) pla...
Aims: We aim to investigate if the environment (characterised by the host dark matter halo mass) pla...
Aims: We aim to investigate if the environment (characterised by the host dark matter halo mass) pla...
We present a detailed investigation into the effects of galaxy environment on their star formation r...
Aims: We aim to investigate if the environment (characterised by the host dark matter halo mass) pla...
We present observations of 18 galaxies from the Galaxy And Mass Assembly (GAMA) survey made with the...
We present observations of 18 galaxies from the Galaxy And Mass Assembly (GAMA) survey made with the...
We present observations of 18 galaxies from the Galaxy And Mass Assembly (GAMA) survey made with the...
We present observations of 18 galaxies from the Galaxy And Mass Assembly (GAMA) survey made with the...
We present observations of 18 galaxies from the Galaxy And Mass Assembly (GAMA) survey made with the...
We present observations of 18 galaxies from the Galaxy And Mass Assembly (GAMA) survey made with the...
We present observations of 18 galaxies from the Galaxy And Mass Assembly (GAMA) survey made with ...
We present observations of 18 galaxies from the Galaxy And Mass Assembly (GAMA) survey made with the...
We present observations of 18 galaxies from the Galaxy And Mass Assembly (GAMA) survey made with the...
We present observations of 18 galaxies from the Galaxy And Mass Assembly (GAMA) survey made with the...
Aims: We aim to investigate if the environment (characterised by the host dark matter halo mass) pla...
Aims: We aim to investigate if the environment (characterised by the host dark matter halo mass) pla...
Aims: We aim to investigate if the environment (characterised by the host dark matter halo mass) pla...
We present a detailed investigation into the effects of galaxy environment on their star formation r...
Aims: We aim to investigate if the environment (characterised by the host dark matter halo mass) pla...