Zobrazeno 1 - 10
of 103
pro vyhledávání: '"HILL, D. T."'
Autor:
Foster, C., Hopkins, A. M., Gunawardhana, M., Lara-Lopez, M. A., Sharp, R. G., Steele, O., Taylor, E. N., Driver, S. P., Baldryi, I. K., Bamford, S. P., Liske, J., Loveday, J., Norberg, P., Peacock, J. A., Alpaslan, M., Bauer, A. E., Bland-Hawthorn, J., Brough, S., Cameron, E., Colless, M., Conselice, C. J., Croom, S. M., Frenk, C. S., Hill, D. T., Jones, D. H., Kelvin, L. S., Kuijken, K., Nichol, R. C., Owers, M. S., Parkinson, H. R., Pimbblet, K. A., Popescu, C. C., Prescott, M., Robotham, A. S. G., Lopez-Sanchez, A. R., Sutherland, W. J., Thomas, D., Tuffs, R. J., van Kampen, E., Wijesinghe, D.
Context: The mass-metallicity relationship (MMR) of star-forming galaxies is well-established, however there is still some disagreement with respect to its exact shape and its possible dependence on other observables. Aims: We measure the MMR in the
Externí odkaz:
http://arxiv.org/abs/1209.1636
Autor:
Driver, S. P., Robotham, A. S. G., Kelvin, L., Alpaslan, M., Baldry, I. K., Bamford, S. P., Brough, S., Brown, M., Hopkins, A. M., Liske, J., Loveday, J., Norberg, P., Peacock, J. A., Andrae, E., Bland-Hawthorn, J., Bourne, N., Cameron, E., Colless, M., Conselice, C. J., Croom, S. M., Dunne, L., Frenk, C. S., Graham, Alister W., Gunawardhana, M., Hill, D. T., Jones, D. H., Kuijken, K., Madore, B., Nichol, R. C., Parkinson, H. R., Pimbblet, K. A., Phillipps, S., Popescu, C. C., Prescott, M., Seibert, M., Sharp, R. G., Sutherland, W. J., Taylor, E. N., Thomas, D., Tuffs, R. J., van Kampen, E., Wijesinghe, D., Wilkins, S.
We use the GAMA I dataset combined with GALEX, SDSS and UKIDSS imaging to construct the low-redshift (z<0.1) galaxy luminosity functions in FUV, NUV, ugriz, and YJHK bands from within a single well constrained volume of 3.4 x 10^5 (Mpc/h)^{3}. The de
Externí odkaz:
http://arxiv.org/abs/1209.0259
Autor:
Loveday, J., Norberg, P., Baldry, I. K., Driver, S. P., Hopkins, A. M., Peacock, J. A., Bamford, S. P., Liske, J., Bland-Hawthorn, J., Brough, S., Brown, M. J. I., Cameron, E., Conselice, C. J., Croom, S. M., Frenk, C. S., Gunawardhana, M., Hill, D. T., Jones, D. H., Kelvin, L. S., Kuijken, K., Nichol, R. C., Parkinson, H. R., Phillipps, S., Pimbblet, K. A., Popescu, C. C., Prescott, M., Robotham, A. S. G., Sharp, R. G., Sutherland, W. J., Taylor, E. N., Thomas, D., Tuffs, R. J., van Kampen, E., Wijesinghe, D.
Galaxy and Mass Assembly (GAMA) is a project to study galaxy formation and evolution, combining imaging data from ultraviolet to radio with spectroscopic data from the AAOmega spectrograph on the Anglo-Australian Telescope. Using data from phase 1 of
Externí odkaz:
http://arxiv.org/abs/1111.0166
Autor:
Prescott, Matthew, Baldry, I. K., James, P. A., Bamford, S. P., Bland-Hawthorn, J., Brough, S., Brown, M. J. I., Cameron, E., Conselice, C. J., Croom, S. M., Driver, S. P., Frenk, C. S., Gunawardhana, M., Hill, D. T., Hopkins, A. M., Jones, D. H., Kelvin, L. S., Kuijken, K., Liske, J., Loveday, J., Nichol, R. C., Norberg, P., Parkinson, H. R., Peacock, J. A., Phillipps, S., Pimbblet, K. A., Popescu, C. C., Robotham, A. S. G., Sharp, R. G., Sutherland, W. J., Taylor, E. N., Tuffs, R. J., van Kampen, E., Wijesinghe, D.
Publikováno v:
Mon.Not.Roy.Astron.Soc. 417 (2011) 1374-1386
We investigate the properties of satellite galaxies that surround isolated hosts within the redshift range 0.01 < z < 0.15, using data taken as part of the Galaxy And Mass Assembly survey. Making use of isolation and satellite criteria that take into
Externí odkaz:
http://arxiv.org/abs/1107.0141
Autor:
Robotham, A. S. G., Norberg, P., Driver, S. P., Baldry, I. K., Bamford, S. P., Hopkins, A. M., Liske, J., Loveday, J., Merson, A., Peacock, J. A., Brough, S., Cameron, E., Conselice, C. J., Croom, S. M., Frenk, C. S., Gunawardhana, M., Hill, D. T., Jones, D. H., Kelvin, L. S., Kuijken, K., Nichol, R. C., Parkinson, H. R., Pimbblet, K. A., Phillipps, S., Popescu, C. C., Prescott, M., Sharp, R. G., Sutherland, W. J., Taylor, E. N., Thomas, D., Tuffs, R. J., van Kampen, E., Wijesinghe, D.
Using the complete GAMA-I survey covering ~142 sq. deg. to r=19.4, of which ~47 sq. deg. is to r=19.8, we create the GAMA-I galaxy group catalogue (G3Cv1), generated using a friends-of-friends (FoF) based grouping algorithm. Our algorithm has been te
Externí odkaz:
http://arxiv.org/abs/1106.1994
Autor:
Gunawardhana, M. L. P., Hopkins, A. M., Sharp, R. G., Brough, S., Taylor, E., Bland-Hawthorn, J., Maraston, C., Tuffs, R. J., Popescu, C. C., Wijesinghe, D., Jones, D. H., Croom, S., Sadler, E., Wilkins, S., Driver, S. P., Liske, J., Norberg, P., Baldry, I. K., Bamford, S. P., Loveday, J., Peacock, J. A., Robotham, A. S. G., Zucker, D. B., Parker, Q. A., Conselice, C. J., Cameron, E., Frenk, C. S., Hill, D. T., Kelvin, L. S., Kuijken, K., Madore, B. F., Nichol, B., Parkinson, H. R., Pimbblet, K. A., Prescott, M., Sutherland, W. J., Thomas, D., van Kampen, E.
The stellar initial mass function (IMF) describes the distribution in stellar masses produced from a burst of star formation. For more than fifty years, the implicit assumption underpinning most areas of research involving the IMF has been that it is
Externí odkaz:
http://arxiv.org/abs/1104.2379
Autor:
Brough, S., Hopkins, A. M., Sharp, R. G., Gunawardhana, M., Wijesinghe, D., Robotham, A. S. G., Driver, S. P., Baldry, I. K., Bamford, S. P., Liske, J., Loveday, J., Norberg, P., Peacock, J. A., Bland-Hawthorn, J. H., Brown, M. J. I., Cameron, E., Croom, S. M., Frenk, C. S., Foster, C., Hill, D. T., Jones, D. H., Kelvin, L. S., Kuijken, K., Nichol, R. C., Parkinson, H. R., Pimbblet, K., Popescu, C. C., Prescott, M., Sutherland, W. J., Taylor, E., Thomas, D., Tuffs, R. J., van Kampen, E.
We present an analysis of the properties of the lowest Halpha-luminosity galaxies (L_Halpha<4x10^32 W; SFR<0.02 Msun/yr) in the Galaxy And Mass Assembly (GAMA) survey. These galaxies make up the the rise above a Schechter function in the number densi
Externí odkaz:
http://arxiv.org/abs/1012.3771
Autor:
Hardcastle, M. J., Virdee, J. S., Jarvis, M. J., Bonfield, D. G., Dunne, L., Rawlings, S., Stevens, J. A., Christopher, N. M., Heywood, I., Mauch, T., Rigopoulou, D., Verma, A., Baldry, I. K., Bamford, S. P., Buttiglione, S., Cava, A., Clements, D. L., Cooray, A., Croom, S. M., Dariush, A., De Zotti, G., Eales, S., Fritz, J., Hill, D. T., Hughes, D., Hopwood, R., Ibar, E., Ivison, R. J., Jones, D. H., Loveday, J., Maddox, S. J., Michalowski, M. J., Negrello, M., Norberg, P., Pohlen, M., Prescott, M., Rigby, E. E., Robotham, A. S. G., Rodighiero, G., Scott, D., Sharp, R., Smith, D. J. B., Temi, P., van Kampen, E.
We use the Herschel-ATLAS science demonstration data to investigate the star-formation properties of radio-selected galaxies in the GAMA-9h field as a function of radio luminosity and redshift. Radio selection at the lowest radio luminosities, as exp
Externí odkaz:
http://arxiv.org/abs/1009.5866
Autor:
Jarvis, Matt J., Smith, D. J. B., Bonfield, D. G., Hardcastle, M. J., Falder, J. T., Stevens, J. A., Ivison, R. J., Auld, R., Baes, M., Baldry, I. K., Bamford, S. P., Bourne, N., Buttiglione, S., Cava, A, Cooray, A., Dariush, A., de Zotti, G., Dunlop, J. S., Dunne, L., Dye, S., Eales, S., Fritz, J., Hill, D. T., Hopwood, R., Hughes, D. H., Ibar, E., Jones, D. H., Kelvin, L., Lawrence, A., Leeuw, L., Loveday, J., Maddox, S. J., Michalowski, M. J., Negrello, M., Norberg, P., Pohlen, M., Prescott, M., Rigby, E. E., Robotham, A., Rodighiero, G., Scott, D., Sharp, R., Temi, P., Thompson, M. A., van der Werf, P., Vlahakis, C., White, G.
We use data from the Herschel-ATLAS to investigate the evolution of the far-infrared--radio correlation over the redshift range 05sigma sources in the Herschel-ATLAS Science Demonstration Field
Externí odkaz:
http://arxiv.org/abs/1009.5390
Autor:
Driver, S. P., Hill, D. T., Kelvin, L. S., Robotham, A. S. G., Liske, J., Norberg, P., Baldry, I. K., Bamford, S. P., Hopkins, A. M., Loveday, J., Peacock, J. A., Andrae, E., Bland-Hawthorn, J., Brough, S., Brown, M. J. I., Cameron, E., Ching, J. H. Y., Colless, M., Conselice, C. J., Croom, S. M., Cross, N. J. G., De Propris, R., Dye, S., Drinkwater, M. J., Ellis, S., Graham, Alister W., Grootes, M. W., Gunawardhana, M., Jones, D. H., van Kampen, E., Maraston, C., Nichol, R. C., Parkinson, H. R., Phillipps, S., Pimbblet, K., Popescu, C. C., Prescott, M., Roseboom, I. G., Sadler, E. M., Sansom, A. E., Sharp, R. G., Smith, D. J. B., Taylor, E., Thomas, D., Tuffs, R. J., Wijesinghe, D., Dunne, L., Frenk, C. S., Jarvis, M. J., Madore, B. F., Meyer, M. J., Seibert, M., Staveley-Smith, L., Sutherland, W. J., Warren, S. J.
The Galaxy And Mass Assembly (GAMA) survey has been operating since February 2008 on the 3.9-m Anglo-Australian Telescope using the AAOmega fibre-fed spectrograph facility to acquire spectra with a resolution of R~1300 for 120,862 SDSS selected galax
Externí odkaz:
http://arxiv.org/abs/1009.0614