Zobrazeno 1 - 7
of 7
pro vyhledávání: '"Parkinson, Hannah R."'
Autor:
Hill, David T., Kelvin, Lee S., Driver, Simon P., Robotham, Aaron S. G., Cameron, Ewan, Cross, Nicholas, Andrae, Ellen, Baldry, Ivan K., Bamford, Steven P., Bland-Hawthorn, Joss, Brough, Sarah, Conselice, Christopher J., Dye, Simon, Hopkins, Andrew M., Liske, Jochen, Loveday, Jon, Norberg, Peder, Peacock, John A., Croom, Scott M., Frenk, Carlos S., Graham, Alister W., Jones, D. Heath, Kuijken, Konrad, Madore, Barry F., Nichol, Robert C., Parkinson, Hannah R., Phillipps, Steven, Pimbblet, Kevin A., Popescu, Cristina C., Prescott, Matthew, Seibert, Mark, Sharp, Rob G., Sutherland, Will J., Thomas, Daniel, Tuffs, Richard J, van Kampen, Elco
In order to generate credible 0.1-2 {\mu}m SEDs, the GAMA project requires many Gigabytes of imaging data from a number of instruments to be re-processed into a standard format. In this paper we discuss the software infrastructure we use, and create
Externí odkaz:
http://arxiv.org/abs/1009.0615
Autor:
Driver, Simon P., Norberg, Peder, Baldry, Ivan K., Bamford, Steven P., Hopkins, Andrew M., Liske, Jochen, Loveday, Jon, Peacock, John A., Hill, David T., Kelvin, Lee S., Robotham, Aaron S. G., Cross, Nick J., Parkinson, Hannah R., Prescott, Matt, Conselice, Chris J., Dunne, Loretta, Brough, Sarah, Jones, Heath, Sharp, Rob G., van Kampen, Eelco, Oliver, Seb, Roseboom, Isaac G., Bland-Hawthorn, Joss, Croom, Scott M., Ellis, Simon, Cameron, Ewan, Cole, Shaun, Frenk, Carlos S., Couch, Warrick J., Graham, Alister W., Proctor, Rob, De Propris, Roberto, Doyle, Issi F., Edmondson, Ed M., Thomas, Robert C. Nichol. Daniel, Eales, Steve A., Jarvis, Matt J., Kuijken, Konrad, Lahav, Ofer, Madore, Barry F., Seibert, Mark, Meyer, Martin J., Staveley-Smith, Lister, Phillipps, Steven, Popescu, Cristina C., Sansom, Ann E., Sutherland, Will J., Tuffs, Richard J., Warren, Steven J.
Publikováno v:
Astron.Geophys.50:5.12-5.19,2009
The Galaxy And Mass Assembly (GAMA) project is the latest in a tradition of large galaxy redshift surveys, and is now underway on the 3.9m Anglo-Australian Telescope at Siding Spring Observatory. GAMA is designed to map extragalactic structures on sc
Externí odkaz:
http://arxiv.org/abs/0910.5123
Autor:
Hill, David T., Kelvin, Lee S., Driver, Simon P., Robotham, Aaron S. G., Cameron, Ewan, Cross, Nicholas J. G., Andrae, Ellen, Baldry, Ivan K., Bamford, Steven P., Bland-Hawthorn, Joss, Brough, Sarah, Conselice, Christopher J., Dye, Simon, Hopkins, Andrew M., Liske, Jochen, Loveday, Jon, Norberg, Peder, Peacock, John A., Croom, Scott M., Frenk, Carlos S., Graham, Alister W., Jones, David Heath, Kuijken, Konrad, Madore, Barry F., Nichol, Robert C., Parkinson, Hannah R., Phillipps, Steven, Pimbblet, Kevin A., Popescu, Cristina C., Prescott, Matthew, Seibert, Mark, Sharp, Robert G., Sutherland, Will J., Thomas, Daniel, Tuffs, Richard J., Van Kampen, Eelco
Publikováno v:
Hill, D T, Kelvin, L S, Driver, S P, Robotham, A S G, Cameron, E, Cross, N J G, Andrae, E, Baldry, I K, Bamford, S P, Bland-Hawthorn, J, Brough, S, Conselice, C J, Dye, S, Hopkins, A M, Liske, J, Loveday, J, Norberg, P, Peacock, J A, Croom, S M, Frenk, C S, Graham, A W, Jones, D H, Kuijken, K, Madore, B F, Nichol, R C, Parkinson, H R, Phillipps, S, Pimbblet, K A, Popescu, C C, Prescott, M, Seibert, M, Sharp, R G, Sutherland, W J, Thomas, D, Tuffs, R J & Van Kampen, E 2011, ' Galaxy and Mass Assembly : FUV, NUV, ugrizYJHK Petrosian, Kron and Sérsic photometry ', Monthly Notices of the Royal Astronomical Society, vol. 412, no. 2, pp. 765-769 . https://doi.org/10.1111/j.1365-2966.2010.17950.x
In order to generate credible 0.1–2 μm spectral energy distributions, the Galaxy and Mass Assembly (GAMA) project requires many gigabytes of imaging data from a number of instruments to be reprocessed into a standard format. In this paper, we disc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::c6700b8f0ae448d4c55d23f69c840b09
http://doc.rero.ch/record/289903/files/mnras0412-0765.pdf
http://doc.rero.ch/record/289903/files/mnras0412-0765.pdf
Autor:
Brough, Sarah, Hopkins, Andrew M., Sharp, Robert G., Gunawardhana, M. L. P., Wijesinghe, D. B., Robotham, Aaron S. G., Driver, Simon P., Baldry, Ivan K., Bamford, Steven P., Liske, Jochen, Loveday, Jon, Norberg, Peder, Peacock, John A., Bland-Hawthorn, Joss, Brown, Michael J. I., Cameron, Ewan, Croom, Scott M., Frenk, Carlos S., Foster, C., Hill, David T., Jones, David Heath, Kelvin, Lee S., Kuijken, Konrad, Nichol, Robert C., Parkinson, Hannah R., Pimbblet, Kevin A., Popescu, Cristina C., Prescott, Matthew, Sutherland, Will J., Taylor, Edward N., Thomas, Daniel, Tuffs, Richard J., Van Kampen, Eelco
Publikováno v:
Brough, S, Hopkins, A M, Sharp, R G, Gunawardhana, M L P, Wijesinghe, D B, 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, 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 A, Popescu, C C, Prescott, M, Sutherland, W J, Taylor, E N, Thomas, D, Tuffs, R J & Van Kampen, E 2011, ' Galaxy and Mass Assembly (GAMA) : galaxies at the faint end of the Hα luminosity function ', Monthly Notices of the Royal Astronomical Society, vol. 413, no. 2, pp. 1236-1243 . https://doi.org/10.1111/j.1365-2966.2011.18210.x
We present an analysis of the properties of the lowest Hα-luminosity galaxies (LHα ≤ 4 × 1032 W; SFR < 0.02 Mʘ yr−1, with SFR denoting the star formation rate) in the Galaxy And Mass Assembly survey. These galaxies make up the rise above a Sc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3461::2aa22e2aea6a1b1479e0a8639296fc47
https://researchportal.port.ac.uk/ws/files/1436559/1236.full.pdf
https://researchportal.port.ac.uk/ws/files/1436559/1236.full.pdf
Autor:
Gunawardhana, M. L. P., Hopkins, Andrew M., Sharp, Robert G., Brough, Sarah, Taylor, Edward N., Bland-Hawthorn, Joss, Maraston, Claudia, Tuffs, Richard J., Popescu, Cristina C., Wijesinghe, D. B., Jones, David Heath, Croom, Scott M., Sadler, E. M., Wilkins, S., Driver, Simon P., Liske, Jochen, Norberg, Peder, Baldry, Ivan K., Bamford, Steven P., Loveday, Jon, Peacock, John A., Robotham, Aaron S. G., Zucker, D. B., Parker, Q. A., Conselice, Christopher J., Cameron, Ewan, Frenk, Carlos S., Hill, David T., Kelvin, Lee S., Kuijken, Konrad, Madore, B. F., Nichol, Bob, Parkinson, Hannah R., Pimbblet, Kevin A., Prescott, Matthew, Sutherland, Will J., Thomas, Daniel Georg, Van Kampen, Eelco
Publikováno v:
Gunawardhana, M L P, Hopkins, A M, Sharp, R G, Brough, S, Taylor, E N, Bland-Hawthorn, J, Maraston, C, Tuffs, R J, Popescu, C C, Wijesinghe, D B, Jones, D H, Croom, S M, Sadler, E M, 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 G & Van Kampen, E 2011, ' Galaxy and Mass Assembly (GAMA) : the star formation rate dependence of the stellar initial mass function ', Monthly Notices of the Royal Astronomical Society, vol. 415, no. 2, pp. 1647-1662 . https://doi.org/10.1111/j.1365-2966.2011.18800.x
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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6e9ae15b23386544f7669aedc33b0fe1
http://arxiv.org/abs/1104.2379
http://arxiv.org/abs/1104.2379
Autor:
Hill, David T., Kelvin, Lee S., Driver, Simon P., Robotham, Aaron S. G., Cameron, Ewan, Cross, Nicholas, Andrae, Ellen, Baldry, Ivan K., Bamford, Steven P., Bland-Hawthorn, Joss, Brough, Sarah, Conselice, Christopher J., Dye, Simon, Hopkins, Andrew M., Liske, Jochen, Loveday, Jon, Norberg, Peder, Peacock, John A., Croom, Scott M., Frenk, Carlos S., Graham, Alister W., Jones, D. Heath, Kuijken, Konrad, Madore, Barry F., Nichol, Robert C., Parkinson, Hannah R., Phillipps, Steven, Pimbblet, Kevin A., Popescu, Cristina C., Prescott, Matthew, Seibert, Mark, Sharp, Rob G., Sutherland, Will J., Thomas, Daniel, Tuffs, Richard J, van Kampen, Elco
Publikováno v:
Monthly Notices of the Royal Astronomical Society
In order to generate credible 0.1-2 {\mu}m SEDs, the GAMA project requires many Gigabytes of imaging data from a number of instruments to be re-processed into a standard format. In this paper we discuss the software infrastructure we use, and create
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=arXiv_dedup_::273b98258f0f832f4889cc560c630e2f
https://hdl.handle.net/11858/00-001M-0000-0015-12A3-011858/00-001M-0000-0015-12A1-3
https://hdl.handle.net/11858/00-001M-0000-0015-12A3-011858/00-001M-0000-0015-12A1-3
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