Zobrazeno 1 - 10
of 35
pro vyhledávání: '"Maddox, Steve J."'
Autor:
Smith, Matthew W. L., Ibar, Edo, Maddox, Steve J., Valiante, Elisabetta, Dunne, Loretta, Eales, Stephen, Dye, Simon, Furlanetto, Christina, Bourne, Nathan, Cigan, Phil, Ivison, Rob J., Gomez, Haley, Smith, Daniel J. B., Viaene, Sébastien
We present the largest submillimeter images that have been made of the extragalactic sky. The Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS) is a survey of 660 deg$^2$ with the PACS and SPIRE cameras in five photometric bands: 100, 160,
Externí odkaz:
http://arxiv.org/abs/1712.02361
Autor:
Driver, Simon P., Andrews, Stephen K., da Cunha, Elisabete, Davies, Luke J., Lagos, Claudia, Robotham, Aaron S. G., Vinsen, Kevin, Wright, Angus H., Alpaslan, Mehmet, Bland-Hawthorn, Joss, Bourne, Nathan, Brough, Sarah, Bremer, Malcolm N., Cluver, Michelle, Colless, Matthew, Conselice, Christopher J., Dunne, Loretta, Eales, Steve A., Gomez, Haley, Holwerda, Benne, Hopkins, Andrew M., Kafle, Prajwal R., Kelvin, Lee S., Loveday, Jon, Liske, Jochen, Maddox, Steve J., Phillipps, Steven, Pimbblet, Kevin, Rowlands, Kate, Sansom, Anne E., Taylor, Edward, Wang, Lingyu, Wilkins, Stephen M.
We use the energy-balance code MAGPHYS to determine stellar and dust masses, and dust corrected star-formation rates for over 200,000 GAMA galaxies, 170,000 G10-COSMOS galaxies and 200,000 3D-HST galaxies. Our values agree well with previously report
Externí odkaz:
http://arxiv.org/abs/1710.06628
Autor:
Driver, Simon P., Wright, Angus H., Andrews, Stephen K., Davies, Luke J., Kafle, Prajwal R., Lange, Rebecca, Moffett, Amanda J., Mannering, Elizabeth, Robotham, Aaron S. G., Vinsen, Kevin, Alpaslan, Mehmet, Andrae, Ellen, Baldry, Ivan K., Bauer, Amanda E., Bamford, Steven P., Bland-Hawthorn, Joss, Bourne, Nathan, Brough, Sarah, Brown, Michael J. I., Cluver, Michelle E., Croom, Scott, Colless, Matthew, Conselice, Christopher J., da Cunha, Elisabete, De Propris, Roberto, Drinkwater, Michael, Dunne, Loretta, Eales, Steve, Edge, Alastair, Frenk, Carlos, Graham, Alister W., Grootes, Meiert, Holwerda, Benne W., Hopkins, Andrew M., Ibar, Edo, van Kampen, Eelco, Kelvin, Lee S., Jarrett, Tom, Jones, D. Heath, Lara-Lopez, Maritza A., Lopez-Sanchez, Angel R., Liske, Jochen, Loveday, Jon, Maddox, Steve J., Madore, Barry, Meyer, Martin, Norberg, Peder, Penny, Samantha J., Phillipps, Stephen, Popescu, Cristina, Tuffs, Richard J., Peacock, John A., Pimbblet, Kevin A., Rowlands, Kate, Sansom, Anne E., Seibert, Mark, Smith, Matthew W. L., Sutherland, Will J., Taylor, Edward N., Valiante, Elisabetta, Wang, Lingyu, Wilkins, Stephen M., Williams, Richard
We present the GAMA Panchromatic Data Release (PDR) constituting over 230deg$^2$ 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 galaxies, and are compiled
Externí odkaz:
http://arxiv.org/abs/1508.02076
Autor:
De Geyter, Gert, Baes, Maarten, De Looze, Ilse, Bendo, George J., Bourne, Nathan, Camps, Peter, Cooray, Asantha, De Zotti, Gianfranco, Dunne, Loretta, Dye, Simon, Eales, Steve A., Fritz, Jacopo, Furlanetto, Cristina, Gentile, Gianfranco, Hughes, Thomas M., Ivison, Rob J., Maddox, Steve J., Michałowski, Michał J., Smith, Matthew W. L., Valiante, Elisabetta, Viaene, Sébastien
Interstellar dust in galaxies can be traced either through its extinction effects on the star light, or through its thermal emission at infrared wavelengths. Recent radiative transfer studies of several nearby edge-on galaxies have found an apparent
Externí odkaz:
http://arxiv.org/abs/1505.04567
Autor:
Kohn, Saul A., Michałowski, Michal J., Bourne, Nathan, Baes, Maarten, Fritz, Jacopo, Cooray, Asantha, De Looze, Ilse, De Zotti, Gianfranco, Dannerbauer, Helmut, Dunne, Loretta, Dye, Simon, Eales, Stephen, Furlanetto, Cristina, Gonzalez-Nuevo, Joaquin, Ibar, Edo, Ivison, Rob J., Maddox, Steve J., Scott, Douglas, Smith, Daniel J. B., Smith, Matthew W. L., Symeonidis, Myrto, Valiante, Elisabetta
Gamma-ray bursts (GRBs) are the most energetic phenomena in the Universe; believed to result from the collapse and subsequent explosion of massive stars. Even though it has profound consequences for our understanding of their nature and selection bia
Externí odkaz:
http://arxiv.org/abs/1501.01004
Autor:
Messias, Hugo, Dye, Simon, Nagar, Neil, Orellana, Gustavo, Bussmann, R. Shane, Calanog, Jae, Dannerbauer, Helmut, Fu, Hai, Ibar, Edo, Inohara, Andrew, Ivison, R. J., Negrello, Mattia, Riechers, Dominik A., Sheen, Yun-Kyeong, Amber, Simon, Birkinshaw, Mark, Bourne, Nathan, Clements, Dave L., Cooray, Asantha, De Zotti, Gianfranco, Demarco, Ricardo, Dunne, Loretta, Eales, Stephen, Fleuren, Simone, Lupu, Roxana E., Maddox, Steve J., Michalowski, Michal J., Omont, Alain, Rowlands, Kate, Smith, Dan, Smith, Matt, Valiante, Elisabetta
Publikováno v:
A&A 568, A92 (2014)
[Abridged] Aims: This work focuses on one lensed system, HATLAS J142935.3-002836 (H1429-0028), selected in the Herschel-ATLAS field. Gathering a rich, multi-wavelength dataset, we aim to confirm the lensing hypothesis and model the background source'
Externí odkaz:
http://arxiv.org/abs/1406.4859
Autor:
Bond, Nicholas A., Benford, Dominic J., Gardner, Jonathan P., Amblard, Alexandre, Fleuren, Simone, Blain, Andrew W., Dunne, Loretta, Smith, Daniel J. B., Maddox, Steve J., Hoyos, Carlos, Baes, Maarten, Bonfield, David, Bourne, Nathan, Bridge, Carrie, Buttiglione, Sara, Cava, Antonio, Clements, David, Cooray, Asantha, Dariush, Ali, de Zotti, Gianfranco, Driver, Simon, Dye, Simon, Eales, Steve, Eisenhardt, Peter, Hopwood, Rosalind, Ibar, Edo, Ivison, Rob J., Jarvis, Matt J., Kelvin, Lee, Robotham, Aaron S. G., Temi, Pasquale, Thompson, Mark, Tsai, Chao-Wei, van der Werf, Paul, Wright, Edward L., Wu, Jingwen, Yan, Lin
We describe the infrared properties of sources detected over ~36 deg^2 of sky in the GAMA 15-hr equatorial field, using data from both the Herschel Astrophysical Terahertz Large-Area Survey (H-ATLAS) and Wide-field Infrared Survey (WISE). With 5-sigm
Externí odkaz:
http://arxiv.org/abs/1204.2020
Autor:
Hilton, Matt, Collins, Chris, De Propris, Roberto, Baldry, Ivan K., Baugh, Carlton M., Bland-Hawthorn, Joss, Bridges, Terry, Cannon, Russell, Cole, Shaun, Colless, Matthew, Couch, Warrick J., Dalton, Gavin B., Driver, Simon P., Efstathiou, George, Ellis, Richard S., Frenk, Carlos S., Glazebrook, Karl, Jackson, Carole A., Lahav, Ofer, Lewis, Ian, Lumsden, Stuart, Maddox, Steve J., Madgwick, Darren, Norberg, Peder, Peacock, John A., Peterson, Bruce A., Sutherland, Will, Taylor, Keith
Publikováno v:
Mon.Not.Roy.Astron.Soc.363:661-674,2005
The ROSAT-ESO Flux Limited X-ray (REFLEX) galaxy cluster survey and the 2dF Galaxy Redshift Survey (2dFGRS) respectively comprise the largest, homogeneous X-ray selected cluster catalogue and completed galaxy redshift survey. In this work we combine
Externí odkaz:
http://arxiv.org/abs/astro-ph/0508207
Autor:
Magliocchetti, Manuela, Maddox, Steve J., Hawkins, Ed, Peacock, John A., Bland-Hawthorn, Joss, Bridges, Terry, Cannon, Russell, Cole, Shaun, Colless, Matthew, Collins, Chris, Couch, Warrick, Dalton, Gavin, de Propris, Roberto, Driver, Simon P., Efstathiou, George, Ellis, Richard S., Frenk, Carlos S., Glazebrook, Karl, Jackson, Carole A., Jones, Bryn, Lahav, Ofer, Lewis, Ian, Lumsden, Stuart, Norberg, Peder, Peterson, Bruce A., Sutherland, Will, Taylor, Keith
Publikováno v:
Mon.Not.Roy.Astron.Soc.350:1485,2004
The clustering properties of local, S_{1.4 GHz} > 1 mJy, radio sources are investigated for a sample of 820 objects drawn from the joint use of the FIRST and 2dF Galaxy Redshift surveys. To this aim, we present 271 new bj < 19.45 spectroscopic counte
Externí odkaz:
http://arxiv.org/abs/astro-ph/0312160
Existing observations are consistent with rich clusters of galaxies having no dust on $\simgt$ Mpc scales, while galaxy groups most probably do have dust distributed over $\lesssim$ Mpc scales. Dust in groups accounts for the observed redshift asymme
Externí odkaz:
http://arxiv.org/abs/astro-ph/0302537