Zobrazeno 1 - 10
of 66
pro vyhledávání: '"Sansom, Anne E."'
We present a new library of semi-empirical stellar population models that are based on the empirical MILES and semi-empirical sMILES stellar libraries. The models span a large range of age and metallicity, in addition to an [$\alpha$/Fe] coverage fro
Externí odkaz:
http://arxiv.org/abs/2306.05942
The content and distribution of cool interstellar medium (ISM, <30K) can indicate the evolutionary mechanisms that transform late type to early type galaxies (ETGs). To investigate this, ALMA observations of 12CO[2-1] line emission were obtained for
Externí odkaz:
http://arxiv.org/abs/2210.11101
Autor:
Pennock, Clara M., van Loon, Jacco Th., Anih, Joy O., Maitra, Chandreyee, Haberl, Frank, Sansom, Anne E., Ivanov, Valentin D., Cowley, Michael J., Afonso, José, Antón, Sonia, Cioni, Maria-Rosa L., Craig, Jessica E. M., Filipović, Miroslav D., Hopkins, Andrew M., Nanni, Ambra, Prandoni, Isabella, Vardoulaki, Eleni
Following the discovery of SAGE0536AGN ($z \sim$ 0.14), with the strongest 10-$\mu$m silicate emission ever observed for an Active Galactic Nucleus (AGN), we discovered SAGE0534AGN ($z \sim$ 1.01), a similar AGN but with less extreme silicate emissio
Externí odkaz:
http://arxiv.org/abs/2207.12301
Autor:
Driver, Simon P., Bellstedt, Sabine, Robotham, Aaron S. G., Baldry, Ivan K., Davies, Luke J., Liske, Jochen, Obreschkow, Danail, Taylor, Edward N., Wright, Angus H., Alpaslan, Mehmet, Bamford, Steven P., Bauer, Amanda E., Bland-Hawthorn, Joss, Bilicki, Maciej, Bravo, Matias, Brough, Sarah, Casura, Sarah, Cluver, Michelle E., Colless, Matthew, Conselice, Christopher J., Croom, Scott M., de Jong, Jelte, D'Eugenio, Franceso, De Propris, Roberto, Dogruel, Burak, Drinkwater, Michael J., Dvornik, Andrej, Farrow, Daniel J., Frenk, Carlos S., Giblin, Benjamin, Graham, Alister W., Grootes, Meiert W., Gunawardhana, Madusha L. P., Hashemizadeh, Abdolhosein, Haussler, Boris, Heymans, Catherine, Hildebrandt, Hendrik, Holwerda, Benne W., Hopkins, Andrew M., Jarrett, Tom H., Jones, D. Heath, Kelvin, Lee S., Koushan, Soheil, Kuijken, Konrad, Lara-Lopez, Maritza A., Lange, Rebecca, Lopez-Sanchez, Angel R., Loveday, Jon, Mahajan, Smriti, Meyer, Martin, Moffett, Amanda J., Napolitano, Nicola R., Norberg, Peder, Owers, Matt S., Radovich, Mario, Raouf, Mojtaba, Peacock, John A., Phillipps, Steven, Pimbblet, Kevin A., Popescu, Cristina, Said, Khaled, Sansom, Anne E., Seibert, Mark, Sutherland, Will J., Thorne, Jessica E., Tuffs, Richard J., Turner, Ryan, van der Wel, Arjen, van Kampen, Eelco, Wilkins, Steve M.
In Galaxy And Mass Assembly Data Release 4 (GAMA DR4), we make available our full spectroscopic redshift sample. This includes 248682 galaxy spectra, and, in combination with earlier surveys, results in 330542 redshifts across five sky regions coveri
Externí odkaz:
http://arxiv.org/abs/2203.08539
We present a new library of semi-empirical stellar spectra that is based on the empirical MILES library. A new, high resolution library of theoretical stellar spectra is generated that is specifically designed for use in stellar population studies. W
Externí odkaz:
http://arxiv.org/abs/2104.04822
Autor:
Ferreras, Ignacio, Hopkins, Andrew M., Lagos, Claudia, Sansom, Anne E., Scott, Nicholas, Croom, Scott M., Brough, Sarah
Publikováno v:
2019, MNRAS, 487, 435
The growth channel of massive galaxies involving mergers can be studied via close pairs as putative merger progenitors, where the stellar populations of the satellite galaxies will be eventually incorporated into the massive primaries. We extend our
Externí odkaz:
http://arxiv.org/abs/1905.03266
Autor:
Saintonge, Amelie, Wilson, Christine D., Xiao, Ting, Lin, Lihwai, Hwang, Ho Seong, Tosaki, Tomoka, Bureau, Martin, Cigan, Phillip J., Clark, Christopher J. R., Clements, David L., De Looze, Ilse, Dharmawardena, Thavisha, Gao, Yang, Gear, Walter K., Greenslade, Joshua, Lamperti, Isabella, Lee, Jong Chul, Li, Cheng, Michalowski, Michal J., Mok, Angus, Pan, Hsi-An, Sansom, Anne E., Sargent, Mark, Smith, Matthew W. L., Williams, Thomas, Yang, Chentao, Zhu, Ming, Accurso, Gioacchino, Barmby, Pauline, Bourne, Nathan, Brinks, Elias, Brown, Toby, Chung, Aeree, Chung, Eun Jung, Cibinel, Anna, Coppin, Kristen, Davies, Jonathan, Davis, Timothy A., Eales, Steve, Fanciullo, Lapo, Fang, Taotao, Gao, Yu, Glass, David H. W., Gomez, Haley L., Greve, Thomas, He, Jinhua, Ho, Luis C., Huang, Feng, Jeong, Hyunjin, Jiang, Xuejian, Jiao, Qian, Kemper, Francisca, Kim, Ji Hoon, Kim, Minjin, Kim, Taehyun, Ko, Jongwan, Kong, Xu, Lacaille, Kevin, Lacey, Cedric G., Lee, Bumhyun, Lee, Joon Hyeop, Lee, Wing-Kit, Masters, Karen, Oh, Se-Heon, Papadopoulos, Padelis, Park, Changbom, Park, Sung-Joon, Parsons, Harriet, Rowlands, Kate, Scicluna, Peter, Scudder, Jillian M., Sethuram, Ramya, Serjeant, Stephen, Shao, Yali, Sheen, Yun-Kyeong, Shi, Yong, Shim, Hyunjin, Smith, Connor M. A., Spekkens, Kristine, Tsai, An-Li, Urquhart, Sheona, Verma, Aprajita, Violino, Giulio, Viti, Serena, Wake, David, Wang, Junfeng, Wouterloot, Jan, Yang, Yujin, Yim, Kijeong, Yuan, Fangting, Zheng, Zheng
JINGLE is a new JCMT legacy survey designed to systematically study the cold interstellar medium of galaxies in the local Universe. As part of the survey we perform 850um continuum measurements with SCUBA-2 for a representative sample of 193 Herschel
Externí odkaz:
http://arxiv.org/abs/1809.07336
Autor:
Kelvin, Lee S., Bremer, Malcolm N., Phillipps, Steven, James, Philip A., Davies, Luke J. M., De Propris, Roberto, Moffett, Amanda J., Percival, Susan M., Baldry, Ivan K., Collins, Chris A., Alpaslan, Mehmet, Bland-Hawthorn, Joss, Brough, Sarah, Cluver, Michelle, Driver, Simon P., Hashemizadeh, Abdolhosein, Holwerda, Benne W., Laine, Jarkko, Lara-Lopez, Maritza A., Liske, Jochen, Maciejewski, Witold, Napolitano, Nicola R., Penny, Samantha J., Popescu, Cristina C., Sansom, Anne E., Sutherland, Will, Taylor, Edward N., van Kampen, Eelco, Wang, Lingyu
Using a sample of 472 local Universe (z<0.06) galaxies in the stellar mass range 10.25 < log M*/M_sun < 10.75, we explore the variation in galaxy structure as a function of morphology and galaxy colour. Our sample of galaxies is sub-divided into red,
Externí odkaz:
http://arxiv.org/abs/1804.04470
Autor:
van de Voort, Freeke, Davis, Timothy A., Matsushita, Satoki, Rowlands, Kate, Shabala, Stanislav S., Allison, James R., Ting, Yuan-Sen, Sansom, Anne E., van der Werf, Paul P.
Publikováno v:
MNRAS, 2018, Volume 476, Issue 1, p.122-132
Gas-rich minor mergers contribute significantly to the gas reservoir of early-type galaxies (ETGs) at low redshift, yet the star formation efficiency (SFE; the star formation rate divided by the molecular gas mass) appears to be strongly suppressed f
Externí odkaz:
http://arxiv.org/abs/1801.08140
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