Zobrazeno 1 - 10
of 743
pro vyhledávání: '"P. Phillipps"'
Autor:
E. Shevliakova, S. Malyshev, I. Martinez‐Cano, P. C. D. Milly, S. W. Pacala, P. Ginoux, K. A. Dunne, J. P. Dunne, C. Dupuis, K. L. Findell, K. Ghannam, L. W. Horowitz, T. R. Knutson, J. P. Krasting, V. Naik, P. Phillipps, N. Zadeh, Yan Yu, F. Zeng, Y. Zeng
Publikováno v:
Journal of Advances in Modeling Earth Systems, Vol 16, Iss 5, Pp n/a-n/a (2024)
Abstract We describe the baseline model configuration and simulation characteristics of the Geophysical Fluid Dynamics Laboratory (GFDL)'s Land Model version 4.1 (LM4.1), which builds on component and coupled model developments over 2013–2019 for t
Externí odkaz:
https://doaj.org/article/5353e5d4ef9149b2aa681395e7b84748
Autor:
Ali, Sadman, De Propris, Roberto, Chung, Chul, Phillipps, Steven, Bremer, Malcolm, Onodera, Masato, Sawicki, Marcin, Desprez, Guillaume, Gwyn, Stephen
We measure the evolution of the rest-frame $NUV-V$ colors for early-type galaxies in clusters at $0
Externí odkaz:
http://arxiv.org/abs/2403.08301
Autor:
Ahmed, U. T., Hopkins, A. M., Ware, J., Gordon, Y. A., Bilicki, M., Brown, M. J. I., Cluver, M., Gürkan, G., López-Sánchez, Á. R., Leahy, D. A., Marchetti, L., Phillipps, S., Prandoni, I., Seymour, N., Taylor, E. N., Vardoulaki, E.
We demonstrate the importance of radio selection in probing heavily obscured galaxy populations. We combine Evolutionary Map of the Universe (EMU) Early Science data in the Galaxy and Mass Assembly (GAMA) G23 field with the GAMA data, providing optic
Externí odkaz:
http://arxiv.org/abs/2312.11883
Autor:
Holwerda, B. W., Phillipps, S., Weerasooriya, S., Bovill, M. S., Brough, S., Brown, M. J. I., Robertson, C., Cook, K.
Groups of galaxies are the intermediate density environment in which much of the evolution of galaxies is thought to take place. In spectroscopic redshift surveys, one can identify these as close spatial redshift associations. However, spectroscopic
Externí odkaz:
http://arxiv.org/abs/2309.16875
Autor:
D'Silva, Jordan C. J., Driver, Simon P., Lagos, Claudia D. P., Robotham, Aaron S. G., Bellstedt, Sabine, Davies, Luke J. M., Thorne, Jessica E., Bland-Hawthorn, Joss, Bravo, Matias, Holwerda, Benne, Phillipps, Steven, Seymour, Nick, Siudek, Malgorzata, Windhorst, Rogier A.
We use the Galaxy and Mass Assembly (GAMA) and the Deep Extragalactic Visible Legacy Survey (DEVILS) observational data sets to calculate the cosmic star formation rate (SFR) and active galactic nuclei (AGN) bolometric luminosity history (CSFH/CAGNH)
Externí odkaz:
http://arxiv.org/abs/2306.16040
Autor:
Dev, Ajay, Driver, Simon P., Meyer, Martin, Roychowdhury, Sambit, Rhee, Jonghwan, Stevens, Adam R. H., Lagos, Claudia del P., Bland-Hawthorn, Joss, Catinella, Barbara, Hopkins, A. M., Loveday, Jonathan, Obreschkow, Danail, Phillipps, Steven, Robotham, Aaron S. G.
We determine the atomic hydrogen (HI) to halo mass relation (HIHM) using Arecibo Legacy Fast ALFA survey HI data at the location of optically selected groups from the Galaxy and Mass Assembly (GAMA) survey. We make direct HI detections for 37 GAMA gr
Externí odkaz:
http://arxiv.org/abs/2305.12750
Autor:
Phillipps, S., Bellstedt, S., Bremer, M. N., De Propris, R., James, P. A., Casura, S., Liske, J., Holwerda, B. W.
The star formation rate in galaxies is well known to correlate with stellar mass (the `star-forming main sequence'). Here we extend this further to explore any additional dependence on galaxy surface brightness, a proxy for stellar mass surface densi
Externí odkaz:
http://arxiv.org/abs/2211.15998
Autor:
Smith, Dominic, Haberzettl, Lutz, Porter, L. E., Porter-Temple, Ren, Henry, Christopher P. A., Holwerda, Benne, Lopez-Sanchez, A. R., Phillipps, Steven, Graham, Alister W., Brough, Sarah, Pimbblet, Kevin A., Liske, Jochen, Kelvin, Lee S., Robertson, Clayton D., Roemer, Wade, Walmsley, Michael, O'Ryan, David, Geron, Tobias
Galaxies broadly fall into two categories: star-forming (blue) galaxies and quiescent (red) galaxies. In between, one finds the less populated ``green valley". Some of these galaxies are suspected to be in the process of ceasing their star-formation
Externí odkaz:
http://arxiv.org/abs/2211.08355
Autor:
Thorne, Jessica E., Robotham, Aaron S. G., Bellstedt, Sabine, Davies, Luke J. M., Cook, Robin H. W., Cortese, Luca, Holwerda, Benne, Phillipps, Steven, Siudek, Malgorzata
Gas-phase metallicities of galaxies are typically measured through auroral or nebular emission lines, but metallicity also leaves an imprint on the overall spectral energy distribution (SED) of a galaxy and can be estimated through SED fitting. We us
Externí odkaz:
http://arxiv.org/abs/2210.13696
Autor:
Crossett, J. P., McGee, S. L., Ponman, T. J., Ramos-Ceja, M. E., Brown, M. J. I., Maughan, B. J., Robotham, A. S. G., Willis, J. P., Wood, C., Bland-Hawthorn, J., Brough, S., Driver, S. P., Holwerda, B. W., Hopkins, A. M., Loveday, J., Owers, M. S., Phillipps, S., Pierre, M., Pimbblet, K. A.
Publikováno v:
A&A 663, A2 (2022)
We investigate the properties of 232 optical spectroscopically selected groups from the Galaxy And Mass Assembly (GAMA) survey that overlap the XXL X-ray cluster survey. X-ray aperture flux measurements combined with GAMA group data provides the larg
Externí odkaz:
http://arxiv.org/abs/2203.14200