Zobrazeno 1 - 10
of 2 039
pro vyhledávání: '"P. McKelvie"'
Autor:
Fraser-McKelvie, A., van de Sande, J., Gadotti, D. A., Emsellem, E., Brown, T., Fisher, D. B., Martig, M., Bureau, M., Gerhard, O., Battisti, A. J., Bland-Hawthorn, J., Catinella, B., Combes, F., Cortese, L., Croom, S. M., Davis, T. A., Falcón-Barroso, J., Fragkoudi, F., Freeman, K. C., Hayden, M. R., McDermid, R., Ciraulo, B. Mazzilli, Mendel, J. T., Pinna, F., Poci, A., Rutherford, T. H., de Sá-Freitas, C., Silva-Lima, L. A., Valenzuela, L. M., van de Ven, G., Wang, Z., Watts, A. B.
The vertical evolution of galactic discs is governed by the sub-structures within them. We examine the diversity of kinematic sub-structure present in the first 12 galaxies observed from the GECKOS survey, a VLT/MUSE large programme providing a syste
Externí odkaz:
http://arxiv.org/abs/2411.03430
Autor:
Ristea, Andrei, Cortese, Luca, Groves, Brent, Fraser-McKelvie, A., Obreschkow, Danail, Glazebrook, Karl
The circular velocity function (CVF) of galaxies is a fundamental test of the $\Lambda$ Cold Dark Matter (CDM) paradigm as it traces the variation of galaxy number densities with circular velocity ($v_{\rm{circ}}$), a proxy for dynamical mass. Previo
Externí odkaz:
http://arxiv.org/abs/2409.05081
Autor:
Tuntipong, Sujeeporn, van de Sande, Jesse, Croom, Scott M., Barsanti, Stefania, Bland-Hawthorn, Joss, Brough, Sarah, Bryant, Julia J., Casura, Sarah, Fraser-McKelvie, Amelia, Lawrence, Jon S., Ristea, Andrei, Sweet, Sarah M., Zafar, Tayyaba
Milky Way Analogues (MWAs) provide an alternative insight into the various pathways that lead to the formation of disk galaxies with similar properties to the Milky Way. In this study, we explore different selection techniques for identifying MWAs in
Externí odkaz:
http://arxiv.org/abs/2408.12223
Autor:
Watts, Adam B., Cortese, Luca, Catinella, Barbara, Fraser-McKelvie, Amelia, Emsellem, Eric, Coccato, Lodovico, van de Sande, Jesse, Brown, Toby H., Ascasibar, Yago, Battisti, Andrew, Boselli, Alessandro, Davis, Timothy A., Groves, Brent, Thater, Sabine
Stellar feedback-driven outflows are important regulators of the gas-star formation cycle. However, resolving outflow physics requires high resolution observations that can only be achieved in very nearby galaxies, making suitable targets rare. We pr
Externí odkaz:
http://arxiv.org/abs/2404.12616
Autor:
Rigamonti, Fabio, Cortese, Luca, Bollati, Francesco, Covino, Stefano, Dotti, Massimo, Fraser-McKelvie, A., Haardt, Francesco
We investigate the relevance of kinematically identified bulges, discs and their role relative to galaxy quenching. We utilize an analysis of the SDSS-MaNGA survey conducted with the GPU-based code BANG which simultaneously models galaxy photometry a
Externí odkaz:
http://arxiv.org/abs/2403.09812
Autor:
Croom, S. M., van de Sande, J., Vaughan, S. P., Rutherford, T. H., Lagos, C. P., Barsanti, S., Bland-Hawthorn, J., Brough, S., Bryant, J. J., Colless, M., Cortese, L., D'Eugenio, F., Fraser-McKelvie, A., Goodwin, M., Lorente, N. P. F., Richards, S. N., Ristea, A., Sweet, S. M., Yi, S. K., Zafar, T.
Publikováno v:
MNRAS, Volume 529, Issue 4, April 2024, Pages 3446-3468
We use the SAMI Galaxy Survey to examine the drivers of galaxy spin, $\lambda_{R_e}$, in a multi-dimensional parameter space including stellar mass, stellar population age (or specific star formation rate) and various environmental metrics (local den
Externí odkaz:
http://arxiv.org/abs/2402.06877
Autor:
Vaughan, Sam P., van de Sande, Jesse, Fraser-McKelvie, A., Croom, Scott, McDermid, Richard, Liquet-Weiland, Benoit, Barsanti, Stefania, Cortese, Luca, Brough, Sarah, Sweet, Sarah, Bryant, Julia J., Goodwin, Michael, Lawrence, Jon
We use the SAMI galaxy survey to study the the kinematic morphology-density relation: the observation that the fraction of slow rotator galaxies increases towards dense environments. We build a logistic regression model to quantitatively study the de
Externí odkaz:
http://arxiv.org/abs/2402.03676
Autor:
Ristea, Andrei, Cortese, Luca, Fraser-McKelvie, Amelia, Catinella, Barbara, van de Sande, Jesse, Croom, Scott M., Swinbank, Mark
The stellar mass Tully-Fisher relation (STFR) and its scatter encode valuable information about the processes shaping galaxy evolution across cosmic time. However, we are still missing a proper quantification of the STFR slope and scatter dependence
Externí odkaz:
http://arxiv.org/abs/2311.13251
Pearson's chi-squared test, from 1900, is the standard statistical tool for "hypothesis testing on distributions": namely, given samples from an unknown distribution $Q$ that may or may not equal a hypothesis distribution $P$, we want to return "yes"
Externí odkaz:
http://arxiv.org/abs/2310.09408
Autor:
Sharma, Anubhav, Masters, Karen L., Stark, David V., Garland, James, Drory, Niv, Fraser-McKelvie, Amelia, Weijmans, Anne-Marie
Gas rich galaxies are typically star-forming. We make use of HI-MaNGA, a program of HI follow-up for the Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey of the Sloan Digital Sky Surveys to construct a sample of unusual neutral hydr
Externí odkaz:
http://arxiv.org/abs/2309.04854