Zobrazeno 1 - 7
of 7
pro vyhledávání: '"Maria, Manolopoulou"'
Autor:
Paul Giles, Phil A. James, Maria Manolopoulou, K. Furnell, R. D. Wilkinson, Pedro T. P. Viana, Chris A. Collins, Carlos Vergara, Lee S. Kelvin, Ivan K. Baldry, A. Bermeo, Sunayana Bhargava, Robert G. Mann, Matt Hilton, John P. Stott, Julian A. Mayers, A. Kathy Romer
Publikováno v:
Furnell, K E, Collins, C A, Kelvin, L S, Baldry, I K, James, P A, Manolopoulou, M, Mann, R G, Giles, P A, Bermeo, A, Hilton, M, Wilkinson, R, Romer, A K, Vergara, C, Bhargava, S, Stott, J P, Mayers, J & Viana, P 2021, ' The Growth of Intracluster Light in XCS-HSC Galaxy Clustersfrom 0.1 < z < 0.5 ', Monthly Notices of the Royal Astronomical Society, vol. 502, no. 2, pp. 2419-2437 . https://doi.org/10.1093/mnras/stab065
We estimate the Intracluster Light (ICL) component within a sample of 18 clusters detected in XMM Cluster Survey (XCS) data using deep ($\sim$ 26.8 mag) Hyper Suprime Cam Subaru Strategic Program DR1 (HSC-SSP DR1) $i$-band data. We apply a rest-frame
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b6e7d6193713fe619653858924893618
https://doi.org/10.1093/mnras/stab065
https://doi.org/10.1093/mnras/stab065
Publikováno v:
Manolopoulou, M, Hoyle, B, Mann, R G, Sahlen, M & Nadathur, S 2021, ' Environmental dependence of X-ray and optical properties of galaxy clusters ', Monthly Notices of the Royal Astronomical Society, vol. 500, no. 2, pp. 1953-1963 . https://doi.org/10.1093/mnras/staa3341
Galaxy clusters are widely used to constrain cosmological parameters through their properties, such as masses, luminosity and temperature distributions. One should take into account all kind of biases that could affect these analyses in order to obta
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e6bcc7deb71c9e0fa32537b173189c89
https://researchportal.port.ac.uk/ws/files/25155544/staa3341.pdf
https://researchportal.port.ac.uk/ws/files/25155544/staa3341.pdf
Autor:
R. D. Wilkinson, Matt Hilton, P. Rooney, Chris A. Collins, Tesla E. Jeltema, C. Vergara, Maria Manolopoulou, Pedro T. P. Viana, John P. Stott, A. Bermeo, Paul Giles, A. K. Romer, E. Swann, S. Rosborough, K. Sabirli, Julian A. Mayers, Sunayana Bhargava
There have been several reports of a detection of an unexplained excess of X-ray emission at $\simeq$ 3.5 keV in astrophysical systems. One interpretation of this excess is the decay of sterile neutrino dark matter. The most influential study to date
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c830796bb93e79f02ae39c156e973ecb
https://doi.org/10.1093/mnras/staa1829
https://doi.org/10.1093/mnras/staa1829
Dark Energy Surveyed Year 1 results: calibration of cluster mis-centring in the redMaPPer catalogues
Autor:
W. G. Hartley, C. Stern, Devon L. Hollowood, John P. Stott, Ramon Miquel, A. Bermeo, B. Flaugher, Martin Sahlén, Chris A. Collins, Eli S. Rykoff, Elisabeth Krause, Tesla E. Jeltema, Yanxi Zhang, Shantanu Desai, C. J. Miller, Arya Farahi, A. A. Plazas, J. Gschwend, Marcelle Soares-Santos, M. E. C. Swanson, M. Costanzi, Xi Chen, Vinu Vikram, J. P. Dietrich, R. H. Schindler, Juan Garcia-Bellido, W. C. Wester, E. Bertin, David J. Brooks, M. Klein, A. Carnero Rosell, J. Carretero, Peter Melchior, Sunayana Bhargava, M. Smith, Eduardo Rozo, Jennifer L. Marshall, Daniel Gruen, G. Gutierrez, S. W. Allen, D. L. Burke, Peter Doel, R. D. Wilkinson, Maria Manolopoulou, S. Allam, Robert A. Gruendl, Pablo Fosalba, K. Honscheid, H. T. Diehl, V. Scarpine, S. Everett, G. Tarle, August E. Evrard, Ricardo L. C. Ogando, Julian A. Mayers, J. De Vicente, Ben Hoyle, Daniel Thomas, Felipe Menanteau, Robert G. Mann, M. A. G. Maia, A. von der Linden, G. Morris, Risa H. Wechsler, E. Suchyta, Matt Hilton, S. Serrano, M. Carrasco Kind, C. Vergara Cervantes, Marcos Lima, I. Sevilla-Noarbe, Enrique Gaztanaga, N. Kuropatkin, M. Splettstoesser, Adam Mantz, L. N. da Costa, Joshua A. Frieman, Douglas L. Tucker, Kyler Kuehn, Paul Giles, A. K. Romer, Santiago Avila, Keith Bechtol, F. J. Castander, Pedro T. P. Viana, E. J. Sanchez
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2019, 487 (2), pp.2578-2593. ⟨10.1093/mnras/stz1361⟩
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2019, 487 (2), pp.2578-2593. ⟨10.1093/mnras/stz1361⟩
Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual)
Universidade de São Paulo (USP)
instacron:USP
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2019, 487 (2), pp.2578-2593. ⟨10.1093/mnras/stz1361⟩
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2019, 487 (2), pp.2578-2593. ⟨10.1093/mnras/stz1361⟩
Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual)
Universidade de São Paulo (USP)
instacron:USP
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
The center determination of a galaxy cluster from an optical cluster finding algorithm can be offset from theoretical prescriptions or $N$-body definitions of its host halo center. These offsets impact the recovered cluster statistics, affecting both
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::debd3002da00ae696baab94cd2d9efe5
Autor:
Manolis Plionis, Maria Manolopoulou
We study the possible rotation of cluster galaxies, developing, testing and applying a novel algorithm which identifies rotation, if such does exist, as well as its rotational centre, its axis orientation, rotational velocity amplitude and, finally,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4cefeef899de9d66197a50a1be565dde
Autor:
Michaela, Diehl, Maria, Manolopoulou, Jörn, Risse, Tilman, Kranert, Christian, Menzel, Natascha, Döbert, Frank, Grünwald
Publikováno v:
Acta medica Austriaca. 31(3)
Twenty patients suffering from malignancy received furosemide, twenty patients were examined by FDG-PET without diuretics. Urine volume and radioactivity were measured before and after acquisition. Bladder activity was evaluated qualitatively and qua
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=pmid________::33e3cf039e3125e38876d831cff412c5
https://pubmed.ncbi.nlm.nih.gov/15515481
https://pubmed.ncbi.nlm.nih.gov/15515481
Autor:
H. Wilcox, Pedro T. P. Viana, John P. Stott, A. Kathy Romer, Ayumu Terukina, David Bacon, Julian A. Mayers, Maria Manolopoulou, Andrew R. Liddle, Ross Hood, Christopher J. Miller, Nicola Mehrtens, Kazuya Koyama, Matt Hilton, P. Rooney, Martin Sahlén, Chris A. Collins, Robert C. Nichol, Gong-Bo Zhao, Robert G. Mann
Publikováno v:
Wilcox, H, Bacon, D, Nichol, R C, Rooney, P J, Terukina, A, Romer, A K, Koyama, K, Zhao, G-B, Hood, R, Mann, R G, Hilton, M, Manolopoulou, M, Sahlen, M, Collins, C A, Liddle, A R, Mayers, J A, Mehrtens, N, Miller, C J, Stott, J P & Viana, P T P 2015, ' The XMM Cluster Survey : testing chameleon gravity using the profiles of clusters ', Monthly Notices of the Royal Astronomical Society, vol. 452, no. 2, pp. 1171-1183 . https://doi.org/10.1093/mnras/stv1366
Wilcox, H, Bacon, D, Nichol, R C, Rooney, P J, Terukina, A, Romer, A K, Koyama, K, Zhao, G-B, Hood, R, Mann, R G, Hilton, M, Manolopoulou, M, Sahlen, M, Collins, C A, Liddle, A R, Mayers, J A, Mehrtens, N, Miller, C J, Stott, J P & Viana, P T P 2015, ' The XMM Cluster Survey : Testing chameleon gravity using the profiles of clusters ', Monthly Notices of the Royal Astronomical Society, vol. 452, no. 2, pp. 1171-1183 . https://doi.org/10.1093/mnras/stv1366
Wilcox, H, Bacon, D, Nichol, R C, Rooney, P J, Terukina, A, Romer, A K, Koyama, K, Zhao, G-B, Hood, R, Mann, R G, Hilton, M, Manolopoulou, M, Sahlen, M, Collins, C A, Liddle, A R, Mayers, J A, Mehrtens, N, Miller, C J, Stott, J P & Viana, P T P 2015, ' The XMM Cluster Survey : Testing chameleon gravity using the profiles of clusters ', Monthly Notices of the Royal Astronomical Society, vol. 452, no. 2, pp. 1171-1183 . https://doi.org/10.1093/mnras/stv1366
The chameleon gravity model postulates the existence of a scalar field that couples with matter to mediate a fifth force. If it exists, this fifth force would influence the hot X-ray emitting gas filling the potential wells of galaxy clusters. Howeve
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1d0c6d104a82eed2d779303228a7918a
https://researchonline.ljmu.ac.uk/id/eprint/1976/1/MNRAS-2015-Wilcox-1171-83.pdf
https://researchonline.ljmu.ac.uk/id/eprint/1976/1/MNRAS-2015-Wilcox-1171-83.pdf