Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Manolopoulou, Maria"'
Autor:
Furnell, Kate E., Collins, Chris A., Kelvin, Lee S., Baldry, Ivan K., James, Phil A., Manolopoulou, Maria, Mann, Robert G., Giles, Paul A., Bermeo, Alberto, Hilton, Matthew, Wilkinson, Reese, Romer, A. Kathy, Vergara, Carlos, Bhargava, Sunayana, Stott, John P., Mayers, Julian, Viana, Pedro
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:
http://arxiv.org/abs/2101.01644
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:
http://arxiv.org/abs/2010.12671
Autor:
Ebrahimpour, Leyla, Viana, Pedro T. P., Manolopoulou, Maria, Vergara-Cervantes, Carlos, Romer, A. Kathy, Bhargava, Sunayana, Giles, Paul, Bermeo-Hernandez, Alberto, Collins, Chris A., Hilton, Matt, Hoyle, Ben, Liddle, Andrew R., Mann, Robert G., Mayers, Julian A., Miller, Christopher J., Nichol, Robert C., Rooney, Philip J., Sahlén, Martin, Stott, John P.
We characterize the X-ray luminosity--temperature ($L_{\rm X}-T$) relation using a sample of 353 clusters and groups of galaxies with temperatures in excess of 1 keV, spanning the redshift range $0.1 < z < 0.6$, the largest ever assembled for this pu
Externí odkaz:
http://arxiv.org/abs/1805.03465
Autor:
Wilcox, Harry, Bacon, David, Nichol, Robert C., Rooney, Philip J., Terukina, Ayumu, Romer, A. Kathy, Koyama, Kazuya, Zhao, Gong-Bo, Hood, Ross, Mann, Robert G., Hilton, Matt, Manolopoulou, Maria, Sahlen, Martin, Collins, Chris A., Liddle, Andrew R., Mayers, Julian A., Mehrtens, Nicola, Miller, Christopher J., Stott, John P., Viana, Pedro T. P.
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:
http://arxiv.org/abs/1504.03937
Autor:
Manolopoulou, Maria
Galaxy clusters are very useful astronomical tools; they are used as a means to study galaxy formation and evolution, large scale structure, but also as probes to constrain cosmological parameters. This work aims to explore some of the uses of galaxy
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______463::b69dc86e8be442ae8503aa554fda1dda
http://hdl.handle.net/1842/35894
http://hdl.handle.net/1842/35894
Autor:
Viana, Pedro T P, Manolopoulou, Maria, Vergara-Cervantes, Carlos, A Kathy Romer, Sunayana Bhargava, Giles, Paul, Bermeo-Hernandez, Alberto, Collins, Chris A, Hilton, Matt, Hoyle, Ben, Liddle, Andrew R, Mann, Robert G, Mayers, Julian A, Miller, Christopher J, Nichol, Robert C, Rooney, Philip J, Sahlén, Martin, Stott, John P
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4a862f39e8ffbdeccd1b8c4c32a1c7db
Autor:
Furnell, Kate E, Collins, Chris A, Kelvin, Lee S, Baldry, Ivan K, James, Phil A, Manolopoulou, Maria, Mann, Robert G, Giles, Paul A, Bermeo, Alberto, Hilton, Matthew, Wilkinson, Reese, Romer, A Kathy, Vergara, Carlos, Bhargava, Sunayana, Stott, John P, Mayers, Julian, Viana, Pedro
Publikováno v:
Monthly Notices of the Royal Astronomical Society; Apr2021, Vol. 502 Issue 2, p2419-2437, 19p
Autor:
Diehl, Michaela1 M.Diehl@em.uni-frankfurt.de, Manolopoulou, Maria1, Risse, Jörn1, Kranert, Tilman1, Menzel, Christian1, Döbert, Natascha1, Grünwald, Frank1
Publikováno v:
Acta Medica Austriaca. 2004, Vol. 31 Issue 3, p76-78. 3p. 1 Chart.
Autor:
Ebrahimpour, Leyla, Viana, Pedro T. P., Manolopoulou, Maria, Vergara-Cervantes, Carlos, Romer, A. Kathy, Bhargava, Sunayana, Giles, Paul, Bermeo-Hernandez, Alberto, Collins, Chris A., Hilton, Matt, Hoyle, Ben, Andrew Liddle, Mann, Robert G., Mayers, Julian A., Miller, Christopher J., Nichol, Robert C., Rooney, Philip J., Sahlén, Martin, Stott, John P.
Publikováno v:
INSPIRE-HEP
We characterize the X-ray luminosity--temperature ($L_{\rm X}-T$) relation using a sample of 353 clusters and groups of galaxies with temperatures in excess of 1 keV, spanning the redshift range $0.1 < z < 0.6$, the largest ever assembled for this pu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5363bd8561eeca4e28a273116ec72c51
http://inspirehep.net/record/1672420
http://inspirehep.net/record/1672420