A new step forward in realistic cluster lens mass modelling: Analysis of Hubble Frontier Field Cluster Abell S1063 from joint lensing, X-ray and galaxy kinematics data

Autor: Beauchesne, Benjamin, Clément, Benjamin, Hibon, Pascale, Limousin, Marceau, Eckert, Dominique, Kneib, Jean-Paul, Richard, Johan, Natarajan, Priyamvada, Jauzac, Mathilde, Montes, Mireia, Mahler, Guillaume, Claeyssens, Adélaïde, Jeanneau, Alexandre, Koekemoer, Anton M., Lagattuta, David, Pagul, Amanda, Sánchez, Javier

We present a new method to simultaneously/self-consistently model the mass distribution of galaxy clusters that combines constraints from strong lensing features, X-ray emission and galaxy kinematics measurements. We are able to successfully decompos

Externí odkaz: http://arxiv.org/abs/2301.10907

The BUFFALO HST Survey

Autor: Steinhardt, Charles L., Jauzac, Mathilde, Acebron, Ana, Atek, Hakim, Capak, Peter, Davidzon, Iary, Eckert, Dominique, Harvey, David, Koekemoer, Anton M., Lagos, Claudia D. P., Mahler, Guillaume, Montes, Mireia, Niemiec, Anna, Nonino, Mario, Oesch, P. A., Richard, Johan, Rodney, Steven A., Schaller, Matthieu, Sharon, Keren, Strolger, Louis-Gregory, Allingham, Joseph, Amara, Adam, Bah'e, Yannick, Boehm, Celine, Bose, Sownak, Bouwens, Rychard J., Bradley, Larry D., Brammer, Gabriel, Broadhurst, Tom, Canas, Rodrigo, Cen, Renyue, Clement, Benjamin, Clowe, Douglas, Coe, Dan, Connor, Thomas, Darvish, Behnam, Diego, Jose M., Ebeling, Harald, Edge, A. C., Egami, Eiichi, Ettori, Stefano, Faisst, Andreas L., Frye, Brenda, Furtak, Lukas J., Gomez-Guijarro, C., Gonzalez, J. D. Remolina, Gonzalez, Anthony, Graur, Or, Gruen, Daniel, Hensley, Hagan, Hovis-Afflerbach, Beryl, Jablonka, Pascale, Jha, Saurabh W., Jullo, Eric, Kneib, Jean-Paul, Kokorev, Vasily, Lagattuta, David J., Limousin, Marceau, von der Linden, Anja, Linzer, Nora B., Lopez, Adrian, Magdis, Georgios E., Massey, Richard, Masters, Daniel C., Maturi, Matteo, McCully, Curtis, McGee, Sean L., Meneghetti, Massimo, Mobasher, Bahram, Moustakas, Leonidas A., Murphy, Eric J., Natarajan, Priyamvada, Neyrinck, Mark, O'Connor, Kyle, Oguri, Masamune, Pagul, Amanda, Rhodes, Jason, Rich, R. Michael, Robertson, Andrew, Sereno, Mauro, Shan, Huanyuan, Smith, Graham P., Sneppen, Albert, Squires, Gordon K., Tam, Sut-Ieng, Tchernin, Celine, Toft, Sune, Umetsu, Keiichi, Weaver, John R., van Weeren, R. J., Williams, Liliya L. R., Wilson, Tom J., Yan, Lin, Zitrin, Adi

The Beyond Ultra-deep Frontier Fields and Legacy Observations (BUFFALO) is a 101 orbit + 101 parallel Cycle 25 Hubble Space Telescope Treasury program taking data from 2018-2020. BUFFALO will expand existing coverage of the Hubble Frontier Fields (HF

Externí odkaz: http://arxiv.org/abs/2001.09999

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Is diffuse intracluster light a good tracer of the galaxy cluster matter distribution?

Autor: R. L. C. Ogando, Brian Yanny, Enrique Gaztanaga, Antonella Palmese, E. Suchyta, S. Everett, August E. Evrard, M. A. G. Maia, Matt Hilton, Tesla E. Jeltema, A. Choi, J. Carretero, Douglas L. Tucker, Kyler Kuehn, G. Tarle, K. Honscheid, M. Costanzi, Michel Aguena, J. Gschwend, David J. James, M. Carrasco Kind, Ofer Lahav, D. L. Burke, Pablo Fosalba, Scarpine, Markus Rau, Chang Chihway, B. Flaugher, S. Allam, Robert A. Gruendl, T. M. C. Abbott, D. L. Hollowood, David J. Brooks, A. A. Plazas, M. March, Basilio X. Santiago, Ben Hoyle, Josh Frieman, Jesse B. Golden-Marx, J. Annis, J. De Vicente, E. J. Sanchez, Mohr Joe, N. Kuropatkin, T. N. Varga, L. N. da Costa, Santiago Avila, Chihway Chang, Jennifer L. Marshall, F. Paz-Chinchón, Michael Schubnell, H. Sampaio-Santos, Pagul Amanda, Joe Zuntz, M. Smith, Daniel Gruen, T. Shin, D. W. Gerdes, M. Gatti, Samuel Hinton, G. Gutierrez, Risa H. Wechsler, Matt J. Jarvis, Yanxi Zhang, Ramon Miquel, E. Bertin, Peter Doel, K. Herner, H. T. Diehl, Juan Garcia-Bellido

Publikováno v: Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2021, 501 (1), pp.1300-1315. ⟨10.1093/mnras/staa3680⟩
Biblos-e Archivo. Repositorio Institucional de la UAM
instname

We explore the relation between diffuse intracluster light (central galaxy included) and the galaxy cluster (baryonic and dark) matter distribution using a sample of 528 clusters at $0.2\leq z \leq 0.35$ found in the Dark Energy Survey (DES) Year 1 d

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8b5865bbc708ff12480ff64f3328dd0d