The WaZP galaxy cluster sample of the dark energy survey year 1

Autor: G. Tarle, David J. Brooks, Antonella Palmese, David J. James, Josh Frieman, M. A. G. Maia, Pablo Fosalba, F. Paz-Chinchón, Michael Schubnell, M. Smith, Agnès Ferté, Samuel Hinton, Christophe Benoist, E. Suchyta, Basilio X. Santiago, August E. Evrard, G. Gutierrez, I. Ferrero, Sunayana Bhargava, J. Carretero, R. D. Wilkinson, B. Flaugher, H. Sampaio-Santos, Peter Melchior, Santiago Avila, K. Honscheid, R. L. C. Ogando, J. De Vicente, S. Everett, M. Carrasco Kind, S. Desai, Ramon Miquel, I. Sevilla-Noarbe, Juan Garcia-Bellido, Ofer Lahav, M. Soares-Santos, N. Kuropatkin, L. N. da Costa, Robert Morgan, A. Carnero Rosell, M. Costanzi, Marcos Lima, D. L. Hollowood, S. Serrano, Chun-Hao To, E. J. Sanchez, Douglas L. Tucker, Kyler Kuehn, Paul Giles, E. Bertin, J. Gschwend, Peter Doel, H. T. Diehl, David Bacon, S. Allam, Robert A. Gruendl, Tesla E. Jeltema, A. A. Plazas, Michel Aguena, A. K. Romer

Publikováno v: Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2021, 502 (3), pp.4435-4456. ⟨10.1093/mnras/stab264⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname

Aguena, M., et al.
We present a new (2+1)D galaxy cluster finder based on photometric redshifts called Wavelet Z Photometric (WaZP) applied to DES first year (Y1A1) data. The results are compared to clusters detected by the South Pole Telescope

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2bf100add5832cf598f9ac7736f86453
https://hal.archives-ouvertes.fr/hal-02939982

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