Zobrazeno 1 - 9
of 9
pro vyhledávání: '"C. P. Haines"'
Publikováno v:
Astronomy & Astrophysics. 658:A190
(Abridged) We explored 18 clusters from LoCuSS at z~0.2 with ACReS spectra of ~1800 cluster members at R
Comment: Accepted for publication in A&A; 10 pages, 4 figures, 3 tables; language edited version
Comment: Accepted for publication in A&A; 10 pages, 4 figures, 3 tables; language edited version
Autor:
John E. Carlstrom, J. Démoclès, Alexis Finoguenov, Rossella Martino, Pasquale Mazzotta, Graham P. Smith, C. P. Haines, Arya Farahi, Daniel P. Marrone, August E. Evrard, Sarah L. Mulroy, H. Bourdin, Sean L. McGee, Nobuhiro Okabe, Zubair Abdulla, Christine O'Donnell
Publikováno v:
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2019, 484 (1), pp.60-80. ⟨10.1093/mnras/sty3484⟩
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2019, 484 (1), pp.60-80. ⟨10.1093/mnras/sty3484⟩
Mon.Not.Roy.Astron.Soc., 2019, 484 (1), pp.60-80. ⟨10.1093/mnras/sty3484⟩
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2019, 484 (1), pp.60-80. ⟨10.1093/mnras/sty3484⟩
We present a simultaneous analysis of galaxy cluster scaling relations between weak-lensing mass and multiple cluster observables, across a wide range of wavelengths, that probe both gas and stellar content. Our new hierarchical Bayesian model simult
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4714dbf65c5e605acf550562f589883e
Autor:
Graham P. Smith, Rossella Martino, Alexis Finoguenov, Ian G. McCarthy, Keiichi Umetsu, Yannick M. Bahé, M. Lieu, Paul Edward May, Sarah L. Mulroy, Arif Babul, Pasquale Mazzotta, Hervé Bourdin, August E. Evrard, Daniel P. Marrone, Nobuhiro Okabe, Mathilde Jauzac, Toshifumi Futamase, F. Ziparo, C. P. Haines, James E. Taylor
Publikováno v:
Monthly notices of the Royal Astronomical Society : letters, 2016, Vol.456(1), pp.L74-L78 [Peer Reviewed Journal]
We test the assumption of hydrostatic equilibrium in an X-ray luminosity selected sample of 50 galaxy clusters at $0.15
Comment: 5 pages, 1 figure, accepted by MNRAS
Comment: 5 pages, 1 figure, accepted by MNRAS
Autor:
J. Démoclès, Nobuhiro Okabe, Steven Gillman, Eiichi Egami, C. P. Haines, Sean L. McGee, Graham P. Smith, Sarah L. Mulroy
Publikováno v:
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2017, 472 (3), pp.3246-3255. ⟨10.1093/mnras/stx2108⟩
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2017, 472 (3), pp.3246-3255. ⟨10.1093/mnras/stx2108⟩
Monthly Notices of the Royal Astronomical Society, 2017, 472 (3), pp.3246-3255. ⟨10.1093/mnras/stx2108⟩
Mon.Not.Roy.Astron.Soc., 2017, 472 (3), pp.3246-3255. ⟨10.1093/mnras/stx2108⟩
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2017, 472 (3), pp.3246-3255. ⟨10.1093/mnras/stx2108⟩
Monthly Notices of the Royal Astronomical Society, 2017, 472 (3), pp.3246-3255. ⟨10.1093/mnras/stx2108⟩
We study a sample of 19 galaxy clusters in the redshift range $0.15
Comment: 11 Pages, 9 Figures, 3 Tables. MNRAS, in press
Comment: 11 Pages, 9 Figures, 3 Tables. MNRAS, in press
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::17ae4e6ae31c84390e031ee60de6f4c1
http://arxiv.org/abs/1708.05971
http://arxiv.org/abs/1708.05971
Autor:
Paola Merluzzi, Michael A. Dopita, Amata Mercurio, Sabine Schindler, A Rifatto, C. P. Haines, G. Busarello, Dominik Steinhauser, Russell J. Smith
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 429:1747-1773
We study the case of a bright (L>L*) barred spiral galaxy from the rich cluster A3558 in the Shapley supercluster core (z=0.05) undergoing ram-pressure stripping. Integral-field spectroscopy, complemented by multi-band imaging, allows us to reveal th
Autor:
Alexis Finoguenov, M. J. Pereira, Arif Babul, Eiichi Egami, C. P. Haines, Sarah L. Mulroy, Daniel P. Marrone, Nobuhiro Okabe, Graham P. Smith, Rossella Martino
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Artículos CONICYT
CONICYT Chile
instacron:CONICYT
Artículos CONICYT
CONICYT Chile
instacron:CONICYT
We present the first scaling relation between weak-lensing galaxy cluster mass, $M_{WL}$, and near-infrared luminosity, $L_K$. Our results are based on 17 clusters observed with wide-field instruments on Subaru, the United Kingdom Infrared Telescope,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::eee1dce61a2481d8548ffdb900d656c8
http://arxiv.org/abs/1407.1767
http://arxiv.org/abs/1407.1767
Autor:
Graham P. Smith, Alastair J. R. Sanderson, C. P. Haines, G. Busarello, Eiichi Egami, T. D. Rawle, Arif Babul, Alexis Finoguenov, Paola Merluzzi, Nobuhiro Okabe, M. J. Pereira
We present an analysis of the levels and evolution of star formation activity in a representative sample of 30 massive galaxy clusters at 0.1510^10 M_sun) star-forming cluster galaxies within r200 are found to be systematically 28% lower than their c
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2518bb97718e52860001b81bea0b54f0
Autor:
David J. E. Floyd, Stanislav S. Shabala, Kevin A. Pimbblet, C. P. Haines, Amelia Fraser-McKelvie
[Abridged] We present an analysis of optical spectroscopically-identified AGN to M*+1 in a sample of 6 self-similar SDSS galaxy clusters at z=0.07. These clusters are specifically selected to lack significant substructure at bright limits in their ce
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ab0eeb5f4e8386a5e6484fb4fddc736a
Autor:
F. Ziparo, Eiichi Egami, T. D. Rawle, Alexis Finoguenov, Sean Moran, Graham P. Smith, M. J. Pereira, C. P. Haines, Nobuhiro Okabe, Sean L. McGee, Arif Babul
Publikováno v:
Astrophysical Journal
Artículos CONICYT
CONICYT Chile
instacron:CONICYT
Artículos CONICYT
CONICYT Chile
instacron:CONICYT
We present a study of the spatial distribution and kinematics of star-forming galaxies in 30 massive clusters at 0.15 < z < 0.30, combining wide-field Spitzer 24 μm and GALEX near-ultraviolet imaging with highly complete spectroscopy of cluster memb