Zobrazeno 1 - 10 of 43 pro vyhledávání: '"C. Rodriguez-Gonzalvez"'
1
Spectroscopic Confirmation and Velocity Dispersions for 20 Planck Galaxy Clusters at 0.16 < z < 0.78
Autor: S. A. Stanford, Charles R. Lawrence, Jean-Baptiste Melin, Simona Mei, Daniel Stern, Hyunjin Shim, S. Amodeo, Ranga-Ram Chary, C. Rodriguez-Gonzalvez, James G. Bartlett, Francine R. Marleau
Publikováno v: Astrophys.J.
Astrophys.J., 2018, 853 (1), pp.36. 〈10.3847/1538-4357/aa98dd〉
Astrophys.J., 2018, 853 (1), pp.36. ⟨10.3847/1538-4357/aa98dd⟩
We present Gemini and Keck spectroscopic redshifts and velocity dispersions for 20 clusters detected via the Sunyaev–Zel'dovich (SZ) effect by the Planck space mission, with estimated masses in the range 2.3 x 10^(14) M⊙ < M^(Pl)_(500) < 9.4 x 10
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2481719d5b689678be64c50b2e0e76e0
https://hal.archives-ouvertes.fr/hal-01703664
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2
CARMA observations of massive Planck-discovered cluster candidates at z>0.5 associated with WISE overdensities: Breaking the size-flux degeneracy
Autor: Jean-Baptiste Melin, Ranga-Ram Chary, Farhan Feroz, Malak Olamaie, Stephen Muchovej, C. Rodriguez-Gonzalvez, Timothy W. Shimwell
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, 2017, 464, pp.2378. ⟨10.1093/mnras/stw2392⟩
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (ISSN 0035-8711)
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2017, 464, pp.2378. ⟨10.1093/mnras/stw2392⟩
Mon.Not.Roy.Astron.Soc., 2017, 464, pp.2378. 〈10.1093/mnras/stw2392〉
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (ISSN 0035-8711), 464, 2378-2395
Monthly Notices of the Royal Astronomical Society, 2017, 464, pp.2378. ⟨10.1093/mnras/stw2392⟩
We use a Bayesian software package to analyze CARMA-8 data towards 19 unconfirmed Planck SZ-cluster candidates from Rodriguez-Gonzalvez et al. (2015), that are associated with significant overdensities in WISE. We used two cluster parameterizations,
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5201c417f51c762e334edcf4beaf7161
https://hal.archives-ouvertes.fr/hal-01554185
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3
Sunyaev-Zel'dovich observations with AMI of the hottest galaxy clusters detected in the XMM-Newton Cluster Survey
Autor: Farhan Feroz, Michel P. Schammel, Anthony Lasenby, Clare Rumsey, Natasha Hurley-Walker, Michael P. Hobson, A. Kathy Romer, David Titterington, Elizabeth Waldram, Anna M. M. Scaife, Yvette C. Perrott, Keith Grainge, Malak Olamaie, Paul F. Scott, E. J. Lloyd-Davies, C. Rodriguez-Gonzalvez, Thomas M. O. Franzen, Richard D. E. Saunders, Guy G. Pooley
Publikováno v: Monthly Notices of the Royal Astronomical Society. 433:2920-2937
We have obtained deep Sunyaev–Zel’dovich (SZ) observations towards 15 of the hottest XMM Cluster Survey (XCS) clusters that can be observed with the Arcminute Microkelvin Imager (AMI). We use a Bayesian analysis to quantify the significance of ou
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cd462c13a84ed467afb912178b5c4876
https://doi.org/10.1093/mnras/stt932
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4
The radio source count at 93.2 GHz from observations of 9C sources using AMI and CARMA
Autor: C. Rodriguez-Gonzalvez, Natasha Hurley-Walker, I. H. Whittam, Elizabeth Waldram, Michel P. Schammel, Irina I. Stefan, Anthony Lasenby, David Titterington, R. Bolton, Michael P. Hobson, Keith Grainge, Guy G. Pooley, Yvette C. Perrott, Timothy W. Shimwell, Matthew L. Davies, John M. Carpenter, Richard D. E. Saunders, Anna M. M. Scaife, Julia M. Riley, David A. Green, Paul F. Scott, Malak Olamaie, T. M. O. Franzen
Publikováno v: Monthly Notices of the Royal Astronomical Society. 430:1961-1969
We present results from follow-up observations of a sample of 80 radio sources, originally detected as part of the 15.2-GHz Ninth Cambridge (9C) survey. The observations were carried out, close to simultaneously, at two frequencies: 15.7 GHz, using t
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::daee6263b10f46657b1a1fbdc3579038
https://doi.org/10.1093/mnras/stt016
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5
A blind detection of a large, complex, Sunyaev-Zel’dovich structure★
Autor: M. Crofts, Jonathan T. L. Zwart, D. M. Odell, Natasha Hurley-Walker, John Ely, J. Czeres, M. L. Davies, Roger Dace, Harry Smith, Anthony Lasenby, E. M. Waldram, M. Olamaie, M. Felvus, Keith Grainge, Michael L. Brown, Michael P. Hobson, O. Norris, W. Flynn, D. Bly, T. Culverhouse, William F. Grainger, Ghassan Yassin, Richard D. E. Saunders, V. Quy, Philip J. Marshall, P. Biddulph, Timothy W. Shimwell, Ricardo Génova-Santos, A. R. Brown, Anna M. M. Scaife, J. Schofield, C. M. Holler, R. Jilley, R. W. Barker, M. Velić, David Titterington, Guy G. Pooley, J. Geisbüsch, B. A. Wood, R. D'Alessandro, D. Hammett, F. Newton, S. West, C. Rodriguez-Gonzalvez, C. Clementson, Michel P. Schammel, Paul F. Scott, C. Shaw, Marian Pospieszalski, T. Kaneko, Roger C. Boysen, Farhan Feroz, T. M. O. Franzen, R. Kneissl, Y. C. Perrott J. C. Pober, K. Duggan, Katy Lancaster, I. Northrop, P. Doherty
Publikováno v: Monthly Notices of the Royal Astronomical Society. 423:1463-1473
We present an interesting Sunyaev-Zel'dovich (SZ) detection in the first of the Arcminute Microkelvin Imager (AMI) 'blind', degree-square fields to have been observed down to our target sensitivity of 100{\mu}Jy/beam. In follow-up deep pointed observ
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::314e5a91efc059fa4761627da718db24
https://doi.org/10.1111/j.1365-2966.2012.20970.x
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7
Akademický článek
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8
Akademický článek
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9
Akademický článek
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10
Future Science Prospects for AMI
Autor: Keith Grainge, P {Alexander}, Richard Battye, M {Birkinshaw}, A {Blain}, M {Bremer}, Sarah Bridle, M {Brown}, R {Davis}, Clive Dickinson, A {Edge}, G {Efstathiou}, R {Fender}, M {Hardcastle}, J {Hatchell}, M {Hobson}, M {Jarvis}, B {Maughan}, I {McHardy}, M {Middleton}, A {Lasenby}, R {Saunders}, G {Savini}, A {Scaife}, G {Smith}, M {Thompson}, G {White}, K {Zarb-Adami}, J {Allison}, J {Buckle}, A {Castro-Tirado}, M {Chernyakova}, R {Deane}, F {Feroz}, R {Genova Santos}, D {Green}, D {Hannikainen}, I {Heywood}, N {Hurley-Walker}, R {Kneissl}, K {Koljonen}, S {Kulkarni}, S {Markoff}, C {MacTavish}, M {McCollough}, S {Migliari}, J M {Miller}, J {Miller-Jones}, M {Olamaie}, Z {Paragi}, T {Pearson}, G {Pooley}, K {Pottschmidt}, R {Rebolo}, J {Richer}, J {Riley}, J {Rodriguez}, C {Rodriguez-Gonzalvez}, A {Rushton}, P {Savolainen}, P {Scott}, T {Shimwell}, M {Tavani}, J {Tomsick}, V {Tudose}, K {van der Heyden}, A {van der Horst}, A {Varlotta}, E {Waldram}, J {Wilms}, A {Zdziarski}, J {Zwart}, Y {Perrott}, C {Rumsey}, M {Schammel}
Publikováno v: University of Manchester-PURE
NASA Astrophysics Data System
The Arcminute Microkelvin Imager (AMI) is a telescope specifically designed for high sensitivity measurements of low-surface-brightness features at cm-wavelength and has unique, important capabilities. It consists of two interferometer arrays operati
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cffb6e062983cf7d54f15c19308945df
https://research.manchester.ac.uk/en/publications/5cecc657-6f3f-4271-92e4-83a3d2db31f5
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