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Start Over Author "Birkinshaw, M" Journal monthly notices of the royal astronomical society
223 results on '"Birkinshaw, M"'

2. The XXL Survey – XLVIII. X-ray follow-up of distant XXL clusters: masses, scaling relations, and AGN contamination

Author

Duffy, R T, primary, Logan, C H A, additional, Maughan, B J, additional, Eckert, D, additional, Birkinshaw, M, additional, Clerc, N, additional, Ettori, S, additional, Gastaldello, F, additional, Koulouridis, E, additional, Pierre, M, additional, Ricci, M, additional, Sereno, M, additional, Valtchanov, I, additional, and Willis, J P, additional

Published
2022
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3. XXL Survey – XLVIII. X-ray follow-up of distant XXL clusters: masses, scaling relations, and AGN contamination†.

Author

Duffy, R T, Logan, C H A, Maughan, B J, Eckert, D, Birkinshaw, M, Clerc, N, Ettori, S, Gastaldello, F, Koulouridis, E, Pierre, M, Ricci, M, Sereno, M, Valtchanov, I, and Willis, J P

Subjects
REDSHIFT, X-rays, ACTIVE galactic nuclei, GALAXY clusters
Abstract

We use deep follow-up XMM–Newton observations of six clusters discovered in the XXL Survey at z > 1 to gain robust measurements of their X-ray properties and to investigate the extent to which scaling relations at low redshift are valid at z > 1. This sample is unique as it has been investigated for active galactic nucleus (AGN) contamination, which ensures measurements are not undermined by systematic uncertainties, and pushes to lower mass at higher redshift than is usually possible, for example with Sunyaev–Zel'dovich (SZ) selected clusters. We determine the flux contribution of point sources to the XXL cluster flux in order to test for the presence of AGN in other high-redshift cluster candidates, and find 3XLSS J231626.8−533822 to be a point source misclassified as a cluster and 3XLSS J232737.3−541618 to be a genuine cluster. We present the first attempt to measure the hydrostatic masses in a bright subsample of z > 1 X-ray selected galaxy clusters with a known selection function. Periods of high particle background significantly reduced the effective exposure times of observations (losing >50 per cent in some cases) limiting the power of this study. When combined with complementary SZ selected cluster samples at higher masses, the data appear broadly consistent with the self-similar evolution of the low redshift scaling relations between intracluster medium properties and cluster mass, suggesting that properties such as the X-ray temperature, gas mass, and SZ signal remain reliable mass proxies even at high redshift. [ABSTRACT FROM AUTHOR]

Published
2022
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9. The X-ray ribs within the cocoon shock of Cygnus A

Author

Duffy, R T, primary, Worrall, D M, additional, Birkinshaw, M, additional, Nulsen, P E J, additional, Wise, M W, additional, de Vries, M N, additional, Snios, B, additional, Mathews, W G, additional, Perley, R A, additional, Hardcastle, M J, additional, Rafferty, D A, additional, McNamara, B R, additional, Edge, A C, additional, McKean, J P, additional, Carilli, C L, additional, Croston, J H, additional, Godfrey, L E H, additional, and Laing, R A, additional

Published
2018
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10. Candidate high-z protoclusters among the Planck compact sources, as revealed by Herschel–SPIRE

Author

Greenslade, J, primary, Clements, D L, additional, Cheng, T, additional, De Zotti, G, additional, Scott, D, additional, Valiante, E, additional, Eales, S, additional, Bremer, M N, additional, Dannerbauer, H, additional, Birkinshaw, M, additional, Farrah, D, additional, Harrison, D L, additional, Michałowski, M J, additional, Valtchanov, I, additional, Oteo, I, additional, Baes, M, additional, Cooray, A, additional, Negrello, M, additional, Wang, L, additional, van der Werf, P, additional, Dunne, L, additional, and Dye, S, additional

Published
2018
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12. AMI-LA observations of the SuperCLASS supercluster

Author

Riseley, C J, primary, Grainge, K J B, additional, Perrott, Y C, additional, Scaife, A M M, additional, Battye, R A, additional, Beswick, R J, additional, Birkinshaw, M, additional, Brown, M L, additional, Casey, C M, additional, Demetroullas, C, additional, Hales, C A, additional, Harrison, I, additional, Hung, C-L, additional, Jackson, N J, additional, Muxlow, T, additional, Watson, B, additional, Cantwell, T M, additional, Carey, S H, additional, Elwood, P J, additional, Hickish, J, additional, Jin, T Z, additional, Razavi-Ghods, N, additional, Scott, P F, additional, and Titterington, D J, additional

Published
2017
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13. The SCUBA-2 Cosmology Legacy Survey: the nature of bright submm galaxies from 2 deg2 of 850-μm imaging

Author

Michałowski, Michał J., primary, Dunlop, J. S., additional, Koprowski, M. P., additional, Cirasuolo, M., additional, Geach, J. E., additional, Bowler, R. A. A., additional, Mortlock, A., additional, Caputi, K. I., additional, Aretxaga, I., additional, Arumugam, V., additional, Chen, Chian-Chou, additional, McLure, R. J., additional, Birkinshaw, M., additional, Bourne, N., additional, Farrah, D., additional, Ibar, E., additional, van der Werf, P., additional, and Zemcov, M., additional

Published
2017
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15. The SCUBA-2 Cosmology Legacy Survey: 850 μm maps, catalogues and number counts

Author

Geach, J. E., primary, Dunlop, J. S., additional, Halpern, M., additional, Smail, Ian, additional, van der Werf, P., additional, Alexander, D. M., additional, Almaini, O., additional, Aretxaga, I., additional, Arumugam, V., additional, Asboth, V., additional, Banerji, M., additional, Beanlands, J., additional, Best, P. N., additional, Blain, A. W., additional, Birkinshaw, M., additional, Chapin, E. L., additional, Chapman, S. C., additional, Chen, C-C., additional, Chrysostomou, A., additional, Clarke, C., additional, Clements, D. L., additional, Conselice, C., additional, Coppin, K. E. K., additional, Cowley, W. I., additional, Danielson, A. L. R., additional, Eales, S., additional, Edge, A. C., additional, Farrah, D., additional, Gibb, A., additional, Harrison, C. M., additional, Hine, N. K., additional, Hughes, D., additional, Ivison, R. J., additional, Jarvis, M., additional, Jenness, T., additional, Jones, S. F., additional, Karim, A., additional, Koprowski, M., additional, Knudsen, K. K., additional, Lacey, C. G., additional, Mackenzie, T., additional, Marsden, G., additional, McAlpine, K., additional, McMahon, R., additional, Meijerink, R., additional, Michałowski, M. J., additional, Oliver, S. J., additional, Page, M. J., additional, Peacock, J. A., additional, Rigopoulou, D., additional, Robson, E. I., additional, Roseboom, I., additional, Rotermund, K., additional, Scott, Douglas, additional, Serjeant, S., additional, Simpson, C., additional, Simpson, J. M., additional, Smith, D. J. B., additional, Spaans, M., additional, Stanley, F., additional, Stevens, J. A., additional, Swinbank, A. M., additional, Targett, T., additional, Thomson, A. P., additional, Valiante, E., additional, Wake, D. A., additional, Webb, T. M. A., additional, Willott, C., additional, Zavala, J. A., additional, and Zemcov, M., additional

Published
2016
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16. The SCUBA-2 Cosmology Legacy Survey: the EGS deep field – I. Deep number counts and the redshift distribution of the recovered cosmic infrared background at 450 and 850 μ m

Author

Zavala, J. A., primary, Aretxaga, I., additional, Geach, J. E., additional, Hughes, D. H., additional, Birkinshaw, M., additional, Chapin, E., additional, Chapman, S., additional, Chen, Chian-Chou, additional, Clements, D. L., additional, Dunlop, J. S., additional, Farrah, D., additional, Ivison, R. J., additional, Jenness, T., additional, Michałowski, M. J., additional, Robson, E. I., additional, Scott, Douglas, additional, Simpson, J., additional, Spaans, M., additional, and van der Werf, P., additional

Published
2016
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17. Deep observations of the Super-CLASS supercluster at 325 MHz with the GMRT: the low-frequency source catalogue

Author

Riseley, C. J., primary, Scaife, A. M. M., additional, Hales, C. A., additional, Harrison, I., additional, Birkinshaw, M., additional, Battye, R. A., additional, Beswick, R. J., additional, Brown, M. L., additional, Casey, C. M., additional, Chapman, S. C., additional, Demetroullas, C., additional, Hung, C.-L., additional, Jackson, N. J., additional, Muxlow, T., additional, and Watson, B., additional

Published
2016
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21. DeepChandraobservations of Pictor A

Author

Hardcastle, M. J., primary, Lenc, E., additional, Birkinshaw, M., additional, Croston, J. H., additional, Goodger, J. L., additional, Marshall, H. L., additional, Perlman, E. S., additional, Siemiginowska, A., additional, Stawarz, Ł., additional, and Worrall, D. M., additional

Published
2015
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22. AMI-LA observations of the SuperCLASS supercluster.

Author

Riseley, C. J., Grainge, K. J. B., Perrott, Y. C., Scaife, A. M. M., Battye, R. A., Beswick, R. J., Birkinshaw, M., Brown, M. L., Casey, C. M., Demetroullas, C., Hales, C. A., Harrison, I., Hung, C.-L., Jackson, N. J., Muxlow, T., Watson, B., Cantwell, T. M., Carey, S. H., Elwood, P. J., and Hickish, J.

Subjects
SUPERCLUSTERS, GALAXY spectra, GALAXIES, RADIO astronomy, ASTROMETRIC telescopes
Abstract

We present a deep survey of the Super-Cluster Assisted Shear Survey (SuperCLASS) supercluster – a region of sky known to contain five Abell clusters at redshift z ∼ 0.2 – performed using the Arcminute Microkelvin Imager (AMI) Large Array (LA) at 15.5 GHz. Our survey covers an area of approximately 0.9 deg2.We achieve a nominal sensitivity of 32.0 μJy beam−1 towards the field centre, finding 80 sources above a 5σ threshold. We derive the radio colour– colour distribution for sources common to three surveys that cover the field and identify three sources with strongly curved spectra – a high-frequency-peaked source and two GHz-peakedspectrum sources. The differential source count (i) agrees well with previous deep radio source counts, (ii) exhibits no evidence of an emerging population of star-forming galaxies, down to a limit of 0.24 mJy, and (iii) disagrees with some models of the 15 GHz source population. However, our source count is in agreement with recent work that provides an analytical correction to the source count from the Square Kilometre Array Design Study (SKADS) Simulated Sky, supporting the suggestion that this discrepancy is caused by an abundance of flat-spectrum galaxy cores as yet not included in source population models. [ABSTRACT FROM AUTHOR]

Published
2018
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23. Physical conditions of the interstellar medium of high-redshift, strongly lensed submillimetre galaxies from theHerschel-ATLAS

Author

Valtchanov, I, Virdee, J, Ivison, RJ, Swinyard, B, van der Werf, P, Rigopoulou, D, da Cunha, E, Lupu, R, Benford, DJ, Riechers, D, Smail, I, Jarvis, M, Pearson, C, Gomez, H, Hopwood, R, Altieri, B, Birkinshaw, M, Coia, D, Conversi, L, Cooray, A, De Zotti, G, Dunne, L, Frayer, D, Leeuw, L, Marston, A, Negrello, M, Portal, MS, Scott, D, Thompson, MA, Vaccari, M, Baes, M, Clements, D, Michałowski, MJ, Dannerbauer, H, Serjeant, S, Auld, R, Buttiglione, S, Cava, A, Dariush, A, Dye, S, Eales, S, Fritz, J, Ibar, E, Maddox, S, Pascale, E, Pohlen, M, Rigby, E, Rodighiero, G, Smith, DJB, Temi, P, Carpenter, J, Bolatto, A, and Gurwell, M

Published
2011

26. The SCUBA-2 Cosmology Legacy Survey: the nature of bright submm galaxies from 2 deg2 of 850-μm imaging.

Author

Michałowski, Michał J., Dunlop, J. S., Koprowski, M. P., Cirasuolo, M., Geach, J. E., Bowler, R. A. A., Mortlock, A., Caputi, K. I., Aretxaga, I., Arumugam, V., Chian-Chou Chen, McLure, R. J., Birkinshaw, M., Bourne, N., Farrah, D., Ibar, E., van der Werf, P., and Zemcov, M.

Subjects
COSMIC dust, INTERSTELLAR reddening, GALACTIC evolution, REDSHIFT, STAR formation, SUBMILLIMETER astronomy
Abstract

We present physical properties [redshifts (z), star-formation rates (SFRs) and stellar masses (Mstar)] of bright (S850 ≥ 4 mJy) submm galaxies in the ≃2 deg2 COSMOS and UDS fields selected with SCUBA-2/JCMT.We complete the galaxy identification process for all (≃2000) S/N ≥ 3.5 850-μm sources, but focus our scientific analysis on a high-quality subsample of 651 S/N ≥ 4 sources with complete multiwavelength coverage including 1.1-mm imaging. We check the reliability of our identifications, and the robustness of the SCUBA-2 fluxes by revisiting the recent ALMA follow-up of 29 sources in our sample. Considering >4mJy ALMA sources, our identification method has a completeness of ≃86 per cent with a reliability of ≃92 per cent, and only ≃15–20 per cent of sources are significantly affected by multiplicity (when a secondary component contributes >1/3 of the primary source flux). The impact of source blending on the 850-μmsource counts as determined with SCUBA-2 ismodest; scaling the single-dish fluxes by ≃0.9 reproduces the ALMA source counts. For our final SCUBA- 2 sample, we find median z = 2.40+0.10 −0.04, SFR = 287 ± 6M⊫ yr−1 and log(Mstar/M⊫) = 11.12 ± 0.02 (the latter for 349/651 sources with optical identifications). These properties clearly locate bright submm galaxies on the high-mass end of the ‘main sequence’ of starforming galaxies out to z ≃ 6, suggesting that major mergers are not a dominant driver of the high-redshift submm-selected population. Their number densities are also consistent with the evolving galaxy stellar mass function. Hence, the submm galaxy population is as expected, albeit reproducing the evolution of the main sequence of star-forming galaxies remains a challenge for theoretical models/simulations. [ABSTRACT FROM AUTHOR]

Published
2017
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27. The SCUBA-2 Cosmology Legacy Survey: 850 µm maps, catalogues and number counts.

Author

Geach, J. E., Dunlop, J. S., Halpern, M., Smail, Ian, van der Werf, P., Alexander, D. M., Almaini, O., Aretxaga, I., Arumugam, V., Asboth, V., Banerji, M., Beanlands, J., Best, P. N., Blain, A. W., Birkinshaw, M., Chapin, E. L., Chapman, S. C., Chen, C-C., Chrysostomou, A., and Clarke, C.

Subjects
SUBMILLIMETER astronomy, TELESCOPES, GALACTIC redshift, PHENOMENOLOGICAL theory (Physics), GALACTIC evolution, METAPHYSICAL cosmology
Abstract

We present a catalogue of ~3000 submillimetre sources detected (=3.5s) at 850 µm over ~5 deg² surveyed as part of the James Clerk Maxwell Telescope (JCMT) SCUBA-2 Cosmology Legacy Survey (S2CLS). This is the largest survey of its kind at 850 µm, increasing the sample size of 850 µm selected submillimetre galaxies by an order of magnitude. The wide 850 µm survey component of S2CLS covers the extragalactic fields: UKIDSS-UDS, COSMOS, Akari-NEP, Extended Groth Strip, Lockman Hole North, SSA22 and GOODS-North. The average 1s depth of S2CLS is 1.2 mJy beam-1, approaching the SCUBA-2 850 µm confusion limit, which we determine to be sc ≈ 0.8 mJy beam-1.We measure the 850 µm number counts, reducing the Poisson errors on the differential counts to approximately 4 per cent at S850 ≈ 3 mJy. With several independent fields, we investigate field-to-field variance, finding that the number counts on 0.5°-1° scales are generally within 50 per cent of the S2CLS mean for S850 > 3 mJy, with scatter consistent with the Poisson and estimated cosmic variance uncertainties, although there is a marginal (2s) density enhancement in GOODS-North. The observed counts are in reasonable agreement with recent phenomenological and semi-analytic models, although determining the shape of the faint-end slope (S850 < 3 mJy) remains a key test. The large solid angle of S2CLS allows us to measure the bright-end counts: at S850 > 10 mJy there are approximately 10 sources per square degree, and we detect the distinctive up-turn in the number counts indicative of the detection of local sources of 850 µm emission, and strongly lensed high-redshift galaxies. All calibrated maps and the catalogue are made publicly available. [ABSTRACT FROM AUTHOR]

Published
2017
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29. Deep Chandra observations of Pictor A.

Author

Hardcastle, M. J., Lenc, E., Birkinshaw, M., Croston, J. H., Goodger, J. L., Marshall, H. L., Perlman, E. S., Siemiginowska, A., Stawarz, Ł., and Worrall, D. M.

Subjects
ATOMIC charges, ELECTRON distribution, MAGNETIC fields, ELECTROMAGNETIC theory, FIELD theory (Physics)
Abstract

We report on deep Chandra observations of the nearby broad-line radio galaxy Pictor A, which we combine with new Australia Telescope Compact Array (ATCA) observations. The new X-ray data have a factor of 4 more exposure than observations previously presented and span a 15 yr time baseline, allowing a detailed study of the spatial, temporal and spectral properties of theAGN, jet, hotspot and lobes.We present evidence for further time variation of the jet, though the flare that we reported in previouswork remains the most significantly detected time-varying feature. We also confirm previous tentative evidence for a faint counterjet. Based on the radio through X-ray spectrum of the jet and its detailed spatial structure, and on the properties of the counterjet, we argue that inverse-Compton models can be conclusively rejected, and propose that the X-ray emission from the jet is synchrotron emission from particles accelerated in the boundary layer of a relativistic jet. For the first time, we find evidence that the bright western hotspot is also time-varying in X-rays, and we connect this to the small-scale structure in the hotspot seen in high-resolution radio observations. The new data allow us to confirm that the spectrum of the lobes is in good agreement with the predictions of an inverse-Compton model and we show that the data favour models in which the filaments seen in the radio images are predominantly the result of spatial variation of magnetic fields in the presence of a relatively uniform electron distribution. [ABSTRACT FROM AUTHOR]

Published
2016
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35. Erratum: One Centimetre Receiver Array-prototype observations of the CRATES sources at 30 GHz

Author

Peel, M. W., primary, Gawroński, M. P., additional, Battye, R. A., additional, Birkinshaw, M., additional, Browne, I. W. A., additional, Davis, R. J., additional, Feiler, R., additional, Kus, A. J., additional, Lancaster, K., additional, Lowe, S. R., additional, Pazderska, B. M., additional, Pazderski, E., additional, Roukema, B. F., additional, and Wilkinson, P. N., additional

Published
2011
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36. Physical conditions of the interstellar medium of high-redshift, strongly lensed submillimetre galaxies from the Herschel-ATLAS★

Author

Valtchanov, I., primary, Virdee, J., additional, Ivison, R. J., additional, Swinyard, B., additional, van der Werf, P., additional, Rigopoulou, D., additional, da Cunha, E., additional, Lupu, R., additional, Benford, D. J., additional, Riechers, D., additional, Smail, Ian, additional, Jarvis, M., additional, Pearson, C., additional, Gomez, H., additional, Hopwood, R., additional, Altieri, B., additional, Birkinshaw, M., additional, Coia, D., additional, Conversi, L., additional, Cooray, A., additional, De Zotti, G., additional, Dunne, L., additional, Frayer, D., additional, Leeuw, L., additional, Marston, A., additional, Negrello, M., additional, Portal, M. Sanchez, additional, Scott, D., additional, Thompson, M. A., additional, Vaccari, M., additional, Baes, M., additional, Clements, D., additional, Michałowski, M. J., additional, Dannerbauer, H., additional, Serjeant, S., additional, Auld, R., additional, Buttiglione, S., additional, Cava, A., additional, Dariush, A., additional, Dye, S., additional, Eales, S., additional, Fritz, J., additional, Ibar, E., additional, Maddox, S., additional, Pascale, E., additional, Pohlen, M., additional, Rigby, E., additional, Rodighiero, G., additional, Smith, D. J. B., additional, Temi, P., additional, Carpenter, J., additional, Bolatto, A., additional, Gurwell, M., additional, and Vieira, J. D., additional

Published
2011
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37. One Centimetre Receiver Array-prototype observations of the CRATES sources at 30 GHz

Author

Peel, M. W., primary, Gawroński, M. P., additional, Battye, R. A., additional, Birkinshaw, M., additional, Browne, I. W. A., additional, Davis, R. J., additional, Feiler, R., additional, Kus, A. J., additional, Lancaster, K., additional, Lowe, S. R., additional, Pazderska, B. M., additional, Pazderski, E., additional, Roukema, B. F., additional, and Wilkinson, P. N., additional

Published
2010
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39. 30 GHz observations of sources in the Very Small Array fields

Author

Gawroński, M. P., primary, Peel, M. W., additional, Lancaster, K., additional, Battye, R. A., additional, Birkinshaw, M., additional, Browne, I. W. A., additional, Davies, M. L., additional, Davis, R. J., additional, Feiler, R., additional, Franzen, T. M. O., additional, Génova-Santos, R., additional, Kus, A. J., additional, Lowe, S. R., additional, Pazderska, B. M., additional, Pazderski, E., additional, Pooley, G. G., additional, Roukema, B. F., additional, Waldram, E. M., additional, and Wilkinson, P. N., additional

Published
2010
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42. High-energy particle acceleration at the radio-lobe shock of Centaurus A

Author

Croston, J. H., primary, Kraft, R. P., additional, Hardcastle, M. J., additional, Birkinshaw, M., additional, Worrall, D. M., additional, Nulsen, P. E. J., additional, Penna, R. F., additional, Sivakoff, G. R., additional, Jordán, A., additional, Brassington, N. J., additional, Evans, D. A., additional, Forman, W. R., additional, Gilfanov, M., additional, Goodger, J. L., additional, Harris, W. E., additional, Jones, C., additional, Juett, A. M., additional, Murray, S. S., additional, Raychaudhury, S., additional, Sarazin, C. L., additional, Voss, R., additional, and Woodley, K. A., additional

Published
2009
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45. The XMM-Large Scale Structure catalogue: X-ray sources and associated optical data. Version I

Author

Pierre, M., primary, Chiappetti, L., additional, Pacaud, F., additional, Gueguen, A., additional, Libbrecht, C., additional, Altieri, B., additional, Aussel, H., additional, Gandhi, P., additional, Garcet, O., additional, Gosset, E., additional, Paioro, L., additional, Ponman, T. J., additional, Read, A. M., additional, Refregier, A., additional, Starck, J.- L., additional, Surdej, J., additional, Valtchanov, I., additional, Adami, C., additional, Alloin, D., additional, Alshino, A., additional, Andreon, S., additional, Birkinshaw, M., additional, Bremer, M., additional, Detal, A., additional, Duc, P.- A., additional, Galaz, G., additional, Jones, L., additional, Le Fevre, J.- P., additional, Le Fevre, O., additional, Maccagni, D., additional, Mazure, A., additional, Quintana, H., additional, Rottgering, H. J. A., additional, Sprimont, P.- G., additional, Tasse, C., additional, Trinchieri, G., additional, and Willis, J. P., additional

Published
2007
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46. The XMM-LSS survey: the Class 1 cluster sample over the initial 5 deg2 and its cosmological modelling

Author

Pacaud, F., primary, Pierre, M., additional, Adami, C., additional, Altieri, B., additional, Andreon, S., additional, Chiappetti, L., additional, Detal, A., additional, Duc, P.-A., additional, Galaz, G., additional, Gueguen, A., additional, Le Fèvre, J.-P., additional, Hertling, G., additional, Libbrecht, C., additional, Melin, J.-B., additional, Ponman, T. J., additional, Quintana, H., additional, Refregier, A., additional, Sprimont, P.-G., additional, Surdej, J., additional, Valtchanov, I., additional, Willis, J. P., additional, Alloin, D., additional, Birkinshaw, M., additional, Bremer, M. N., additional, Garcet, O., additional, Jean, C., additional, Jones, L. R., additional, Le Fèvre, O., additional, Maccagni, D., additional, Mazure, A., additional, Proust, D., additional, Röttgering, H. J. A., additional, and Trinchieri, G., additional

Published
2007
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50. Erratum: The XMM Large-Scale Structure survey: an initial sample of galaxy groups and clusters to a redshift z < 0.6

Author

Willis, J. P., primary, Pacaud, F., additional, Valtchanov, I., additional, Pierre, M., additional, Ponman, T., additional, Read, A., additional, Andreon, S., additional, Altieri, B., additional, Quintana, H., additional, Santos, S. Dos, additional, Birkinshaw, M., additional, Bremer, M., additional, Duc, P.-A., additional, Galaz, G., additional, Gosset, E., additional, Jones, L., additional, and Surdej, J., additional

Published
2005
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