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21 results on '"Birkinshaw, M"'

1. The XXL Survey

Author

Adam, R., primary, Ricci, M., additional, Eckert, D., additional, Ade, P., additional, Ajeddig, H., additional, Altieri, B., additional, André, P., additional, Artis, E., additional, Aussel, H., additional, Beelen, A., additional, Benoist, C., additional, Benoît, A., additional, Berta, S., additional, Bing, L., additional, Birkinshaw, M., additional, Bourrion, O., additional, Boutigny, D., additional, Bremer, M., additional, Calvo, M., additional, Cappi, A., additional, Catalano, A., additional, De Petris, M., additional, Désert, F.-X., additional, Doyle, S., additional, Driessen, E. F. C., additional, Faccioli, L., additional, Ferrari, C., additional, Gastaldello, F., additional, Giles, P., additional, Gomez, A., additional, Goupy, J., additional, Hahn, O., additional, Hanser, C., additional, Horellou, C., additional, Kéruzoré, F., additional, Koulouridis, E., additional, Kramer, C., additional, Ladjelate, B., additional, Lagache, G., additional, Leclercq, S., additional, Lestrade, J.-F., additional, Macías-Pérez, J. F., additional, Madden, S., additional, Maughan, B., additional, Maurogordato, S., additional, Maury, A., additional, Mauskopf, P., additional, Monfardini, A., additional, Muñoz-Echeverría, M., additional, Pacaud, F., additional, Perotto, L., additional, Pierre, M., additional, Pisano, G., additional, Pompei, E., additional, Ponthieu, N., additional, Revéret, V., additional, Rigby, A., additional, Ritacco, A., additional, Romero, C., additional, Roussel, H., additional, Ruppin, F., additional, Sereno, M., additional, Schuster, K., additional, Sievers, A., additional, Tintoré Vidal, G., additional, Tucker, C., additional, and Zylka, R., additional

Published
2024
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2. The XXL Survey I. Scientific Motivations - Xmm-Newton Observing Plan - Follow-up Observations and Simulation Programme

Author

Pierre, M, Pacaud, F, Adami, C, Alis, S, Altieri, B, Baran, N, Benoist, C, Birkinshaw, M, Bongiorno, A, Bremer, M. N, Brusa, M, Butler, A, Ciliegi, P, Chiappetti, L, Clerc, N, Corasaniti, P. S, Coupon, J, De Breuck, C, Democles, J, Desai, S, Delhaize, J, Devriendt, J, Dubois, Y, Snowden, Steven L, and Eckert, D

Subjects
Astrophysics
Abstract

The quest for the cosmological parameters that describe our universe continues to motivate the scientific community to undertake very large survey initiatives across the electromagnetic spectrum. Over the past two decades, the Chandra and XMM-Newton observatories have supported numerous studies of X-ray-selected clusters of galaxies, active galactic nuclei (AGNs), and the X-ray background. The present paper is the first in a series reporting results of the XXL-XMM survey; it comes at a time when the Planck mission results are being finalized. Aims. We present the XXL Survey, the largest XMM programme totaling some 6.9 Ms to date and involving an international consortium of roughly 100 members. The XXL Survey covers two extragalactic areas of 25 deg2 each at a point-source sensitivity of approx. 5 x 10(exp 15) erg/s/sq cm in the [0.5-2] keV band (completeness limit). The surveys main goals are to provide constraints on the dark energy equation of state from the space-time-distribution of clusters of galaxies and to serve as a pathfinder for future, wide-area X-ray missions. We review science objectives, including cluster studies, AGN evolution, and large-scale structure, that are being conducted with the support of approximately 30 follow-up programs. Methods. We describe the 542 XMM observations along with the associated multi- and numerical simulation programmes. We give a detailed account of the X-ray processing steps and describe innovative tools being developed for the cosmological analysis. Results. The paper provides a thorough evaluation of the X-ray data, including quality controls, photon statistics, exposure and background maps, and sky coverage. Source catalogue construction and multi-associations are briefly described. This material will be the basis for the calculation of the cluster and AGN selection functions, critical elements of the cosmological and science analyses. Conclusions. The XXL multi- data set will have a unique lasting legacy value for cosmological and extragalactic studies and will serve asa calibration resource for future dark energy studies with clusters and other X-ray selected sources. With the present article, we release the XMM XXL photon and smoothed images along with the corresponding exposure maps.

Published
2016
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3. The XXL Survey

Author

Ricci, M., primary, Adam, R., additional, Eckert, D., additional, Ade, P., additional, André, P., additional, Andrianasolo, A., additional, Altieri, B., additional, Aussel, H., additional, Beelen, A., additional, Benoist, C., additional, Benoît, A., additional, Berta, S., additional, Bideaud, A., additional, Birkinshaw, M., additional, Bourrion, O., additional, Boutigny, D., additional, Bremer, M., additional, Calvo, M., additional, Cappi, A., additional, Chiappetti, L., additional, Catalano, A., additional, De Petris, M., additional, Désert, F.-X., additional, Doyle, S., additional, Driessen, E. F. C., additional, Faccioli, L., additional, Ferrari, C., additional, Fotopoulou, S., additional, Gastaldello, F., additional, Giles, P., additional, Gomez, A., additional, Goupy, J., additional, Hahn, O., additional, Horellou, C., additional, Kéruzoré, F., additional, Koulouridis, E., additional, Kramer, C., additional, Ladjelate, B., additional, Lagache, G., additional, Leclercq, S., additional, Lestrade, J.-F., additional, Macías-Pérez, J. F., additional, Maughan, B., additional, Maurogordato, S., additional, Mauskopf, P., additional, Monfardini, A., additional, Pacaud, F., additional, Perotto, L., additional, Pierre, M., additional, Pisano, G., additional, Pompei, E., additional, Ponthieu, N., additional, Revéret, V., additional, Ritacco, A., additional, Romero, C., additional, Roussel, H., additional, Ruppin, F., additional, Sánchez Portal, M., additional, Schuster, K., additional, Sereno, M., additional, Shu, S., additional, Sievers, A., additional, Tucker, C., additional, and Umetsu, K., additional

Published
2020
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4. The XXL Survey

Author

Šlaus, B., primary, Smolčić, V., additional, Novak, M., additional, Fotopoulou, S., additional, Ciliegi, P., additional, Jurlin, N., additional, Ceraj, L., additional, Tisanić, K., additional, Birkinshaw, M., additional, Bremer, M., additional, Chiappetti, L., additional, Horellou, C., additional, Huynh, M., additional, Intema, H., additional, Kolokythas, K., additional, Pierre, M., additional, Raychaudhury, S., additional, and Rottgering, H., additional

Published
2020
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5. The XXL Survey

Author

Eyles, R. A. J., primary, Birkinshaw, M., additional, Smolčić, V., additional, Horellou, C., additional, Huynh, M., additional, Butler, A., additional, Delhaize, J., additional, Vignali, C., additional, and Pierre, M., additional

Published
2019
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6. The intergalactic magnetic field probed by a giant radio galaxy

Author

O’Sullivan, S. P., primary, Machalski, J., additional, Van Eck, C. L., additional, Heald, G., additional, Brüggen, M., additional, Fynbo, J. P. U., additional, Heintz, K. E., additional, Lara-Lopez, M. A., additional, Vacca, V., additional, Hardcastle, M. J., additional, Shimwell, T. W., additional, Tasse, C., additional, Vazza, F., additional, Andernach, H., additional, Birkinshaw, M., additional, Haverkorn, M., additional, Horellou, C., additional, Williams, W. L., additional, Harwood, J. J., additional, Brunetti, G., additional, Anderson, J. M., additional, Mao, S. A., additional, Nikiel-Wroczyński, B., additional, Takahashi, K., additional, Carretti, E., additional, Vernstrom, T., additional, van Weeren, R. J., additional, Orrú, E., additional, Morabito, L. K., additional, and Callingham, J. R., additional

Published
2019
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7. The XXL Survey

Author

Pacaud, F., primary, Pierre, M., additional, Melin, J.-B., additional, Adami, C., additional, Evrard, A. E., additional, Galli, S., additional, Gastaldello, F., additional, Maughan, B. J., additional, Sereno, M., additional, Alis, S., additional, Altieri, B., additional, Birkinshaw, M., additional, Chiappetti, L., additional, Faccioli, L., additional, Giles, P. A., additional, Horellou, C., additional, Iovino, A., additional, Koulouridis, E., additional, Le Fèvre, J.-P., additional, Lidman, C., additional, Lieu, M., additional, Maurogordato, S., additional, Moscardini, L., additional, Plionis, M., additional, Poggianti, B. M., additional, Pompei, E., additional, Sadibekova, T., additional, Valtchanov, I., additional, and Willis, J. P., additional

Published
2018
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8. The XXL Survey

Author

Guglielmo, V., primary, Poggianti, B. M., additional, Vulcani, B., additional, Adami, C., additional, Gastaldello, F., additional, Ettori, S., additional, Fotoupoulou, S., additional, Koulouridis, E., additional, Ramos Ceja, M. E., additional, Giles, P., additional, McGee, S., additional, Altieri, B., additional, Baldry, I., additional, Birkinshaw, M., additional, Bolzonella, M., additional, Bongiorno, A., additional, Brown, M., additional, Chiappetti, L., additional, Driver, S., additional, Elyiv, A., additional, Evrard, A., additional, Garilli, B., additional, Grootes, M., additional, Guennou, L., additional, Hopkins, A., additional, Horellou, C., additional, Iovino, A., additional, Lidman, C., additional, Liske, J., additional, Maurogordato, S., additional, Owers, M., additional, Pacaud, F., additional, Paltani, S., additional, Pierre, M., additional, Plionis, M., additional, Ponman, T., additional, Robotham, A., additional, Sadibekova, T., additional, Scodeggio, M., additional, Sereno, M., additional, Smolčić, V., additional, Tuffs, R., additional, Valtchanov, I., additional, Vignali, C., additional, and Willis, J., additional

Published
2018
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9. The XXL Survey

Author

Horellou, C., primary, Intema, H. T., additional, Smolčić, V., additional, Nilsson, A., additional, Karlsson, F., additional, Krook, C., additional, Tolliner, L., additional, Adami, C., additional, Benoist, C., additional, Birkinshaw, M., additional, Caretta, C., additional, Chiappetti, L., additional, Delhaize, J., additional, Ferrari, C., additional, Fotopoulou, S., additional, Guglielmo, V., additional, Kolokythas, K., additional, Pacaud, F., additional, Pierre, M., additional, Poggianti, B. M., additional, Ramos-Ceja, M. E., additional, Raychaudhury, S., additional, Röttgering, H. J. A., additional, and Vignali, C., additional

Published
2018
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10. The XXL Survey

Author

Marulli, F., primary, Veropalumbo, A., additional, Sereno, M., additional, Moscardini, L., additional, Pacaud, F., additional, Pierre, M., additional, Plionis, M., additional, Cappi, A., additional, Adami, C., additional, Alis, S., additional, Altieri, B., additional, Birkinshaw, M., additional, Ettori, S., additional, Faccioli, L., additional, Gastaldello, F., additional, Koulouridis, E., additional, Lidman, C., additional, Le Fèvre, J.-P., additional, Maurogordato, S., additional, Poggianti, B., additional, Pompei, E., additional, Sadibekova, T., additional, and Valtchanov, I., additional

Published
2018
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11. The XXL Survey

Author

Logan, C. H. A., primary, Maughan, B. J., additional, Bremer, M. N., additional, Giles, P., additional, Birkinshaw, M., additional, Chiappetti, L., additional, Clerc, N., additional, Faccioli, L., additional, Koulouridis, E., additional, Pacaud, F., additional, Pierre, M., additional, Ramos-Ceja, M. E., additional, Vignali, C., additional, and Willis, J., additional

Published
2018
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12. The XXL Survey

Author

Adami, C., primary, Pompei, E., additional, Sadibekova, T., additional, Clerc, N., additional, Iovino, A., additional, McGee, S. L., additional, Guennou, L., additional, Birkinshaw, M., additional, Horellou, C., additional, Maurogordato, S., additional, Pacaud, F., additional, Pierre, M., additional, Poggianti, B., additional, and Willis, J., additional

Published
2016
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13. The XXL Survey

Author

Pacaud, F., primary, Clerc, N., additional, Giles, P. A., additional, Adami, C., additional, Sadibekova, T., additional, Pierre, M., additional, Maughan, B. J., additional, Lieu, M., additional, Le Fèvre, J. P., additional, Alis, S., additional, Altieri, B., additional, Ardila, F., additional, Baldry, I., additional, Benoist, C., additional, Birkinshaw, M., additional, Chiappetti, L., additional, Démoclès, J., additional, Eckert, D., additional, Evrard, A. E., additional, Faccioli, L., additional, Gastaldello, F., additional, Guennou, L., additional, Horellou, C., additional, Iovino, A., additional, Koulouridis, E., additional, Le Brun, V., additional, Lidman, C., additional, Liske, J., additional, Maurogordato, S., additional, Menanteau, F., additional, Owers, M., additional, Poggianti, B., additional, Pomarède, D., additional, Pompei, E., additional, Ponman, T. J., additional, Rapetti, D., additional, Reiprich, T. H., additional, Smith, G. P., additional, Tuffs, R., additional, Valageas, P., additional, Valtchanov, I., additional, Willis, J. P., additional, and Ziparo, F., additional

Published
2016
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14. The XXL Survey

Author

Pierre, M., primary, Pacaud, F., additional, Adami, C., additional, Alis, S., additional, Altieri, B., additional, Baran, N., additional, Benoist, C., additional, Birkinshaw, M., additional, Bongiorno, A., additional, Bremer, M. N., additional, Brusa, M., additional, Butler, A., additional, Ciliegi, P., additional, Chiappetti, L., additional, Clerc, N., additional, Corasaniti, P. S., additional, Coupon, J., additional, De Breuck, C., additional, Democles, J., additional, Desai, S., additional, Delhaize, J., additional, Devriendt, J., additional, Dubois, Y., additional, Eckert, D., additional, Elyiv, A., additional, Ettori, S., additional, Evrard, A., additional, Faccioli, L., additional, Farahi, A., additional, Ferrari, C., additional, Finet, F., additional, Fotopoulou, S., additional, Fourmanoit, N., additional, Gandhi, P., additional, Gastaldello, F., additional, Gastaud, R., additional, Georgantopoulos, I., additional, Giles, P., additional, Guennou, L., additional, Guglielmo, V., additional, Horellou, C., additional, Husband, K., additional, Huynh, M., additional, Iovino, A., additional, Kilbinger, M., additional, Koulouridis, E., additional, Lavoie, S., additional, Le Brun, A. M. C., additional, Le Fevre, J. P., additional, Lidman, C., additional, Lieu, M., additional, Lin, C. A., additional, Mantz, A., additional, Maughan, B. J., additional, Maurogordato, S., additional, McCarthy, I. G., additional, McGee, S., additional, Melin, J. B., additional, Melnyk, O., additional, Menanteau, F., additional, Novak, M., additional, Paltani, S., additional, Plionis, M., additional, Poggianti, B. M., additional, Pomarede, D., additional, Pompei, E., additional, Ponman, T. J., additional, Ramos-Ceja, M. E., additional, Ranalli, P., additional, Rapetti, D., additional, Raychaudury, S., additional, Reiprich, T. H., additional, Rottgering, H., additional, Rozo, E., additional, Rykoff, E., additional, Sadibekova, T., additional, Santos, J., additional, Sauvageot, J. L., additional, Schimd, C., additional, Sereno, M., additional, Smith, G. P., additional, Smolčić, V., additional, Snowden, S., additional, Spergel, D., additional, Stanford, S., additional, Surdej, J., additional, Valageas, P., additional, Valotti, A., additional, Valtchanov, I., additional, Vignali, C., additional, Willis, J., additional, and Ziparo, F., additional

Published
2016
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16. Survey of planetary nebulae at 30 GHz with OCRA-p

Author

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

Published
2009
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17. The XMM-Newton serendipitous survey

Author

Barcons, X., primary, Carrera, F. J., additional, Ceballos, M. T., additional, Page, M. J., additional, Bussons-Gordo, J., additional, Corral, A., additional, Ebrero, J., additional, Mateos, S., additional, Tedds, J. A., additional, Watson, M. G., additional, Baskill, D., additional, Birkinshaw, M., additional, Boller, T., additional, Borisov, N., additional, Bremer, M., additional, Bromage, G. E., additional, Brunner, H., additional, Caccianiga, A., additional, Crawford, C. S., additional, Cropper, M. S., additional, Della Ceca, R., additional, Derry, P., additional, Fabian, A. C., additional, Guillout, P., additional, Hashimoto, Y., additional, Hasinger, G., additional, Hassall, B. J. M., additional, Lamer, G., additional, Loaring, N. S., additional, Maccacaro, T., additional, Mason, K. O., additional, McMahon, R. G., additional, Mirioni, L., additional, Mittaz, J. P. D., additional, Motch, C., additional, Negueruela, I., additional, Osborne, J. P., additional, Panessa, F., additional, Pérez-Fournon, I., additional, Pye, J. P., additional, Roberts, T. P., additional, Rosen, S., additional, Schartel, N., additional, Schurch, N., additional, Schwope, A., additional, Severgnini, P., additional, Sharp, R., additional, Stewart, G. C., additional, Szokoly, G., additional, Ullán, A., additional, Ward, M. J., additional, Warwick, R. S., additional, Wheatley, P. J., additional, Webb, N. A., additional, Worrall, D., additional, Yuan, W., additional, and Ziaeepour, H., additional

Published
2007
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20. XLIV. Sunyaev-Zel’dovich mapping of a low-mass cluster at z ∼ 1: a multi-wavelength approach

Author

Ricci, M., Adam, R., Eckert, D., Ade, P., André, P., Andrianasolo, A., Altieri, B., Aussel, H., Beelen, A., Benoist, C., Benoît, A., Berta, S., Bideaud, A., Birkinshaw, M., Bourrion, O., Boutigny, D., Bremer, M., Calvo, M., Cappi, A., Chiappetti, L., Catalano, A., De Petris, M., Désert, F.-X., Doyle, S., Driessen, E. F. C., Faccioli, L., Ferrari, C., Fotopoulou, S., Gastaldello, F., Giles, P., Gomez, A., Goupy, J., Hahn, O., Horellou, C., Kéruzoré, F., Koulouridis, E., Kramer, C., Ladjelate, B., Lagache, G., Leclercq, S., Lestrade, J.-F., Macías-Pérez, J. F., Maughan, B., Maurogordato, S., Mauskopf, P., Monfardini, A., Pacaud, F., Perotto, L., Pierre, M., Pisano, G., Pompei, E., Ponthieu, N., Revéret, V., Ritacco, A., Romero, C., Roussel, H., Ruppin, F., Sánchez Portal, M., Schuster, K., Sereno, M., Shu, S., Sievers, A., Tucker, C., and Umetsu, K.

Subjects
Astrophysics::Cosmology and Extragalactic Astrophysics
Abstract

High-mass clusters at low redshifts have been intensively studied at various wavelengths. However, while more distant objects at lower masses constitute the bulk population of future surveys, their physical state remain poorly explored to date. In this paper, we present resolved observations of the Sunyaev-Zel’dovich (SZ) effect, obtained with the NIKA2 camera, towards the cluster of galaxies XLSSC 102, a relatively low-mass system (M500 ∼ 2 × 1014 M⊙) at z = 0.97 detected from the XXL survey. We combine NIKA2 SZ data, XMM-Newton X-ray data, and Megacam optical data to explore, respectively, the spatial distribution of the gas electron pressure, the gas density, and the galaxies themselves. We find significant offsets between the X-ray peak, the SZ peak, the brightest cluster galaxy, and the peak of galaxy density. Additionally, the galaxy distribution and the gas present elongated morphologies. This is interpreted as the sign of a recent major merging event, which induced a local boost of the gas pressure towards the north of XLSSC 102 and stripped the gas out of the galaxy group. The NIKA2 data are also combined with XXL data to construct the thermodynamic profiles of XLSSC 102, obtaining relatively tight constraints up to about ∼r500, and revealing properties that are typical of disturbed systems. We also explore the impact of the cluster centre definition and the implication of local pressure substructure on the recovered profiles. Finally, we derive the global properties of XLSSC 102 and compare them to those of high-mass-and-low-redshift systems, finding no strong evidence for non-standard evolution. We also use scaling relations to obtain alternative mass estimates from our profiles. The variation between these different mass estimates reflects the difficulty to accurately measure the mass of low-mass clusters at z ∼ 1, especially with low signal-to-noise ratio data and for a disturbed system. However, it also highlights the strength of resolved SZ observations alone and in combination with survey-like X-ray data. This is promising for the study of high redshift clusters from the combination of eROSITA and high resolution SZ instruments and will complement the new generation of optical surveys from facilities such as LSST and Euclid.\ud\udKey words: techniques: high angular resolution / galaxies: clusters: individual: XLSSC 102 / galaxies: clusters: intracluster medium / X-rays: galaxies: clusters

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21. The XXL Survey

Author

Paul Giles, Cathy Horellou, Stefano Ettori, Elias Koulouridis, C. Lidman, V. Smolvcic, Mark Birkinshaw, C. Adami, M. Bolzonella, S. Paltani, T. Sadibekova, Matt S. Owers, R. J. Tuffs, Florian Pacaud, L. Chiappetti, B. Garilli, L. Guennou, S. Maurogordato, Jochen Liske, Andrii Elyiv, Trevor J. Ponman, Meiert W. Grootes, A. Iovino, M. E. Ramos Ceja, Mauro Sereno, Michael J. I. Brown, Sean L. McGee, J. L. Willis, Bruno Altieri, I. Valtchanov, Andrew M. Hopkins, Ivan K. Baldry, Angela Bongiorno, S. Fotoupoulou, Aaron S. G. Robotham, Bianca M. Poggianti, V. Guglielmo, Cristian Vignali, Simon P. Driver, August E. Evrard, Fabio Gastaldello, Benedetta Vulcani, M. Plionis, Marco Scodeggio, Marguerite Pierre, University of St Andrews. School of Physics and Astronomy, Guglielmo, V., Poggianti, B.M., Vulcani, B., Adami, C., Gastaldello, F., Ettori, S., Fotoupoulou, S., Koulouridis, E., Ramos Ceja, M.E., Giles, P., McGee, S., Altieri, B., Baldry, I., Birkinshaw, M., Bolzonella, M., Bongiorno, A., Brown, M., Chiappetti, L., Driver, S., Elyiv, A., Evrard, A., Garilli, B., Grootes, M., Guennou, L., Hopkins, A., Horellou, C., Iovino, A., Lidman, C., Liske, J., Maurogordato, S., Owers, M., Pacaud, F., Paltani, S., Pierre, M., Plionis, M., Ponman, T., Robotham, A., Sadibekova, T., Scodeggio, M., Sereno, M., Smolčić, V., Tuffs, R., Valtchanov, I., Vignali, C., Willis, J., Laboratoire d'Astrophysique de Marseille (LAM), and Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)

Subjects
luminosity function, mass function [Galaxies], Stellar mass, astro-ph.GA, FOS: Physical sciences, Astrophysics, clusters: general [Galaxies], 01 natural sciences, Virial theorem, galaxies: groups: general, 0103 physical sciences, QB Astronomy, Infrarot-Astrophysik - Abteilung Hinton, 010303 astronomy & astrophysics, QC, luminosity function [galaxies], QB, Physics, [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph], 85A04, 010308 nuclear & particles physics, X-ray, DAS, Astronomy and Astrophysics, Virial mass, evolution [Galaxies], Astrophysics - Astrophysics of Galaxies, NATURAL SCIENCES. Physics, Redshift, Galaxy, PRIRODNE ZNANOSTI. Fizika, galaxies: luminosity function, groups: general [Galaxies], QC Physics, [SDU]Sciences of the Universe [physics], galaxies: clusters: general, mass function, Space and Planetary Science, Homogeneous, Astrophysics of Galaxies (astro-ph.GA), X-rays: galaxies: clusters, galaxies: luminosity function, mass function, galaxies: clusters [X-rays], Halo, galaxies: evolution
Abstract

The fraction of galaxies bound in groups in the nearby Universe is high (50% at z~0). Systematic studies of galaxy properties in groups are important in order to improve our understanding of the evolution of galaxies and of the physical phenomena occurring within this environment. We have built a complete spectrophotometric sample of galaxies within X-ray detected, optically spectroscopically confirmed groups and clusters (G&C), covering a wide range of halo masses at z, 20 pages, 18 figures, 6 tables, accepted for publication in A&A

Published
2018

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