Table A.1
First series of XXL articles.
| Num. | The XXL Survey | Authors |
|
|
||
| I | Scientific motivations −XMM-Newton observing plan − | Pierre, Pacaud, Adami et al. |
| Follow-up observations and simulation programme | ||
| II | The bright cluster sample | Pacaud, Clerc, Giles et al. |
| III | Luminosity-temperature relation of the bright cluster sample | Giles, Maughan, Pacaud et al. |
| IV | Mass-temperature relation of the bright cluster sample | Lieu, Smith, Giles et al. |
| V | Detection of the Sunyaev-Zel’dovich effect | Mantz, Abdul, Carlstrom et al. |
| of the redshift 1.9 galaxy cluster XLSSU J021744.1-034536 with CARMA | ||
| VI | The 1000 brightest X-ray point sources | Fotopoulou, Pacaud, Paltani et al. |
| VII | A supercluster of galaxies at z = 0.43 | Pompei, Adami, Eckert et al. |
| VIII | MUSE characterisation of intra-cluster light in a z = 0.53 cluster of galaxies | Adami, Pompei, Sadibekova et al. |
| IX | Optical overdensity and radio continuum analysis of a supercluster at z = 0.43 | Baran, Smolčić, Milaković et al. |
| X | Weak-lensing mass − | Ziparo, Smith, Mulroy et al. |
| K-band luminosity relation for groups and clusters of galaxies | ||
| XI | ATCA 2.1 GHz continuum observations | Smolčić, Delahize, Huynh et al. |
| XII | Optical spectroscopy of X-ray selected clusters | Koulouridis, Poggianti, Altieri et al. |
| and the frequency of AGNs in superclusters | ||
| XIII | The baryon content of the bright cluster sample | Eckert, Ettori, Coupon et al. |
| XIV | AAOmega redshifts for the southern XXL field | Lidman, Ardila, Owers et al. |
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