Sunyaev-Zeldovich Effect (SZE) surveys have finally and successfully opened anew window to study the cosmic large-scale structure in a more promising waythan previous methods. We have performed a coordinated SZE, X-ray, andoptical/MIR survey to best understand the potential of this new survey techniqueand obtained the first exciting multi-wavelength detections. Here we propose toextent the current small test area applying the new XMM-Newton mosaic mode,which allows us to adapt our survey optimally to the depth of the SZE surveysallowing for about 100 cluster detections with XMM.
Publications
XMM-Newton detection of two clusters of galaxies with strong SPT Sunyaev-Zeldovich effect signatures |Suhada R. Song J. et al. | A&A | 514-3 | 2010 | 2010A&A...514L...3S | http://ui.adsabs.harvard.edu/#abs/2010A&A...514L...3S
The XXL Survey. I. Scientific motivations - XMM-Newton observing plan - Follow-up observations and simulation programme |Pierre M. Pacaud F. et al. | A&A | 592-1 | 2016 | 2016A&A...592A...1P | http://ui.adsabs.harvard.edu/#abs/2016A&A...592A...1P
The XXL Survey. III. Luminosity-temperature relation of the bright cluster sample |Giles P. A. Maughan B. J. et al. | A&A | 592-3 | 2016 | 2016A&A...592A...3G | http://ui.adsabs.harvard.edu/#abs/2016A&A...592A...3G
The XXL Survey. VIII. MUSE characterisation of intracluster light in a z ~ 0.53 cluster of galaxies |Adami C. Pompei E. et al. | A&A | 592-7 | 2016 | 2016A&A...592A...7A | http://ui.adsabs.harvard.edu/#abs/2016A&A...592A...7A
The XXL Survey. IX. Optical overdensity and radio continuum analysis of a supercluster at z = 0.43 |Baran N. Smolcic V. et al. | A&A | 592-8 | 2016 | 2016A&A...592A...8B | http://ui.adsabs.harvard.edu/#abs/2016A&A...592A...8B
The XXL Survey. X. K-band luminosity - weak-lensing mass relation for groups and clusters of galaxies |Ziparo F. Smith G. P. et al. | A&A | 592-9 | 2016 | 2016A&A...592A...9Z | http://ui.adsabs.harvard.edu/#abs/2016A&A...592A...9Z
Cosmological hydrodynamical simulations of galaxy clusters: X-ray scaling relations and their evolution |Truong N. Rasia E. et al. | MNRAS | 474-4089 | 2018 | 2018MNRAS.474.4089T | http://ui.adsabs.harvard.edu/#abs/2018MNRAS.474.4089T
An optically-selected cluster catalog at redshift 0.1 < z < 1.1 from the Hyper Suprime-Cam Subaru Strategic Program S16A data |Oguri Masamune Lin Yen-Ting et al. | PASJ | 70-20 | 2018 | 2018PASJ...70S..20O | http://ui.adsabs.harvard.edu/#abs/2018PASJ...70S..20O
A large sample of shear-selected clusters from the Hyper Suprime-Cam Subaru Strategic Program S16A Wide field mass maps |Miyazaki Satoshi Oguri Masamune et al. | PASJ | 70-27 | 2018 | 2018PASJ...70S..27M | http://ui.adsabs.harvard.edu/#abs/2018PASJ...70S..27M
A matched filter approach for blind joint detection of galaxy clusters in X-ray and SZ surveys |Tarrio P. Melin J.-B. | A&A | 614-82 | 2018 | 2018A&A...614A..82T | http://ui.adsabs.harvard.edu/#abs/2018A&A...614A..82T
The XXL Survey. XXVI. Optical and near-infrared identifications of the ATCA 2.1 GHz radio sources in the XXL-S Field |Ciliegi Paolo Jurlin Nika et al. | A&A | 620-11 | 2018 | 2018A&A...620A..11C | http://ui.adsabs.harvard.edu/#abs/2018A&A...620A..11C
The XXL Survey: XXX. Characterisation of the XLSSsC N01 supercluster and analysis of the galaxy stellar populations |Guglielmo V. Poggianti B. M. et al. | A&A | 620-15 | 2018 | 2018A&A...620A..15G | http://ui.adsabs.harvard.edu/#abs/2018A&A...620A..15G
The XXL Survey. XXXI. Classification and host galaxy properties of 2.1 GHz ATCA XXL-S radio sources |Butler Andrew Huynh Minh et al. | A&A | 620-16 | 2018 | 2018A&A...620A..16B | http://ui.adsabs.harvard.edu/#abs/2018A&A...620A..16B
The dependence of the X-ray AGN clustering on the properties of the host galaxy |Mountrichas G. Georgakakis A. | MNRAS | 483-1374 | 2019 | 2019MNRAS.483.1374M | http://ui.adsabs.harvard.edu/#abs/2019MNRAS.483.1374M
The XXL Survey. XVIII. ATCA 2.1 GHz radio source catalogue and source counts for the XXL-South field |Butler Andrew Huynh Minh et al. | A&A | 620-3 | 2018 | 2018A&A...620A...3B | http://ui.adsabs.harvard.edu/#abs/2018A&A...620A...3B
Quantifying baryon effects on the matter power spectrum and the weak lensing shear correlation |Schneider Aurel Teyssier Romain et al. | JCAP | 3-20 | 2019 | 2019JCAP...03..020S | http://ui.adsabs.harvard.edu/#abs/2019JCAP...03..020S
The XXL Survey. XXXVII. The role of the environment in shaping the stellar population properties of galaxies at 0.1 <= z <= 0.5 |Guglielmo V. Poggianti B. M. et al. | A&A | 625-112 | 2019 | 2019A&A...625A.112G | http://ui.adsabs.harvard.edu/#abs/2019A&A...625A.112G
The XXL Survey. XXXVI. Evolution and black hole feedback of high-excitation and low-excitation radio galaxies in XXL-S |Butler Andrew Huynh Minh et al. | A&A | 625-111 | 2019 | 2019A&A...625A.111B | http://ui.adsabs.harvard.edu/#abs/2019A&A...625A.111B
On the fast quenching of young low-mass galaxies up to z u0303 0.6: new spotlight on the lead role of environment |Moutard Thibaud Sawicki Marcin et al. | MNRAS | 479-2147 | 2018 | 2018MNRAS.479.2147M | http://ui.adsabs.harvard.edu/#abs/2018MNRAS.479.2147M
Stellar mass-halo mass relation for the brightest central galaxies of X-ray clusters since z u0303 0.65 |Erfanianfar G. Finoguenov A. et al. | A&A | 631-175 | 2019 | 2019A&A...631A.175E | http://ui.adsabs.harvard.edu/#abs/2019A&A...631A.175E
The XXL Survey. XXXVIII. Scatter and correlations of X-ray proxies in the bright XXL cluster sample |Sereno Mauro Ettori Stefano et al. | A&A | 632-54 | 2019 | 2019A&A...632A..54S | http://ui.adsabs.harvard.edu/#abs/2019A&A...632A..54S
An obscured AGN population hidden in the VIPERS galaxies: identification through spectral energy distribution decomposition |Pouliasis E. Mountrichas G. et al. | MNRAS | 495-1853 | 2020 | 2020MNRAS.495.1853P | http://ui.adsabs.harvard.edu/#abs/2020MNRAS.495.1853P
The EXOD search for faint transients in XMM-Newton observations: Method and discovery of four extragalactic Type I X-ray bursters |Pastor-Marazuela I. Webb N. A. et al. | A&A | 640-124 | 2020 | 2020A&A...640A.124P | http://ui.adsabs.harvard.edu/#abs/2020A&A...640A.124P
The XXL Survey. XLII. Detection and characterisation of the galaxy population of distant galaxy clusters in the XXL-N/VIDEO field: A tale of variety |Trudeau A. Garrel C. et al. | A&A | 642-124 | 2020 | 2020A&A...642A.124T | http://ui.adsabs.harvard.edu/#abs/2020A&A...642A.124T
The XXL Survey. XLIV. Sunyaev-Zeldovich mapping of a low-mass cluster at z u223c 1: a multi-wavelength approach |Ricci M. Adam R. et al. | A&A | 642-126 | 2020 | 2020A&A...642A.126R | http://ui.adsabs.harvard.edu/#abs/2020A&A...642A.126R
Weak-lensing clusters from HSC survey first-year data: Mitigating the dilution effect of foreground and cluster-member galaxies |Hamana Takashi Shirasaki Masato | PASJ | 72-78 | 2020 | 2020PASJ...72...78H | http://ui.adsabs.harvard.edu/#abs/2020PASJ...72...78H
The XXL Survey. XLIII. The quasar radio loudness dichotomy exposed via radio luminosity functions obtained by combining results from COSMOS and XXL-S X-ray selected quasars |Ceraj L. Smolu010diu0107 V. et al. | A&A | 642-125 | 2020 | 2020A&A...642A.125C | http://ui.adsabs.harvard.edu/#abs/2020A&A...642A.125C
GAMA/XXL: X-ray point sources in low-luminosity galaxies in the GAMA G02/XXL-N field |Nwaokoro E. Phillipps S. et al. | MNRAS | 502-3101 | 2021 | 2021MNRAS.502.3101N | http://ui.adsabs.harvard.edu/#abs/2021MNRAS.502.3101N
Active gas features in three HSC-SSP CAMIRA clusters revealed by high angular resolution analysis of MUSTANG-2 SZE and XXL X-ray observations |Okabe Nobuhiro Dicker Simon et al. | MNRAS | 501-1701 | 2021 | 2021MNRAS.501.1701O | http://ui.adsabs.harvard.edu/#abs/2021MNRAS.501.1701O
Understanding X-ray and optical selection of galaxy clusters: a comparison of the XXL and CAMIRA cluster catalogues obtained in the common XXL-HSC SSP area |Willis J. P. Oguri M. et al. | MNRAS | 503-5624 | 2021 | 2021MNRAS.503.5624W | http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5624W
Galaxy properties of type 1 and 2 X-ray selected AGN and a comparison among different classification criteria |Mountrichas G. Buat V. et al. | A&A | 653-70 | 2021 | 2021A&A...653A..70M | http://ui.adsabs.harvard.edu/#abs/2021A&A...653A..70M
XXL-HSC: An updated catalogue of high-redshift (z u2265 3.5) X-ray AGN in the XMM-XXL northern field. Constraints on the bright end of the soft log N-log S |Pouliasis E. Georgantopoulos I. et al. | A&A | 658-175 | 2022 | 2022A&A...658A.175P | http://ui.adsabs.harvard.edu/#abs/2022A&A...658A.175P
The XMM cluster survey: exploring scaling relations and completeness of the dark energy survey year 3 redMaPPer cluster catalogue |Upsdell E. W. Giles P. A. et al. | MNRAS | 522-5267 | 2023 | 2023MNRAS.522.5267U | http://ui.adsabs.harvard.edu/#abs/2023MNRAS.522.5267U
The XXL Survey. LI. Pressure profile and YSZ u2212 M scaling relation in three low-mass galaxy clusters at z u223c 1 observed with NIKA2 |Adam R. Ricci M. et al. | A&A | 684-A18 | 2024 | 2024A&A...684A..18A | http://ui.adsabs.harvard.edu/#abs/2024A&A...684A..18A
The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII O VIII and Fe L-shell Transitions |Pan Zeyang Qu Zhijie et al. | ApJS | 271-62 | 2024 | 2024ApJS..271...62P | http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P
Robust constraints on feebly interacting particles using XMM-Newton |Luque Pedro De la Torre Balaji Shyam | PhRvD | 109-L101305 | 2024 | 2024PhRvD.109j1305L | http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L
Multimessenger search for electrophilic feebly interacting particles from supernovae |Luque Pedro De la Torre Balaji Shyam | PhRvD | 109-103028 | 2024 | 2024PhRvD.109j3028L | http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L
The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations. Since Earths atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
European Space Agency, Prof Hans Boehringer, 2010, 'Testing Cosmological SZE-X-ray-Multi-Wavelength Galaxy Cluster Surveys', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-13azing
