We propose to complete, by an additional 5 deg2, the XMM-LSS Survey regionoverlying the Spitzer/SWIRE field. This field already has CFHTLS and Integralcoverage, and will encompass about 10 deg2. The resulting multi-wavelengthmedium-depth survey, which complements XMM and Chandra deep surveys, willprovide a unique view of large-scale structure over a wide range of redshift,and will show active galaxies in the full range of environments. The completecoverage by optical and IR surveys provides high-quality photometric redshifts,so that cosmological results can quickly be extracted. In the spirit of a Legacysurvey, we will make the raw X-ray data immediately public. Multi-bandcatalogues and images will also be made available on short time scales.
Six More Quasars at Redshift 6 Discovered by the Canada-France High-z Quasar Survey |Willott Chris J. Delorme Philippe et al. | AJ | 137-3541 | 2009 | 2009AJ....137.3541W | http://ui.adsabs.harvard.edu/#abs/2009AJ....137.3541W
Angular correlation functions of X-ray point-like sources in the full exposure XMM-LSS field |Elyiv A. Clerc N. et al. | A&A | 537-131 | 2012 | 2012A&A...537A.131E | http://ui.adsabs.harvard.edu/#abs/2012A&A...537A.131E
The XMM Cluster Survey: optical analysis methodology and the first data release |Mehrtens Nicola Romer A. Kathy et al. | MNRAS | 423-1024 | 2012 | 2012MNRAS.423.1024M | http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.1024M
An XMM-Newton Survey of the Soft X-ray Background. I. The O VII and O VIII Lines Between l = 120 and l = 240 |Henley David B. Shelton Robin L. | ApJS | 187-388 | 2010 | 2010ApJS..187..388H | http://ui.adsabs.harvard.edu/#abs/2010ApJS..187..388H
The WIRCAM Deep Infrared Cluster Survey. I. Groups and clusters at z ⪆ 1.1 |Bielby R. M. Finoguenov A. et al. | A&A | 523-66 | 2010 | 2010A&A...523A..66B | http://ui.adsabs.harvard.edu/#abs/2010A&A...523A..66B
The cosmological analysis of X-ray cluster surveys - II. Application of the CR-HR method to the XMM archive |Clerc N. Sadibekova T. et al. | MNRAS | 423-3561 | 2012 | 2012MNRAS.423.3561C | http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.3561C
An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities |Henley David B. Shelton Robin L. | ApJS | 202-14 | 2012 | 2012ApJS..202...14H | http://ui.adsabs.harvard.edu/#abs/2012ApJS..202...14H
Using the Bright Ultrahard XMM-Newton survey to define an IR selection of luminous AGN based on WISE colours |Mateos S. Alonso-Herrero A. et al. | MNRAS | 426-3271 | 2012 | 2012MNRAS.426.3271M | http://ui.adsabs.harvard.edu/#abs/2012MNRAS.426.3271M
A systematic cross-search for radio/infrared counterparts of XMM- Newton sources |Combi J. A. Albacete Colombo J. F. et al. | Ap&SS | 331-53 | 2011 | 2011Ap&SS.331...53C | http://ui.adsabs.harvard.edu/#abs/2011Ap&SS.331...53C
The XMM-Large Scale Structure catalogue - II. X-ray sources and associated multiwavelength data |Chiappetti L. Clerc N. et al. | MNRAS | 429-1652 | 2013 | 2013MNRAS.429.1652C | http://ui.adsabs.harvard.edu/#abs/2013MNRAS.429.1652C
Mining the gap: evolution of the magnitude gap in X-ray galaxy groups from the 3-square-degree XMM coverage of CFHTLS |Gozaliasl G. Finoguenov A. et al. | A&A | 566-140 | 2014 | 2014A&A...566A.140G | http://ui.adsabs.harvard.edu/#abs/2014A&A...566A.140G
The XMM-LSS survey: the Class 1 cluster sample over the extended 11 deg2 and its spatial distribution |Clerc N. Adami C. et al. | MNRAS | 444-2723 | 2014 | 2014MNRAS.444.2723C | http://ui.adsabs.harvard.edu/#abs/2014MNRAS.444.2723C
Revisiting the relationship between 6 mum and 2-10 keV continuum luminosities of AGN |Mateos S. Carrera F. J. et al. | MNRAS | 449-1422 | 2015 | 2015MNRAS.449.1422M | http://ui.adsabs.harvard.edu/#abs/2015MNRAS.449.1422M
The XMM Cluster Survey: predicted overlap with the Planck Cluster Catalogue |Viana Pedro T. P. da Silva Antonio et al. | MNRAS | 422-1007 | 2012 | 2012MNRAS.422.1007V | http://ui.adsabs.harvard.edu/#abs/2012MNRAS.422.1007V
Sunyaev-Zeldovich effect or not? Detecting the main foreground effect of most galaxy clusters |Xiao Weike Chen Chen et al. | MNRAS | 432-41 | 2013 | 2013MNRAS.432L..41X | http://ui.adsabs.harvard.edu/#abs/2013MNRAS.432L..41X
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
Brightest group galaxies: stellar mass and star formation rate (paper I) |Gozaliasl Ghassem Finoguenov Alexis et al. | MNRAS | 458-2762 | 2016 | 2016MNRAS.458.2762G | http://ui.adsabs.harvard.edu/#abs/2016MNRAS.458.2762G
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
Ensemble X-ray variability of active galactic nuclei. II. Excess variance and updated structure function |Vagnetti F. Middei R. et al. | A&A | 593-55 | 2016 | 2016A&A...593A..55V | http://ui.adsabs.harvard.edu/#abs/2016A&A...593A..55V
SPIDERS: the spectroscopic follow-up of X-ray selected clusters of galaxies in SDSS-IV |Clerc N. Merloni A. et al. | MNRAS | 463-4490 | 2016 | 2016MNRAS.463.4490C | http://ui.adsabs.harvard.edu/#abs/2016MNRAS.463.4490C
The XMM Cluster Survey: the halo occupation number of BOSS galaxies in X-ray clusters |Mehrtens Nicola Romer A. Kathy et al. | MNRAS | 463-1929 | 2016 | 2016MNRAS.463.1929M | http://ui.adsabs.harvard.edu/#abs/2016MNRAS.463.1929M
The rapid assembly of an elliptical galaxy of 400 billion solar masses at a redshift of 2.3 |Fu Hai Cooray Asantha et al. | Natur | 498-338 | 2013 | 2013Natur.498..338F | http://ui.adsabs.harvard.edu/#abs/2013Natur.498..338F
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
X-ray-bright optically faint active galactic nuclei in the Subaru Hyper Suprime-Cam wide survey |Terashima Yuichi Suganuma Makoto et al. | PASJ | 70-36 | 2018 | 2018PASJ...70S..36T | http://ui.adsabs.harvard.edu/#abs/2018PASJ...70S..36T
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
X-ray versus infrared selection of distant galaxy clusters: a case study using the XMM-LSS and SpARCS cluster samples |Willis J. P. Ramos-Ceja M. E. et al. | MNRAS | 477-5517 | 2018 | 2018MNRAS.477.5517W | http://ui.adsabs.harvard.edu/#abs/2018MNRAS.477.5517W
The XMM-SERVS survey: new XMM-Newton point-source catalogue for the XMM-LSS field |Chen C.-T. J. Brandt W. N. et al. | MNRAS | 478-2132 | 2018 | 2018MNRAS.478.2132C | http://ui.adsabs.harvard.edu/#abs/2018MNRAS.478.2132C
Imaging Plasma Density Structures in the Soft X-Rays Generated by Solar Wind Charge Exchange with Neutrals |Sibeck David G. Allen R. et al. | SSRv | 214-79 | 2018 | 2018SSRv..214...79S | http://ui.adsabs.harvard.edu/#abs/2018SSRv..214...79S
Is there a relationship between AGN and star formationin IR-bright AGNs? |Dai Y. Sophia Wilkes Belinda J. et al. | MNRAS | 478-4238 | 2018 | 2018MNRAS.478.4238D | http://ui.adsabs.harvard.edu/#abs/2018MNRAS.478.4238D
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
A new clean catalogue of extragalactic non-nuclear X-ray sources in nearby galaxies |Earnshaw H. P. Roberts T. P. et al. | MNRAS | 483-5554 | 2019 | 2019MNRAS.483.5554E | http://ui.adsabs.harvard.edu/#abs/2019MNRAS.483.5554E
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
Constraining the Dark-matter Halo Mass of Isolated Low-surface-brightness Galaxies |Kovacs Orsolya E. Bogdan Akos | ApJ | 879-12 | 2019 | 2019ApJ...879L..12K | http://ui.adsabs.harvard.edu/#abs/2019ApJ...879L..12K
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
A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). II. Physical Properties Derived from the SED Fitting with Optical Infrared and Radio Data |Toba Yoshiki Yamashita Takuji et al. | ApJS | 243-15 | 2019 | 2019ApJS..243...15T | http://ui.adsabs.harvard.edu/#abs/2019ApJS..243...15T
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
Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline |Hollowood Devon L. Jeltema Tesla et al. | ApJS | 244-22 | 2019 | 2019ApJS..244...22H | http://ui.adsabs.harvard.edu/#abs/2019ApJS..244...22H
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
Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters |Palmese A. Annis J. et al. | MNRAS | 493-4591 | 2020 | 2020MNRAS.493.4591P | http://ui.adsabs.harvard.edu/#abs/2020MNRAS.493.4591P
X-ray properties of the X-CLASS-redMaPPer galaxy cluster sample: the luminosity-temperature relation |Molham Mona Clerc Nicolas et al. | MNRAS | 494-161 | 2020 | 2020MNRAS.494..161M | http://ui.adsabs.harvard.edu/#abs/2020MNRAS.494..161M
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
A Comparison of X-Ray Photon Indices among the Narrow- and Broad-line Seyfert 1 Galaxies |Ojha Vineet Chand Hum et al. | ApJ | 896-95 | 2020 | 2020ApJ...896...95O | http://ui.adsabs.harvard.edu/#abs/2020ApJ...896...95O
SPIDERS: overview of the X-ray galaxy cluster follow-up and the final spectroscopic data release |Clerc N. Kirkpatrick C. C. et al. | MNRAS | 497-3976 | 2020 | 2020MNRAS.497.3976C | http://ui.adsabs.harvard.edu/#abs/2020MNRAS.497.3976C
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
Implications of the Environments of Radio-detected Active Galactic Nuclei in a Complex Protostructure at z u223c 3.3 |Shen Lu Lemaux Brian C. et al. | ApJ | 912-60 | 2021 | 2021ApJ...912...60S | http://ui.adsabs.harvard.edu/#abs/2021ApJ...912...60S
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 RapidXMM upper limit server: X-ray aperture photometry of the XMM-Newton archival observations |Ruiz A. Georgakakis A. et al. | MNRAS | 511-4265 | 2022 | 2022MNRAS.511.4265R | http://ui.adsabs.harvard.edu/#abs/2022MNRAS.511.4265R
The Solar Cycle Temporal Variation of the Solar Wind Charge Exchange X-Ray Lines |Qu Zhijie Koutroumpa Dimitra et al. | ApJ | 930-21 | 2022 | 2022ApJ...930...21Q | http://ui.adsabs.harvard.edu/#abs/2022ApJ...930...21Q
The Redshift Evolution of Ultraluminous X-Ray Sources out to z 0.5: Comparison with X-Ray Binary Populations and Contribution to the Cosmic X-Ray Background |Scott Barrows R. Comerford Julia M. et al. | ApJ | 932-27 | 2022 | 2022ApJ...932...27S | http://ui.adsabs.harvard.edu/#abs/2022ApJ...932...27S
A fresh look at AGN spectral energy distribution fitting with the XMM-SERVS AGN sample |Marshall Adam Auger-Williams Matthew W. et al. | MNRAS | 515-5617 | 2022 | 2022MNRAS.515.5617M | http://ui.adsabs.harvard.edu/#abs/2022MNRAS.515.5617M
The value-added catalogue of ASAS-SN eclipsing binaries: parameters of 30 000 detached systems |Rowan D. M. Jayasinghe T. et al. | MNRAS | 517-2190 | 2022 | 2022MNRAS.517.2190R | http://ui.adsabs.harvard.edu/#abs/2022MNRAS.517.2190R
Detection of radio-AGN in dust-obscured galaxies using deep uGMRT radio continuum observations |Kayal Abhijit Singh Veeresh et al. | JApA | 43-84 | 2022 | 2022JApA...43...84K | http://ui.adsabs.harvard.edu/#abs/2022JApA...43...84K
Hard X-Ray to Radio Multiwavelength SED Analysis of Local U/LIRGs in the GOALS Sample with a Self-consistent AGN Model including a Polar-dust Component |Yamada Satoshi Ueda Yoshihiro et al. | ApJS | 265-37 | 2023 | 2023ApJS..265...37Y | http://ui.adsabs.harvard.edu/#abs/2023ApJS..265...37Y
Search and Characterization of Remnant Radio Galaxies in the XMM-LSS Deep Field |Dutta Sushant Singh Veeresh et al. | ApJ | 944-176 | 2023 | 2023ApJ...944..176D | http://ui.adsabs.harvard.edu/#abs/2023ApJ...944..176D
Identification and Characterization of a Large Sample of Distant Active Dwarf Galaxies in XMM-SERVS |Zou Fan Brandt W. N. et al. | ApJ | 950-136 | 2023 | 2023ApJ...950..136Z | http://ui.adsabs.harvard.edu/#abs/2023ApJ...950..136Z
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
Observational properties of active galactic nucleus obscuration during the peak of accretion growth |Vijarnwannaluk Bovornpratch Akiyama Masayuki et al. | MNRAS | 529-3610 | 2024 | 2024MNRAS.529.3610V | http://ui.adsabs.harvard.edu/#abs/2024MNRAS.529.3610V
X-ray spectral properties of dust-obscured galaxies in the XMM-SERVS coverage of the XMM-LSS field |Kayal Abhijit Singh Veeresh | MNRAS | 531-830 | 2024 | 2024MNRAS.531..830K | http://ui.adsabs.harvard.edu/#abs/2024MNRAS.531..830K
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, Dr Marguerite Pierre, 2008, 'The XMM Large Scale Structure Survey', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-xyfomia