|Title||Precision Mass-Observable Cluster Calibration with the HSC and ACTPol surveys|
|Author||Dr Nobuhiro Okabe|
|Description||We propose a systematic study to calibrate how various galaxy cluster observables scale with mass, using precision, HSC-derived, weak lensing mass measurements and make a stringent test of the assumption of hydrostatic equilibrium of clusters. The exquisite quality of multi-band HSC imaging will enable us to improve both the precision and accuracy of weak-lensing mass measurements, and allow us to significantly reduce systematic error for individual cluster mass measurements. By combining these weak lensing mass measurements wit deep XMM-Newton X-ray and ACTPol Sunyaev-Zel.dovich effect data, we will have an unprecedented ability to constrain the physical state of the intracluster medium. Our project provides an essential bridge to future, cluster-based, cosmological studies by eROSITA.|
|Publication||X-Ray Morphological Analysis of the Planck ESZ Clusters . Lovisari, Lorenzo, Forman, William R., et all. . ApJ . 846-51 . 2017 . 2017ApJ...846...51L ,
On the Connection between Turbulent Motions and Particle Acceleration in Galaxy Clusters . Eckert, D., Gaspari, M., et all. . ApJ . 843-29 . 2017 . 2017ApJ...843L..29E ,
Multiwavelength study of X-ray luminous clusters in the Hyper Suprime-Cam Subaru Strategic Program S16A field . Miyaoka, Keita, Okabe, Nobuhiro, et all. . PASJ . 70-22 . 2018 . 2018PASJ...70S..22M ,
X-ray scaling relations from a complete sample of the richest maxBCG clusters . Ge, Chong, Sun, Ming, et all. . MNRAS . 484-1946 . 2019 . 2019MNRAS.484.1946G ,
ComPRASS: a Combined Planck-RASS catalogue of X-ray-SZ clusters . Tarrio, P., Melin, J.-B., . A&A . 626-7 . 2019 . 2019A&A...626A...7T ,
X-Ray Scaling Relations for a Representative Sample of Planck-selected Clusters Observed with XMM-Newton . Lovisari, Lorenzo, Schellenberger, Gerrit, et all. . ApJ . 892-102 . 2020 . 2020ApJ...892..102L ,
A Comparison of X-Ray Photon Indices among the Narrow- and Broad-line Seyfert 1 Galaxies . Ojha, Vineet, Chand, Hum, et all. . ApJ . 896-95 . 2020 . 2020ApJ...896...95O ,
The XMM Cluster Survey: new evidence for the 3.5-keV feature in clusters is inconsistent with a dark matter origin . Bhargava, S., Giles, P. A., et all. . MNRAS . 497-656 . 2020 . ...ef=" http://ui.adsabs.harvard.edu/#abs/2020MNRAS.497..656B" > 2020MNRAS.497..656B ,
|Instrument||EMOS1, EMOS2, EPN, OM, RGS1, RGS2|
|Mission Description||The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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.
|Publisher And Registrant||European Space Agency|
|Credit Guidelines||European Space Agency, 2017-02-19T23:00:00Z, 076287, 17.56_20190403_1200. https://doi.org/10.5270/esa-iixn9uu|