Searching for Emission from the Warm-Hot Intergalactic Medium

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Searching for emission from the warm-hot intergalactic medium Yoh Takei (ISAS/JAXA) Takaya Ohashi1, Kosuke Sato2,3, Ikuyuki Mitsuishi4, Enzo Branchini5, Eugenio Ursino5, Alessandra Corsi6 1: Tokyo Metropolitan U.; 2: Kanazawa U.; 3: MIT; 4: ISAS/JAXA; 5: Roma Tre U.; 6: INAF-IASF-Rome Evolution of the Universe 1(00(#+(2.Small scale Past 3,+4) GRBs • Current Universe is a !"# Stars $%&$'()$%& consequence of SNRs • structure formaiton by :"";3(-7.8. "&+$-<0"&)Starburst gravity, galaxies/ *)+,-),+".Galaxies AGNs • and chemical enrichment /%+0()$%& and feedback from smaller scale to larger scale. 56,4)"+.%,)47$+)4.8. "9%6,)$%& Clusters Structure formation Clusters • The warm-hot intergalactic ! !";4<$/) medium (WHIM) is largest structures in the local Universe, tracing distribution Feedback& Enrichment =1>."0$44$%& of dark matter and imprinting =1>.(34%+?)$%& ! Present WHIM ! enrichment history. 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    Draft version August 6, 2018 A Preprint typeset using LTEX style emulateapj v. 5/2/11 X-RAY ABSORPTION BY THE WARM-HOT INTERGALACTIC MEDIUM IN THE HERCULES SUPERCLUSTER Bin Ren1,2, Taotao Fang1,3, David A. Buote3 (Received; Revised; Accepted) Draft version August 6, 2018 ABSTRACT The “missing baryons”, in the form of warm-hot intergalactic medium (WHIM), are expected to reside in cosmic filamentary structures that can be traced by signposts such as large-scale galaxy superstructures. The clear detection of an X-ray absorption line in the Sculptor Wall demonstrated the success of using galaxy superstructures as a signpost to search for the WHIM. Here we present an XMM-Newton Reflection Grating Spectrometer (RGS) observation of the blazar Mkn 501, located in the Hercules Supercluster. We detected an O VII Kα absorption line at the 98.7% level (2.5σ) at the redshift of the foreground Hercules Supercluster. The derived properties of the absorber are consistent with theoretical expectations of the WHIM. We discuss the implication of our detection for the search for the “missing baryons”. While this detection shows again that using signposts is a very effective strategy to search for the WHIM, follow-up observations are crucial both to strengthen the statistical significance of the detection and to rule out other interpretations. A local, z ∼ 0 O VII Kα absorption line was also clearly detected at the 4σ level, and we discuss its implications for our understanding of the hot gas content of our Galaxy. Subject headings: BL Lacertae objects: individual (Markarian 501) — cosmology: observations — diffuse radiation — X-rays: diffuse background — X-rays: galaxies: clusters 1.
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