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- 件名arachnoid web spine surgery ......cquisition for the manipulation of image contras...
- 並列タイトル等（連結）Arachnoid web of the spine confirme......cquisition for the manipulation o......e contrast (3D-COSMIC) magnetic resonance imaging :...
- 並列タイトル等Arachnoid web of the spine confirme......cquisition for the manipulation o......e contrast (3D-COSMIC) magnetic resonance imaging :...
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- 並列タイトル等（連結）... and growth of the cosmicweb : proceedings of the International ...... and growth of the cosmic web : proceedings of the International Astronomical Un...
- 並列タイトル等... and growth of the cosmicweb : proceedings of the International ...... and growth of the cosmic web : proceedings of the International Astronomical Un...
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- 著者標目Hayles, N. Katherine
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- 並列タイトル等（連結）Astronomers observe a nascent galaxy stuck to the cosmic web
- 並列タイトル等Astronomers observe a nascent galaxy stuck to the cosmic web
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- 参照Classification of cosmic structures for......h observations The impact of fila......f subhaloes on the shape and orientation of halo...
- 並列タイトル等（連結）The cosmic web
- 並列タイトル等The cosmic web
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- 参照Can HI 21-cm lines trace the missing baryons in the filamentary structures?
- 並列タイトル等（連結）<i>Radio emission in the cosmic web</i>
- 並列タイトル等<i>Radio emission in the cosmic web</i>
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- 並列タイトル等（連結）Exploration of Magnetic Fields in the Cosmic Web with the SKA
- 並列タイトル等Exploration of Magnetic Fields in the Cosmic Web with the SKA
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- 並列タイトル等（連結）Multiscale phenomenology of the cosmic web
- 並列タイトル等Multiscale phenomenology of the cosmic web
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- 参照An excess of dusty starbursts related to the Spiderweb galaxy
- 並列タイトル等（連結）The Cosmic Web and RX J1347.5−1145
- 並列タイトル等The Cosmic Web and RX J1347.5−1145
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- 参照...bservations of the Perseus Cluster The turbulent pres...... relations and their evolution A ...... a filament of the cosmic web X-ray properti......nd clusters On the role of AGN feedback on the thermal and chemod...... properties of the hot intraclust......aces Exploring the effects of gal......Shocks and Non-thermal Particles ...... PROPERTIES OF THE WARM-HOT INTER......e evolution in the density-strati......tistics: using the minimum spanni......-invariance of the iron enrichment in the hot haloes of ......o-electronics ATHENA WFI optical ...... status toward the end of the instrument pha......on overcoating THE ROTATION OF THE HOT GAS AROUN...
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- 要約等...as detected by the Australian Squ......ne-formula> in the Sloan Digital ......SS) footprint. The burst has a la......>) compared to the expected cosmic average at its......ed analysis of the ultraviolet an......al emission of the host galaxy and estimate the host DM contri......rk complements theirs and reports the analysis of the optical data of galaxies in the foreground of ......der to explore their contributions to the FRB signal. Together, the two studies de......FRB sightline, the first study of......ining our Keck Cosmic Web Imager (KCWI) ......a, we estimate the expected cosmic dispersion mea......{DM}}_{\mathrm{cosmic}}$?> </jats:tex-math> ...
- 参照Constraining the Cosmic Baryon Distrib......ter haloes and cosmic dispersion measures
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- 要約等... <jats:p>The connections among galaxies, the dark matter haloes where they form and the properties of the large-scale Cosmic Web still need to ......angled. We use the cosmological h......tion TNG100 of the IllustrisTNG s......te to quantify the effects played by the large-scale de......sity field and the Cosmic Web morphology on the relation betwe......amical mass in the range ${\ge}6.......shift z = 0. A Cosmic Web class (knot, f......each region of the volume using a......verdensity and Cosmic Web class. The latter two qua......ate with each other, but are not ......degenerate. Furthermore, we find that at fixed h...
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- 要約等...netized today. The origin of magnetic fields in the intergalactic ...... extensions to the physics of the standard model......of magnetizing the universe at la...... well known is the fact that stan......ally possesses the same potential......anism based on the exchange of mo....... Operating in the neighborhood o......sources during the epoch of reion...... comparable to the distance betwe......on, summing up the contributions ......g into account the distribution o......chanism leaves the IGM, at the end of reioniz......take over, for the magnetic fields strengths in the current cosmic web.</jats:p>
- 参照Workshop Summary “The Power of Faraday Tomography”
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- 要約等... properties of the ensemble of superclusters in the cosmic web evolve with ti......simulations of the evolution of the cosmic web using the Λ cold dark ma......rresponding to the present epoch ......rclusters, and the number of supe......s functions of the threshold dens...... properties of the ensemble of superclusters in the cosmic web. We calculated the distributions ......, and followed the time evolution......of galaxies of the Sloan Digital ......ionary epochs. The geometrical di......ecrease during the evolution of the cosmic web, and the luminosities o......cal influence. The stability of f......lusters during the evolution is an important pro...
- 参照...uster: Mapping the light and dark......z = 0.55 using the subaru hyper suprime-cam
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- 要約等<jats:p>The detection of the radio signal f......m filaments in the cosmic web is crucial to ......ios. We review the status of the different attempts to detect the cosmic web at radio wavel......is is put into the context of the advanced simulations of cosmic magnetism carried out in the last few years......pts of imaging the cosmic web with the MWA and LOFAR ......enesis models, the complexity beh......equencies that the SKA and LOFAR2......ey to removing the existing uncer......ies related to the contribution o......ble to isolate the contribution f......onnection with the origin of extragalactic magne...
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- 要約等<jats:p>We report the discovery of d......o 4.5, tracing cosmic web filaments on s......of 2.5−4 cMpc. These structures h......c> emitters in the MUSE Extremely......ion located in the <jats:italic>H......p Field. Among the 22 overdense r......rkably, 70% of the total Ly<jats:......uminosity from these filaments co......es from beyond the circumgalactic......ion powered by the cosmic UV background ....... We find that the bulk of this d...... reproduced by the unresolved Ly<...... provided that the faint end of the Ly<jats:italic......jats:sup>, and the clustering of these Ly<jats:ital......tor < 1/6). If these Ly<jats:italic>α</jats:ital...
- 著者標目...Kusakabe J. Matthee L. Michel-Dansac T. Nanayakk...
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- 参照The eROSITA view of the Abell 3391/95 ......ase study from the Magneticum cos......n distribution The impact of fila......f subhaloes on the shape and orie......tion of haloes The Bias from Hydr......axies based on the local mass den......s according to the Viewing Direction Discovery o...
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- 参照...toclusters and the Cosmic Web
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- 参照Classification of cosmic structures for galaxies with ...
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- 要約等...ts:p>Measuring the properties of ......fields through the effect of Fara...... to understand the origin and evolution of cosmic magnetism. Her...... use data from the LOFAR Two-Metr......) to calculate the Faraday rotati......By considering the RM difference ......ted sources on the sky), we stati......ically isolate the contribution o......s to ΔRM along the line of sight ......erence between the ΔRM distributions of the physical and n......airs, limiting the excess Faraday......mit of 4 nG on the cosmological c......e also compare the RM data with a......gnetization of the large-scale st......be rejected by the current data; while stronger ...