'Cluster cores' diaporamas de présentation

Yusei Koyama (ISAS/JAXA)

??????? 2014/6/5 @ ???????. Yusei Koyama (ISAS/JAXA). Star Formation Main Sequence and Beyond: tracking down the environ-mental i mpacts on the S FR-M ? relation out to z~2. M A H A L O -Subaru collaboration. = SFR-M ? relation for star-forming galaxies. Starburst. merger. disk.

459 views • 25 slides

New and Odds on Globular Cluster Stellar Populations: an Observational Point of View

New and Odds on Globular Cluster Stellar Populations: an Observational Point of View (The Snapshot Database) G.Piotto, I. King, S. Djorgovski and G. Bono, S. Cassisi, M. Catelan, F. De Angeli , G. Meylan, A. Recio Blanco , A. Renzini, M. Rich, I. Saviane, M. Zoccali.

384 views • 24 slides

Cluster and Density wave --- cluster structures in 28 Si and 12 C---

350 views • 21 slides

High resolution spectroscopy & wide field:

High resolution spectroscopy & wide field:. prospects for Clusters and WHIM. Silvano Molendi (IASF Milano/INAF). Setting the context. Hot topics identified in ASI 2004 Feasibility Study for GC and IGM Workpackage. Cluster outer regions Cool cores Hard Excess emission

409 views • 20 slides

Yusei Koyama (NAOJ)

TMT science workshop @ Asahi- seimei building , 16/ 10/2013. From MAHALO-Subaru to ALOHA-TMT: unveiling internal physics of distant galaxies across environment. Yusei Koyama (NAOJ).

353 views • 17 slides

WFXRT vs. eROSITA

WFXRT vs. eROSITA. PSF 4-5 arcsec vs 12-14 arcsec Ef.Area 1300 cm2 vs. 2000 cm2 Instr Bkg. Similar. Sensitivity to diffuse emission will be different. Because of different PSF,FOV and observing strategy. WFXRT out to Rvir eROSITA 0.5-0.6 Rvir. Deep Pointings.

261 views • 12 slides