Takayuki Tamura Job Log: 1月 2015

2015年1月30日金曜日

Subaru HSC white paper

ver 1.2
http://www.astro.princeton.edu/~strauss/hsc_main.pdf

2015年1月29日木曜日

Formation of Galaxy Clusters

http://adsabs.harvard.edu/abs/2012ARA%26A..50..353K
http://www.annualreviews.org/doi/abs/10.1146/annurev-astro-081811-125502?journalCode=astro

Kravtsov and Borgani 2012

Mark Voit

http://www.pa.msu.edu/~voit/Mark.html

A nice review,
Voit 2005
http://adsabs.harvard.edu/abs/2005RvMP...77..207V
Tracing cosmic evolution with clusters of galaxies

2015年1月27日火曜日

銀河団における巨大なエネルギーの流れを発見

http://www-utheal.phys.s.u-tokyo.ac.jp/wordpress/pr2014/

2015年1月26日月曜日

XMM Large Scale Structure Surbey (LSS)

http://wela.astro.ulg.ac.be/themes/spatial/xmm/LSS/

2015年1月25日日曜日

知のバリアフリー: 「障害」で学びを拡げる

出版　2014
嶺重慎/京都大学学術出版会

ユニバーサル天文学

amazon http://goo.gl/vQrESp

https://www.facebook.com/kyoto.d.support

小石、地球の来歴を語る

amazon review

Jan Zalasiewicz

Nice stories about earth, oceans, animals, and ourselves.

2015年1月23日金曜日

The Atlas of Radio/X-ray Associations (ARXA, 2010 PASA 27 283)

http://quasars.org/arxa.htm
Eric Flesch, 2010

(copied)
These are 602 570 optical objects which are associated to radio/X-ray detections from the NVSS, FIRST, SUMSS, XMM, Chandra, or ROSAT RASS, PSPC, HRI and WGA survey catalogs. All association detections are shown, across all these catalogs. Also displayed: the calculated probability that the optical object is in turn a quasar, galaxy, star, or erroneous association. The optical object is identified from the literature, if known.

http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=V%2F134

(2015-01-23)
Useful data from a large set of catalogs.

I will use this for identification of X-ray observations of Abell2199.

2015年1月22日木曜日

「あすか」小特集

(2014-12)
2001 日本物理学会　
井上他

http://ci.nii.ac.jp/vol_issue/nels/AN00196952/ISS0000137024_ja.html

(2015-01-22)
大学院の頃に観測で利用したＸ線天文衛星「あすか」。
その科学的な成果のまとめです。
時間がたっても参考になります。

A WISE View of a nearby Supercluster A2199

http://adsabs.harvard.edu/abs/2012ApJ...752…64H
http://iopscience.iop.org/0004-637X/752/1/64/

Hwang et al. 2012

ASTRO-H White Paper - Clusters of Galaxies and Related Science

http://arxiv.org/abs/1412.1176

2014-12
Kitayama et al.

(2015-01-22)
Collaborated with ASTRO-H SWG, I contributed to this work.

(copy, abstract)
The next generation X-ray observatory ASTRO-H will open up a new dimension in the study of galaxy clusters by achieving for the first time the spectral resolution required to measure velocities of the intracluster plasma, and extending at the same time the spectral coverage to energies well beyond 10 keV. This white paper provides an overview of the capabilities of ASTRO-H for exploring gas motions in galaxy clusters including their cosmological implications, the physics of AGN feedback, dynamics of cluster mergers as well as associated high-energy processes, chemical enrichment of the intracluster medium, and the nature of missing baryons and unidentified dark matter.