Astrophysical Integrated Research Environment 周建锋、杨洋清华大学天体物理中心.

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Presentation transcript:

Astrophysical Integrated Research Environment 周建锋、杨洋清华大学天体物理中心

Contents Some BackgroundsSome Backgrounds Main Components of AIREMain Components of AIRE Current StatusCurrent Status Scientific Results HighlightsScientific Results Highlights Future PlanFuture Plan

INTEGRAL / IBIS (ISGRI) SWID = : Start from Raw Data

2 : Use Multi-band Data as Much as Possible

3 : Do Collaborations as Much as Possible Radio : Interferometry …, AIPS, AIPS++, Difmap… Optical : Photometry …, IRAF, MIDAS … X-ray : Coded-mask …, HEADAS …. Provide a web-based collaborative research environment for astrophysicists.

DPC (Data Processing Center)

VLBI Data Processing

HST Data Processing Via IRAF

Chandra Data Processing Via CIAO

Provide a simple but effective way to do collaborative researchProvide a simple but effective way to do collaborative research HTML and DPC interfaces.HTML and DPC interfaces. CARPS (Collaborative Astrophysical Research Project System )

Current Status of AIRE

8 Data Processing Servers, with 20 Intel Xeon or AMD Opteron CPUs, 22GB memory and 7TB hard disks. Fast Internet Connection to the outside data centers (download 200~600GB/Day from single data center). 5~30 online users. 18 collaborative research projects.

Scientific Results Highlights I X-Ray Triple Rings around the M87 Jets in the Central Virgo Cluster Feng, Hua; Zhang, Shuang-Nan; Lou, Yu-Qing; Li, Ti-Pei 2004ApJ...607L..95F 1. Non-Gaussianity due to Possible Residual Foreground Signals in WMAP 1st-year Data Using Spherical Wavelet Approaches Xin Liu, Shuang Nan Zhang, 2005ApJ L2005ApJ L 2. A Cross-Correlation Analysis of WMAP and EGRET Data in Wavelet Space Xin Liu, Shuang Nan Zhang, 2006ApJ...636L...1L 2006ApJ...636L...1L

Scientific Results Highlights II Optimization of interferometric array configurations by ``sieving'' u - v points Su, Y.; Nan, R. D.; Peng, B.; Roddis, N.; Zhou, J. F. Astronomy & Astrophysics 414, 389 – 397 (2004) Fu-Yan Bian, Yu-Qing Lou, Xiao-Feng Wang, Yang Yang, Tsinghua Center for Astrophysics (THCA), Tsinghua University, Beijing , China and Yu-Lei Qiu, National Astronomical Observatories of China (NAOC), report the discovery of an apparent new supernova of about mag 17.4 on unfiltered archival CCD images taken on 2005 December UT using the 0.8-m THCA-NAOC Telescope (TNT) during the THCA Supernova Survey. The candidate supernova was located at R.A. = 09h08m42s.33, Decl. = 44o48'51".4 (equinox ), which is 5".9 west and 13".3 north of the center of the galaxy UGC Nothing was visible at the location of the new object on our TNT template images obtained on December 13, November 25, November 13, and October 31, The limiting magnitude of November 25 can reach 18.5 mag. We confirmed this object on 2005 December UT and the magnitude of the object on unfiltered CCD was about 17.3 mag.

Scientific Results Highlights III

Future Plan Improve the Collaboration Environment.Improve the Collaboration Environment. Incorporate AIRE with other VO tools andIncorporate AIRE with other VO tools and standards. standards.

If you are interested in AIRE, please visit website Thanks!