Chandra Electronic Bulletin No. 69 |
******************************************************************************** | | | ccc XX XX OOO | Chandra | CC XX XX OO OO | CXC Electronic | CC XXX OO OO | Number 69 Bulletin | CC XX XX OO OO | February | CCC XX XX OOO | 2008 | | ******************************************************************************** Welcome to the Chandra X-ray Center's Electronic News Bulletin Number 69. CXC Web site: cxc.harvard.edu If you would like to unsubscribe from this alias, simply reply to this message to let us know. Please use this website to update your address or email: http://cxc.harvard.edu/cdo/udb/userdat.html Contents: 1. Chandra Source Catalog Information 2. Goddard Email 3. MARX 4.3 is now available 4. COSPAR: Astrophysical Studies of Neutron Stars 5. Chandra Deep Field South: Merged Products for 2000 and 2007 Observations ------------------------------------------------------------------------------- Item 1. Chandra Source Catalog Information =========================================== Information about the Chandra Source Catalog project, including the catalog requirements and associated documents, is now available on the CXC web site at the following URL: http://cxc.cfa.harvard.edu/csc The catalog web site will be updated regularly as we approach catalog production and release. For those who are unfamiliar with the project, the Chandra Source Catalog will be the definitive catalog of all X-ray sources detected by the Chandra X-ray Observatory. The catalog will include fields of all Galactic latitudes, and sources from the entire detector field of view, although the first catalog release will be restricted to imaging data only. -- Ian Evans for the Chandra Source Catalog project team ------------------------------------------------------------------------------- Item 2. Goddard Email ====================== Goddard Scientists: If your email is changing, please use our webpage to provide us with your new email: http://cxc.harvard.edu/cdo/udb/userdat.html Of course, we request that anyone with new contact information do the same to keep our lists up to date. Thanks all. Nancy Evans Chandra Director's Office ------------------------------------------------------------------------------- Item 3. MARX 4.3 is now available ================================== MARX is a raytrace program that allows a user to simulate the on-orbit performance of the Chandra X-ray Observatory for variety of astrophysical sources. It can output Chandra EVENT files that may be processed using standard CIAO tools. Version 4.3 contains calibration updates, support for large files, and has been ported to Cygwin and MacOSX. The examples on the MARX web pages have been rewritten to reflect the changes in both MARX 4.3 and the CIAO 4 tools. See http://space.mit.edu/cxc/marx/ for more information. John E. Davis, for the MARX team ------------------------------------------------------------------------------- Item 4. Astrophysical Studies of Neutron Stars from Multiwavelengths Observations =============================================================================== == COSPAR SESSION E11 to be held as part of the 37th COSPAR Scientific Assembly Montreal, Canada, July 13-20, 2008 ------------------------------------------------------------------------------- In recent years, we have seen tremendous progress in the field of neutron star research, primarily enabled by multi-wavelength timing, imaging and spectroscopic observations with both ground and space-based observatories. Along with ground-based radio, optical and infra-red telescopes, an array of X-ray and Gamma ray observatories -- such as RXTE, INTEGRAL, Chandra, XMM-Newton and SWIFT -- with broad ranging timing, spectral and imaging capabilities has opened a new era of multi-wavelength investigations. Multi-wavelength observations of the different manifestations of neutron stars like radio pulsars, magnetars, isolated neutron stars etc. offer the opportunity to investigate a wide range of astrophysical problems including the extremes of gravity, density and magnetic field. At the COSPAR assembly in Montreal, 2008, we will have an opportunity to bring together researchers from diverse fields and gauge the direction of future neutron star research with existing and coming observatories, such as GLAST and ASTROSAT. We invite you to participate in this meeting and to submit abstracts for contributed talks or posters via the COSPAR assembly website http://www.cospar-assembly.org/ Session E11. Important Deadlines: -------------------- Abstract Submission : 17 Feb 2008 Applications for Financial Support : 17 Feb 2008 Early Registration : 1 June 2008 Biswajit Paul and Vicky Kaspi for the SOC ------------------------------------------------------------------------------ Solicited Speakers: M. McLaughlin, M. Baring, W. Hermsen, S. Zavlin, A. Pellizzoni, Y. Lyubarsky, F. P. Gavriil, D. Gotz, R. Mignani, M. Muno, E. Amato, P. Slane, G. Pavlov, F. Haberl, D. Kaplan, R. Turolla, Wynn Ho, A. Watts, M. van der Klis, M. Mendez, R. Hynes, T. Mihara, L. Sidoli, P. Jonker, N. Masetti, S. Watanabe ------------------------------------------------------------------------------ * Scientific Organizing Committee * Felix Aharonian, Dipankar Bhattacharya, K. S. Cheng, Andrew Cumming, David Eichler, Alice Harding, Vicky Kaspi, Nobu Kawai, Lucien Kuiper, Maxim Lyutikov, Dick Manchester, Maura McLaughlin, Sandro Mereghetti, Biswajit Paul, Scott Ransom, Bob Rutledge, Rudy Wijnands, Sylvia Zane ------------------------------------------------------------------------------ ------------------------------------------------------------------------------- Item 5. Chandra Deep Field South: Merged Products for 2000 and 2007 Observations =============================================================================== == The old 2000 and the new 2007 data from the Chandra Deep Field South have been custom processed to register all 21 individual observations astrometrically. For more information, see: http://cxc.harvard.edu/cda/whatsnew.html#CDFS2000-2007 This web page provides several download files for three merged sets - 2000 only, 2007 only, and 2000+2007: * Tar file containing the merged event file, exposure map, and image * By-ObsId tar file containing the event list and aspect solution for each of the individual ObsIds * Full resolution linear three-color image of merged datasets * Full resolution enhanced three-color image of merged datasets * Smoothed enhanced three-color image of merged datasets CXC Data Systems ------------------------------------------------------------------------------- This Electronic Bulletin is used for the dissemination of important announcements and information about the Chandra X-Ray Observatory to members of the community. If you wish to unsubscribe from the list, simply reply to this email to let us know. |
Last modified: 12/03/10
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