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Announcements of Upcoming Meetings

Notice that this list is not meant to be all-inclusive, but concentrates on meetings of potential interest to X-ray, gamma-ray, cosmic-ray, and gravitational astrophysicists. The HEASARC also maintains a list of on-line proceedings of high-energy astrophysics meetings. Updates, corrections, and/or suggestions about meetings should be sent to drake@olegacy.gsfc.nasa.gov

Other Sources of Information on Upcoming Meetings

Liz Bryson's list of International Astronomy meetings
Jet Propulsion Laboratory (JPL) Space Calendar


High Energy Astrophysics meetings

2009 July 3: International X-Ray Observatory (IXO) Science Study Team Meeting

2009 July 8 - 10: Workshop on Supernova Remnants and Pulsar Wind Nebulae in the Chandra Era

2009 July 12 - 18: 12th Marcel Grossmann Meeting

2009 July 13 - 17: TeV Particle Astrophysics 2009

2009 July 26 - 31: CosmoStats09 & GREAT08 Challenge Workshop

2009 August 3 - 5: NEUTRON STARS: TIMING IN AN EXTREME ENVIRONMENT: JOINT DISCUSSION AT THE XXVII IAU GENERAL ASSEMBLY

2009 August 6 - 7: HOT INTERSTELLAR MATTER IN ELLIPTICAL GALAXIES: JOINT DISCUSSION AT THE XXVII IAU GENERAL ASSEMBLY

2009 August 10 - 14: IAU Symposium 267: Evolution of Galaxies and Central Black Holes: Feeding and Feedback

2009 September 7 - 11: X-ray Astronomy 2009: Present Status, Multiwavelength Approach and Future Perspectives

2009 September 11 - 12: Black Holes in Binary Systems: Observations versus Theory

2009 September 21: Chandra Calibration Review

2009 September 22 - 25: Ten Years of Science with Chandra: Chandra's First Decade of Discovery

2009 October 4 - 8: 4th INTERNATIONAL WORKSHOP ON ASTRONOMY AND RELATIVISTIC ASTROPHYSICS: New Phenomena and New States of Matter in the Universe in the AUGER, SLAC, LHC, FERMI, FAIR/GSI and GEO/LIGO Era

2009 October 7 - 9: Science with the New Generation of High Energy Gamma-ray Experiments: SCINEGHE-VII Workshop

2009 October 13 - 17: INTEGRAL Workshop: The Extreme Sky: Sampling the Universe above 10 keV

2009 November 2 - 5: 2009 Fermi Symposium

2009 November 17 -20: Swift Mission Conference: Celebrating 5 Years

2010 March 1 - 4: High Energy Astrophysics Division (HEAD) Meeting

2010 March 15 - 17: High-Resolution X-ray Spectroscopy: Past, Present, and Future

2010 July 18 - 25: 38th Scientific Assembly of the Committee on Space Research (COSPAR) and Associated Events: COSPAR 2010


Other Selected Astronomy, Physics and Space Science meetings

2009 June 29 - July 10: 1st Summer School on Multiwavelength Astronomy

2009 August 3 - 14: IAU XXVII General Assembly

2009 October 26 - 28: Reionization to Exoplanets: Spitzer's Growing Legacy

2010 January 3 - 7: American Astronomical Society Meeting 215


Selected Astronomy-related Technology (e.g., Detectors) meetings


Selected Astronomy-related Physics, Computational, Data Analysis, Software or Statistics meetings


Selected Space Science-related Education and Public Outreach meetings


High Energy Astrophysics meetings

International X-ray Observatory (IXO) Science Study Team Meeting

Dates: 2009 July 3
Place: Otaru, Hokkaido, Japan

The International X-ray Observatory (IXO) is an X-ray telescope with joint participation from NASA, the European Space Agency (ESA), and Japan's Aerospace Exploration Agency (JAXA). This project supersedes both NASA's Constellation-X and ESA's XEUS mission concepts.

IXO will be launched circa 2020. This meeting will feature presentations by the Science Definition Team (SDT), the Instrument Working Group (IWG), the Telescope Working Group (IWG), and the ESA, JAXA, and NASA projects.

This meeting will be held just after the Suzaku Conference from June 29 through July 2 held in the same location (Otaru, Japan). It is strongly advised that the attendants of the Suzaku Conference extend their stay one more day to learn more about the exciting future mission IXO.

Workshop on Supernova Remnants and Pulsar Wind Nebulae in the Chandra Era

Dates: 2009 July 8 - 10
Early deadline for both registration and abstract submission for contributed talks and poster presentations: 2009 April 29
Final registration and abstract submission deadline for poster presentations only: 2009 May 20
Place: Boston, Massachusetts, USA

X-ray observatories are advancing our understanding of a wide range of astrophysical processes, and profoundly so in the field of supernova remnants. The Chandra X-ray Observatory's superior spatial and spectral resolution, for example, are probing the structure and evolution of supernova remnant ejecta, diffusive shock acceleration processes, and interactions between supernova remnants and pulsar wind nebulae down to the sub-arcsecond level. This conference highlights both observational and theoretical studies of SNR, emphasizing recent X-ray observations of Galactic SNR. All aspects of SNR research will be explored including shock acceleration, electron/ion temperature equilibration, pulsar wind nebulae, connections between SNR ejecta and SN processes, and SNR interactions with the circumstellar and interstellar medium. The goals are to discuss outstanding problems in SNR research, and the most direct path forward in coming years.

Contact snr09 "at" cfa.harvard.edu for more information.

12th Marcel Grossmann Meeting

Dates: 2009 July 12 - 18
Deadline for Hotel Reservations: 2009 May 20
Deadline for Early Registration and Abstract Submission: 2009 June 1
Place: Paris, France

The scientific objective of these meetings is to bring together scientists from diverse backgrounds in order to deepen our understanding of spacetime structures and review the status of experiments testing Einstein's theory of gravitation. The range of topics is broad: from more abstract classical gravitational theories, quantum gravity, and string theories all the way to relativistic astrophysics and an outlook towards future observational missions.

As well as plenary sessions, there will also be parallel sessions, as follows:

A. String Theory and Quantum Gravity
B. Black Holes: Theory
C. Astrophysics of Neutron Stars and Black Holes
D. Theoretical Cosmology
E. Gamma Ray Bursts: Theory and Observation
F. Mathematical and General Theories
G. Experimental Gravitation
H. History of Relativity
I. Analytic and Numerical Methods
L. Cosmological Models
M. Observational Cosmology
N. Astroparticle Physics
O. Gravitational Waves

TeV Particle Astrophysics 2009

Dates: 2009 July 13 - 17
Deadline for Abstract Submission and Regular Registration: 2009 June 15
Place: Menlo Park, California, USA

Particle astrophysics is now a busy intersection between particle physics, astrophysics and cosmology. In 2009, the Large Hadron Collider will begin taking data and start its exploration of the TeV scale and physics beyond the Standard Model. The Fermi Gamma-ray Space Telescope (FGST) launched in June 2008, and it will have passed its one year anniversary by the time of the conference. Many results have already been reported, and there will be considerably more by the time of the conference. We expect more interesting results from Pamela and ATIC. In addition, ground-based gamma ray telescopes including HESS, MAGIC, VERITAS, MILAGRO and ARGO have been observing gamma-rays at the TeV scale and higher with unprecedented accuracy for years. We also expect new exciting results from Auger. Neutrino experiments such as Antares and IceCube are starting to run at similar and higher energies. Underground experiments that focus on dark matter direct detection, neutrino mass measurement, and gravitational wave detection, are all making rapid progress.

This conference aims to understand what we can learn from the present and upcoming observational results from both the LHC and a broad range of astrophysical searches. It will provide an occasion for theorists and experimentalists to discuss the latest and upcoming results in these fields, to consider new strategies, technologies and collaborative efforts to address some of the most pressing questions in physics today, including the nature of dark matter and the origin of cosmic rays.

CosmoStats09 and GREAT08 Challenge Workshop

Dates: 2009 July 26 - 31
Deadline for Priority Registration: 2009 February 28
Place: Ascona, Switzerland

In the last ten years, a wealth of observational data has revolutionized cosmology. The purpose of this workshop is to bring together world-class leading figures in cosmology, particle physics and from the statistical community in order to exchange knowledge and experience in dealing with large and complex data sets, and to meet the challenge of upcoming large cosmological surveys. Topics to be covered include: statistical challenges in cosmology and particle physics, discovery issues, peta-scale inference, and Frequentists vs Bayesians.

Furthermore, CosmoStats09 will host the GRavitational lEnsing Accuracy Testing 2008 (GREAT08) Challenge Final Workshop. Observed galaxy images appear distorted due to gravitational lensing and their shapes must be precisely disentangled from observational effects of sampling, convolution and noise. The GREAT08 Challenge is open to all, and aimed at those from outside the gravitational lensing community, including statistical inference, inverse problems and computational learning. It runs from October 2008 until April 2009. The GREAT08 Challenge contains 200 GB of simulated images, containing 30 million galaxy images. For the main competition, participants are asked to extract 5400 numbers from 170 GB of data.

NEUTRON STARS: TIMING IN AN EXTREME ENVIRONMENT: JOINT DISCUSSION AT THE XXVII IAU GENERAL ASSEMBLY

Dates: 2009 August 3 - 5
Place: Rio de Janeiro, Brazil

Astronomical systems harboring a neutron star, from isolated and binary radio pulsars to magnetars and accreting X-ray binaries, constitute a unique tool for the study of matter under extreme conditions. Testing General Relativity in the strong-field regime and the determination of the equation of state of neutron matter are major goals which appear more and more within reach. The availability of high-energy missions such as XMM-Newton, Chandra and Suzaku for energy spectra and RossiXTE for fast time variability, as well as the discovery of a new binary radio pulsar, have spurred these lines of research. The results from high-energy Cherenkov experiments like MAGIC and HESS are opening a new window to study the extreme environment close to compact objects. Agile and GLAST will be fully operational, providing an unprecedented view of this type of systems. The proposed Joint Discussion aims at getting together experts in these fields for an analysis of the current situation and a view toward future prospects. 2009 will be the fourteenth year of operation of RossiXTE and it will mark the 10-year anniversary of the launch of XMM-Newton and Chandra. The Indian satellite for X-ray astronomy ASTROSAT will be in orbit, providing crucial fast-timing information. In addition, ESA, NASA and JAXA are currently analyzing the possibility of joining forces by merging the two major X-ray programs (Constellation-X and XEUS) into one large mission and we expect that the conclusions reached in this JD will help shape up the science program for it. All these constitute an ideal milestone for such a meeting. The proposed program includes ten major topics for which two solicited talks are envisioned, together with a small number of selected contributed talks. An additional session, distributed through the two days, will address future instrumentation for timing analysis. A poster session is also envisioned. A IAU JD provides an ideal setting for such a meeting and will allow discussions focused to these topics. Although the emphasis is on time variability, all aspects will be addressed, from radio observations to high-resolution spectra and high-energy emission.

The principal topics to be discussed:

    * quasi-periodic oscillations from mHz to kHz
    * X-ray bursts and superbursts
    * millisecond X-ray pulsars
    * AXP/SGR and magnetars
    * isolated neutron stars
    * very-high energy emission from neutron stars
    * gravitational waves from neutron stars
    * neutron-star equation of state and strong gravity
    * future instrumentation for timing

Hot Interstellar Matter in Elliptical Galaxies, Joint Discussion 8 at the IAU XXVII General Assembly

Dates: 2009 August 6 - 7
Place: Rio de Janeiro, Brazil

The physical properties of the hot interstellar matter in elliptical galaxies are directly related with the formation and evolution of elliptical galaxies via star formation episodes, environmental effects such as stripping, infall, and mergers, and growth of super-massiveblack holes. While the recent successful Chandra and XMM-Newton X-ray space missions have provided a large amount of high quality observational data on the hot ISM in elliptical galaxies, a number of important issues are still poorly understood, including the metal abundance discrepancy in some X-ray faint galaxies, the deviation from the solar abundance ratio of alpha elements, the wide range of hot gas contents for a given stellar mass, the effects of AGN-feedback on the dynamics and energetics of the hot ISM. This conference is intended to review the observational constraints available on the physical properties of the hot ISM and to confront the predictions of the latest simulations and analytical models of the dynamical/chemical evolution with observations.

IAU Symposium 267: Evolution of Galaxies and Central Black Holes: Feeding and Feedback

Dates: 2009 August 10 - 14
Deadline for Abstract Submission for Contributed Talks: 2009 February 2
Deadline for Early Registration: 2009 March 1
Deadline for Regular Registration: 2009 July 24
Place: Rio de Janeiro, Brazil

It is now widely recognized that nuclear activity is an important ingredient in shaping the evolution of galaxies. With the advent of techniques for estimating AGN black hole masses, even at large redshifts, and the availability of large quasar samples over a broad range of redshifts and selected at wavelengths ranging from the radio to the X-ray, the field has undergone transformational change. A major focus has become observational and theoretical investigation of nuclear activity in the context of the galactic environment, which can be described in terms of "feeding" and "feedback." AGN feeding is tightly correlated with redshift-dependent star formation in the host galaxy. AGN feedback, in the form of relativistic jets, massive winds, and intense radiation, has been invoked to solve a broad range of problems that arise in Cold Dark Matter-based models of galaxy formation: setting the critical mass scale for galaxies, regulating cooling in clusters, and shutting down star formation. Such feedback, feeding, and their mutual interaction might possibly account for the tight relationship between galactic bulge mass and central black hole mass.

The purpose of the symposium is to bring together researchers, both theorists and observers, from different specializations to better define the current global landscape and to motivate new lines of research. The timing of this symposium is propitious: HST is expected to be in its first full cycle after SM4 refurbishment, and ALMA, JWST, and LSST will be on the near-term horizon. The scientific program is as follows:

Session 1. The first galaxies and black holes

Session 2. Quasar and supermassive black hole demographics

Session 3. Multi-wavelength properties of AGN and their hosts

Session 4. Black hole masses, scaling relationships, and their evolution

Session 5. Accretion and feeding

Session 6. Outflows and feedback

Session 7. The Big Picture: Large-scale effects of feedback on galaxies and their environment

X-ray Astronomy 2009: Present Status, Multiwavelength Approach and Future Perspectives

Dates: 2009 September 7 - 11
(Extended) Deadline for Early Registration and Abstract Submission: 2009 May 15
Deadline for Final Registration: 2009 July 1
Place: Bologna, Italy

Third in a decadal series of X-ray astronomy conferences in Bologna, this meeting will highlight the contribution of XMM-Newton and Chandra observatories, ten years after their launch. Emphasis will be given on cosmic source multiwavelength studies and associated synergies with major facilities at all wavelengths, and on the perspectives for future high energy astrophysics missions.

The main scientific issues to be addressed are:

* STELLAR OBJECTS AND SUPERNOVA REMNANTS

	 - Cool and hot stars
	 - Star-forming regions 
	 - Neutron Stars
	 - Supernovae and SN remnants and pulsar wind nebulae
	 - Pulsars and Soft Gamma-Ray Repeaters 

* BLACK HOLES AND COMPACT OBJECTS  

        - Matter under extreme conditions 
        - Physics of Accretion and Ejection
	- X-rays as probes of General Relativity
	- Particle acceleration   
        - Evolution of Super-massive Black Holes
	- Black Hole-Galaxy Co-Evolution and Feedback processes

* GALAXIES AND CLUSTERS OF GALAXIES 

	-  Star formation across cosmic time 
	-  Physical processes in clusters and groups 
	-  Metal enrichement of the ICM 
	-  Interaction of cluster components 
	-  WHIM 
	-  Clusters of galaxies as cosmological probes

* PRESENT and FUTURE MISSIONS 

	- XMM, Chandra, Suzaku  
	- RossiXTE, INTEGRAL, Swift 
	- Simbol X, NuStar, EXIST, ASTRO-H
	- JANUS, GEMS, WFXT 
	- IXO 
	- Synergies with other wavelengths.

Black Holes in Binary Systems: Observations versus Theory

Dates: 2009 September 11 - 12
Deadline for Submission of Contributions: 2009 July 15
Place: Ferrara, Italy

The main goal of this workshop is to establish the current state of art in our understanding of the Physics of Black Hole sources, their spectral and timing signatures and to formulate the key fundamental problems of BH Physics and General Relativity, which can be addressed by future X-ray spectroscopic, timing and polarimetry missions.

Topics of the Workshop are:

  *  Spectra and variability of black-hole binaries
  *  Towards the measurement of fundamental parameters
  *  Spectral features, hard tails and annihilation lines
  *  Expectations from X-ray polarimetric observations of BH candidates. 

Chandra Calibration Review

Dates: 2009 September 21
Place: Boston, Massachusetts, USA

The Chandra Calibration Review (CCR) is held in order to disseminate and advance our understanding of the performance and capabilities of the Chandra X-ray Observatory. It is intended to share the Chandra teams' knowledge of the detectors, gratings, mirrors, and aspect system with the community while encouraging participation and feedback in the process of calibrating the observatory. Reports are solicited on various aspects of Chandra calibration.

This year, we will be holding the Calibration Review in conjunction with the Chandra's First Decade of Discovery symposium at the Seaport Hotel in Boston, Massachusetts. Calibration talks will be presented on Monday September 21, and calibration-related posters will be displayed throughout the symposium, which runs from Tuesday, September 22 through Friday, September 25.

Registration for the CCR is free and available through the Chandra's First Decade of Discovery website.

Ten Years of Science with Chandra: Chandra's First Decade of Discovery

Dates: 2009 September 22 - 25
Deadline for Oral Presentation Abstracts: 2009 July 10
Deadline for Other Abstracts and Hotel Reservations: 2009 August 21
Deadline for General and Student Registration: 2009 September 4
Place: Boston, Massachusetts, USA

This will be the fifth symposium in a series highlighting unique imaging and spectroscopic results from NASA's Chandra X-Ray Observatory. This event will celebrate key science results from the first ten years of operation of the Chandra X-ray Observatory. The focus will be on results which have had the largest impact on Astrophysics, including: The Cosmic Evolution of AGN, AGN outflows, evolutionary processes in clusters of galaxies, source populations and diffuse emission from normal galaxies, physical processes at the Galactic center, high spatial and spectral studies of neutron star physics, supernova remnants and star forming regions. It will also cover recent results from the XMM-Newton, Suzaku, Fermi Swift, INTEGRAL, RXTE and AGILE missions, as well as related theoretical results.

4th INTERNATIONAL WORKSHOP ON ASTRONOMY AND RELATIVISTIC ASTROPHYSICS (IWARA 2009): New Phenomena and New States of Matter in the Universe in the AUGER, SLAC, LHC, FERMI, FAIR/GSI and GEO/LIGO Era

Dates: 2009 October 4 - 8
Place: Maresias, Sao Paulo, Brazil

The main purpose of the event is to offer new opportunities for personal and professional growth of our students. For this reason, we feel it is very important to keep the series of meetings that began in 2003 in which astrophysicists, astronomers and scientists working in nuclear, and high-energy particle physics, for the first time in this series, meet with the intention of showing the latest results on a variety of topics involving new phenomena and new states of matter in the universe and therefore interact with their peers from around the world. The previous IWARA meetings were in 2003 (Olinda, Pernambuco, Brazil), 2005 (Natal, Rio Grande do Norte, Brazil), and 2007, Joao Pessoa, Paraiba, Brazil).

"New Phenomena and New States of Matter in the Universe' is the motto of this event. The topics of the workshop include General Relativity, Gravitation, Cosmology, Heavy Ion Collisions and the Quark-Gluon Plasma, White Dwarfs, Neutron Stars and Pulsars, Black Holes, Gamma Ray Bursts, High-Energy Cosmic Rays, Gravitational Waves, Dark Matter and Dark Energy, Strange Matter and Strange Stars, Antimatter and Ion Research, and Cosmic Matter in the Laboratory. Related topics are welcome.

Science with the New Generation of High Energy Gamma-ray Experiments: SCINEGHE-VII Workshop

Dates: 2009 October 7 - 9
Deadline for Registration: mid-September
Place: Assisi, Perugia, Italy

This is the seventh workshop in a series after six successful editions in Perugia (2003), Bari (2004), Cividale del Friuli (2005), Elba Island (2006), Villa Mondragone (2007) and Padova (2008).

Fundamental research on the nature of matter at the high energy frontier takes place in three main fields: accelerator-based particle physics, high energy astrophysics, and the cosmology of the early universe. The study of astroparticle physics can have significant implications for collider physics at the LHC, and, at the same time, the LHC project provides the laboratory to perform measurements of great importance for cosmic ray astrophysics and cosmology. By the end of this year the Large Hadron Collider will begin taking data and start the exploration of the TeV scale physics and of the physics beyond the Standard Model. The Fermi Gamma-Ray Space Telescope mission has started in June 2008 and, after nearly one year of excellent performance on orbit, is producing a huge number of physics results, some of them already published and many more will be available by the time of the workshop. Interesting results will be also available from PAMELA, ATIC and Auger on cosmic ray physics. Ground based experiments (HESS, MAGIC, VERITAS, MILAGRO and ARGO) have been observing photons at the TeV scale with unprecedented accuracy and will also provide new results for the incoming years. Finally neutrino experiments and underground experiments for direct observation of dark matter and neutrino mass measurement are doing rapid progress.

The workshop will be distributed over 3 days, aiming to bring together researchers with different scientific backgrounds, High Energy Physics and High Energy Astrophysics, to share interests and to exchange new results in the various fields. Participation and abstract submission of young researchers and PhD students are strongly encouraged.

INTEGRAL Workshop: The Extreme Sky: Sampling the Universe above 10 keV

Dates: 2009 October 13 - 17
Start of Online Registration: 2009 June 15
Deadline for Abstract Submission of Contributed Talks/Posters: 2009 August 15
Place: Otranto (Lecce), Italy

All-sky surveys form the foundation of observational astronomy as they provide:

    * statistics on the types and distribution of celestial objects which 
         populate the Galaxy and the Universe
    * the ability to discover new classes of sources
    * a means of selecting specific types of objects for further 
         studies/observations

With respect to other surveys, those at high energies (above 10 keV) are particularly interesting as they probe the energy domain where fundamental changes from thermal to non-thermal sources/phenomena are expected, where the effects of absorption are drastically reduced, and a clearer picture of the Universe is possible. This is also the energy range where most of the extreme astrophysical behaviour is taking place, e.g. cosmic acceleration, explosions and accretion onto black holes and neutron stars. Recently a number of surveys have been performed in the keV to TeV energy range.

The objective of this workshop is to gather all the knowledge collected so far above 10 keV, to compare and contrast the results obtained in the various bands in the light of physical models and ultimately provide indications for future progress. The meeting is aimed at bringing together scientists active across the high energy range in order to focus on the opportunities offered by this new window both from the observational and theoretical viewpoints, while a dedicated section will also be devoted to discuss future mission ideas. The meeting will consist of invited talks and contributions which are welcome as either posters or as short interventions. There will be time for open discussions throughout. Finally, this meeting is a perfect way in which to celebrate with friends and colleagues INTEGRAL's 7th birthday and 7 years of success in gamma-ray astronomy.

The workshop will be organized in sessions dedicated to:

    * The soft gamma-ray sky: Surveys and observations from: INTEGRAL, SWIFT, 
          SUZAKU, MAXI etc
    * The high energy gamma-ray sky: Surveys and observations from: AGILE, 
          FERMI, HESS, MAGIC etc
    * The search for counterparts: Synergies between surveys: 
          The multi-waveband approach
    * Comparing and contrasting the two skies: Similarities and differences: 
          which theoretical implications, New source typologies: 
          what have we learnt
    * Prospects for future missions above 10 keV: Decadal Survey, Cosmic 
          Vision national programs etc.

2009 Fermi Symposium

Dates: 2009 November 2 - 5
Place: Washington, DC, USA

The 2009 Fermi Symposium is dedicated to results and prospects for scientific exploration of the Universe with the Fermi Gamma-ray Space Telescope and related studies. The symposium comes shortly after the Fermi data release, offering an opportunity for the astrophysical community to share in the excitement of discoveries being made with the Fermi instruments. Topics include: blazars and other active galactic nuclei, pulsars, gamma-ray bursts, supernova remnants, diffuse gamma radiation, unidentified gamma-ray sources, and searches for dark matter. The meeting will be held in downtown Washington, D.C,. near the U.S. Capitol Building.

Swift Mission Conference: Celebrating 5 Years

Dates: 2009 November 17 - 20
Deadline for Early Registration: 2009 October 1
Place: State College, Pennsylvania, USA

The goal of the Swift Mission Conference is to bring together scientists who have worked with Swift data in the last five years to talk about science results and discuss strategies for the future.

Swift is a highly successful NASA mission. Although Swift's primary task still is to observe gamma-ray bursts, it is one of the most versatile missions ever flown. With its multiwavelength and fast-scheduling capacity, the mission is ideal for multiwavelength and/or monitoring programs. Thus, it has been used for AGNs, supernovae, variable stars, transients, comets, and other phenomena. Swift has observed the closest objects (comets) and, with GRB 050904, 080913, and 090423, some of the most distant objects in the universe.

The future will bring new opportunities for Swift with increasing capacities in the GeV and TeV energy ranges from Fermi, AGILE, VERITAS, MAGIC, and HESS, and with gravitational wave detectors such as LIGO, VIRGO, and GEO, and the neutrino detectors ICECUBE and ANTARES.

High Energy Astrophysics Division (HEAD) of the AAS Meeting

Dates: 2010 March 1 - 4
Place: Hawaii, USA

High-Resolution X-ray Spectroscopy: Past, Present, and Future

Dates: 2010 March 15-17
Deadline for Abstract Submission: 2009 November 1
Deadline for Regular Registration: 2010 January 15
Deadline for Late Registration: 2010 March 1
Place: Utrecht, The Netherlands

High-resolution X-ray spectroscopy has become a powerful tool for astrophysics since the launch of Chandra and XMM-Newton, now 10 years ago. The grating spectrometers on both instruments still continue to provide excellent data, while imaging calorimeters are being prepared for future missions like Astro-H and IXO. The synergy with other wavelength bands like the UV will be boosted by the addition of COS to HST. X-ray spectroscopy offers unique diagnostics to study almost any object in the Universe. In this meeting we foresee presentations on highlights and the state-of-the-art of X-ray spectroscopy for a broad range of objects and on the prospects for future studies.

38th Scientific Assembly of the Committee on Space Research (COSPAR) and Associated Events: COSPAR 2010

Dates: 2010 July 18 - 25
First Date for Abstract Submission: 2009 August 21
Deadline for Abstract Submission: 2010 February 19
Place: Bremen, Germany

Topics of COSPAR 2010 include:

Approximately 90 meetings covering the fields of COSPAR Scientific
Commissions (SC) and Panels:
- SC A:  The Earth's Surface, Meteorology and Climate 
- SC B:  The Earth-Moon System, Planets, and Small Bodies of the Solar System
- SC C:  The Upper Atmospheres of the Earth and Planets Including Reference 
         Atmospheres
- SC D:  Space Plasmas in the Solar System, Including Planetary Magnetospheres 
- SC E:  Research in Astrophysics from Space 
- SC F:  Life Sciences as Related to Space 
- SC G:  Materials Sciences in Space 
- SC H:  Fundamental Physics in Space 
- Panel on Satellite Dynamics (PSD)
- Panel on Scientific Ballooning (PSB)
- Panel on Potentially Environmentally Detrimental Activities in Space (PEDAS)
- Panel on Radiation Belt Environment Modelling (PRBEM)
- Panel on Space Weather (PSW)
- Panel on Planetary Protection (PPP)
- Panel on Capacity Building (PCB)
- Panel on Education (PE)
- Panel on Exploration (PEX)
- Special events:  Interdisciplinary lectures, space agency round table, etc.

For further details, contact:

The COSPAR Secretariat, 
c/o CNES, 2 place Maurice Quentin, 
75039 Paris Cedex 01, 
France 
Tel:     +33 1 44 76 75 10 
Fax:     +33 1 44 76 74 37
Email:   cospar@cosparhq.cnes.fr 
Website: http://www.cospar-assembly.org/

Other Selected Astronomy, Physics and Space Science meetings

1st Summer School on Multiwavelength Astronomy

Dates: June 29 - July 10
Deadline for Grant Applications and Registration: 2009 March 15
Place: Paris, France

Our current understanding of accretion onto black holes and neutrons stars has greatly evolved in the past 20 years, thanks in large part to the large amount of scientific data available at all wavelengths.

In the X- and gamma-rays these advances have been made possible by satellites such as XMM-Newton, Chandra, INTEGRAL, RXTE, Swift, and Suzaku, while new missions, like the Fermi Gamma-Ray Observatory, promise new discoveries. The same is true for radio astronomy, with many discoveries from existing world-leading radio-astronomical observatories such the ATCA, the VLA, the VLBA, the EVN, and MERLIN, with a range of major planned upgrades to these facilities, plus additional facilities planned and under construction.

Clearly, given these developments, the need for more researchers to exploit the enormous volume of available and upcoming scientific data, both by analyzing these data and interpreting them, is pressing. In this context, we announce an international summer school to provide young researchers the necessary expertise/skill to independently conduct data-analysis related to high energies and radio astrophysics.

The school will focus on X-ray/Gamma-ray and radio data analysis, with one week spent on each topic. The program will cover a mixture of practical hands-on data analysis sessions (using, for example, AIPS, Miriad, HEADAS, CIAO, and XMM-SAS). The school will also include science talks and complementary skills training. Priority will be given to hands-on sessions of data-analysis.

The audience targeted by the school is primarily PhD students and possibly post-docs.

----------------- application form / cut here ------------------------

To be sent to: mwschool@black-hole.eu

			   APPLICATION FORM
----------------------------------------------------------------------
	    1st Summer School on Multiwavelength Astronomy
----------------------------------------------------------------------
		       29 June - 10 July  2009
----------------------------------------------------------------------
			    Paris, France
----------------------------------------------------------------------

Last name:
First Name :
Title (Ms/Mr/Dr.):

Age:
Sex (F/M):

Position:

Address:

E-mail:
Tel:
Fax:

Scientific interests:

Application for support (Y/N):
Financial support required (Y/N):

I have attached the following files IN PDF FORMAT:

Curriculum Vitae (Y/N):
Letter of motivation (Y/N):
Letter of recommendation (Y/N):

Note: only complete applications can be considered

----------------- application form / cut here -----------------------

IAU XXVII General Assembly

Dates: 2009 August 3 - 14
(Extended) Deadline for On-line Abstract Submission: 2009 March 31
Deadline for Early On-line Registration: 2009 May 1
Regular On-line Registration: 2009 May 2 - July 24
Start of On-site Registration: 2009 August 3
Place: Rio de Janeiro, Brazil

Reionization to Exoplanets: Spitzer's Growing Legacy

Dates: 2009 October 26 - 28
Deadline for Early Registration: 2009 August 15
Deadline for Late Off-Site Registration: 2009 October 16
Place: Pasadena, California, USA

The 2009 Spitzer Science Center Conference, 'Reionization to Exoplanets: Spitzer's Growing Legacy', will occur shortly after the end of Spitzer's highly successful cryogenic mission, and at the start of the Spitzer warm mission. The meeting will celebrate the accomplishments of the cryogenic mission, and assess future opportunities in the fields where Spitzer's impact has been greatest. In particular, the meeting will be organized into five half day sessions, with each session focusing on a single science topic. The five session topics are:

1. Exoplanets and Exoplanetary Systems (planets, atmospheres, planetary systems, solar system)
2. Star Formation (molecular cloud cores, protoplanetary and debris disks, planet formation)
3. The Early Universe (structure and galaxy formation, young galaxies, star formation, stellar populations)
4. The Dusty Universe (nearby galaxies, starbursts, (U)LIRGs, sub-mm galaxies, AGNs)
5. The Galaxy (Galactic structure, interstellar medium).

In support of the Warm Spitzer mission, all Spitzer Cycle 6 Exploration Science teams are invited to hold team meetings during the conference. Please send the organizers an email to reserve space and time for your special break-out session. Meeting space for other Spitzer-related teams that wish to hold team meetings during the conference will be provided on an "as available" basis.

The oral program will consist entirely of invited reviews. All other attendees are urged to submit poster presentations on any aspect of astrophysical theory or observations related to the Spitzer mission.

American Astronomical Society Meeting 215

Dates: 2010 January 3 - 7
Place: Washington, DC, USA

Selected Astronomy-related Technology (e.g., Detectors) meetings

None

Selected Astronomy-related Physics, Computational, Data Analysis, Software or Statistics meetings

None

Selected Space Science-related Education and Public Outreach meetings

None


Page Author: Stephen Drake


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