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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 March 17 - 18: High-Resolution X-ray Spectroscopy School

2009 March 19 - 20: 3rd High-Resolution X-ray Spectroscopy Workshop

2009 March 30 - April 1: STScI Conference on Observational Signatures of Black Hole Mergers

2009 March 30 - April 3: The First PANDA Symposium on Products of Astrophysical Outflows

2009 April 27 - 30: The coming of Age of X-ray Polarimetry

2009 May 2 - 5: 2009 "April" American Physical Society Meeting

2009 May 13 - 15: RICAP09 2nd Roma International Conference on Astro-Particle Physics

2009 May 18 - 20: Supersoft X-ray Sources - New Developments

2009 May 19 - 21: Multi-Messenger Relativistic Astrophysics 2009

2009 June 1 - 5: The Monster's Fiery Breath: Feedback in Galaxies, Groups, and Clusters

2009 June 21 - 26: Windows on the Universe: XXIth Rencontres de Blois

2009 June 22 - 26: Accretion and Ejection in AGN: A Global View

2009 June 28 - July 3: The Many Faces of Centaurus A

2009 June 29 - July 3: 9th XMM-Newton SAS Workshop

2009 June 29 - July 2: The Energetic Cosmos: from Suzaku to ASTRO-H (3rd Suzaku Conference)

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 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 21: Chandra Calibration Workshop

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, LHC, FAIR/GSI and GEO/LIGO Era

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

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 March 26 - 27: Beyond JWST: The Next Steps in UV-Optical-NIR Space Astronomy

2009 May 4 - 7: The search for Life in the Universe (Spring 2009 STScI Symposium)

2009 June 7 - 11: American Astronomical Society Meeting 214

2009 June 8 - 10: Bridging Laboratory and Astrophysics: From the Infrared to the Submm: A Meeting-in-a-Meeting (MiM) during the 214th AAS Meeting

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

2009 August 3 - 14: IAU XXVII General Assembly

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

2009 March 22 - 26: 16th Atomic Processes in Plasmas Conference: APiP-2009


Selected Space Science-related Education and Public Outreach meetings


High Energy Astrophysics meetings

High-Resolution X-ray Spectroscopy School

Dates: 2009 March 17 - 18
Deadline for Registration and Abstracts: 2009 February 1
Place: Dorking, Surrey, UK

3rd High-Resolution X-ray Spectroscopy Workshop

Dates: 2009 March 19 - 20
Deadline for Registration and Abstracts: 2009 February 1
Place: Dorking, Surrey, UK

The 'new beginning' with the integration of XEUS and Con-X into IXO, the many other X-ray astronomy missions under study aimed at high spectral resolution, together with the high quality data that XMM-Newton and Chandra will hopefully continue to procure for a while yet, promise further expansion and strengthening of the high resolution X-ray spectroscopy field. We therefore invite you to attend the high resolution X-ray spectroscopy workshop, to take place on 19-20 March 2009 at the UCL Mullard Space Science Laboratory.

For the first time this year we will also be running a 'high resolution X-ray spectroscopy school', prior to the workshop, on 17-18 March 2009. Aimed at PhD students and postdocs working both in and outside X-ray astronomy, it will be an opportunity to learn the principles and practice of high resolution X-ray spectroscopy as applied to a range of stellar, Galactic and extragalactic sources.

For further details, a list of the invited speakers, and registration, see: http://www.mssl.ucl.ac.uk/~ajb/workshop3/. There will be a limited number of places, so we advise participants to register as soon as possible.

Observational Signatures of Black Hole Mergers (STScI Conference)

Dates: 2007 March 30 - April 1
Deadline for Hotel Reservations at Conference Rate: 2009 March 10
Place: Baltimore, Maryland, USA

Motivated by recent advances in numerical relativity and with an eye towards the future of gravitational wave observatories, we are pleased to announce a conference on the observational signatures of supermassive black hole mergers, including electromagnetic signals detectable today. The primary goal of this meeting is to bring together theorists and observers from a number of different fields and foster the communication that is critical for moving forward in actually detecting and characterizing the properties of merging black holes over a wide range of time-scales. To this end, the conference will be structured around a relatively small number of plenary sessions with a large amount of time dedicated for discussion. The topice to be covered are:

Black Holes in Galaxy Mergers and Evolution
Black Hole Merger Mechanisms ("The Final Parsec Problem")
Gravitational Waves
Electromagnetic Counterparts
Gravitational Recoil
Imprint on Galaxy Structure
Spin as a Probe of Black Hole Evolution
Next-generation Observatories

First PANDA Symposium on Products of Astrophysical Outflows

Dates; 2009 March 30 - April 3
Deadline for Early Registration: 2009 February 15
Deadline for Abstract Submission: 2009 February 20
Place: Lijiang, Yunnan, China

This is the first of a new Symposia series aimed at establishing and fostering collaborations among young post doctoral fellows (0-6 years from graduation) from the Pacific/Asiatic scientific community with their peers across the globe. Besides enabling scientific mobility and networking, the organizers are also aiming in providing young researchers with a forum to exchange ideas on current and future projects. To this end, the meeting will include several tutorials from senior lecturers during the first day, and three evening lectures, in the following days. The Symposia should take place every 2 years and the first three should be held in China near Panda natural reserves.

Topics include:

    * Bubbles and Super Bubbles
    * Planetary Nebulae
    * Stellar Winds and Jets
    * AGNs
    * Supernovae Remnants
    * Magnetars and GRBs

The coming of Age of X-ray Polarimetry

Dates: 2009 April 27 - 30
Deadline for Regular Registration: Now through 2009 February 28
Deadline for Late Registration: 2009 March 1 - April 27
Place: Rome, Italy

The advent of a new generation of X-ray polarimeters, to be combined with large area X-ray telescopes, has renewed interests in the X-ray polarimetry, as demonstrated by the several polarimetric missions recently proposed to various space agencies. The possibility to have a X-ray polarimetric mission operating in the near future is indeed concrete, not forgetting that a polarimeter is one of the candidate instruments to be part of the focal plane of the International X-Ray Observatory (IXO). After more than four years from the last X-ray Polarimetry Workshop (February 2004), the organizers believe it is time to hold a conference with the aim of discussing the present status and perspectives of instruments as well as to review and discuss the theoretical models. They would like not only to gather the community actively involved in X-ray polarimetry (both on the instrumental and theoretical sides), but also and foremost to stimulate the interest in a wider community, hampered so far by the lack of observational perspectives.

2009 "April" American Physical Society Meeting

Dates: 2009 May 2 - 5
Deadline for Abstract Submission: 2009 January 9 at 5:00 pm EST
Deadline for Housing Reservations: 2009 February 13 or April 1 (?)
Deadline for Early Bird Registration: 2009 February 27
Deadline for Late Registration: 2009 April 3
Place: Denver, Colorado, USA

The theme of this year's "April APS" meeting will be "New Eyes on the Universe: 400 years since Galileo's Telescope". The April Meeting, which brings together nuclear, particle, gravitational, accelerator, plasma, and astrophysicists, will have a strong focus on astrophysics this year, featuring 4 astrophysics plenary talks (of the 9 total), 19 invited sessions on astrophysical topics and two town meetings (JDEM and the Decadal Survey).

Some activities related to the Astronomy 2010 decadal survey will be held at this meeting. A special Town Hall session will be held on Monday night May 4th and two invited sessions will be held on Tuesday May 5th entitled New Facilities in Particle Astrophysics I & II.

RICAP09 2nd Roma International Conference on Astro-Particle Physics

Dates: 2009 May 13 - 15
Place: Frascati, Rome, Italy

RICAP09 (Roma International Conference on Astro-Particle Physics) is the second edition of a series of International Conferences entirely dedicated to high energy cosmic rays study, organized by the three public Universities and INFN Sections in Rome (University and INFN of Roma La Sapienza, University and INFN of Roma Tor Vergata and University and INFN of Roma Tre).

In these institutions there is an intense activity on Astro-Particle physics, visible in the participation to major experimental projects in the field (AGILE, AMS, ANTARES, ARGO, AUGER, FERMI, NEMO, PAMELA, ...) and in a deep and fruitful theoretical work.

The Conference will be held every two years. The first edition was held at the University of Roma La Sapienza, the second edition will be hosted by the University of Roma Tor Vergata and the third edition will be at Roma Tre.

Supersoft X-ray Sources - New Developments

Dates: 2009 May 18 - 20
Deadline for Abstract Submission: 2009 March 13
Deadline for Hotel Bookings: 2009 April 7
Place: Villafranca, near Madrid, Spain

After the discovery of supersoft X-ray sources (SSS) with the Einstein Observatory, the detection of about a dozen luminous SSS in the Magellanic Clouds in the ROSAT all-sky survey data established luminous SSS as a class of objects. Later, ROSAT pointed observations revealed SSS also in the Milky Way and other nearby galaxies.

XMM-Newton and Chandra have been in orbit for about one decade. High-resolution X-ray spectra of SSS are crucial for our understanding of the emission process in these systems. With their high-sensitivity instrumentation SSS can be investigated in more distant galaxies. XMM-Newton and Chandra surveys of M 31 revealed that most SSS in M 31 are identified with optical novae with various durations of the SSS state lasting from months to more than 10 years. Monitoring observations with Swift allow us to investigate the spectral evolution during the SSS state. The aim of the workshop is to summarise the present status of supersoft X-ray sources research from the observational as well as the theoretical side in order to identify the most critical unsolved problems.

Multi-Messenger Relativistic Astrophysics 2009

Dates: 2009 May 19 - 21
Deadline for Abstract Submission and Registration: 2009 April 15
Place: Atlanta, Georgia, USA

The School of Physics at the Georgia Institute of Technology is pleased to announce the inaugural conference of the Center for Relativistic Astrophysics (CRA): Multi-Messenger Relativistic Astrophysics 2009. The newly established CRA is devoted to interdisciplinary research and education in multi-messenger astrophysics, linking high energy, particle and gravitational astrophysics. This inaugural conference is an opportunity for participants to share their insights and experience on research focusing on extreme astrophysical phenomena such as merger of black holes and neutron stars, central engines of active galactic nuclei, gamma ray bursts, and sources of the high energy cosmic rays and neutrinos.

The Monster's Fiery Breath: Feedback in Galaxies, Groups, and Clusters

Dates: 2009 June 1 - 5
Pre-Registration: Open
Place: Madison, Wisconsin, USA

The past decade has shown that black hole growth and the formation of large scale structure are intimately linked. With the astrophysical community having largely converged on this view, the scientific task at hand is to determine the nature, strength, and ultimate relevance of this link. In honor of the 10th anniversary of the Chandra X-ray Observatory, which has been instrumental in demonstrating the importance of feedback and in anticipation of the first year of GLAST, which will be instrumental in making the next step towards a consistent picture of how black hole growth and large scale structure formation are coupled, as well as the next generation of low frequency radio telescopes, the 2009 Wisconsin meeting on feedback from galaxies to clusters will bring together a broad group of researchers with one common goal: To lay the path for the next decade of work on feedback in structure formation.

Windows on the Universe: XXIth Rencontres de Blois

Dates: 2009 June 21 - 26
Deadline for Conference Registration, Abstract Submission and Hotel Reservation: 2009 April 15
Place: Blois, Loire Valley, France

'Windows on the Universe' will emphasize that our current understanding of the Universe is intimately related to the wide variety of techniques, experimental, observational and theoretical, now available to study it. The year 2009 has been dubbed "World year of astronomy"; it is in fact the 400th anniversary of Galileo's first use of a telescope to study the sky, and also the 400th anniversary of the publication of Kepler's laws of planetary motion, which led ultimately to our understanding of gravitational forces.

Windows on the Universe will be organised around a number of basic themes, including:

    * The electromagnetic window
    * The gravitational window
    * The astroparticle window
    * Accelerator physics
    * Fundamental processes

Accretion and Ejection in AGN: A Global View

Dates: 2009 Jun 22 - 26
Deadline for Pre-Registration: 2009 January 14
Deadline for Registration and Abstract Submission: 2009 April 15
Place: Como, Italy

The workshop will cover major observational and theoretical aspects of fuelling, accretion disks, outflows and relativistic jets in AGN, with emphasis on their interconnection and relation to environment. These topics are essentially multiwavelength in nature but rely especially on the high-energy side of the electromagnetic spectrum (X-rays, GeV and TeV gamma-rays). In particular, results from the AGILE and FERMI Gamma-Ray Telescopes and the second generation of Cherenkov telescope arrays will be presented.

The covered topics will include:

    * Fueling supermassive black holes and AGN activity
    * Accretion "modes"
    * Accretion Disks and Outflows
    * News from AGILE/FERMI and Cherenkov Telescopes
    * Jets - Structure and emission mechanisms at small and large scale
    * Radio-quiet vs. radio-loud AGN: what makes the difference?
    * Feed back from radio-loud/radio-quiet AGN
    * Accretion and ejection: a balance?

The Many Faces of Centaurus A

Dates: 2009 June 28 - July 3
Deadline for Registration:2009 February - April
Place: Sydney, Australia

This conference aims to bring together a broad range of astronomers and high-energy physicists that traditionally form separate research communities but are all involved in some way in the detailed studies of the very nearby, active, massive galaxy Centaurus A/NGC 5128. Since its discovery as a radio source 60 years ago, the radio galaxy Centaurus A (NGC 5128) has attracted great interest from the international astrophysics and high energy physics communities, and yet this will be the first conference devoted to this intriguing source.

9th XMM-Newton SAS (Science Analysis Software) Workshop

Dates: 2009 June 29 - July 3
Deadline for Apllications: 2009 March 31
Place: Villafranca del Castillo, near Madrid, Spain

SAS Workshops aim at providing XMM-Newton users with a basic introduction to the procedures and techniques to successfully reduce and analyse XMM-Newton data. The 4-day workshop is organised around 4 half-days of presentations and 4 half-days of practical training sessions. An extra day can be allocated for practical training sessions upon demand. The sessions cover all aspects of data reduction and data analysis for all the X-ray cameras on-board XMM-Newton, as well as for its Optical Monitor.

Interested persons are encouraged to send an email through the XMM-Newton Helpdesk no later than Tuesday, March 31, 2009. Please specify in the subject line:
Subject: Interest in participating in the 9th XMM-Newton SAS Workshop
and provide the following information:

Name                   :
Organisation           :
Address                :
Country                :
Phone                  :
E-mail                 :
Main Research Field    :
Do you need means of transportation between pre-booked
accommodation at El Escorial and Venue at ESAC ?               : YES/NO
Will you bring your own laptop ?                               : YES/NO
Interested in having an extra 5th day for practical sessions ? : YES/NO
Would you like to have an introductory session to XSPEC ?      : YES/NO

No fee is required to attend the SAS Workshop. We regret that no financial support is available for Workshop participants.

The Energetic Cosmos: from Suzaku to ASTRO-H (3rd Suzaku Conference)

Dates: 2009 June 29 - July 2
Registration: Now Open
Deadline for Registration and Abstract Submission: 2009 March 16
Deadline for Registration (if not giving a paper) and for Hotel Booking: 2009 April 13
Place: Otaru, Hokkaido, Japan

Since the launch on 2005 July 10, the cosmic X-ray satellite Suzaku has been operating successfully under a close Japan-US collaboration. Thanks to the unprecedented broad-band coverage provided by the XRT+XIS and the HXD, aided by their low backgrounds and good energy responses, a large amount of scientific results are accumulating. In the International Year of Astronomy 2009, it is our hope to harvest them, and assemble them into novel research paradigms that innovate our view of The Energetic Cosmos.

These attempts will further strengthen the ASTRO-H (previously known as NeXT) project, Suzaku's successor, which is making a steady progress toward its launch around 2013. Our scope also includes NuStar and Simbol-X, and further extends to the genuine one-world X-ray mission, IXO. At the same time, the Fermi Gamma-Ray Space Telescope is producing excellent initial results. The MAXI (Monitor of All-Sky X-ray Image) experiment, to be onboard the ISS Japan Experimental Module, is also ready for launch in May 2009.

Given these plentiful high-energy astrophysics results, the 3rd Suzaku conference has been organized. This conference follows the first one held at Kyoto/Japan in December 2006, and the second at San Diego/California in December 2007. The conference will be organized so as to highlight common physics among different types of objects, rather than treating them separately. Focusing mainly on the results obtained with Suzaku, the conference will also cover new results from related missions, Chandra, XMM-Newton, INTEGRAL, Swift, Fermi, and others.

Topics to be covered include:

- Particle acceleration in cosmic shocks and jets (SNRs, Blazars,GRBs,..)
- X-ray diagnostics of cosmic hot plasmas (Galactic diffuse, SNRs, 
    clusters,..)
- Magnetic activities in stellar objects (pulsars/magnetars, WDs, 
    stellar flares,.. )
- Primary and reprocessed emissions from accreting objects (BHBs,LMXBs, 
    ULXs, AGNs, ..)
- X-ray views of the evolution of the universe (GRBs, AGNs, clusters, ..)
- Highlights from the Fermi Space Gamma-Ray Telescope
- Status of the MAXI experiment
- From Suzaku to ASTRO-H and other missions, and further to IXO

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.

TeV Particle Astrophysics 2009

Dates: 2009 July 13 - 17
Place: Menlo Park, California, USA

In 2009 the Large Hadron Collider is scheduled to start exploring the TeV frontier searching for signals of Physics beyond the Standard Model. Meanwhile satellite experiments exploring high energy, Fermi GLAST and Pamela, and a number of ground based TeV telescopes have been in operation for some time. In addition, underground direct detection experiments contiunue to make considerable progress in exploring limits on dark matter. This Meeting will focus on the contributions of astrophysical observations, direct detection experiments, and TeV accelerator results, that are probing fundamental physics at the TeV scale of particle physics. The aim of the meeting is to enable understanding of what we have and can learn from recent and upcoming experiments exploring the TeV scale and above.

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
Deadline for Early Registration and Abstract Submission: 2009 May 1
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.

Chandra Calibration Workshop

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

The Chandra Calibration Workshop (CCW) is held regularly for the dissemination and advancement of 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. Abstracts are solicited on various aspects of Chandra calibration.

This year, we will again be holding the CCW in conjunction with a Chandra anniversary symposium, the Ten Years of Science with Chandra Symposium (see next item). Calibration talks will be presented on Monday September 21, prior to the Symposium. Calibration-related posters will be displayed throughout the Symposium, which runs from Tuesday, September 22 through Friday, September 25.

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

Dates: 2009 September 22 - 25
Place: Boston, Massachusetts, USA

The fifth in a series, this meeting will highlight key science results from the first ten years of operation of the Chandra X-ray Observatory. To stay informed about the Symposium, subscribe to the mailing list. Send email to majordomo@head.cfa.harvard.edu with "subscribe chandra10" (without the quotation marks) in the body of the message.

4th INTERNATIONAL WORKSHOP ON ASTRONOMY AND RELATIVISTIC ASTROPHYSICS (IWARA 2009): New Phenomena and New States of Matter in the Universe in the AUGER, LHC, 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.

High Energy Astrophysics Division (HEAD) of the AAS Meeting

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

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

Beyond JWST: The Next Steps in UV-Optical-NIR Space Astronomy

Dates: 2009 March 26 - 27
Place: Baltimore, Maryland, USA

The Association of Universities for Research in Astronomy (AURA) is sponsoring a workshop to engage the UV/optical/Near-IR (UVOIR) astronomy community to discuss its long-term goals for space-based astronomy and astrophysics. The meeting will provide the community with an opportunity to look forward on a 25-year horizon to identify the scientific opportunities enabled by large and very large space telescopes and to outline a path forward that will form the basis for a community-led report to the NRC 2010 Decadal Review Committee.

The focus of the workshop program will be heavily science-based with topics covering:

-	Detection & Characterization of Exoplanets
-	Solar System
-	Local Galactic Neighborhood
-	Star Formation and Evolution
-	IGM and Chemical Evolution of Universe
-	Galaxy Formation & Evolution
-	Cosmology: Dark Matter/Lensing/Dark Energy

Representatives from NASA Astrophysics Mission Concept Studies that are relevant to UVOIR space astrophysics are also being invited to give short presentations. Additional presentations will include NASA and ESA long-range plans and advanced technological possibilities for UVOIR telescopes.

The Search for Life in the Universe (Spring 2009 STScI Symposium)

Dates: 2009 May 4 - 7
Deadline for Early Registration: 2009 March 1
Place: Baltimore, Maryland, USA

The concept that life might exist elsewhere besides the Earth has intrigued humankind for centuries. Technology has now enabled this fundamental question to be pursued with substantial international scientific vigor. Within the Solar System several Mars probes, as well probes to the moons of Jupiter (Europa) and Saturn (Titan), are being developed with specific emphasis on the development of in-situ instrumentation to detect the presence of life. Beyond the Solar System, the search for life signs has gained momentum with the rapid growth in the number of known exoplanets. While the detection of exoplanets is challenging conventional views of planet formation, it has also created opportunities for new observational methods to detect and characterize habitability and bio-signatures. And the study of life on Earth has revealed surprising constraints on the limits of life with the discovery of extremophiles capable of surviving in near-freezing, near-boiling, non-aqueous, or high radiation environments.

The STScI 2009 Spring Symposium will divide discussion of the motivations and expectations for the search for life in the universe into three distance domains that each require markedly different observational approaches and speakers from multiple disciplines: detecting Life within 50 AU of Earth, detecting life within 100 pc of Earth, and detecting life beyond 100 pc from Earth.

The program will consist of invited talks and contributed posters. Specific scientific themes have been selected for each day:

May 4 (day 1): "Milepost Zero: Life on Earth"
May 5 (day 2): "The Search for Life Within 50 A.U"
May 6 (day 3): "The Search for Life Within 100 pc"
May 7 (day 4): "The Search for Life in the Galaxy"

American Astronomical Society Meeting 214

Dates: 2009 June 7 - 11
Deadline for Abstracts: 2009 March 2 at 9:00pm EST
Deadline for Early Registration: 2009 March 20
Deadline for Regular Registration: 2009 April 30
Deadline for Late Abstracts: 2009 April 30 at 9:00pm EST
Deadline for Late (Off-Site) Registration: 2009 June 1
Place: Pasadena, California, USA

Bridging Laboratory and Astrophysics: From the Infrared to the Submm: a Meeting-in-a-Meeting (MiM) at the 214th Meeting of the American Astronomical Society (see above)

Dates: 2009 June 8 - 10
Deadlines: Same as for the Main AAS Meeting
Place: Pasadena, California, USA

This 3 day Meeting-in-a-Meeting will be devoted to the interplay between laboratory astrophysics and IR, FIR and Submm astronomy. The sessions will discuss current and future missions and facilities that operate in this domain and their laboratory astrophysics needs. Astronomy is an observational science detecting photons generated by atomic/molecular/chemical, and solid-state physics. The astrophysically motivated studies, which consist of both laboratory experiments and theoretical calculations, are collectively known as laboratory astrophysics. This Meeting-in-a-Meeting will consist of six sessions that will discuss the nature and evolution of molecules, dust and ices from stellar and planetary formation regions to circumstellar, planetary nebulae and diffuse ISM environments to comets and planets. The sessions map the sub areas of laboratory astrophysics in the IR, FIR and Submm domains and cover the study of molecules, dust and ices. Each session will include talks focusing on major mission projects and key data needs, related experimental and theoretical work, all illustrating the important role of laboratory astrophysics in support of current and future missions and facilities. There will be an associated poster session on astronomical observations and laboratory astrophysics of molecules, dust and ices in the IR - Submm. Student participation is particularly encouraged.

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

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

16th Atomic Processes in Plasmas Conference: ApiP-2009

Dates: 2009 March 22 - 26

Deadline for Abstract Submission and Early Registration: 2009 January 16
Deadline for Final Registration: 2009 March 16
Place: Monterey, California, USA

Topics covered:

High-energy density physics

    * laser and pulsed-power facilities
    * fast-ignition and inertial fusion

Astrophysical plasmas
Magnetic-fusion plasmas

    * ITER, DIII-D, JET, etc.

Bench-top scale plasmas

    * table-top lasers, EBITs

Next generation light sources

    * LCLS, DESY, free-electron lasers

Fundamental atomic data
Fundamental modeling and Plasma diagnostics 

Selected Space Science-related Education and Public Outreach meetings

None


Page Author: Stephen Drake


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