Conférences - Astronomie, astrophysique et cosmologie

Conference-Service.com met à la disposition de ses visiteurs des listes de conférences et réunions dans le domaine scientifique. Ces listes sont publiées pour le bénéfice des personnes qui cherchent une conférence, mais aussi, bien sûr, pour celui des organisateurs. Noter que, malgré tout le soin que nous apportons à la vérification des données entrées dans nos listes, nous ne pouvons accepter de responsabilité en ce qui concerne leur exactitude ou étendue. Pensez donc à vérifier les informations présentées avec les organisateurs de la conférence ou de la réunion avant de vous engager à y participer!

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1.
 
IAU Symposia: Astroinformatics
ID
761850
Dates
29 sep 2016 - 04 oct 2016
Lieu
Sorrento, Italie
Résumé
The proposed symposium will bring together world-class experts to address the methodological and technological challenges posed by massive data sets produced by the new generation of telescopes and observatories. Astronomy is at the forefront of Big Data science with exponentially growing data volumes and data rates, now entering the petascale regime at optical, infrared and radio wavelengths. The data structures are not simple, and the procedures for using them to gain astrophysical insights are not obvious. Astronomy is truly becoming data-driven in the ways that are both quantitatively and qualitatively different from the past. The informational content of the modern data sets is so high that archival research and data mining not merely profitable, but practically obligatory; researchers who obtain the data can only extract a small fraction of the science that is enabled by it.
2.
 
XV Latin American Regional IAU meeting
ID
757594
Date de début
02 oct 2016
Lieu
Cartagena de Indias, Colombie
3.
 
XV Latin American Regional IAU Meeting
ID
761353
Dates
02 oct 2016 - 07 oct 2016
Lieu
Cartagena, Colombie
Résumé
From October 3 to 7, 2016, Colombia is hosting the XV LARIM 2016 (Latin American Regional IAU Meeting). This is the most important meeting among the community of astronomy and astrophysics in Latin America and represents an important milestone for Colombia into the IAU (International Astronomical Union).   The meeting's agenda responds to one of the main needs for astronomers and astrophysicists in our country: the internationalization of scientific production in these areas, as well as the formation of human talent, both carried out by the country over the last years.   The event includes several educational and scientific public and private sectors which have committed to providing financial and logistical support for the successful completion of it. Additionally, this is an important opportunity to consolidate a joint research agenda, sponsored by the strong support of the International Astronomical Union (IAU).
4.
 
The ISM-SPP Olympian School of Astrophysics 2016
ID
794029
Date de début
03 oct 2016
Lieu
Paralia Katerini's, Mount Olympus, Grèce
5.
 
Stars: from collapse to collapse
ID
799461
Dates
03 oct 2016 - 07 oct 2016
Lieu
Special Astrophysical Observatory, Nizhnij Arkhyz, Russie
6.
 
IAUS 326: Research in Astronomy Education: Far Reaching Impacts and Future Directions
ID
734594
Date de début
04 oct 2016
Lieu
Heidelberg, Allemagne
7.
 
IAU Symposia: Research in Astronomy Education - Far Reaching Impacts and Future Directions
ID
761948
Dates
04 oct 2016 - 07 oct 2016
Lieu
Heidelberg, Allemagne
Résumé
Astronomy education research has become a respected subdiscipline of astronomy. Scientific results from this field have great potential to enhance the teaching and learning of astronomy for learners of many ages. New results and research methodologies from the cognition and learning sciences domains are now able to influence the work of astronomy educators, enabling them to make informed innovations for the teaching of astronomy. Generally, professional astronomers who have responsibilities that include teaching are not aware of the results of astronomy education research, and this Symposium can help expand attendee's awareness of results, as well as providing a forum for active experts in astronomy education to jointly plan the research agenda for the upcoming decade. Thus, the central objective of the meeting is aiming at an increase of the quality and impact of astronomy education.
Sujets apparentés
8.
 
4th National Conference on Space Science & Technology
ID
835967
Dates
07 oct 2016 - 09 oct 2016
Lieu
Karachi, Pakistan
Résumé
The Institute of Space & Planetary Astrophysics, University of Karachi, Karachi, Pakistan is organizing “4th National Conference on Space Science & Technology” on October 7-9, 2016 at University of Karachi, Karachi for celebrating “World Space Week 2016”. This conference is to be held in collaboration with SUPARCO and Higher Education Commission, Pakistan.
Contact
Faisal Afridi;     Email.: fakafridi@hotmail.com
Sujets
Astronomy / Radio Astronomy, Astrophysics, Computational Astrophysics, Cosmology, Satellite Communication / GNSS, Space Antennas, Space Technology & Industry, Flight Dynamics / Aerodynamics, Space Plasma, Remote Sensing & GIS, Solar System & Extrasolar Planets, Climate Change, Astro-Chemistry Space-Biology, Planetary Atmospheric Sciences, Climatology & Meteorology, Renewable Energy, Environmental Sciences / Natural Hazards and Physical Oceanography.
9.
 
IWARA 2016 — 7th International Workshop on Astronomy and Relativistic Astrophysics
ID
793921
Date de début
09 oct 2016
Lieu
Gramado, RS, Brésil
10.
 
IAU Symposium 327: Fine Structure and Dynamics of the Solar Atmosphere
ID
794257
Date de début
09 oct 2016
Lieu
Cartagena de Indias, Colombie
11.
 
IWARA2016 — 7th International Workshop on Astronomy and Relativistic Astrophysics
ID
782407
Dates
09 oct 2016 - 13 oct 2016
Lieu
GRAMADO, RIO GRANDE DO SUL, Brésil
Résumé
Our understanding of the origin of the Universe, of its evolution and the physical laws that govern its behavior, as well as on the different states of matter that make up its evolutionary stage, reached in recent years levels never before imagined. This is due mainly to the new and recent discoveries in astronomy and relativistic astrophysics as well as to experiments on particle and nuclear physics that made the traditional boundaries of knowledge on physics to be overcome. As a result we have presently a new understanding about the Universe in its two extreme domains, the very large and the very small: the recognition of the deep connections that exist between quarks and the cosmos. Based on the understanding of the intimate relationship between quarks and cosmos, the IWARA meetings is focused on topics that connect these two extreme physical domains.
Contact
Cesar Augusto Zen Vasconcellos;     Tél.: [+555191527996];     Email.: iwara2016@gmail.com
Sujets
New phenomena and new states of matter in the Universe, General Relativity, gravitation and cosmology, white dwarfs, neutron stars, pulsars and black holes, gamma-ray emission in the Universe, high energy cosmic rays and gravitational waves, strong magnetic fields in compact stars and in galaxies, ultra-strong magnetic fields in neutron star mergers, strange matter, strange stars, quark stars and magnetars, strong magnetic fields and the cosmic microwave background, dark matter and dark energy, antimatter in the Universe, strong magnetic fields in the Universe, heavy ion collisions and the formation of the quark-gluon plasma, and topics related.
12.
 
IAU Symposia: Fine Structure and Dynamics of the Solar Atmosphere
ID
761881
Dates
09 oct 2016 - 13 oct 2016
Lieu
Cartagena, Colombie
Résumé
The scientific goal of this symposium is to discuss recent results on the processes shaping the structure of the solar atmosphere and driving plasma eruptions and explosive events.  Activity of the solar atmosphere entails numerous multi-scale processes. State-of-the-art solar instrumentation is revealing the dynamics of the Sun with unprecedented temporal and spatial resolutions. Together with advanced numerical simulations these investigations are making new steps in our understanding of the complex dynamical structure of the solar atmosphere.  
13.
 
11th INTEGRAL Conference: gamma-rays and beyond
ID
757641
Date de début
10 oct 2016
Lieu
Amsterdam, Pays-Bas
14.
 
Hot-wiring the Transient Universe V
ID
757600
Date de début
10 oct 2016
Lieu
Villanova University, Pennsylvania, États-Unis
15.
 
Hot-wiring the Transient Universe V
ID
781673
Dates
10 oct 2016 - 14 oct 2016
Lieu
Pennsylvania, États-Unis
Résumé
Hot-wiring the Transient Universe 5 will explore opportunities and challenges of massively parallel time domain surveys coupled with rapid coordinated multi-wavelength follow-up observations. The interdisciplinary agenda includes future and ongoing science investigations, information infrastructure for publishing observations in real time, as well as novel data science to classify events and systems to optimize follow-up campaigns. Time domain astronomy is at the fore of modern astrophysics and crosses fields from solar physics and solar system objects, through stellar variability, to explosive phenomena at galactic and cosmological distances. Recent rapid progress by instruments in space and on the ground has been toward a continuous record of the electromagnetic sky with ever increasing coverage, sensitivity, and temporal resolution. With the advent of gravitational wave and neutrino observatories we are witnessing the birth of multi-messenger astronomy.
16.
 
JINA-CEE/TRIUMF Workshop: Recoil Separators for Nuclear Astrophysicsp
ID
807470
Dates
11 oct 2016 - 12 oct 2016
Lieu
Vancouver, Canada
17.
 
Astronomical Data Analysis Software and Systems (ADASS) XXVI
ID
780797
Date de début
16 oct 2016
Lieu
Trieste, Italie
Sujets apparentés
18.
 
Shining from the heart of darkness: black hole accretion and jets
ID
794133
Date de début
16 oct 2016
Lieu
Kathmandu, Népal
19.
 
The Local Truth: Galactic Star-formation and Feed-back in the SOFIA Era - Celebrating 50 years of airborne astronomy
ID
780826
Date de début
16 oct 2016
Lieu
Asilomar Conference Grounds, Pacific Grove, CA, États-Unis
20.
 
DPS 2016 — 48th Meeting of the American Astronomical Society Division for Planetary Sciences
ID
651491
Dates
16 oct 2016 - 21 oct 2016
Lieu
Pasadena, États-Unis
Résumé
The mission of the American Astronomical Society is to enhance and share humanity’s scientific understanding of the Universe. The Society, through its publications, disseminates and archives the results of astronomical research. The Society also communicates and explains our understanding of the universe to the public., The Society facilitates and strengthens the interactions among members through professional meetings and other means. The Society supports member divisions representing specialized research and astronomical interests., The Society represents the goals of its community of members to the nation and the world. The Society also works with other scientific and educational societies to promote the advancement of science., The Society, through its members, trains, mentors and supports the next generation of astronomers. The Society supports and promotes increased participation of historically underrepresented groups in astronomy., The Society assists its members to develop their skills in the fields of education and public outreach at all levels. The Society promotes broad interest in astronomy, which enhances science literacy and leads many to careers in science and engineering.,
Sujets apparentés
21.
 
IAU Symposium 328: Living Around Active Stars
ID
771986
Date de début
17 oct 2016
Lieu
Maresias, Brésil
22.
 
New York City Gaia Sprint
ID
794251
Date de début
17 oct 2016
Lieu
Simons Center for Computational Astrophysics, NYC, États-Unis
23.
 
IAU Symposia: Living around Active Stars
ID
761968
Dates
17 oct 2016 - 21 oct 2016
Lieu
Maresias, Brésil
Résumé
The activity of stars such as the Sun modulates the environment within their astrospheres. This variable forcing is mediated via stellar magnetic fields, radiative and energetic particulate flux, stellar winds and magnetic storms. In turn this influences planetary atmospheres, climate and habitability. Studies of this intimate relationship between the parent star, its astrophere and the planets that it hosts have reached a certain level of maturity within our own solar system – fueled both by advances in theoretical modelling and a host of satellites that observe the Sun-Earth system. Based on this understanding the first attempts are being made to understand Star-Planet interactions and their coupled evolution, which have relevance for habitability and the search for habitable planets in other stellar environments.
24.
 
SciNeGHE2016 - 11th Workshop on Science with the New Generation of High Energy Gamma-rays Experiments
ID
822066
Date de début
18 oct 2016
Lieu
Pise, Italie
25.
 
SciNeGHE 2016 — 11th Workshop on Science with the New generation of High Energy Gamma-ray Experiments
ID
818021
Dates
18 oct 2016 - 21 oct 2016
Lieu
Pise, Italie
Résumé
The 2016 edition of the SciNeGHE workshops will focus on observations of extreme gamma-ray sources in a multimessenger context, with special attention to connections with gravitational waves observations and theory.
Contact
Email.: scineghe2016@pi.infn.it
26.
 
AGN Reverberation Mapping: the pc Scale Garden of Massive Black Holes
ID
822085
Date de début
24 oct 2016
Lieu
Lijiang, Chine
27.
 
The galaxy life-cycle. From activity to quiescence, and back, across cosmic times
ID
794401
Date de début
24 oct 2016
Lieu
Venise, Italie
28.
 
8th Huntsville Gamma-Ray Burst Symposium
ID
830154
Date de début
24 oct 2016
Lieu
Huntsville, AL, États-Unis
29.
 
Exploring the Universe with JWST - II
ID
799575
Dates
24 oct 2016 - 28 oct 2016
Lieu
Universit de Montral, Montral, Canada
Résumé
This conference is in the same spirit as the one held in the Netherlands at ESTEC (ESA headquarter) in October 2015.
30.
 
The galaxy life-cycle. From activity to quiescence, and back, across cosmic times.
ID
795153
Dates
24 oct 2016 - 28 oct 2016
Lieu
Venise, Italie
31.
 
SMA Science in the Next Decade
ID
811379
Date de début
27 oct 2016
Lieu
Taipei, Taïwan
Résumé
The Submillimeter Array (SMA) has provided forefront capabilities for high spatial and spectral resolution observations at submillimeter wavelengths from its excellent site on Mauna Kea, Hawaii since 2004. SMA observations have resulted in new insights into a wide variety of astrophysical phenomena, from protoplanetary disks to high redshift galaxies. The much larger international Atacama Large Millimeter/submillimeter Array (ALMA) is now in routine operation at millimeter and submillimeter wavelengths. To maintain a leading role in the ALMA era, the SMA project has embarked on an ambitious, staged, strategic upgrade to dramatically improve its sensitivity and observing speed. The new wideband SMA -- the wSMA -- will be ideally suited to spectral line surveys and studies of submillimeter sources in the time domain, as well as a wealth of other applications. This workshop will provide a forum for astronomers from the SMA collaboration and user community to promote, discuss, and elaborate key science cases for wSMA observations in the next decade. The workshop will also facilitate the forging of collaborations to help realize these new science opportunities.
32.
 
7th KIAS workshop on Cosmology and Structure Formation
ID
822103
Date de début
30 oct 2016
Lieu
Korea Insititute for Advanced Study (KIAS), Corée du Sud
33.
 
7th KIAS workshop on Cosmology and Structure Formation
ID
829069
Dates
30 oct 2016 - 04 nov 2016
Lieu
Seoul, Corée du Sud
Résumé
Our understanding of the distribution of matter in the Universe has made rapid progress in recent years. Increasingly sophisticated simulations on both small and large scales, coupled with high quality galaxy data has introduced a new era of precision cosmology. The aim of this workshop is to review the latest theoretical, computational and observational advances in cosmology and large scale structure, and to promote collaboration between specialists in different fields.
Contact
Stephen Appleby;     Email.: stephen@kias.re.kr
Sujets
Large Scale Structure, Cosmic Microwave Background, Formation and Evolution of Galaxies, Reionization of the Universe, Dark Energy, Dark Matter
34.
 
Stardust Final Conference on Asteroids and Space Debris
ID
807332
Date de début
31 oct 2016
Lieu
ESTEC, Pays-Bas
35.
 
Chemical Abundances in Gaseous Nebulae
ID
794507
Date de début
02 nov 2016
Lieu
Campos do Jordo, So Paulo, Brésil
36.
 
Gaia 2016 Data Release #1 Workshop
ID
799460
Dates
02 nov 2016 - 04 nov 2016
Lieu
European Space Astronomy Centre (ESAC), Madrid, Espagne
37.
 
SPARCS 2016: SKA Pathfinders Radio Continuum Surveys 2016
ID
834853
Date de début
03 nov 2016
Lieu
International Centre Goa (ICG), Goa, Inde
38.
 
NuSTAR Science Meeting 2016
ID
834860
Date de début
15 nov 2016
Lieu
Pasadena, CA, États-Unis
39.
 
Preparing for SN science in the LSST era: A kick-off workshop
ID
834947
Date de début
16 nov 2016
Lieu
Pittsburgh, PA, États-Unis
40.
 
Gaia Data Workshop
ID
830207
Date de début
21 nov 2016
Lieu
Heidelberg, Allemagne
41.
 
European Conference on Laboratory Astrophysics ECLA2016 - Gas on the Rocks
ID
822054
Date de début
21 nov 2016
Lieu
Madrid, Espagne
42.
 
Exploring the X-ray Transient and variable Sky
ID
834891
Date de début
21 nov 2016
Lieu
Pavia, Italie
43.
 
NARIT COMAC2016 Workshop "Simulating Galaxies And Beyond"
ID
836250
Date de début
21 nov 2016
Lieu
Chiang Mai, Thaïlande
44.
 
International Symposium on Neutron Star Matter (NSMAT2016)
ID
824769
Dates
21 nov 2016 - 24 nov 2016
Lieu
Sendai, Japon
45.
 
GASP 2016 — 2016 E&F White Research conference on Galactic Archaeology and Stellar Physics
ID
799615
Dates
21 nov 2016 - 25 nov 2016
Lieu
Canberra, Australie
Résumé
Galactic Archaeology aims at unveiling the Milky Way’s history by studying the fossil record preserved in stellar light. Large surveys are targeting samples of 105 to 106 stars to measure their chemical compositions. Together with distances, ages and 3D velocities, the chemical information will have a revolutionary impact on understanding galaxy formation. Stellar physics combines the observations with theoretical interpretations of the structure of stars. This knowledge is essential to decipher the observed chemical patterns within the Galaxy’s stellar populations. Major new developments in stellar physics have a direct impact on understanding the observational data. This conference will bring together world-leading experts on Galactic Archaeology and Stellar physics in order to exploit the wealth of information provided by new and on-going surveys of the Galaxy.
46.
 
ECLA 2016 — European Conference on Laboratory Astrophysics - Gas on the Rocks
ID
797181
Dates
21 nov 2016 - 25 nov 2016
Lieu
Madrid, Espagne
Résumé
Over the last decade European research activities in the field of laboratory astrophysics have experienced an impressive increase in their potential to address astrophysical problems, in particular by providing essential information on the physical and chemical processes leading to chemical complexity in space resulting in star and planet formation. These activities have been motivated by the interpretation of astronomical observations obtained with single dish telescopes and short baseline interferometers. The wealth of data obtained with ALMA, space facilities (Herschel, Spitzer, Rosetta, the coming JWST, E-ELT), and other ground based observatories (VLTI, NOEMA, ...), require new methodologies for the astrophysical modeling that will lead to new challenges for laboratory astrophysics. This conference aims to address the state of the art in laboratory astrophysics within the context of these new astrophysical data and to improve communication and collaboration between astrophysicists, physicists and (geo) chemists. Hence, the conference structure will consist of invited talks presenting topics in astrophysics and planetary science and related laboratory astrophysics activities. Contributing talks will be selected to complement the topics from the astrophysical, laboratory, and theoretical/modeling points of view. The conference will cover studies in many fields such as spectroscopy, analytical (geo) chemistry, reactivity, nanoscience, and quantum chemistry, pertaining to different matter components (gas, plasma, PAHs, ices, dust, solid surfaces, ...).
Sujets
1. Comets, asteroids, meteorites and the primitive Solar System nebula: formation and evolution 2. Protoplanetary disks and planet formation 3. Planet, Moon, and exoplanet surfaces and atmospheres 4. The signatures of the evolving interstellar medium 5. Dense Clouds: the gas-ice interface and molecular complexity 6. Chemical fingerprints of star formation 7. The late stages of star evolution: dust formation 8. Supernovae and shocks: high-energy processing of matter
47.
 
Summer school Antennas for Radio Telescopes
ID
839827
Dates
21 nov 2016 - 25 nov 2016
Lieu
Stellenbosch, Afrique du Sud
Résumé
The School will address the specific challenges facing antenna designers and others working in radio astronomy applications. In addition to topics covering specific antenna technologies used in the state of the art instruments, background on basic radio astronomical methods and performance metrics will be provided, as well as an introduction to some basic calibration and imaging techniques. The School will provide participants with a solid understanding of what is required from the antenna systems to yield the best possible instruments for different applications.
Contact
Prof. Dirk de Villiers (ddv@sun.ac.za) and Dr. Albert Lysko (alysko@csir.co.za).;     Tél.: [+27 12 841 4609];     Email.: alysko@csir.co.za
Sujets
antenna, radiotelescope, radio telescope, radio astronomy, reflector antennas, dense aperture arrays, sparse array antennas, calibration
48.
 
CosPA 2016
ID
834934
Date de début
28 nov 2016
Lieu
The University of Sydney, Sydney, Australie
49.
 
629. WE-Heraeus-Seminar "Exoplanets: Bridging the Gap between Theory and Observations"
ID
822078
Date de début
28 nov 2016
Lieu
Bad Honnef, Allemagne
Sujets apparentés
50.
 
The 6th Subaru International Conference — Panoramas of the Evolving Cosmos
ID
794302
Date de début
28 nov 2016
Lieu
Hiroshima, Japon
51.
 
CosPA 2016 — 13th International Symposium on Cosmology and Particle Astrophysics
ID
811245
Dates
28 nov 2016 - 02 dec 2016
Lieu
Sydney, Australie
Résumé
The 13th International Symposium on Cosmology and Particle Astrophysics (CosPA 2016) will be hosted by the University of Sydney from November 28 to December 2, 2016 at the Sydney Nanoscience Hub, located on the University's Camperdown Campus. CosPA 2016 will bring together theorists, experimentalists, and observers working in the fields of particle physics, cosmology, and astrophysics to discuss the latest results and ideas, and prospects for progress.
Sujets
Particle astrophysics, dark matter and dark energy, cosmic microwave background and large-scale structure, inflation and early universe cosmology, gravity and gravitational waves
52.
 
IAU Symposia: The lives and death-throes of massive stars
ID
761890
Dates
28 nov 2016 - 02 dec 2016
Lieu
Auckland, Nouvelle-Zélande
Résumé
Research on Massive Stars is undergoing a period of rapid progress. While these stars are relatively few in number they are the main driver of chemical and dynamical evolution in galaxies via their stellar winds and explosive deaths in core-collapse supernovae. Our understanding of massive stars is going through a remarkable time of change with long held convictions being shown to be incomplete. This evidence arises from new research concerning the formation and evolution of massive stars and linking this to their deaths in core-collapse supernovae. Now is a fortuitous time to make significant advances in massive star research. We propose a meeting with the central rationale to bring together the two communities that study massive stars and their supernovae.
53.
 
ACCRETION PROCESSES IN SYMBIOTIC STARS AND RELATED OBJECTS. First Chile-Korea-Gemini Workshop on Stellar Astrophysics.
ID
822126
Date de début
04 dec 2016
Lieu
La Serena, Chili
54.
 
631. WE-Heraeus-Seminar: Stellar aggregates over mass and spatial scales
ID
811351
Date de début
05 dec 2016
Lieu
Physikzentrum Bad Honnef, Allemagne
55.
 
Stellar aggregates over mass and spatial scales
ID
822117
Date de début
05 dec 2016
Lieu
Physikzentrum Bad Honnef, Allemagne
56.
 
7 years of MAXI : monitoring X-ray transients
ID
836356
Date de début
05 dec 2016
Lieu
Wako, Saitama, Japon
57.
 
Workshop on Solar & Stellar Astronomy Big Data
ID
830177
Date de début
05 dec 2016
Lieu
Washington, DC, États-Unis
58.
 
Monitoring the Non-thermal Universe
ID
839236
Dates
07 dec 2016 - 09 dec 2016
Lieu
Cochem, Allemagne
Résumé
The goal of this workshop is to bring people together who are either working on monitoring or are involved in monitoring at different wavelengths. The far goal is to setup a global monitoring network at all wavelengths.
Contact
Daniela Dorner;     Email.: hap-mon@lists.rwth-aachen.de
59.
 
SEARCH FOR LIFE: FROM EARLY EARTH TO EXOPLANETS
ID
799599
Dates
11 dec 2016 - 16 dec 2016
Lieu
Quy Nhon, Viêt Nam
Résumé
This international conference, endorsed by IAU and Division of Planetary Sciences and Astrobiology, is the third of a series of conferences on « Planets, Exoplanets and Astrobiology ». It will be preceeded by a 2 day Training School on « Basics of Astrobiology » for students and young researchers (December 9th-11th – see “Program“). Both the Training School and Conference will be held at ICISE* and hosted by the Rencontres du Vietnam
60.
 
The physics of groups and galaxy properties therein
ID
811398
Date de début
12 dec 2016
Lieu
Institut d'Astrophysique de Paris, France
61.
 
The hydride toolbox
ID
830217
Date de début
12 dec 2016
Lieu
Paris, France
62.
 
229th American Astronomical Society
ID
803772
Date de début
03 jan 2017
Lieu
Grapevine, TX, États-Unis
63.
 
ZTF Community Workshop at AAS 229
ID
836243
Date de début
03 jan 2017
Lieu
Grapevine, TX, États-Unis
64.
 
10 Escuela de Astronoma Observacional para Estudiantes Latinoamericanos "ESAOBELA"
ID
834961
Date de début
08 jan 2017
Lieu
Observatorio Astronmico Nacional de Tonantzintla, , Mexique
65.
 
2nd Fudan Winter School on Astrophysical Black Holes
ID
836342
Date de début
09 jan 2017
Lieu
Shanghai, Chine
66.
 
Confronting MHD Theories of Accretion Disks with Observations
ID
757540
Date de début
09 jan 2017
Lieu
Kavli Institute for Theoretical Physics, Santa Bar, États-Unis
Sujets apparentés
67.
 
Wide Band Spectral and Timing Studies of Cosmic X-ray Sources
ID
835067
Date de début
10 jan 2017
Lieu
Tata Institute of Fundamental Research, Mumbai, Inde
68.
 
New Directions in Theoretical Physics 2
ID
836297
Date de début
11 jan 2017
Lieu
Edinburgh, Royaume-Uni
69.
 
The Dawn of Galaxies
ID
794293
Date de début
14 jan 2017
Lieu
Obergurgl, Autriche
70.
 
2017 ESO Calibration Workshop: the second generation VLT instruments and friends
ID
830080
Date de début
16 jan 2017
Lieu
Santiago (ESO Office), Chili
71.
 
Star Formation and mass assembly in high redshift galaxies
ID
813360
Dates
16 jan 2017 - 20 jan 2017
Lieu
Bad Moos , Italie
Résumé
This workshop is organized as the ending event of the ASTRODEEP project.

Building on the latest results from Great Observatories (in orbit and on the ground), we will discuss the nature and evolution of high redshift galaxies, with a particular emphasis on the consistency between the star-formation and the mass assembly processes. We aim at bringing together members of the CANDELS and the GOODS-Herschel collaborations, as well as external scientists interested in the topics, to present their latest results and the perspectives for the next future.

72.
 
Beyond the Solar Neighborhood: Entering into the GAIA Era
ID
813425
Dates
23 jan 2017 - 27 jan 2017
Lieu
Bad Moos , Italie
73.
 
Ushering in the New Age of Microlensing from Space: 21st International Microlensing Conference
ID
803859
Date de début
01 fév 2017
Lieu
Pasadena, California, États-Unis
Résumé
We happily invite the exoplanet community to the 21st International Microlensing Conference entitled "Ushering in the New Age of Microlensing from Space". The field of gravitational microlensing is burgeoning, in particular due to the success of several space-spaced missions. We will highlight breaking results from K2's Campaign 9 ( K2C9 ), which constitutes the first combined ground- and space-based microlensing survey, as well as progress in Spitzer's program of obtaining "satellite parallaxes." Talks on ground-based surveys and advances in theory will also be featured prominently. Finally, we will have a number of talks on the revolutionary promise of the WFIRST mission for exoplanet science, which was recently approved to enter Phase A. Together these endeavors provide invaluable insight into topics such as the Galactic distribution of exoplanets, the abundance of free-floating planets, and the demographics of cold exoplanets.
Sujets apparentés
74.
 
International Workshop on Spectral Stellar Libraries
ID
835086
Date de début
06 fév 2017
Lieu
Campos de Jordo, So Paulo, Brésil
75.
 
Disks, Dynamos, and Data: Confronting MHD Accretion Theory with Observations
ID
836235
Date de début
06 fév 2017
Lieu
Kavli Institute for Theoretical Physics, Santa Bar, États-Unis
76.
 
The Physics of the ISM 6 years of ISM-SPP 1573: what have we learned?
ID
835138
Date de début
13 fév 2017
Lieu
Cologne, Allemagne
77.
 
COSPAR Capacity Building Workshop in High Energy Astrophysics
ID
821980
Date de début
20 fév 2017
Lieu
Viedma, Argentine
78.
 
IAU Symposium 331 - SN 1987A 30 years later: Cosmic Rays and Nuclei from Supernovae and their aftermaths
ID
824647
Date de début
20 fév 2017
Lieu
Saint Gilles Les Bains, La Runion Island, France
79.
 
IAU Symposium 331 — SN 1987A, 30 years later – Cosmic Rays and Nuclei from Supernovae and their aftermaths
ID
821929
Dates
20 fév 2017 - 24 fév 2017
Lieu
Saint Gilles - Réunion Island, France
Résumé
Supernovae (SNe), along with their remnants, are central in many active fields of research as the key sources of cosmic high-energy particles and heavy elements, the privileged sites of cosmic dust formation, and the primary agents of chemical and dynamical evolution of galaxies. Moreover, they are among the rare celestial events visible with the naked eye. Yet, many open issues still need to be deeply explored such as the nature of the SN progenitors and the final stages of stellar evolution, explosion mechanisms and nucleosynthesis, shock acceleration processes and the question of the origin of cosmic rays.
Sujets
Massive Stars as SN progenitors, Supernovae as stellar explosive outcomes, Supernova explosion mechanisms, Supernova outcomes and impacts, Particle acceleration and Origin of Cosmic Rays, SN 1987A, thirty years later, Non-thermal multi-wavelength/multi-messenger data on Supernovae and their remnants.
80.
 
The remarkable life of a BCG
ID
813424
Dates
20 fév 2017 - 24 fév 2017
Lieu
Bad Moos , Italie
Résumé
In the last years a strong effort has been devoted to the study of the brightest cluster galaxies (BCG). Several studies are focusing on BCG properties adopting a multi-wavelength approach, other are using numerical and semi-analitical models to describe BCG formation and evolution. These works have been fostered by extensive follow-up of newly discovered SZ clusters at high-redshift, by in-depth studies with Hubble such as CLASH, and a rapidly increasing amount of data in the radio and submm bands thanks to ALMA and the upgraded JVLA. This strong interest in the origin and evolution of BCG is mainly due to their unique role in the context of galaxy formation, evolution of galaxy clusters, and interactions between nuclear activity and surrounding diffuse baryons. With this workshop we intend to bring together the most active researchers in this field to discuss the latest results, and compare the outcomes of new observational campaigns with numerical simulations and semi-analitical models.
81.
 
Frontiers in Theoretical and Applied Physics (astrophysics is one of the main conference themes)
ID
807360
Date de début
22 fév 2017
Lieu
American University of Sharjah (AUS), Dubai, Émirats arabes unis
Résumé
In partnership with the Emirates Mars Mission and Mohammed Bin Rashid Space Center (MBRSC), the Department of Physics at American University of Sharjah (AUS) is proud to host the international conference Frontiers in Theoretical and Applied Physics |UAE 2017 (FTAPS 2017). The aim of the conference is to provide a forum for physicists, astronomers, and space and material scientists from around the world to present the latest developments in the various dynamic fields of physics. The conference will provide ample opportunity to exchange ideas on rising research issues in physics, astrophysics, and space and material science, and to promote regional and international collaborations.
82.
 
The Mysteries and Inner Workings of Massive Stars
ID
734532
Date de début
27 fév 2017
Lieu
KITP, Santa Barbara, États-Unis
83.
 
Star Formation from Cores to Clusters
ID
836292
Date de début
06 mar 2017
Lieu
Santiago, Chili
84.
 
47th Saas-Fee Advanced Course: Supernovae, cosmic explosions
ID
811377
Date de début
12 mar 2017
Lieu
Villars-sur-Ollon, Suisse
85.
 
On the Origin (and Evolution) of Baryonic Galaxy Halos
ID
807385
Date de début
13 mar 2017
Lieu
Galapagos Islands, Équateur
86.
 
IAUS332 Astrochemistry VII - Through the Cosmos from Galaxies to Planets
ID
835071
Date de début
20 mar 2017
Lieu
Puerto Varas, Chili
87.
 
Science with the Hubble and James Webb Space Telescopes. V
ID
835092
Date de début
20 mar 2017
Lieu
Venise, Italie
88.
 
Phenomena, Physics, and Puzzles Of Massive Stars and their Explosive Outcomes
ID
836245
Date de début
20 mar 2017
Lieu
Kavli Institute for Theoretical Physics, Santa Bar, États-Unis
89.
 
FORMATION AND DYNAMICAL EVOLUTION OF EXOPLANETS
ID
807345
Date de début
26 mar 2017
Lieu
Aspen, Colorado, États-Unis
Sujets apparentés
90.
 
QUASARS AT ALL COSMIC EPOCHS
ID
836300
Date de début
02 avr 2017
Lieu
PADOVA, Italie
91.
 
QUASARS AT ALL COSMIC EPOCHS
ID
835639
Dates
02 avr 2017 - 07 avr 2017
Lieu
PADOVA, Italie
Résumé
Quasars have been discovered slightly more than 50 years ago. All the improvement in telescope light gathering and in computing power notwithstanding, we still miss a clear connection between observational properties and theory for quasars, as provided, for example, by the H-R diagram for stars. We do not yet have a complete self-consistent view of nuclear activity with predictive power, as we do for main-sequence stellar sources. At the same time quasars offer many “windows open onto the unknown.” On small scales, quasar properties depend on phenomena very close to the black hole event horizon. On large scales, quasars may effect evolution of host galaxies and their circum-galactic environments. Quasars’ potential to map the matter density of the Universe and help reconstruct the Universe’s spacetime geometry is still largely unexploited.

The time is ripe for a critical assessment of our present knowledge of quasars as accreting black holes and of their evolution across the cosmic time. The aim of this meeting is to review and contextualize the main observational scenarios following an empirical approach, to present and discuss the accretion scenario, and then to analyze how a closer connection between theory and observation can be achieved, identifying those aspects of our understanding that are still on a shaky terrain and are therefore uncertain knowledge.

Contact
MAURO D'ONOFRIO;     Tél.: [+39-049-8278233];     Email.: mauro.donofrio@unipd.it
Sujets
1. observational properties of quasars as luminous active galactic nuclei 2. accretion processes on supermassive black holes 3. contextualization and connection between theory and observation for the emitting region of quasars 4. quasar evolution over cosmic time and quasars as cosmological tools 5. feedback and environment of active galaxies and quasars
92.
 
Physics of the Intra-Cluster Medium
ID
835189
Date de début
03 avr 2017
Lieu
Pékin, Chine
93.
 
Big Questions in Astrophysics - the next decades
ID
836313
Date de début
03 avr 2017
Lieu
Lund, Suède
94.
 
44th IOP Plasma Physics Conference
ID
836422
Dates
03 avr 2017 - 06 avr 2017
Lieu
Worcester College, Oxford, Royaume-Uni
Résumé
This conference covers all aspects of plasma physics, including Magnetic and Inertial confinement fusion, Astrophysical and Space Plasmas, Low Density and Technological/Industrial Plasmas, High Energy Density and Laser Plasmas, Dusty and Complex plasmas, Plasma Surface interactions, Plasma Applications including Medical applications and Plasma Diagnostics
95.
 
PICM — Physics of the Intra-Cluster Medium
ID
833537
Dates
03 avr 2017 - 07 avr 2017
Lieu
Pékin, Chine
Résumé
The Intra Cluster Medium (ICM) constitutes the largest baryonic component of galaxy clusters. It is affected by gravitational and non-gravitational processes due to the interaction with the cluster galaxy population. It is now widely recognized that the cluster environment plays a fundamental role in determining the evolution of its galaxy population. In turn, feedback in cluster cores offer the unique opportunity to understand the interactions between star formation events and nuclear activity within the surrounding medium.

Theoretical models and numerical simulations have been developed in order to capture the complexity of this interaction and to understand when, where, and how feedback takes place. At the same time the ICM is an important diagnostic of the dynamics of the cluster itself, and an exhaustive understanding of its properties is crucial for a full understanding of the growth of cosmic structures at large, and the measurement of cosmological parameters. This workshop will focus on the physics of the ICM and its relation with the different mass components of galaxy clusters. The aim is to provide an overview of the many exciting recent results at vastly different wavelengths (Radio, SZ, sub-mm, IR, optical, X-ray, gamma-ray) and use them to challenge theoretical models and advanced numerical simulations.

Contact
Heng Yu;     Email.: picm@bnu.edu.cn
Sujets
galaxy cluster, AGN, intra-cluster medium, bulk motion, hydrodynamical simulation, high-z protocluster, cosmology
96.
 
Asteroids, Comets, Meteors 2017
ID
822133
Date de début
10 avr 2017
Lieu
Edificio Polifuncional Jos Luis Massera, Montevide, Uruguay
97.
 
The Galaxy-Halo Connection Across Cosmic Time
ID
771974
Date de début
24 avr 2017
Lieu
Kavli Institute for Theoretical Physics, Santa Bar, États-Unis
98.
 
Fundamental Physics with the Square Kilometre Array
ID
812675
Dates
01 mai 2017 - 05 mai 2017
Lieu
Flic-en-Flac, Maurice
Résumé
The Square Kilometre Array (SKA) will be the world’s largest and most powerful radio telescope. When the SKA begins operations early in the next decade, it will deliver spectacular new data sets that are expected to transform our understanding of physics, astronomy and cosmology.

To fully realise the potential of the SKA as a machine for fundamental physics, the SKA organisation seeks to engage the theoretical physics community in the science case and design considerations for the full array. To initiate this discussion, we will be holding a focused workshop in May 2017, in which we aim to bring together radio astronomers and theorists to jointly consider ways in which the SKA can test and explore fundamental physics.

99.
 
Impacts in planetary systems
ID
835208
Date de début
15 mai 2017
Lieu
Lund Observatory, Suède
Sujets apparentés
100.
 
Quantifying and Understanding the Galaxy-Halo Connection
ID
836244
Date de début
15 mai 2017
Lieu
Kavli Institute for Theoretical Physics, Santa Bar, États-Unis
101.
 
2nd Advanced School on Exoplanetary Science: Astrophysics of Exoplanetary Atmospheres
ID
824717
Date de début
22 mai 2017
Lieu
Vietri sul Mare (Salerno), Italie
Sujets apparentés
102.
 
ASES2 — 2nd Advanced School on Exoplanetary Science: ASTROPHYSICS OF EXOPLANETARY ATMOSPHERES
ID
824474
Dates
22 mai 2017 - 26 mai 2017
Lieu
Vietri sul Mare (Salerno), Italie
Résumé
The 2nd Advanced School on Exoplanetary Science will be held at the International Institute for Advanced Scientific Studies (IIASS) in Vietri sul Mare (Salerno), Italy from 22 to 26 May, 2017. The School - taking place in the enchanting Amalfi Coast - is aimed to provide a comprehensive, state-of-the-art picture of a variety of relevant aspects of the fast-developing, highly interdisciplinary field of exoplanets research. The Lecture topics of the 2nd year of School will be focused on the Atmospheres of Exoplanets. The Lectures will be delivered by four senior researchers to an audience of graduate students, Ph.D. students and young post-docs.
Contact
Luigi Mancini;     Tél.: [+49 (0) 6221 528 454];     Email.: mancini@mpia.de
Sujets
exoplanets, exoplanet atmospheric models, exoplanet-atmosphere observational techniques, molecular spectroscopy, solar-system atmospheres
103.
 
PROTOPLANETARY DISKS AND PLANET FORMATION AND EVOLUTION
ID
811383
Date de début
29 mai 2017
Lieu
Garching by Munich, Allemagne
Sujets apparentés
104.
 
FOE2017: Fifty One Erg
ID
830197
Date de début
05 jui 2017
Lieu
Corvallis, OR, États-Unis
105.
 
Globular cluster systems and their host galaxies
ID
813434
Dates
05 jui 2017 - 09 jui 2017
Lieu
Bad Moos , Italie
Résumé
The formation and evolution of globular cluster (GC) systems is still an unsolved problem of modern astrophysics despite years of study. New observations have revealed that the distribution of sizes, masses and mass-to-light ratios of small stellar systems is largely continuous thanks to the discovery of a growing number of ultracompact dwarf galaxies and related objects, all of which have properties remarkably similar to GCs. At the same time, steady progress is being made in characterising the properties of GC systems, not only in our own Milky Way, but also in a growing number of local Universe galaxies. All these new observations add new pieces to the puzzle of how and where GCs form, starting as early as the epoch of reionization within the first billion years after the Big Bang, and then continuing through the hierarchical assembly of their host galaxies. GC systems are also providing new insight on the properties of galaxy halos at large radii. Simulations have now reached the size and mass scales relevant for direct modelling of GC system formation in a cosmological context. This meeting will bring together the leading observers and theorists from diverse backgrounds to review the current state of the field, discuss existing scenarios, and stimulate the exploration of new collaborative proposals for future modeling and for observations with next-generation telescopes.

The meeting will place GC systems in the context of their host galaxy and the interplay between them.

106.
 
Gordon Research Seminar Origins of Solar Systems
ID
835194
Date de début
17 jui 2017
Lieu
Mount Holyoke College, South Hadley, MA, États-Unis
107.
 
Nuclear Physics in Astrophysics
ID
822178
Date de début
18 jui 2017
Lieu
Catania, Italie
108.
 
Gordon Research Conference Origins of Solar Systems: Making a Habitable Planet
ID
822108
Date de début
18 jui 2017
Lieu
Mount Holyoke College, South Hadley, MA, États-Unis
109.
 
NPA8 — 8th Nuclear Physics in Astrophysics International Conference
ID
811413
Dates
18 jui 2017 - 23 jui 2017
Lieu
Catania, Italie
110.
 
EWASS 2017 (European Week of Astronomy and Space Science)
ID
824729
Date de début
26 jui 2017
Lieu
Prague, République tchèque
111.
 
Wide Field Infrared Survey Telescope: Science with WFIRST
ID
824582
Date de début
26 jui 2017
Lieu
Baltimore, MD, États-Unis
112.
 
Forging Connections: From Nuclei to the Cosmic Web
ID
836271
Date de début
26 jui 2017
Lieu
Michigan State University, East Lansing, MI, États-Unis
113.
 
Advances in Theoretical Cosmology in Light of Data
ID
824622
Date de début
04 jul 2017
Lieu
Nordita, Stockholm, Suède
114.
 
IAUS 334: Rediscovering our Galaxy
ID
824612
Date de début
10 jul 2017
Lieu
Potsdam, Allemagne
115.
 
Eighth Meeting on Hot Subdwarfs and Related Objects
ID
822165
Date de début
10 jul 2017
Lieu
Cracovie, Pologne
116.
 
Early stages of Galaxy Cluster Formation: Mergers, High-z Clusters, and Protoclusters
ID
836203
Date de début
17 jul 2017
Lieu
Garching, Allemagne
117.
 
Transiting Exoplanets
ID
807391
Date de début
17 jul 2017
Lieu
Keele University, Royaume-Uni
118.
 
IAU Symposium 335: Space Weather of the Heliosphere: Processes and Forecasts
ID
824676
Date de début
17 jul 2017
Lieu
University of Exeter, Devon, Royaume-Uni
119.
 
CHEOPS Science Workshop V
ID
794275
Date de début
24 jul 2017
Lieu
Schloss Seggau, Autriche
120.
 
TAUP 2017 — XV International Conference on Topics in Astroparticle and Underground Physics
ID
823252
Dates
24 jul 2017 - 28 jul 2017
Lieu
Sudbury, ON, Canada
Résumé
The biennial TAUP series covers recent experimental and theoretical developments in astroparticle physics by invited plenary review talks and parallel workshop sessions of invited and contributed presentations. Topics covered by the conference are; Cosmology and particle physics; Dark matter and its detection; Neutrino physics and astrophysics; Gravitational waves; High-energy astrophysics and cosmic rays
Sujets
Astroparticle Physics, Dark Matter, Cosmology, Neutrino Physics, Gravitational Waves, Cosmic Rays, High-energy Astrophysics
121.
 
TAUP 2017 — XV International Conference on Topics in Astroparticle and Underground Physics
ID
835200
Dates
25 jul 2017 - 29 jul 2017
Lieu
Sudbury, Ontario, Canada
122.
 
Understanding cosmological observations
ID
794065
Date de début
30 jul 2017
Lieu
Benasque, Espagne
123.
 
SMG20 - Twenty years of submillimetre galaxies; star-forming galaxies at high redshifts
ID
836398
Date de début
31 jul 2017
Lieu
Durham, Japon
124.
 
2017 NATIONAL ASTRONOMY TEACHING SUMMIT
ID
835242
Date de début
07 aou 2017
Lieu
Florida Gulf Coast University in Ft. Myers, Florid, États-Unis
125.
 
EPRV III — The Third Workshop on Extremely Precise Radial Velocities
ID
831739
Dates
07 aou 2017 - 13 aou 2017
Lieu
University Park, États-Unis
Résumé
This workshop is for teams around the world to share techniques for advancing precise radial velocity work towards 10 cm/s precision in coming years. Building on the success of the first two workshops at Penn State in 2010 and Yale in 2015, the focus on this workshop will be on the performance of the next generation of precise Doppler instruments, including hardware, statistical techniques for signal extraction and interpretation, and stellar jitter modeling and mitigation.
Contact
Jason Wright;     Email.: jtw13@psu.edu
126.
 
16th Divisional Meeting of the High Energy Astrophysics Division (HEAD) of the AAS
ID
632072
Date de début
16 aou 2017
Lieu
Jackson Hole, Wyoming, États-Unis
127.
 
The PLATO Mission Conference 2017: Exoplanetary systems in the PLATO era
ID
836339
Date de début
05 sep 2017
Lieu
University of Warwick, Royaume-Uni
128.
 
MODEST 17 - Modelling and observing dense stellar systems
ID
835252
Date de début
18 sep 2017
Lieu
Prague, République tchèque
129.
 
The many Scales of the Universe: Galaxies, their Suns, and their Planets
ID
794167
Date de début
18 sep 2017
Lieu
Gttingen, Allemagne
130.
 
MODEST 17 — Modelling and observing dense stellar systems
ID
831514
Dates
18 sep 2017 - 22 sep 2017
Lieu
Prague, République tchèque
Contact
Jaroslav Haas;     Email.: haas@sirrah.troja.mff.cuni.cz
Sujets
Galactic centre / nuclear star clusters, Young star clusters and star forming regions, Stellar dynamics and numerical methods, Stellar populations in star clusters, Blue stragglers / stellar collisions and their products, Compact objects in star clusters, Astrophysical sources of gravitational waves, Dynamics of (exo)planetary systems in star clusters, New observational frontiers (LIGO, GAIA, JWST, FAST...)
131.
 
Planet Formation and Evolution 2017
ID
835295
Date de début
25 sep 2017
Lieu
Jena, Allemagne
Sujets apparentés
132.
 
Astrobiology 2017, Research meeting by IAU's Commission F3.
ID
836252
Date de début
26 nov 2017
Lieu
Coyhaique, Chili
133.
 
231st American Astronomical Society Meeting
ID
651267
Dates
07 jan 2018 - 11 jan 2018
Lieu
National Harbor, États-Unis
Résumé
American Astronomical Society 231st Meeting
134.
 
The Small-Scale Structure of Cold(?) Dark Matter
ID
836215
Date de début
09 avr 2018
Lieu
KITP, Santa Barbara, California, États-Unis
135.
 
42nd COSPAR Scientific Assembly and Associated Events
ID
835333
Date de début
14 jul 2018
Lieu
Pasadena, CA, États-Unis
136.
 
COOL STARS 20: Cambridge Workshop on Cool Stars, Stellar Systems and the Sun
ID
836352
Date de début
29 jul 2018
Lieu
Cambriege/Boston MA, États-Unis
AIP Conference Proceedings
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Dernière mise à jour: 22 Septembre 2016