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|
EXOPLANETS Detection, Formation & Dynamics IAU Symposium 249 Oct. 22-26, 2007 Suzhou, China |
| Announcements and FAQs |  |
| Announcements | |
| Submission to Proceedings | |
| More details about the proceedings can be found at
webpage Proceedings. Please submit your manuscript for refereeing by email to iaus249@nju.edu.cn. At this moment, we need only ONE read-able file (pdf or ps) containing both the text and all figures. Make sure your file is smaller than 5MB. If you need to contain large files (e.g. large pictures of very-high-resolution) in your paper, please find an accessible place by yourself and cite the URL in your manuscript. | |
| Final Announcement | |
|
The program of the conference has come out, please go to the Program page to see it. Due to the limited conference time, it is impossible to give every contributor an oral talk. We have to discard some interesting topics proposed by our participants. Those participants with names listed on the program please prepare your oral talks. The time for a talk is 20 minutes (invited talk 30 minutes). Other contributors are invited to present your works as posters. Any speaker who wants to
use the computer supplied by the conference please bring your
presentation in a flash disk, portable hard disk or CD/DVD. We
do NOT use floppy disk, and please make sure your portable
device is able to be connected to the USB port. Please copy your
stuff to the conference computer during the Coffee Breaks on the
day before your talk.
For poster contribution, the poster should be the A0 size (841 x 1189 mm) and in a portrait orientation. We will print a booklet including the abstracts of all contributions, so we need your abstract before Oct. 11. Please submit your abstracts on line immediately. You need to input your (first and last) name, the title of your contribution and the abstract (prepared in LaTeX format) on the webpage. Have a look at the Participants page. If you can see your own name on it but can not see the contribution title of yours, that means, we did not receive your abstract on-line, please submit immediately. We have left some printable notes in Chinese and English on the Travel & Visa page. If you think they are helpful, print them out and bring them with you. Every participant is asked to bring the receipt of your bank transferring for the registration fee, in case the treasurer needs it to check the account. And as you may know from this page, we still have some unrecognized remitters. If possible, please send an email to iaus249@nju.edu.cn to tell your flight number, arrival time and arrival airport. Thank you for your cooperation! Wish you a pleasant trip and see you in Suzhou! | |
| Conference Site | |
A sketch-map showing the Hotels and the Conference Center looks like: | |
| About the Poster Session | |
| A list of all Posters is below. They will be posted in two sessions.
The first poster session is from the beginning of conference to 10:00am of Oct. 24; and the second one from then on to the end of the conference.
Those posters numbered with odd numbers (P01, P03,...) are in the first session and those with odd numbers in the second session. Poster Contributions to IAU Symposium No.249 Exoplanets: Detection, Formation & Dynamics Oct.22-26, 2007, Suzhou, China Miss Alapini, Aude P01: Precise relative temperature calibration of solar-type stars using equivalent width ratios of spectral lines Miss Alves De Oliveira, Catarina P02: Disk signatures in a new population of low mass YSOs in Rho Ophiuchus Dr. Andrei, Alexandre Humberto P03: Long Term Variation Trend of the Pluto-Charon System Mr. Baluev, Roman Vladimirovich P04: Effect of unknown inclination in the mass distribution of exoplanets Mr. Baruteau, Clement P05: On the corotation torque in radiatively inefficient disks Miss Batista, Virginie P06: HOLMES: real time analysis of photometric data to hunt for extra solar planets via microlensing Dr. Carmona Gonzalez, Andres P07: Studies of gas in protoplanetary disks using high-resolution IR spectroscopy Miss Chavero, Carolina Andrea P08: A Global Evolution of Resolved Debris Disks Prof. Cuntz, Manfred
P09: Orbital
Stability Criteria for Planets in Stellar Binary Systems Miss Davis, Erica P11: Formation and Detectability of Earth-Size Planets Around Alpha Centauri B Dr. Psychoyos, Dionyssia P12: Planetary dynamics in the 1/1 resonance: The symmetric periodic orbits and their families Mr. Fleming, Scott William P13: Results From Testing of a Monolithic Interferometer with Keck ET at APO and Plans for the Future: Towards ET DFDI Long-Term Stability and High Precision Miss Gayon, Julie and Prof. Bois, Eric J. P14: Retrograde resonances in compact multi-planetary systems : a feasible stabilizing mechanism Mr. Geisler, Ronny P15: Target Selection for the Astrometric Planet Search ESPRI with PRIMA at VLTI Dr. Genda, Hidenori P16: Formation of Heavy Element Rich Giant Planets by Giant Impacts Dr. Gu, Pin-Gao P17: Internal Waves Driven by Stellar Irradiation in a Non-synchronized Hot Jupiter Dr. Gu, Sheng-hong P18: Photometric follow-up observations of the SuperWASP transiting planet candidates Dr. Hara, Tetsuya
P19: On the
Transfer of Meteorites (and Life?) from Earth to the GI 581
System Dr. Hebb, Leslie P21: Search for Planets Transiting the M-dwarf Debris Disk Host, AU Mic Dr. Helling, Christiane P22: Comparison of cloud models for brown dwarfs Mr. Hori, Yasunori P23: Observational effects on the core mass and the total mass of heavier elements of gas giants and implication for J6 Mr. Janson, Markus P24: Differential imaging search for the giant planet Epsilon Eri b with ESO-VLT Dr. Ji, Jianghui
P25:
Baroclinic Generation of Vortensity and Rossby-Wave-Instability
in an Embedded Planet-Disk System Dr. Kane, Stephen P27: Cadence Optimisation and Exoplanetary Parameter Sensivitity Miss Kato, Mariko P28: Modification of angular velocity distribution and concentration of the dust particles by inhomogeneous growth of MRI in proto-planetary disks Dr. Kitiashvili, Irina P29: Modeling of the Axis Rotational Evolution of “Hot Jupiter” Planets Miss Kretke, Katherine Anne P30: Planet Formation around Intermediate Mass Stars Prof. Krot, Alexander Mikhailovich P31: The main planetary dynamics problem solving based on spheroidal bodies theory Mr. Laibe, Guillaume P32: 3D SPH Simulations of grain growth in protoplanetary disks Mr. Li, Jian P33: The origin of the Neptune Trojan 2005 TN53 Miss Liu, Yujuan P34: A substellar Companion to the Intermediate-Mass Giant 11 Com Mr. Lyra, Wladimir P35: Turbulence-assisted planetary growth Mr. Ma, Da-Zhu
P36: An
Extension of Nacozy’s Approach to Correcting All Orbital
Elements of Each Body in Planetary Dynamics Dr. Marchi, Simone P38: The World Space Observatory for UV (WSO-UV): implications for exoplanets studies P39: First light of AquEye, the fast multichannel photometer for the 1.82m telescope at Asiago Cima Ekar P40: Search for massive Earth around SARG astereosismic targets Mr. Muto, Takayuki P41: The Effect of Poloidal Magnetic Field on Type I Planetary Migration Dr. Niedzielski, Andrzej P42: The Penn State/Torun Centre for Astronomy Search for Planets Around Evolved Stars Prof. Noyes, Robert W. P43: HAT-P-6b: A Hot Jupiter transiting a bright F star Mr. Ogihara, Masahiro P44: Formation of Terrestrial Planets from Planetesimals around M Dwarfs Dr. O'Toole, Simon John P45: Selection effects in Doppler velocity Planet Searches Dr. Plavchan, Peter
P46:
Prospecting for Transits in 2MASS Mr. Omiya, Masashi P48: A Korea-Japan Planet Search Program: Current status and discovery of a brown dwarf candidate Dr. Rahvar Nematabad, Sohrab P49: Xallarap Microlensing detection of exoplanets Mr. Regandell, Samuel P50: Places where planets form Mr. Robles, Jose A P51: How Typical is the Sun? Miss Rojas, Barbara Denisse P52: Metallicity detemination of M dwarfs in the NIR Dr. Schuetz, Oliver P53: Astromineralogy of protoplanetary disks Dr. Schwarz, Richard P54: Orbital stability of fictitious Trojans in Extrasolar planetary systems Dr. Sozzetti, Alessandro P55: Observational Tests of Planet Formation Models Mr. Tachinami, Chihiro P56: Thermal evolution and magnetism of terrestrial planets Dr. Tubbs, Robert Nigel P57: Software, strategy and error budget for the Exoplanet Search with PRIma (ESPRI) Mr. Van Der Plas, Gerrit P58: Using [OI] emission as a tracer for the shape of - and gaps in - circumstellar disks Dr. Von Braun, Kaspar P59: Observational Window Functions in Planet Transit Searches Miss Wang, Su P60: Analysis of Near-separatrix Motion in Planetary systems Dr. Wang, Xiao-Bin P61: Photometric observation of the transiting planet WASP-1b Prof. Weng, Zihua
P62:
Planetary Dynamic Characteristics in Modified Gravitational
Field Mr. Xie, Ji-Wei
P64: Effects
of dissipating gas drag on plantesimal accretion in binary
systems Mr. Zhang, Hui P66: On the Orbital Evolution of Multiple Protoplanets Embedded in a Protostellar Disk Mr. Zhao, Haibin P67: Photometric Performances of NEOST and the further exoplanet observation Mr. Zhao, Ming P68: Closure Phase Studies toward Direct Detection of Light from Hot Jupiters Dr. Zhou, Jilin P69: Post-oligarchic Evolution of Protoplanetary Embryos and the Stability of Planetary Systems P70: Planetesimal Accretion onto Growing Proto–Gas Giant Planets Mr. Zhao Gang P71: On the Dynamical Lifetime of the Solar System Mr. Dong, Ruobing P72: Origin of dust disk around a young white dwarf
Mr. Wang, Yan P73: Origin of Disks and Supply of Metals in DZ White Dwarfs
Miss Li, Shuling P74: Giant impact, planetary merger, and diversity of planetary-core mass
Miss Zhang, Xiaojia P75: Retention of protoplanetary cores near the Snowline
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| Unknown Remittance | |
| We have more money from unknowns. Below we list the annotations we found on the bank file. CARLY HALLMAN 40USD BONNIEIKOSSLFF 150USD If you are or you know the remitter(s), please contact us at iaus249@nju.edu.cn. | |
| Frequently Asked Questions and Answers | |
| Q: What's the process to make a sucessful attendance? | |
| A: You should follow this process: 1. finish the on-line registration; 2. pay the registration fee; 3. get the invitation letter; 4. get the visa; 5. book a hotel room; 6. find a flight ticket | |
| Q: Shall I register and pay the registration fee? | |
| A: Yes. Everyone, including members of SOC and invited speakers, shall provide necessary information by completing the on-line registration and pay the fee. Please note there is discount for early bird registration before August 31. | |
| Q: Can I pay the registration fee from the IAU grants? | |
| A: Yes. If you have obtained the IAU grants, we can charge your registration fee from the grants. But you need to send an email to iaus249@nju.edu.cn to state this. The IAU grants is in the currency of CHF, we will charge the the right amount in USD (250 for staff member and 150 for students) on August 31 with the exchange rate on that day. | |
| Q: Can I pay through credit card? | |
| A: No. You can pay the registration fee through wire transferring. All other money should be paid by cash on desk at your arriving. | |
| Q: Who will pay the bank charge for the money transferring? | |
| A: The participant. We need to receive the right amount of 250USD (staff member) or 150USD (student) in our account. | |
| Q: How to apply for a visa to travel in China? | |
| A: Generally speaking, it should be quite easy. Please ask the nearest Chinese Embassy or Consulate early. We have heard that many people just ask for a tourist visa to travel. After your registration, an invitation letter will be sent to you by airmail. In some (unusual) cases, the visa office may require a "visa requisition form" (it will be in Chinese) from us, so we would send it to you along with the invitation. For this purpose, you need to supply your passport number. Please send an email to iaus249@nju.edu.cn to give us your (and your accompanier's) passport number. | |
| Q: Will you arrange more tours after the conference? | |
| A: Sorry, No. But we will try to offer some help for you. | |
For your information, the electrical system
in China is 220V 50Hz and the most popular plug & socket is the
oblique flat blades (like a 'V') with ground.