博士后

序號

招收方向

專業背景等要求

合作導師

郵箱

是否招收外籍

1

銀河系分子云的巡天觀測研究。

Survey Study of Galactic Molecular Clouds.

熟練毫米波譜線觀測,在分子云觀測研究方向有科學產出。

Good at millimeter-wave line observations with publications in the study of interstellar molecular clouds.

楊戟

jiyang@pmo.ac.cn

2

21-cm cosmology: intensity mapping, and epoch of reionization;

Cosmic microwave background radiation;

Large-scale structure formation.

Good background in cosmology, some knowledge level in radio astronomy, and strong programming skills.


馬寅哲

Ma@ukzn.ac.za

3

星系形成的流體模擬研究。

Hydro-dynamical simulation of galaxyformation;

宇宙大尺度結構。

large-scale structure formation of the universe.

galaxy formation using hydro-dynamical simulation;

galaxy formation and large-scale structure of the universe, experience with using observational data, especially using the luminous red galaxies.


康熙

kangxi@pmo.ac.cn

4

弱引力透鏡信號測量技術;

圖像疊加技術;

弱引力透鏡理論研究。

具備良好的編程能力,有一定的引力透鏡研究背景或具有熟練的圖像處理技術。



李國亮

guoliang@pmo.ac.cn

5

通過對分子云與星團進行多波段觀測與數據處理分析,研究銀河系內的分子云恒星形成過程。

Multi-Wavelength studies of molecular clouds and stellar clusters to understand the star-forming process of the Milky Way;

通過使用國內國際大型射電、毫米波等觀測設備,研究河外星系中的分子氣體、塵埃以及恒星形成的性質。

Study molecular gas (especially dense gas), dust and their relationships with star-formation activity of external galaxies.

具有豐富的數據處理經驗,能夠進行獨立的科研能力。


高煜

yugao@pmo.ac.cn

6

先進天基太陽天文臺”是即將工程立項并計劃于2022年發射的我國第一顆太陽探測衛星,圍繞該衛星有效載荷未來觀測數據分析軟件及有關科學開展研究。

ASO-S is the first Chinese solar satellite which will be launched in 2022. The mission of the position will concentrate on the data analysis software and scientific objective dedicated researches.

太陽物理研究方向博士學位獲得者,提供能夠證明自己勝任該博士后位置的材料(如論文等)。

PhD in solar physics.


甘為群

wqgan@pmo.ac.cn

7

The origin of cosmic rays and multi-wavelength study of supernova remnants.

Ph.D in astrophysics. Familiar with radiative processes, plasma physics, and particle acceleration and transport theory.


劉四明

liusm@pmo.ac.cn

8

暗物質間接探測。

dark matter indirect detection;

高能天體物理。

high energy astrophysics.

具有Fermi-LAT數據處理經驗,在暗物質或高能天體物理研究領域有較好的工作基礎。

The applicants should major in dark matter indirect detection or high energy astrophysics and have experience on data analysis of Fermi-LAT.


范一中

yzfan@pmo.ac.cn

9

高能天體物理X射線/紫外彌漫源光譜研究。

High-energy astrophysics: X-ray/UV spectroscopy for diffuse plasmas;

近鄰星系多波段研究。

Muti-wavelength studies for nearby galaxies;

星系流體數值模擬研究。

Hydro-dynamical simulations for galaxies;

紫外空間探測技術。

Technologies for UV space detection.



需要天體物理、物理或者光學設計專業的博士,有國外經歷者優先。申請材料包括簡介、發表文章、2封推薦信。

The group of X-ray/UV science and space detection in PMO invites the applications for a couple of postdoc positions in the field of High-energy astrophysics: X-ray/UV spectroscopy for diffuse plasmas; Muti-wavelength studies for nearby galaxies; Hydro-dynamical simulations for galaxies; and Technologies for UV space detection. The successful applicants will collaborate with Prof. Ji, L. and her group. The positions are available for 2 years, funding for research travel and equipment is also provided. Additional benefits such as housing can be provided by PMO. The preferred starting date is Oct. 1st 2017 although it can be negotiable.

A requirement for employment is the possession of the Ph.D. diploma in Astrophysics、physics or Optics, a list of publications, a statement of scientific interests and plans (2 pages) and two letters of recommendation. For full consideration, the applications should be received by Sep.1st, 2017. The review of applications will begin soon after this date and continue until the positions are filled. Applications (in pdf format) and questions concerning the positions should be sent to ji@pmo.ac.cn


紀麗

ji@pmo.ac.cn

10

Thermal infrared remote sensing;

Geology, Petrology or Spectroscopy.

has a background of related discipline;

has published at least one paper in the international journal.


吳昀昭

wu@pmo.ac.cn


 
 
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■地址:
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