Participants | ||||
Name |
Affiliation |
Status |
Seminar |
|
1 |
À뱂 ÀÓ |
¼¼Á¾´ëÇб³ |
Student |
|
2 |
ÀÓÇü¹¬ ÀÓ |
¼¼Á¾´ëÇб³ |
Student |
|
3 |
¿ø±â ¹Ú |
¼¼Á¾´ëÇб³/ARCSEC |
Doctor |
TBD |
4 |
Á¤¿¬ Á¶ |
Ãæ³²´ëÇб³ |
Professor |
TBD |
5 |
¹ü¼® ¿° |
Ãæ³²´ëÇб³ |
Student |
High Redshift Simulations using the GALEX Ultraviolet Images of Nearby Galaxies |
6 |
¼® ±è |
Ãæ³²´ëÇб³ õ¹®¿ìÁÖ°úÇаú |
Student |
Ultraviolet properties of Early-Type dwarf Galaxies in the Virgo Cluster. |
7 |
¼öâ ÀÌ |
Ãæ³²´ëÇб³ |
Professor |
|
8 |
¼öÁ¾ ¹Ú |
°æÈñ´ëÇб³ |
Professor |
MIR Camera for Japanese Space IR Telescope SPICA |
9 |
±ÔÇö ä |
¼¼Á¾´ëÇб³ |
Professor |
Dark Enery, Halo Mass Functions and Lens Statistics |
10 |
¸í½Å ÀÓ |
¼¿ï´ëÇб³ |
Professor |
TBD |
11 |
Á¾¼ö ±è |
Çѱ¹Ãµ¹®¿¬±¸¿ø |
Doctor |
|
12 |
â¹ü ¹Ú |
°íµî°úÇпø |
Professor |
Sciences of the SDSS-III Survey |
13 |
¿µ·¡ ±è |
°íµî°úÇпø |
Doctor |
Cosmological Parameter Estimation from LSS Topology |
14 |
À±¿µ ÃÖ |
°íµî°úÇпø |
Professor |
Environmental dependence of AGN activity |
15 |
È«¹è ¾È |
ºÎ»ê´ëÇб³ |
Professor |
Morphology and Environment of nearby galaxies |
16 |
Á¤ÁÖ ¼Õ |
°æÈñ´ëÇб³ |
Doctor |
|
17 |
¼º¼ö ±è |
°æÈñ´ëÇб³ |
Professor |
|
18 |
Á¾È¯ ÀÌ |
¼¿ï´ëÇб³ |
Student |
|
19 |
±â¿ø ÀÌ |
°æºÏ´ëÇб³/ARCSEC |
Professor |
|
20 |
±¤È£ ÀÌ |
¼¿ï´ëÇб³ |
Student |
|
21 |
À±Çö ·ù |
°æºÏ´ëÇб³ |
Student |
|
22 |
À±Èñ ÀÌ |
°æºÏ´ëÇб³ |
Student |
The Nuclear Regions of Nearyby Galaxies |
23 |
ÀÀÁø Àü |
°íµî°úÇпø |
Professor |
|
24 |
µµ±Õ ±è |
Yonsei Univ, KIAS |
Student |
|
25 |
ÁÖÇÑ ±è |
°íµî°úÇпø |
Doctor |
Subhalo-Galaxy Correspondence Model |
26 |
ÇöÁø ¹è |
¿¬¼¼´ëÇб³ |
Student |
|
27 |
µ¿Çö ÀÌ |
¿¬¼¼´ëÇб³ |
Student |
|
28 |
È£ ÀÌ |
¿¬¼¼´ëÇб³ Àڿܼ± ¿ìÁÖ¸Á¿ø°æ ¿¬±¸´Ü |
Student |
|
29 |
¹ÌÈ ÇÑ |
¿¬¼¼´ëÇб³ |
Student |
|
30 |
kiyun yun |
Dept. Astronomy. Yonsei Univ. S.Korea. |
Student |
|
31 |
Çö¿µ ÀÌ |
¿¬¼¼´ëÇб³ |
Student |
|
32 |
µÎȯ ÇÑ |
°æºÏ´ëÇб³ |
Student |
Han, D.-H. Type Ia Supernoave in the SDSS Stripe 82 |
33 |
¹Î¼± ±è |
õ¹®¿¬±¸¿ø |
Doctor |
|
34 |
Çü¸ñ ÀÌ |
¼¿ï´ëÇб³ |
Professor |
Preliminary results of NEP Wide Survey of AKARI |
35 |
¼®Áø À± |
¿¬¼¼´ëÇб³ |
Professor |
|
36 |
ÀºÇõ ±è |
¼¿ï´ëÇб³ |
Doctor |
Galactic Globular Clusters in SDSS |
37 |
º´¿ø °í |
°íµî°úÇпø |
Professor |
Dark Matter Candidates in Particle Physics |
38 |
Á¤¿í ±è |
°íµî°úÇпø |
Professor |
Neutrino Physics and Cosmology |
39 |
ÁØÇù ÀÌ |
¼¿ï´ëÇб³ |
Student |
Multiwavelength Properties of the SDSS Galaxies in Various Classes |
40 |
¼®Ãµ ÀÌ |
Institute of Physics, Academia Sinica. |
Doctor |
Large Scale Strucure and Modified Gravity |
41 |
Kevin Schawinski Schawinski |
University of Oxford |
Doctor |
The Star Formation and Black Hole Accretion Histories of SDSS Early-type Galaxies |
42 |
À̼®¿µ Yi |
¿¬¼¼´ëÇб³ |
Professor |
Specific star formation rates of SDSS galaxies compared with semi-analytic models |
43 |
ż± ±è |
¿¬¼¼´ëÇб³ |
Student |
The Intrinsic Axis Ratio Distribution of Early-type Galaxies |
44 |
Çý¿ø ¼ |
¿¬¼¼´ëÇб³ õ¹®¿ìÁÖÇаú |
Student |
|
45 |
ÁÖÇå À± |
¿¬¼¼´ëÇб³ õ¹®¿ìÁÖÇаú |
Student |
A Demography of Galaxies in Galaxy Clusters with the Spectro-photometric density measurement. |
46 |
¹«¿µ õ |
Çѱ¹Ãµ¹®¿¬±¸¿ø |
Doctor |
|