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1 Korean Activities in IR Space Missions - Past, Current and Future - Woong-Seob Jeong 1 on behalf of Korean Infrared Astronomy Group 1 KASI, Korea Ramada.

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Presentation on theme: "1 Korean Activities in IR Space Missions - Past, Current and Future - Woong-Seob Jeong 1 on behalf of Korean Infrared Astronomy Group 1 KASI, Korea Ramada."— Presentation transcript:

1 1 Korean Activities in IR Space Missions - Past, Current and Future - Woong-Seob Jeong 1 on behalf of Korean Infrared Astronomy Group 1 KASI, Korea Ramada Hotel, Jeju, 2 nd AKARI Converence, 2012/02/27 ~ 02/29

2 2 Infrared Projects in Korea Experience in the near-IR space instrument Data analysis & scientific research in IR range Space IR Ground IR 2004 2006 2008 2010 2012 2014 2016 KASINICS Ground Near-IR Camera PSICS IR Cryogenic System CIBER Near-IR Camera AKARI DR Pipeline Science Collaborations MIRIS Compact Space IR Camera IGRINS Ground Near-IR Spectrometer

3 3 Participation to AKARI Project Development of data reduction pipeline  Collaborative Work: ESA, ISAS, SNU  SNU: optical simulation, observing simulation, modules of data reduction pipeline for FIS (Far- Infrared Surveyor) Simulated images

4 4 Scientific Products from AKARI 90  m point source map SNR detection in LMC Sky brightness map @ 9  m CIB detected in NEP Field

5 5 Technical Development (1/3) Development of our own IR instrument: KASI Near-Infrared Camera (KASINICS)  Optical system including mirror  Mechanics and cryogenics  Electronics

6 6 Technical Development (2/3) Scientific observations with KASINICS @ Bohyun  FoV : 3.3’x 3.3’(pixel: 0.39”)  J, H, Ks, L, H 2, and H 3 + bands (Gupta et al. 2009) (Burrows et al. 2011) NIR Light curve of Sw J1644+57

7 7 Technical Development (3/3) Proto-model of space infrared cryogenic system (PSICS)  Small mechanical cooler  Cooling system down to 77K  Space use

8 8 Space Observation Program Science & Technology Satellite Series in Korea  1 st satellite: FIMS (Far-ultraviolet Imaging Spectrograph) (2003)  2 nd Satellite: Observation of Space environment by Korean Launcher Naro  3 rd Satellite: MIRIS (Multipurpose Infrared Imaging System) (Seon et al. 2011)

9 9 ST-Satellite III Primary payload : MIRIS  Wide-Area Survey in Near-Infrared Galactic Plane Survey in Paschen  emission line Observation of Low Background Region in Wide bands MIRIS

10 10 Specifications of MIRIS Specifications of Space Observation Camera  Wavelength: 0.9 ~ 2  m − Aperture: 80 mm  Detector FOV: 3.67 o x 3.67 o (Pixel : 51.6 arcsec) (c.f. Nyq. sampling @ 1.6  m = 4.1 arcsec) → limited by satellite stability  Telescope & Sensor Temp.: 180K (Passive Cooling), 90K  Filters (5 filters) I (1.05  m), H (1.6  m), blank Pa  (1.876  m), Pa  Cont

11 11 Pa  Emission Line Survey Galactic Plane, WIM Origin of Warm Ionized Medium  Previous study of WIM: Photoionization model  Recent study of WIM from FIMS: dust scattering  Verification of the dust scattering theory Physical Properties of Interstellar Turbulence Observation: Pa survey  Comparison between Pa (MIRIS) vs. H Monte-Carlo simulation  Uniform dust distribution; E(B-V) = 0.1  Point source or Spherical H II region

12 12 Observation for CIB Cosmic Infrared Background in Near-IR band  CIB from POP III stats  Spectral peak of CIB  Large-scale fluctuation of CIB Matsumoto et al. 2005 Large-scale structure of CIB from IRTS observation 10 100 0.20.40.60.8135 residual_summary IRTS/NIRS model by Totani et al. 2001 Totani et al. 2001 Bernstein et al. 2002 DIRBE/COBE Wright and Rees 2000 Fazio et al. 2004 Madau and Pozzetti 2000 Cambrecy et al. 2001 Surface brightness (nW/m 2 /sr) Wavelength (  m)

13 13 Calibration purpose: 2 orbits /day Simultaneous observation of NEP & SEP in 1 orbit Monitoring of ZL in SEP and NEP: I & H bands  Revision of ZL Model & Removal of ZL component Zodiacal Foreground

14 14 CIBER Sounding Rocket Payload Imagers  Wavelength: 0.9 ~ 2  m − Aperture: 110 mm  FOV: 2 o x 2 o (pixel = 7 arcsec)  Sensor Temp.: 77K  Filters (2 filters) I (1.0  m), H (1.6  m) Spectrometers  LRS (Low Resolution)  NBS (Narrow Band)

15 15 Future Project Ground telescope: GMT Space Telescope  Synergy with GMT  International collaboration  New technical challenge SPICA Project  Near-infrared instrument (heritage from MIRIS)

16 16 Summary International collaborations in the big projects Large Infrared Space Telescope in Korea Space IR Ground IR 2004 2006 2008 2010 2012 2014 2016 KASINICS Ground Near-IR Camera PSICS IR Cryogenic System CIBER Near-IR Camera AKARI DR Pipeline Science Collaborations MIRIS Compact Space IR Camera IGRINS Ground Near-IR Spectrometer SPICA FPC CIBER II GMTNIRS GMT Near-IR Spectrometer


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