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Ji-hyun Kang (KASI)alma.kasi.re.kr/files/2019/townhall/kangj_kasi.pdf · Figure 9. SED fit for NGC...

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Ji-hyun Kang (KASI) Ref : EU Archive science ﬁle

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Page 1: Ji-hyun Kang (KASI)alma.kasi.re.kr/files/2019/townhall/kangj_kasi.pdf · Figure 9. SED fit for NGC 1068 to the mid-IR spectra (black spectrum) with the torus model (long-dashed and

Ji-hyun Kang (KASI)

Ref : EU Archive science file

Page 2: Ji-hyun Kang (KASI)alma.kasi.re.kr/files/2019/townhall/kangj_kasi.pdf · Figure 9. SED fit for NGC 1068 to the mid-IR spectra (black spectrum) with the torus model (long-dashed and

Page 3: Ji-hyun Kang (KASI)alma.kasi.re.kr/files/2019/townhall/kangj_kasi.pdf · Figure 9. SED fit for NGC 1068 to the mid-IR spectra (black spectrum) with the torus model (long-dashed and

Page 4: Ji-hyun Kang (KASI)alma.kasi.re.kr/files/2019/townhall/kangj_kasi.pdf · Figure 9. SED fit for NGC 1068 to the mid-IR spectra (black spectrum) with the torus model (long-dashed and

T-ReCS/Gemini, SOFIA ALMA, JVLA

Page 5: Ji-hyun Kang (KASI)alma.kasi.re.kr/files/2019/townhall/kangj_kasi.pdf · Figure 9. SED fit for NGC 1068 to the mid-IR spectra (black spectrum) with the torus model (long-dashed and

Page 6: Ji-hyun Kang (KASI)alma.kasi.re.kr/files/2019/townhall/kangj_kasi.pdf · Figure 9. SED fit for NGC 1068 to the mid-IR spectra (black spectrum) with the torus model (long-dashed and

Page 7: Ji-hyun Kang (KASI)alma.kasi.re.kr/files/2019/townhall/kangj_kasi.pdf · Figure 9. SED fit for NGC 1068 to the mid-IR spectra (black spectrum) with the torus model (long-dashed and

Page 8: Ji-hyun Kang (KASI)alma.kasi.re.kr/files/2019/townhall/kangj_kasi.pdf · Figure 9. SED fit for NGC 1068 to the mid-IR spectra (black spectrum) with the torus model (long-dashed and

Page 9: Ji-hyun Kang (KASI)alma.kasi.re.kr/files/2019/townhall/kangj_kasi.pdf · Figure 9. SED fit for NGC 1068 to the mid-IR spectra (black spectrum) with the torus model (long-dashed and

Page 10: Ji-hyun Kang (KASI)alma.kasi.re.kr/files/2019/townhall/kangj_kasi.pdf · Figure 9. SED fit for NGC 1068 to the mid-IR spectra (black spectrum) with the torus model (long-dashed and

Page 11: Ji-hyun Kang (KASI)alma.kasi.re.kr/files/2019/townhall/kangj_kasi.pdf · Figure 9. SED fit for NGC 1068 to the mid-IR spectra (black spectrum) with the torus model (long-dashed and

Page 12: Ji-hyun Kang (KASI)alma.kasi.re.kr/files/2019/townhall/kangj_kasi.pdf · Figure 9. SED fit for NGC 1068 to the mid-IR spectra (black spectrum) with the torus model (long-dashed and

Page 13: Ji-hyun Kang (KASI)alma.kasi.re.kr/files/2019/townhall/kangj_kasi.pdf · Figure 9. SED fit for NGC 1068 to the mid-IR spectra (black spectrum) with the torus model (long-dashed and

Page 14: Ji-hyun Kang (KASI)alma.kasi.re.kr/files/2019/townhall/kangj_kasi.pdf · Figure 9. SED fit for NGC 1068 to the mid-IR spectra (black spectrum) with the torus model (long-dashed and

Page 15: Ji-hyun Kang (KASI)alma.kasi.re.kr/files/2019/townhall/kangj_kasi.pdf · Figure 9. SED fit for NGC 1068 to the mid-IR spectra (black spectrum) with the torus model (long-dashed and

Page 16: Ji-hyun Kang (KASI)alma.kasi.re.kr/files/2019/townhall/kangj_kasi.pdf · Figure 9. SED fit for NGC 1068 to the mid-IR spectra (black spectrum) with the torus model (long-dashed and

Page 17: Ji-hyun Kang (KASI)alma.kasi.re.kr/files/2019/townhall/kangj_kasi.pdf · Figure 9. SED fit for NGC 1068 to the mid-IR spectra (black spectrum) with the torus model (long-dashed and

Page 18: Ji-hyun Kang (KASI)alma.kasi.re.kr/files/2019/townhall/kangj_kasi.pdf · Figure 9. SED fit for NGC 1068 to the mid-IR spectra (black spectrum) with the torus model (long-dashed and

Page 19: Ji-hyun Kang (KASI)alma.kasi.re.kr/files/2019/townhall/kangj_kasi.pdf · Figure 9. SED fit for NGC 1068 to the mid-IR spectra (black spectrum) with the torus model (long-dashed and

Page 20: Ji-hyun Kang (KASI)alma.kasi.re.kr/files/2019/townhall/kangj_kasi.pdf · Figure 9. SED fit for NGC 1068 to the mid-IR spectra (black spectrum) with the torus model (long-dashed and

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