20
Ji-hyun Kang (KASI) Ref : EU Archive science file

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

  • Upload
    others

  • View
    0

  • Download
    0

Embed Size (px)

Citation preview

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

Archive & JVO