Staff profile

• Active Galactic Nuclei (AGN), especially X-ray observation and modeling of AGN outflows
• mass loss from massive stars

Journal Article

• Geometry of the X-ray source 1H 0707–495
  Szanecki, M., Niedźwiecki, A., Done, C., Klepczarek, Ł., Lubiński, P., & Mizumoto, M. (2020). Geometry of the X-ray source 1H 0707–495. Astronomy & Astrophysics, 641, Article A89. https://doi.org/10.1051/0004-6361/202038303
• Testing the Lamp-post and Wind Reverberation Models with XMM-Newton Observations of NGC 5506
  Zoghbi, A., Kalli, S., Miller, J. M., & Mizumoto, M. (2020). Testing the Lamp-post and Wind Reverberation Models with XMM-Newton Observations of NGC 5506. Astrophysical Journal, 893(2), Article 97. https://doi.org/10.3847/1538-4357/ab7dc8
• Possible Progression of Mass-flow Processes around Young Intermediate-mass Stars Based on High-resolution Near-infrared Spectroscopy. I. Taurus
  Yasui, C., Hamano, S., Fukue, K., Kondo, S., Sameshima, H., Takenaka, K., Matsunaga, N., Ikeda, Y., Kawakita, H., Otsubo, S., Watase, A., Taniguchi, D., Mizumoto, M., Izumi, N., & Kobayashi, N. (2019). Possible Progression of Mass-flow Processes around Young Intermediate-mass Stars Based on High-resolution Near-infrared Spectroscopy. I. Taurus. Astrophysical Journal, 886(2), Article 115. https://doi.org/10.3847/1538-4357/ab45ee
• First Detection of A–X (0,0) Bands of Interstellar C2 and CN
  Hamano, S., Kawakita, H., Kobayashi, N., Takenaka, K., Ikeda, Y., Matsunaga, N., Kondo, S., Sameshima, H., Fukue, K., Yasui, C., Mizumoto, M., Otsubo, S., Watase, A., Yoshikawa, T., & Kobayashi, H. (2019). First Detection of A–X (0,0) Bands of Interstellar C2 and CN. Astrophysical Journal, 881(2), Article 143. https://doi.org/10.3847/1538-4357/ab2e0f
• Fe i Lines in 0.91–1.33 μm Spectra of Red Giants for Measuring the Microturbulence and Metallicities
  Kondo, S., Fukue, K., Matsunaga, N., Ikeda, Y., Taniguchi, D., Kobayashi, N., Sameshima, H., Hamano, S., Arai, A., Kawakita, H., Yasui, C., Izumi, N., Mizumoto, M., Otsubo, S., Takenaka, K., Watase, A., Asano, A., Yoshikawa, T., & Tsujimoto, T. (2019). Fe i Lines in 0.91–1.33 μm Spectra of Red Giants for Measuring the Microturbulence and Metallicities. Astrophysical Journal, 875(2), https://doi.org/10.3847/1538-4357/ab0ec4
• X-ray reverberation lags of the Fe–K line due to AGN disc winds
  Mizumoto, M., Ebisawa, K., Tsujimoto, M., Done, C., Hagino, K., & Odaka, H. (2019). X-ray reverberation lags of the Fe–K line due to AGN disc winds. Monthly Notices of the Royal Astronomical Society, 482(4), 5316-5326. https://doi.org/10.1093/mnras/sty3056
• Kinetic Energy Transfer from X-Ray Ultrafast Outflows to Millimeter/Submillimeter Cold Molecular Outflows in Seyfert Galaxies
  Mizumoto, M., Izumi, T., & Kohno, K. (2019). Kinetic Energy Transfer from X-Ray Ultrafast Outflows to Millimeter/Submillimeter Cold Molecular Outflows in Seyfert Galaxies. Astrophysical Journal, 871(2), Article 156. https://doi.org/10.3847/1538-4357/aaf814
• Thermally driven wind as the origin of warm absorbers in AGN
  Mizumoto, M., Done, C., Tomaru, R., & Edwards, I. (2019). Thermally driven wind as the origin of warm absorbers in AGN. Monthly Notices of the Royal Astronomical Society, 489(1), 1152-1160. https://doi.org/10.1093/mnras/stz2225
• WINERED High-resolution Near-infrared Line Catalog: A-type Star
  Sameshima, H., Ikeda, Y., Matsunaga, N., Fukue, K., Kobayashi, N., Kondo, S., Hamano, S., Kawakita, H., Yasui, C., Izumi, N., Mizumoto, M., Otsubo, S., Takenaka, K., Watase, A., Asano, A., & Yoshikawa, T. (2018). WINERED High-resolution Near-infrared Line Catalog: A-type Star. Astrophysical Journal Supplement, 239(2), Article 19. https://doi.org/10.3847/1538-4365/aae924
• A newly identified emission-line region around P Cygni
  Mizumoto, M., Kobayashi, N., Hamano, S., Ikeda, Y., Kondo, S., Sameshima, H., Matsunaga, N., Fukue, K., Yasui, C., Izumi, N., Kawakita, H., Nakanishi, K., Nakaoka, T., Otsubo, S., & Maehara, H. (2018). A newly identified emission-line region around P Cygni. Monthly Notices of the Royal Astronomical Society, 481(1), 793-805. https://doi.org/10.1093/mnras/sty2239
• X-ray short-time lags in the Fe-K energy band produced by scattering clouds in active galactic nuclei
  Mizumoto, M., Done, C., Hagino, K., Ebisawa, K., Tsujimoto, M., & Odaka, H. (2018). X-ray short-time lags in the Fe-K energy band produced by scattering clouds in active galactic nuclei. Monthly Notices of the Royal Astronomical Society, 478(1), 971-982. https://doi.org/10.1093/mnras/sty1114
• Can the relativistic light-bending model explain X-ray spectral variations of Seyfert galaxies?
  Mizumoto, M., Moriyama, K., Ebisawa, K., Mineshige, S., Kawanaka, N., & Tsujimoto, M. (2018). Can the relativistic light-bending model explain X-ray spectral variations of Seyfert galaxies?. Publications of Astronomical Society of Japan, 70(3), Article 42. https://doi.org/10.1093/pasj/psy032
• Nature of the warm absorber outflow in NGC 4051
  Mizumoto, M., & Ebisawa, K. (2017). Nature of the warm absorber outflow in NGC 4051. Monthly Notices of the Royal Astronomical Society, 466(3), 3259-3271. https://doi.org/10.1093/mnras/stw3364
• Variabiity of the X-ray broad iron spectral features in active galactic nuclei and black-hole binaries
  Mizumoto, M., Ebisawa, K., Tsujimoto, M., & Inoue, H. (2016). Variabiity of the X-ray broad iron spectral features in active galactic nuclei and black-hole binaries. Astronomische Nachrichten, 337(4-5), 507-511. https://doi.org/10.1002/asna.201612338
• Origin of the X-ray broad iron spectral feature in GRS 1915+105
  Mizumoto, M., Ebisawa, K., Tsujimoto, M., & Inoue, H. (2016). Origin of the X-ray broad iron spectral feature in GRS 1915+105. Publications of Astronomical Society of Japan, 68(SP1), Article S16. https://doi.org/10.1093/pasj/psv125
• Interpretation of the X-ray spectral variation of 1H 0707−495 with a variable double partial covering model
  Mizumoto, M., Ebisawa, K., & Sameshima, H. (2014). Interpretation of the X-ray spectral variation of 1H 0707−495 with a variable double partial covering model. Publications of Astronomical Society of Japan, 66(6), https://doi.org/10.1093/pasj/psu121