Zobrazeno 1 - 10
of 179
pro vyhledávání: '"Hanami, H."'
Autor:
Miyaji, T., Bravo-Navarro, B. A., Tello, J. Díaz, Krumpe, M., Herrera-Endoqui, M., Ikeda, H., Takagi, T., Oi, N., Shogaki, A., Matsuura, S., Kim, H., Malkan, M. A., Hwang, H. S., Kim, T., Ishigaki, T., Hanami, H., Kim, S. J., Ohyama, Y., Goto, T., Matsuhara, H.
Publikováno v:
A&A 689, A83 (2024)
We present a catalog of optical and infrared identifications (ID) of X-ray sources in the AKARI North Ecliptic Pole (NEP) Deep field detected with Chandra covering $\sim 0.34\,{\rm deg^{2}}$ with 0.5-2 keV flux limits ranging $\sim 2 \mathrm{-} 20\ti
Externí odkaz:
http://arxiv.org/abs/2407.13864
Autor:
Ohyama, Y., Wada, T., Matsuhara, H., Takagi, T., Malkan, M., Goto, T., Egami, E., Lee, H. M., Im, M., Kim, J. -H., Pearson, C., Inami, H., Oyabu, S., Usui, F., Burgarella, D., Mazyed, F., Imanishi, M., Jeong, W. -S., Miyaji, T., Tello, J. Díaz, Nakagawa, T., Serjeant, S., Takeuchi, T. T., Toba, Y., White, G. J., Hanami, H., Ishigaki, T.
Publikováno v:
A&A 618, A101 (2018)
Deep MIR surveys have revealed numerous strongly star-forming galaxies at redshift z~<2. Their MIR fluxes are produced by a combination of continuum and PAH emission features. The PAH features can dominate the total MIR flux, but are difficult to mea
Externí odkaz:
http://arxiv.org/abs/1808.04566
Autor:
Matsuhara, H., Wada, T., Oi, N., Takagi, T., Nakagawa, T., Murata, K., Goto, T., Oyabu, S., Takeuchi, T. T., Malek, K., Solarz, A., Ohyama, Y., Miyaji, T., Krumpe, M., Lee, H. M., Im, M., Serjeant, S., Pearson, C. P., White, G. J., Malkan, M. A., Hanami, H., Ishigaki, T., Burgarella, D., Buat, V., Pollo, A.
Publikováno v:
2017, Publications of The Korean Astronomical Society, vol. 32, issue 1, pp. 213-217
The recent updates of the North Ecliptic Pole deep (0.5~deg$^2$, NEP-Deep) multi-wavelength survey covering from X-ray to radio-wave is presented. The NEP-Deep provides us with several thousands of 15~$\mu$m or 18~$\mu$m selected sample of galaxies,
Externí odkaz:
http://arxiv.org/abs/1710.10472
Autor:
Tello, J. Díaz, Miyaji, T., Ishigaki, T., Krumpe, M., Ueda, Y., Brunner, H., Goto, T., Hanami, H., Toba, Y.
Publikováno v:
A&A 604, A14 (2017)
Aims. We report our finding of a high excitation emission line nebula associated with an Ultra Luminous X-ray source (ULX) at $z=$ 0.027, which we found in our Chandra observation of the AKARI North Ecliptic Pole (NEP) Deep Field. Methods. We present
Externí odkaz:
http://arxiv.org/abs/1706.01986
Autor:
Tello, J. Díaz, Donzelli, C., Padilla, N., Akiyama, M., Fujishiro, N., Yoshikawa, T., Hanami, H.
Publikováno v:
A&A 587, A136 (2016)
Aims. We present a spectroscopic study of the properties of 64 Balmer break galaxies that show signs of star formation. The studied sample of star-forming galaxies spans a redshift range from 0.094 to 1.475 with stellar masses in the range 10$^{8}-$1
Externí odkaz:
http://arxiv.org/abs/1601.03077
Autor:
Solarz, A., Pollo, A., Takeuchi, T. T., Małek, K., Matsuhara, H., White, G. J., Pȩpiak, A., Goto, T., Wada, T., Oyabu, S., Takagi, T., Ohyama, Y., Pearson, C. P., Hanami, H., Ishigaki, T., Malkan, M.
Publikováno v:
A&A 582, A58 (2015)
We present a method of selection of 24~$\mu$m galaxies from the AKARI North Ecliptic Pole (NEP) Deep Field down to $150 \mbox{ }\mu$Jy and measurements of their two-point correlation function. We aim to associate various 24 $\mu$m selected galaxy pop
Externí odkaz:
http://arxiv.org/abs/1509.00219
Autor:
Krumpe, M., Miyaji, T., Brunner, H., Hanami, H., Ishigaki, T., Takagi, T., Markowitz, A. G., Goto, T., Malkan, M. A., Matsuhara, H., Pearson, C., Ueda, Y., Wada, T.
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 446, 911 (2015)
We present data products from the 300 ks Chandra survey in the AKARI North Ecliptic Pole (NEP) deep field. This field has a unique set of 9-band infrared photometry covering 2-24 micron from the AKARI Infrared Camera, including mid-infrared (MIR) ban
Externí odkaz:
http://arxiv.org/abs/1409.7697
Autor:
Tello, J. Díaz, Donzelli, C., Padilla, N., Fujishiro, N., Hanami, H., Yoshikawa, T., Hatsukade, 'and' B.
We present a spectroscopic study with the derivation of the physical properties of 37 Balmer break galaxies, which have the necessary lines to locate them in star-forming-AGN diagnostic diagrams. These galaxies span a redshift range from 0.045 to 0.9
Externí odkaz:
http://arxiv.org/abs/1306.0905
Autor:
Nobuta, K., Akiyama, M., Ueda, Y., Watson, M. G., Silverman, J., Hiroi, K., Ohta, K., Iwamuro, F., Yabe, K., Tamura, N., Moritani, Y., Sumiyoshi, M., Kimura, M., Maihara, T., Dalton, G., Lewis, I., Bonfield, D., Lee, H., Lake, E. Curtis, Macaulay, E., Clarke, F., Sekiguchi, K., Simpson, C., Croom, S., Ouchi, M., Hanami, H., Yamada, T.
In order to investigate the growth of super-massive black holes (SMBHs), we construct the black hole mass function (BHMF) and Eddington ratio distribution function (ERDF) of X-ray-selected broad-line AGNs at z~1.4 in the Subaru XMM-Newton Deep Survey
Externí odkaz:
http://arxiv.org/abs/1211.0069
Autor:
Solarz, A., Pollo, A., Takeuchi, T. T., Pepiak, A., Matsuhara, H., Wada, T., Oyabu, S., Takagi, T., Goto, T., Ohyama, Y., Pearson, C. P., Hanami, H., Ishigaki, T.
Context: It is crucial to develop a method for classifying objects detected in deep surveys at infrared wavelengths. We specifically need a method to separate galaxies from stars using only the infrared information to study the properties of galaxies
Externí odkaz:
http://arxiv.org/abs/1203.1931