ASTRO-F/FIS Observing Simulation : Detection Limits for Point Sources

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概要

• 論文の詳細を見る
• Astronomical Society of Japanの論文
• 2003-06-25

著者

• Nishimura Tetsuo

  Subaru Telescope National Astronomical Observatory Of Japan

• Lee Ho-gyu

  Astronomy Program Fprd Department Of Physics And Astronomy Seoul National University

• SHIBAI Hiroshi

  Graduate School of Science, Nagoya University

• KAWADA Mitsunobu

  Graduate School of Science, Nagoya University

• JEONG Woong-Seob

  Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency

• LEE Hyung

  Astronomy Program, FPRD, Department of Physics and Astronomy, Seoul National University

• PAK Soojong

  Department of Astronomy and Space Science, Kyung Hee University

• SOHN Jungjoo

  Department of Physics and Astronomy, Seoul National University

• NAKAGAWA Takao

  The Institute of Space and Astronautical Science

• Nagayama Takahiro

  Department Of Astrophysics Faculty Of Sciences Nagoya University

• WATANABE Masaru

  The Institute of Space and Astronautical Science

• Lee Hyung

  Astronomy Program Fprd Department Of Physics And Astronomy Seoul National University

• SOHN Jungjoo

  Astronomy Program, Department of Physics and Astronomy, FPRD, Seoul National University

• Yamamura Issei

  Jaxa Sagamihara

• Shibai H

  Osaka Univ. Osaka

• Shibai Hiroshi

  Graduate School Of Science Nagoya University

• Yamamura Issei

  Institute Of Space And Astronautical Science Japan Aerospace Exploration Agency

• JEONG Woong-Seob

  Astronomy Program in Graduate School of Earth and Environmental Sciences, Seoul National University

• PAK Soojong

  Astronomy Program in Graduate School of Earth and Environmental Sciences, Seoul National University

• AHN Insun

  Astronomy Program in Graduate School of Earth and Environmental Sciences, Seoul National University

• YAMAMURA Issei

  The Institute of Space and Astronautical Science

• Jeong Woong-seob

  Institute Of Space And Astronautical Science Japan Aerospace Exploration Agency

• Pak Soojong

  Department Of Astronomy And Space Science Kyung Hee University

• Sohn Jungjoo

  Department Of Physics And Astronomy Seoul National University

• Ahn Insun

  Astronomy Program In Graduate School Of Earth And Environmental Sciences Seoul National University

• Shibai H

  Graduate School Of Science Nagoya University

• Kawada Mitsunobu

  Graduate School Of Science Nagoya University

• Lee Hyung

  Astronomy Program In Graduate School Of Earth And Environmental Sciences Seoul National University

• Takato Naruhisa

  Subaru Telescope National Astronomical Observatory Of Japan National Institutes Of Natural Science

• Nishimura Tetsuo

  National Astronomical Observatory Of Japan

• Shibai Hiroshi

  Department Of Earth And Space Science Graduate School Of Science Osaka University

関連論文

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• Multi-Wavelength Analysis of 18μm-Selected Galaxies in the AKARI/Infrared-Camera monitor field towards the North Ecliptic Pole
• Optical Identification of 15μm Sources in the AKARI Performance Verification Field toward the North Ecliptic Pole
• Nature of Infrared Sources in 11μm Selected Sample from Early Data of the AKARI North Ecliptic Pole Deep Survey
• Detection of an Hα Emission Line on a Quasar, RX J1759.4+6638, at z = 4.3 with AKARI
• Properties of UIR Bands in NGC 6946 Based on Mid-Infrared Imaging and Spectroscopy with Infrared Camera on Board AKARI
• AKARI Infrared Imaging of Reflection Nebulae IC 4954 and IC 4955
• Flight Performance of the AKARI Cryogenic System
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• IRTS Observation of the Unidentified 3.3-Micron Band in the Diffuse Galactic Emission
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• AKARI Far-Infrared Source Counts in the Lockman Hole
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• AKARI Detection of the Infrared-Bright Supernova Remnant B0104-72.3 in the Small Magellanic Cloud
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• Near-Infrared Polarization Images of the Orion Molecular Cloud 1 South Region
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• MOIRCS Deep Survey. II : Clustering Properties of K-Band Selected Galaxies in GOODS-North Region
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• Near-Infrared Coronagraphy of the GG Tauri A Binary System
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• First NIR Polarimetry of 30 Doradus
• Near-Infrared Imaging Polarimetry of the Star-Forming Region NGC 2024
• Common Correlations between 60, 100, and 140μm Intensities in the Galactic Plane and Magellanic Clouds
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• Detection of the Mid-Infrared Unidentified Bands in the Diffuse Galactic Emission by IRTS
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• Slow-Scan Observations with the Infrared Camera (IRC) aboard AKARI

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