Infrared Photometric Data of Asteroids with AKARI 
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Asteroid Catalog Using AKARI: AKARI/IRC Mid-Infrared Asteroid Survey 
    Usui, F., Kuroda, D., Mueller, T. G., et al. 
   <Publ. Astron. Soc. Japan, 63, 1117-1138 (2011)>
   =2011PASJ...63.1117U

The Asteroid Catalog Using AKARI IRC Slow-Scan Observations 
    Hasegawa, S., Mueller, T. G., Kuroda, D., et al. 
   <Publ. Astron. Soc. Japan, 65, 34, 1-11 (2013)>
   =2013PASJ...65...34H

(25143) Itokawa: The power of radiometric techniques for the interpretation of 
remote thermal observations in the light of the Hayabusa rendezvous results 
    Mueller, T. G., Hasegawa, S., and Usui, F.
   <Publ. Astron. Soc. Japan, 66, 52, 1-17 (2014)>
   =2014PASJ...66...52M

Hayabusa-2 Mission Target Asteroid 162173 Ryugu (1999 JU3): Searching for 
the Object's Spin-Axis Orientation 
    Mueller, T. G., Durech, J., Ishiguro, M., et al. 
    (submitted to Astronomy & Astrophysics, 2016)
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ADC_Keywords: Solar system ; Minor planets ; Photometry, infrared
Mission_Name: AKARI
Keywords: catalogs - infrared: solar system - minor planets, asteroids -
          space vehicles; instruments - surveys

Description:
   This catalog contains photometric data of 5201 asteroids observed with the 
   infrared astronomical satellite AKARI (Murakami et al. 2007). The catalog 
   objects comprise the near-Earth asteroids, the main belt asteroids, the 
   Cybeles, the Hildas, and the Jovian Trojan asteroids. The observations were 
   performed with the Infrared Camera (IRC; Onaka et al. 2007) on board AKARI 
   by the all-sky survey in 9 or 18 um bands as well as the slow-scan 
   observations in 9 or 18 um bands, and the pointed observations in 3, 4, 7, 
   11, 15, and/or 24 um bands. The all-sky survey (Usui et al. 2011) and the 
   slow-scan observations (Hasegawa et al. 2013) detected asteroids 
   serendipitously, while the pointed observations (Mueller et al. 2014, 2016) 
   intentionally targeted the objects. Note that an asteroid was not observed 
   with two or more bands simultaneously because of the alignment of the focal 
   plane instruments or the filter operation of the detector.

   Data reductions were performed by the following methods: 
      The all-sky survey: The data reduction and flux calibration were applied 
         in the same manner as in the IRC Point Source Catalog 
         (Ishihara et al. 2010). See Usui et al. (2011) for details. 
      The Slow-scan observations: The IRC slow-scan observation data were 
         reduced by the AKARI data reduction tools (Takita et al. 2012). Flux 
         calibration is given in Hasegawa et al. (2013). See Hasegawa et al. 
         (2013) for details. 
      The pointed observations: The imaging data reduction toolkit was applied 
         for data reduction (version 20070104 for (25143) Itokawa, and version 
         20150331 for (162173) Ryugu). Flux calibration is described in Tanabe 
         et al. (2008). See Mueller et al. (2014, 2016) for details. 

See also:
    The Infrared Astronomical Mission AKARI
    Murakami, H., Baba, H., Barthel, P., et al.
   <Publ. Astron. Soc. Japan, 59, S369-S376 (2007)>
   =2007PASJ...59S.369M

    The Infrared Camera (IRC) for AKARI -- Design and Imaging Performance
    Onaka, T., Matsuhara, H., Wada, T., et al. 
   <Publ. Astron. Soc. Japan, 59, S401-S410 (2007)>
   =2007PASJ...59S.401O

    Absolute Photometric Calibration of the Infrared Camera (IRC) aboard AKARI 
    Tanabe, T., Sakon, I., Cohen, M., et al. 
   <Publ. Astron. Soc. Japan, 60, S375--S388 (2008)>
   =2008PASJ...60S.375T

    Albedo, Size, and Surface Characteristics of Hayabusa-2 Sample-Return 
    Target 162173 1999 JU3 from AKARI and Subaru Observations
    Hasegawa, S., Mueller, T. G., Kawakami, K., et al. 
   <Publ. Astron. Soc. Japan, 60, S399-S405 (2008)>
   =2008PASJ...60S.399H

    The AKARI/IRC mid-infrared all-sky survey 
    Ishihara, D., Onaka, T., Kataza, H., et al. 
   <Astro. Astrophys., 514, A1, 1-14 (2010)>
   =2010A&A...514A...1I

    Slow-Scan Observations with the Infrared Camera (IRC) aboard AKARI 
    Takita, S., Ikeda, N., Kitamura, Y., et al. 
   <Publ. Astron. Soc. Japan, 64, 126, 1-8 (2012)>
   =2012PASJ...64..126T

File Summary:
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FileName      Lrecl  Records   Explanations
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ReadMe            80        .   This file
AST_FLUX_V1.txt  169    20780   Photometric data of asteroids
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Byte-by-byte Description of file: AST_FLUX_V1.txt
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  Bytes  Format Units    Label      Explanations
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  1-  6  A6     ---      Number     Asteroid's number
  8- 23  A16    ---      Name       Asteroid's name
 25- 34  A10    ---      Prov_des   Asteroid's provisional designation
 36- 58  A23    ---      Datetime   Observation datetime (UT)
 60- 70  A11    h:m:s    RA         Right ascension (J2000)
 72- 82  A11    d:m:s    Dec        Declination (J2000)
 84- 93  F10.6  Jy       inFlux     In-band flux density 
 95-103  F9.6   Jy     e_inFlux     In-band flux density uncertainty 
105-114  F10.6  Jy       ccFlux     Color-corrected flux density (1)
116-124  F9.6   Jy     e_ccFlux     Color-corrected flux density uncertainty (1)
126-128  A3     um       band       Observed band
130-137  F8.6   au       Rh         Heliocentric distance
139-146  F8.6   au       Delta      "AKARI-centric" distance
148-152  F5.2   deg      Alpha      Phase angle (Sun-Target-Observer angle)
154-158  F5.2   deg      Elong      Elongation angle (Sun-Observer-Target angle)
160-165  A6     ---      Mode       Observational mode (2) 
167-169  A3     ---      Ref        Reference (3) 
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Note (1): 
   Differences in color between asteroids and the calibration stars (mainly 
   K-, M-, and A-type giant stars) need to be considered, because of the wide 
   bandwidths of observed filters. The filter profiles of the IRC are available 
   at:
   http://www.ir.isas.jaxa.jp/AKARI/Observation/support/IRC/RSRF/
   To obtain color-corrected monochromatic flux density, color corrections 
   were applied which is expressed as a polynomial function of the heliocentric 
   distance of the object. See Usui et al. (2011) for details. Note that the 
   data of color-corrected flux density in shorter wavelength (4 um bands) may 
   have large uncertainty due to contamination of reflected sunlight to thermal 
   flux of asteroid. 

Note (2): 
   Observational modes used for detection of asteroid are described as follows: 
    survey: the all-sky survey
    IRC11,IRC51: the slow-scan observations 
    IRC02: the pointed observations 

Note (3): 
   Reference papers of the data are described as follows: 
    U11: Asteroid Catalog Using AKARI: AKARI/IRC Mid-Infrared Asteroid Survey 
         Usui, F., et al. 2011
    H13: The Asteroid Catalog Using AKARI IRC Slow-Scan Observations 
         Hasegawa, S., et al. 2013
    M14: (25143) Itokawa: The power of radiometric techniques for the 
         interpretation of remote thermal observations in the light of 
         the Hayabusa rendezvous results
         Mueller, T. G., et al. 2014
    M16: Hayabusa-2 Mission Target Asteroid 162173 Ryugu (1999 JU3): Searching 
         for the Object's Spin-Axis Orientation 
         Mueller, T. G., et al. 2016

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History:
  * 27-Sep-2016: Documentation prepared by Fumihiko Usui

Author's address:
    Fumihiko Usui, usui(at)cps-jp.org
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(End)                               Fumihiko Usui [Kobe University]  27-Sep-2016