## example for with AO ##

1. Object/field name :
    AP 13B
2. Magnitude/range of magnitudes in a specified NIR band.
    J=19, H=17, K=15.3, L(3.6 micron)=13.6
3. Are photometric conditions necessary? (Yes/No)
    Yes
4. What is the maximum acceptable seeing size (in arcseconds) in the specified NIR band?
    0.7 arcsecond
5. Do you need AO188? (Yes/No)
    Yes
6. If you need AO188, please describe about the AO guide star as follows.
   i. R (or V if not available) magnitude of your AO guide stars.
	R=12
   ii. Separation between your targets and AO guide stars.
        10 arcseconds  (see the finding chart)
   iii. Maximum acceptable FWHM of the point-spread function (PSF) after the AO correction.
        0.2
   iv. Whether the AO guide star is a point source or not. If you use an extended object or a star associated with nebulousity, you must describe a FWHM of its spatial distribution or contrast between the star and nebulousity.
        Point source

7. Right ascension of the target field in format HHMMSS.SSS
    042900.140
8. Declination of the target field in format (+/-)DDMMSS.SS
    +215521.50
9. Equinox of position in format YYYY.Y
    2000.0
10. Filter(s) for observation.
     J, H, K, LP
11. Pixel scale for observation. (20MAS/52MAS)
     52MAS (JHK), 20MAS (LP)
12. Single frame exposure time in seconds.
     5, 2, 2, 0.5
13. Number of coadds at each dithering position.
     2, 5, 5, 20
14. Dither pattern.
     S5*1, S5*1, S5*1, S5*1
15. Dithering size in arcseconds ("DITH" in the above figures).
    9, 9, 9, 4.5
16. Type of target. Use "OBJ" for objects, "STD" for standards.
    OBJ
17. Name of the target, to be written in the OBJECT field of the image FITS header.
    AP 13B


# standard witout AO#

1. Object/field name :
    FS 140
2. Magnitude/range of magnitudes in a specified NIR band.
    J=10.8, H=10.4, K=10.4, Lp=10.3
3. Are photometric conditions necessary? (Yes/No)
    Yes
4. What is the maximum acceptable seeing size (in arcseconds) in the specified NIR band?
    0.7 arcsecond
5. Do you need AO188? (Yes/No)
    No
6. If you need AO188, please describe about the AO guide star as follows.
   i. R (or V if not available) magnitude of your AO guide stars.
   ii. Separation between your targets and AO guide stars.
   iii. Maximum acceptable FWHM of the point-spread function (PSF) after the AO correction.
   iv. Whether the AO guide star is a point source or not. If you use an extended object or a star associated with nebulousity, you must describe a FWHM of its spatial distribution or contrast between the star and nebulousity.

7. Right ascension of the target field in format HHMMSS.SSS
    052900.140
8. Declination of the target field in format (+/-)DDMMSS.SS
    +210002.50
9. Equinox of position in format YYYY.Y
    2000.0
10. Filter(s) for observation.
     J, H, K, LP
11. Pixel scale for observation. (20MAS/52MAS)
     52MAS (JHK), 20MAS (LP)
12. Single frame exposure time in seconds.
     2, 2, 5, 0.5
13. Number of coadds at each dithering position.
     3, 3, 1, 10
14. Dither pattern.
     S5*1, S5*1, S5*1, S5*1
15. Dithering size in arcseconds ("DITH" in the above figures).
    9, 9, 9, 4.5
16. Type of target. Use "OBJ" for objects, "STD" for standards.
    STD
17. Name of the target, to be written in the OBJECT field of the image FITS header.
    FS140