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%TOC% ---+ Instructions to generate fits: Typical header with required keywords/values: SIMPLE = T / BITPIX = -32 /IEEE real 4. Other values: 16, 32, 64, -64 /for 16, 32, 64: use BSCALE and BZERO keys. NAXIS = 3 /datacube NAXIS1 = 512 /size 1st axis. Possible values: 512, 1024, 2048 NAXIS2 = 512 /size 2nd axis, see above H & K band: resolution ~100, N band (8.7-13.1mic) band: R~30. The 3rd axis is the spectral axis. 20 spectral elements are reasonable: NAXIS3 = 20 /size 3rd (spectral) axis. 20 spectral elements , Values of the two spatial axis: Pixels scale is 0.1 millisec for H and K images/cubes, 1mas /pixel for N band CRVAL1 = 0 / center is at 0 offset on sky (Right Ascension) CRPIX1 = 256 / reference pixel would be pixel 256 if NAXIS1=512 CDELT1 = -0.4848136811095E-10 / increment between pixels is is 0.1 millisec (IN RADIANS: MANDATORY),and is 'astronomy oriented (negative)' CRVAL2 = 0 / center is at 0 DEC offset on sky CRPIX2 = 256 / reference pixel is 256 in Delta CDELT2 = 0.4848136811095E-10 / increment is 0.1 millisec. values for the spectral axis: CTYPE3 = 'WAVELENGTH' / MANDATORY: means that Cxxxx3 are in Microns CRPIX3 = 1 / reference pixel(channel) is 1 on 3rd axis CRVAL3 = 2.2 / 2.2 microns for this pix/channel CDELT3 = 0.02 / microns channel width Other mandatory keywords MAGV = 3.3 / magnitude V of star ( for AO) MAGK = 6.6 /K mag for FT MAGH = 4.4 /H mag for FT TOTFLUX = 2.5434E12 /Total flux in the image or cube. The image's values can be in any unit. More keywords are recomended that can give a better view of what is inside the fits file: OBJECT = 'HD 86554' / name (for bookeeping) RA = 0.6800000000000E+02 / Right Ascension RADIANS (for bookeeping) DEC = 0.2600000000000E+02 / Declination RADIANS (for bookeeping) EPOCH = 2008 / Epoch (for bookeeping) EQUINOX = 2008 / Equinox (for bookeeping) ORIGIN = 'MY Simulator' / DATE-OBS= '2005-12-02T00:00:00.00' / Date image/cube produced. ---+ Interferometers configuration: This first table contains the proposed configurations. The spectral resolution is here to improve the (u,v) coverage. For CHARA I am waiting for John's response. | Config # |Interferometer | Number of telescopes | Time for one calibrate point | Spectral resolution |Filter | | 1| Gravity/Matisse/VSI | 4 T | 40 mn | 7 spectral channels |H,K,N| |2| VSI | 6 T | 40 mn | 7 spectral channels |H,K| |3| MROI| 6 T (3x4) | 20 mn | 7 spectral channels |H,K| |4| CHARA| 6 T | | || ---+ Information on images: |Topic | Author | Band | Info/comment| Oifits Generated (Y,N) | Image reconstruction | | AGN| S. Hoenig | | No inclination, low contrast except N, asked for more||| | | |H | Config 1(4T VLTI) |No |No| | | |K | Config 2(6T VLTI) |No |No| | | |N | Config 3(6T MROI) |No |No| | Planet in disk | H. Jang-Condell | | Low contrast, asked for images with gaps| || | | |H | Config 1(4T VLTI) |No |No| | | |K | Config 2(6T VLTI) |No |No| | | |N | Config 3(6T MROI) |No |No| | Supergiant | A. Chiavassa || Convection cells||| | | |H | Config 1(4T VLTI) |No |No| | | |K | Config 2(6T VLTI) |No |No| | | |N | Config 3(6T MROI) |No |No| |Evolved star | T. Verhoelst|| Low contrast envelop shells, circular symmetry, asked for more |No |No| | | |H | Config 1(4T VLTI) |No |No| | | |K | Config 2(6T VLTI) |No |No| | | |N | Config 3(6T MROI) |No |No| -- Main.JeanPhilippeBerger - 29 Apr 2009
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Topic revision: r1 - 2009-04-29
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JeanPhilippeBerger
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