start:astrofotos:virgocluster_sharpstar_405_20260422_400mal60graxsirilgimp1starnetgimp2.jpg
![SIMPLE = T / file does conform to FITS standard
BITPIX = 16 / number of bits per data pixel
NAXIS = 3 / number of data axes
NAXIS1 = 3814 / length of data axis 1
NAXIS2 = 2390 / length of data axis 2
NAXIS3 = 3 / length of data axis 3
EXTEND = T / FITS dataset may contain extensions
COMMENT FITS (Flexible Image Transport System) format is defined in 'Astronomy
COMMENT and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H
BZERO = 0. / Offset data range to that of unsigned short
BSCALE = 1. / Default scaling factor
PROGRAM = 'Siril 1.4.1' / Software that created this HDU
DATE = '2026-05-09T12:39:35' / UTC date that FITS file was created
ROWORDER= 'TOP-DOWN' / Order of the rows in image array
FOCALLEN= 271.609 / [mm] Focal length
XBINNING= 1 / Camera binning mode
YBINNING= 1 / Camera binning mode
XPIXSZ = 4.59999990463257 / [um] Pixel X axis size
YPIXSZ = 4.59999990463257 / [um] Pixel Y axis size
STACKCNT= 1 / Stack frames
OBJCTRA = '12 30 25.880' / [H M S] Image center Right Ascension
OBJCTDEC= '+12 59 44.591' / [D M S] Image center Declination
RA = 187.6078322215 / [deg] Image center Right Ascension
DEC = 12.9957196381853 / [deg] Image center Declination
CTYPE1 = 'RA---TAN-SIP' / TAN (gnomic) projection + SIP distortions
CTYPE2 = 'DEC--TAN-SIP' / TAN (gnomic) projection + SIP distortions
CUNIT1 = 'deg ' / Unit of coordinates
CUNIT2 = 'deg ' / Unit of coordinates
EQUINOX = 2000. / Equatorial equinox
CRPIX1 = 1907.5 / Axis1 reference pixel
CRPIX2 = 1195.5 / Axis2 reference pixel
CRVAL1 = 187.6078322215 / [deg] Axis1 reference value
CRVAL2 = 12.9957196381854 / [deg] Axis2 reference value
LONPOLE = 180. / Native longitude of celestial pole
CDELT1 = -0.00097039173640588 / [deg] X pixel size
CDELT2 = 0.000970340658429196 / [deg] Y pixel size
PC1_1 = -0.993730423218991 / Linear transformation matrix (1, 1)
PC1_2 = -0.11180271002532 / Linear transformation matrix (1, 2)
PC2_1 = 0.111482463494496 / Linear transformation matrix (2, 1)
PC2_2 = -0.993766401290161 / Linear transformation matrix (2, 2)
A_ORDER = 3 / SIP polynomial degree, axis 1, pixel-to-sky
A_0_0 = 0.
A_1_0 = 0.
A_0_1 = 0.
A_2_0 = 2.29631973768908E-07
A_1_1 = -3.16661530707206E-07
A_0_2 = 9.99498876885144E-09
A_3_0 = -5.44657606126471E-10
A_2_1 = -2.53037586168604E-11
A_1_2 = -5.0334558735337E-10
A_0_3 = -3.55140391078357E-11
B_ORDER = 3 / SIP polynomial degree, axis 2, pixel-to-sky
B_0_0 = 0.
B_1_0 = 0.
B_0_1 = 0.
B_2_0 = -7.69062004474646E-08
B_1_1 = 1.12818763914739E-07
B_0_2 = -4.79992208398082E-07
B_3_0 = -1.29031272028323E-11
B_2_1 = -5.97540790321906E-10
B_1_2 = -6.18304552636071E-11
B_0_3 = -4.03811484109476E-10
AP_ORDER= 3 / SIP polynomial degree, axis 1, sky-to-pixel
AP_0_0 = 0.00100528008989444
AP_1_0 = -6.14325407732874E-06
AP_0_1 = -1.53987853926689E-06
AP_2_0 = -2.32087746751692E-07
AP_1_1 = 3.19927155817197E-07
AP_0_2 = -1.02113292988582E-08
AP_3_0 = 5.49881340309269E-10
AP_2_1 = 2.61123187096622E-11
AP_1_2 = 5.08933785325102E-10
AP_0_3 = 3.64582533367397E-11
BP_ORDER= 3 / SIP polynomial degree, axis 2, sky-to-pixel
BP_0_0 = -0.00131104366546618
BP_1_0 = -1.23191071629197E-06
BP_0_1 = -3.74680066617117E-06
BP_2_0 = 7.80028593013161E-08
BP_1_1 = -1.13636248118533E-07
BP_0_2 = 4.83056937457889E-07
BP_3_0 = 1.33056871857251E-11
BP_2_1 = 6.02936572667654E-10
BP_1_2 = 6.32735350348065E-11
BP_0_3 = 4.07008778843989E-10
PLTSOLVD= T / Siril internal solver
HISTORY Astrometrie / Plate Solving
HISTORY Photometrische Farbkalibrierung (Algorithmus: PCC)...](/lib/exe/fetch.php?cache=&w=900&h=563&tok=277491&media=start:astrofotos:virgocluster_sharpstar_405_20260422_400mal60graxsirilgimp1starnetgimp2.jpg "SIMPLE = T / file does conform to FITS standard
BITPIX = 16 / number of bits per data pixel
NAXIS = 3 / number of data axes
NAXIS1 = 3814 / length of data axis 1
NAXIS2 = 2390 / length of data axis 2
NAXIS3 = 3 / length of data axis 3
EXTEND = T / FITS dataset may contain extensions
COMMENT FITS (Flexible Image Transport System) format is defined in 'Astronomy
COMMENT and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H
BZERO = 0. / Offset data range to that of unsigned short
BSCALE = 1. / Default scaling factor
PROGRAM = 'Siril 1.4.1' / Software that created this HDU
DATE = '2026-05-09T12:39:35' / UTC date that FITS file was created
ROWORDER= 'TOP-DOWN' / Order of the rows in image array
FOCALLEN= 271.609 / [mm] Focal length
XBINNING= 1 / Camera binning mode
YBINNING= 1 / Camera binning mode
XPIXSZ = 4.59999990463257 / [um] Pixel X axis size
YPIXSZ = 4.59999990463257 / [um] Pixel Y axis size
STACKCNT= 1 / Stack frames
OBJCTRA = '12 30 25.880' / [H M S] Image center Right Ascension
OBJCTDEC= '+12 59 44.591' / [D M S] Image center Declination
RA = 187.6078322215 / [deg] Image center Right Ascension
DEC = 12.9957196381853 / [deg] Image center Declination
CTYPE1 = 'RA---TAN-SIP' / TAN (gnomic) projection + SIP distortions
CTYPE2 = 'DEC--TAN-SIP' / TAN (gnomic) projection + SIP distortions
CUNIT1 = 'deg ' / Unit of coordinates
CUNIT2 = 'deg ' / Unit of coordinates
EQUINOX = 2000. / Equatorial equinox
CRPIX1 = 1907.5 / Axis1 reference pixel
CRPIX2 = 1195.5 / Axis2 reference pixel
CRVAL1 = 187.6078322215 / [deg] Axis1 reference value
CRVAL2 = 12.9957196381854 / [deg] Axis2 reference value
LONPOLE = 180. / Native longitude of celestial pole
CDELT1 = -0.00097039173640588 / [deg] X pixel size
CDELT2 = 0.000970340658429196 / [deg] Y pixel size
PC1_1 = -0.993730423218991 / Linear transformation matrix (1, 1)
PC1_2 = -0.11180271002532 / Linear transformation matrix (1, 2)
PC2_1 = 0.111482463494496 / Linear transformation matrix (2, 1)
PC2_2 = -0.993766401290161 / Linear transformation matrix (2, 2)
A_ORDER = 3 / SIP polynomial degree, axis 1, pixel-to-sky
A_0_0 = 0.
A_1_0 = 0.
A_0_1 = 0.
A_2_0 = 2.29631973768908E-07
A_1_1 = -3.16661530707206E-07
A_0_2 = 9.99498876885144E-09
A_3_0 = -5.44657606126471E-10
A_2_1 = -2.53037586168604E-11
A_1_2 = -5.0334558735337E-10
A_0_3 = -3.55140391078357E-11
B_ORDER = 3 / SIP polynomial degree, axis 2, pixel-to-sky
B_0_0 = 0.
B_1_0 = 0.
B_0_1 = 0.
B_2_0 = -7.69062004474646E-08
B_1_1 = 1.12818763914739E-07
B_0_2 = -4.79992208398082E-07
B_3_0 = -1.29031272028323E-11
B_2_1 = -5.97540790321906E-10
B_1_2 = -6.18304552636071E-11
B_0_3 = -4.03811484109476E-10
AP_ORDER= 3 / SIP polynomial degree, axis 1, sky-to-pixel
AP_0_0 = 0.00100528008989444
AP_1_0 = -6.14325407732874E-06
AP_0_1 = -1.53987853926689E-06
AP_2_0 = -2.32087746751692E-07
AP_1_1 = 3.19927155817197E-07
AP_0_2 = -1.02113292988582E-08
AP_3_0 = 5.49881340309269E-10
AP_2_1 = 2.61123187096622E-11
AP_1_2 = 5.08933785325102E-10
AP_0_3 = 3.64582533367397E-11
BP_ORDER= 3 / SIP polynomial degree, axis 2, sky-to-pixel
BP_0_0 = -0.00131104366546618
BP_1_0 = -1.23191071629197E-06
BP_0_1 = -3.74680066617117E-06
BP_2_0 = 7.80028593013161E-08
BP_1_1 = -1.13636248118533E-07
BP_0_2 = 4.83056937457889E-07
BP_3_0 = 1.33056871857251E-11
BP_2_1 = 6.02936572667654E-10
BP_1_2 = 6.32735350348065E-11
BP_0_3 = 4.07008778843989E-10
PLTSOLVD= T / Siril internal solver
HISTORY Astrometrie / Plate Solving
HISTORY Photometrische Farbkalibrierung (Algorithmus: PCC)...")
SIMPLE = T / file does conform to FITS standard
BITPIX = 16 / number of bits per data pixel
NAXIS = 3 / number of data axes
NAXIS1 = 3814 / length of data axis 1
NAXIS2 = 2390 / length of data axis 2
NAXIS3 = 3 / length of data axis 3
EXTEND = T / FITS dataset may contain extensions
COMMENT FITS (Flexible Image Transport System) format is defined in 'Astronomy
COMMENT and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H
BZERO = 0. / Offset data range to that of unsigned short
BSCALE = 1. / Default scaling factor
PROGRAM = 'Siril 1.4.1' / Software that created this HDU
DATE = '2026-05-09T12:39:35' / UTC date that FITS file was created
ROWORDER= 'TOP-DOWN' / Order of the rows in image array
FOCALLEN= 271.609 / [mm] Focal length
XBINNING= 1 / Camera binning mode
YBINNING= 1 / Camera binning mode
XPIXSZ = 4.59999990463257 / [um] Pixel X axis size
YPIXSZ = 4.59999990463257 / [um] Pixel Y axis size
STACKCNT= 1 / Stack frames
OBJCTRA = '12 30 25.880' / [H M S] Image center Right Ascension
OBJCTDEC= '+12 59 44.591' / [D M S] Image center Declination
RA = 187.6078322215 / [deg] Image center Right Ascension
DEC = 12.9957196381853 / [deg] Image center Declination
CTYPE1 = 'RA---TAN-SIP' / TAN (gnomic) projection + SIP distortions
CTYPE2 = 'DEC--TAN-SIP' / TAN (gnomic) projection + SIP distortions
CUNIT1 = 'deg ' / Unit of coordinates
CUNIT2 = 'deg ' / Unit of coordinates
EQUINOX = 2000. / Equatorial equinox
CRPIX1 = 1907.5 / Axis1 reference pixel
CRPIX2 = 1195.5 / Axis2 reference pixel
CRVAL1 = 187.6078322215 / [deg] Axis1 reference value
CRVAL2 = 12.9957196381854 / [deg] Axis2 reference value
LONPOLE = 180. / Native longitude of celestial pole
CDELT1 = -0.00097039173640588 / [deg] X pixel size
CDELT2 = 0.000970340658429196 / [deg] Y pixel size
PC1_1 = -0.993730423218991 / Linear transformation matrix (1, 1)
PC1_2 = -0.11180271002532 / Linear transformation matrix (1, 2)
PC2_1 = 0.111482463494496 / Linear transformation matrix (2, 1)
PC2_2 = -0.993766401290161 / Linear transformation matrix (2, 2)
A_ORDER = 3 / SIP polynomial degree, axis 1, pixel-to-sky
A_0_0 = 0.
A_1_0 = 0.
A_0_1 = 0.
A_2_0 = 2.29631973768908E-07
A_1_1 = -3.16661530707206E-07
A_0_2 = 9.99498876885144E-09
A_3_0 = -5.44657606126471E-10
A_2_1 = -2.53037586168604E-11
A_1_2 = -5.0334558735337E-10
A_0_3 = -3.55140391078357E-11
B_ORDER = 3 / SIP polynomial degree, axis 2, pixel-to-sky
B_0_0 = 0.
B_1_0 = 0.
B_0_1 = 0.
B_2_0 = -7.69062004474646E-08
B_1_1 = 1.12818763914739E-07
B_0_2 = -4.79992208398082E-07
B_3_0 = -1.29031272028323E-11
B_2_1 = -5.97540790321906E-10
B_1_2 = -6.18304552636071E-11
B_0_3 = -4.03811484109476E-10
AP_ORDER= 3 / SIP polynomial degree, axis 1, sky-to-pixel
AP_0_0 = 0.00100528008989444
AP_1_0 = -6.14325407732874E-06
AP_0_1 = -1.53987853926689E-06
AP_2_0 = -2.32087746751692E-07
AP_1_1 = 3.19927155817197E-07
AP_0_2 = -1.02113292988582E-08
AP_3_0 = 5.49881340309269E-10
AP_2_1 = 2.61123187096622E-11
AP_1_2 = 5.08933785325102E-10
AP_0_3 = 3.64582533367397E-11
BP_ORDER= 3 / SIP polynomial degree, axis 2, sky-to-pixel
BP_0_0 = -0.00131104366546618
BP_1_0 = -1.23191071629197E-06
BP_0_1 = -3.74680066617117E-06
BP_2_0 = 7.80028593013161E-08
BP_1_1 = -1.13636248118533E-07
BP_0_2 = 4.83056937457889E-07
BP_3_0 = 1.33056871857251E-11
BP_2_1 = 6.02936572667654E-10
BP_1_2 = 6.32735350348065E-11
BP_0_3 = 4.07008778843989E-10
PLTSOLVD= T / Siril internal solver
HISTORY Astrometrie / Plate Solving
HISTORY Photometrische Farbkalibrierung (Algorithmus: PCC)...
- Date:
- 2026/05/09 14:50
- Filename:
- virgocluster_sharpstar_405_20260422_400mal60graxsirilgimp1starnetgimp2.jpg
- Caption:
- SIMPLE = T / file does conform to FITS standard
BITPIX = 16 / number of bits per data pixel
NAXIS = 3 / number of data axes
NAXIS1 = 3814 / length of data axis 1
NAXIS2 = 2390 / length of data axis 2
NAXIS3 = 3 / length of data axis 3
EXTEND = T / FITS dataset may contain extensions
COMMENT FITS (Flexible Image Transport System) format is defined in 'Astronomy
COMMENT and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H
BZERO = 0. / Offset data range to that of unsigned short
BSCALE = 1. / Default scaling factor
PROGRAM = 'Siril 1.4.1' / Software that created this HDU
DATE = '2026-05-09T12:39:35' / UTC date that FITS file was created
ROWORDER= 'TOP-DOWN' / Order of the rows in image array
FOCALLEN= 271.609 / [mm] Focal length
XBINNING= 1 / Camera binning mode
YBINNING= 1 / Camera binning mode
XPIXSZ = 4.59999990463257 / [um] Pixel X axis size
YPIXSZ = 4.59999990463257 / [um] Pixel Y axis size
STACKCNT= 1 / Stack frames
OBJCTRA = '12 30 25.880' / [H M S] Image center Right Ascension
OBJCTDEC= '+12 59 44.591' / [D M S] Image center Declination
RA = 187.6078322215 / [deg] Image center Right Ascension
DEC = 12.9957196381853 / [deg] Image center Declination
CTYPE1 = 'RA---TAN-SIP' / TAN (gnomic) projection + SIP distortions
CTYPE2 = 'DEC--TAN-SIP' / TAN (gnomic) projection + SIP distortions
CUNIT1 = 'deg ' / Unit of coordinates
CUNIT2 = 'deg ' / Unit of coordinates
EQUINOX = 2000. / Equatorial equinox
CRPIX1 = 1907.5 / Axis1 reference pixel
CRPIX2 = 1195.5 / Axis2 reference pixel
CRVAL1 = 187.6078322215 / [deg] Axis1 reference value
CRVAL2 = 12.9957196381854 / [deg] Axis2 reference value
LONPOLE = 180. / Native longitude of celestial pole
CDELT1 = -0.00097039173640588 / [deg] X pixel size
CDELT2 = 0.000970340658429196 / [deg] Y pixel size
PC1_1 = -0.993730423218991 / Linear transformation matrix (1, 1)
PC1_2 = -0.11180271002532 / Linear transformation matrix (1, 2)
PC2_1 = 0.111482463494496 / Linear transformation matrix (2, 1)
PC2_2 = -0.993766401290161 / Linear transformation matrix (2, 2)
A_ORDER = 3 / SIP polynomial degree, axis 1, pixel-to-sky
A_0_0 = 0.
A_1_0 = 0.
A_0_1 = 0.
A_2_0 = 2.29631973768908E-07
A_1_1 = -3.16661530707206E-07
A_0_2 = 9.99498876885144E-09
A_3_0 = -5.44657606126471E-10
A_2_1 = -2.53037586168604E-11
A_1_2 = -5.0334558735337E-10
A_0_3 = -3.55140391078357E-11
B_ORDER = 3 / SIP polynomial degree, axis 2, pixel-to-sky
B_0_0 = 0.
B_1_0 = 0.
B_0_1 = 0.
B_2_0 = -7.69062004474646E-08
B_1_1 = 1.12818763914739E-07
B_0_2 = -4.79992208398082E-07
B_3_0 = -1.29031272028323E-11
B_2_1 = -5.97540790321906E-10
B_1_2 = -6.18304552636071E-11
B_0_3 = -4.03811484109476E-10
AP_ORDER= 3 / SIP polynomial degree, axis 1, sky-to-pixel
AP_0_0 = 0.00100528008989444
AP_1_0 = -6.14325407732874E-06
AP_0_1 = -1.53987853926689E-06
AP_2_0 = -2.32087746751692E-07
AP_1_1 = 3.19927155817197E-07
AP_0_2 = -1.02113292988582E-08
AP_3_0 = 5.49881340309269E-10
AP_2_1 = 2.61123187096622E-11
AP_1_2 = 5.08933785325102E-10
AP_0_3 = 3.64582533367397E-11
BP_ORDER= 3 / SIP polynomial degree, axis 2, sky-to-pixel
BP_0_0 = -0.00131104366546618
BP_1_0 = -1.23191071629197E-06
BP_0_1 = -3.74680066617117E-06
BP_2_0 = 7.80028593013161E-08
BP_1_1 = -1.13636248118533E-07
BP_0_2 = 4.83056937457889E-07
BP_3_0 = 1.33056871857251E-11
BP_2_1 = 6.02936572667654E-10
BP_1_2 = 6.32735350348065E-11
BP_0_3 = 4.07008778843989E-10
PLTSOLVD= T / Siril internal solver
HISTORY Astrometrie / Plate Solving
HISTORY Photometrische Farbkalibrierung (Algorithmus: PCC)
END
- Copyright:
- Siril v1.4.1
- Format:
- JPEG
- Size:
- 2MB
- Width:
- 3814
- Height:
- 2390
← Back to start:astrofotos:winter2526
![SIMPLE = T / file does conform to FITS standard
BITPIX = 16 / number of bits per data pixel
NAXIS = 3 / number of data axes
NAXIS1 = 3814 / length of data axis 1
NAXIS2 = 2390 / length of data axis 2
NAXIS3 = 3 / length of data axis 3
EXTEND = T / FITS dataset may contain extensions
COMMENT FITS (Flexible Image Transport System) format is defined in 'Astronomy
COMMENT and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H
BZERO = 0. / Offset data range to that of unsigned short
BSCALE = 1. / Default scaling factor
PROGRAM = 'Siril 1.4.1' / Software that created this HDU
DATE = '2026-05-09T12:39:35' / UTC date that FITS file was created
ROWORDER= 'TOP-DOWN' / Order of the rows in image array
FOCALLEN= 271.609 / [mm] Focal length
XBINNING= 1 / Camera binning mode
YBINNING= 1 / Camera binning mode
XPIXSZ = 4.59999990463257 / [um] Pixel X axis size
YPIXSZ = 4.59999990463257 / [um] Pixel Y axis size
STACKCNT= 1 / Stack frames
OBJCTRA = '12 30 25.880' / [H M S] Image center Right Ascension
OBJCTDEC= '+12 59 44.591' / [D M S] Image center Declination
RA = 187.6078322215 / [deg] Image center Right Ascension
DEC = 12.9957196381853 / [deg] Image center Declination
CTYPE1 = 'RA---TAN-SIP' / TAN (gnomic) projection + SIP distortions
CTYPE2 = 'DEC--TAN-SIP' / TAN (gnomic) projection + SIP distortions
CUNIT1 = 'deg ' / Unit of coordinates
CUNIT2 = 'deg ' / Unit of coordinates
EQUINOX = 2000. / Equatorial equinox
CRPIX1 = 1907.5 / Axis1 reference pixel
CRPIX2 = 1195.5 / Axis2 reference pixel
CRVAL1 = 187.6078322215 / [deg] Axis1 reference value
CRVAL2 = 12.9957196381854 / [deg] Axis2 reference value
LONPOLE = 180. / Native longitude of celestial pole
CDELT1 = -0.00097039173640588 / [deg] X pixel size
CDELT2 = 0.000970340658429196 / [deg] Y pixel size
PC1_1 = -0.993730423218991 / Linear transformation matrix (1, 1)
PC1_2 = -0.11180271002532 / Linear transformation matrix (1, 2)
PC2_1 = 0.111482463494496 / Linear transformation matrix (2, 1)
PC2_2 = -0.993766401290161 / Linear transformation matrix (2, 2)
A_ORDER = 3 / SIP polynomial degree, axis 1, pixel-to-sky
A_0_0 = 0.
A_1_0 = 0.
A_0_1 = 0.
A_2_0 = 2.29631973768908E-07
A_1_1 = -3.16661530707206E-07
A_0_2 = 9.99498876885144E-09
A_3_0 = -5.44657606126471E-10
A_2_1 = -2.53037586168604E-11
A_1_2 = -5.0334558735337E-10
A_0_3 = -3.55140391078357E-11
B_ORDER = 3 / SIP polynomial degree, axis 2, pixel-to-sky
B_0_0 = 0.
B_1_0 = 0.
B_0_1 = 0.
B_2_0 = -7.69062004474646E-08
B_1_1 = 1.12818763914739E-07
B_0_2 = -4.79992208398082E-07
B_3_0 = -1.29031272028323E-11
B_2_1 = -5.97540790321906E-10
B_1_2 = -6.18304552636071E-11
B_0_3 = -4.03811484109476E-10
AP_ORDER= 3 / SIP polynomial degree, axis 1, sky-to-pixel
AP_0_0 = 0.00100528008989444
AP_1_0 = -6.14325407732874E-06
AP_0_1 = -1.53987853926689E-06
AP_2_0 = -2.32087746751692E-07
AP_1_1 = 3.19927155817197E-07
AP_0_2 = -1.02113292988582E-08
AP_3_0 = 5.49881340309269E-10
AP_2_1 = 2.61123187096622E-11
AP_1_2 = 5.08933785325102E-10
AP_0_3 = 3.64582533367397E-11
BP_ORDER= 3 / SIP polynomial degree, axis 2, sky-to-pixel
BP_0_0 = -0.00131104366546618
BP_1_0 = -1.23191071629197E-06
BP_0_1 = -3.74680066617117E-06
BP_2_0 = 7.80028593013161E-08
BP_1_1 = -1.13636248118533E-07
BP_0_2 = 4.83056937457889E-07
BP_3_0 = 1.33056871857251E-11
BP_2_1 = 6.02936572667654E-10
BP_1_2 = 6.32735350348065E-11
BP_0_3 = 4.07008778843989E-10
PLTSOLVD= T / Siril internal solver
HISTORY Astrometrie / Plate Solving
HISTORY Photometrische Farbkalibrierung (Algorithmus: PCC)...](/lib/exe/fetch.php?cache=&media=start:astrofotos:virgocluster_sharpstar_405_20260422_400mal60graxsirilgimp1starnetgimp2.jpg "SIMPLE = T / file does conform to FITS standard
BITPIX = 16 / number of bits per data pixel
NAXIS = 3 / number of data axes
NAXIS1 = 3814 / length of data axis 1
NAXIS2 = 2390 / length of data axis 2
NAXIS3 = 3 / length of data axis 3
EXTEND = T / FITS dataset may contain extensions
COMMENT FITS (Flexible Image Transport System) format is defined in 'Astronomy
COMMENT and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H
BZERO = 0. / Offset data range to that of unsigned short
BSCALE = 1. / Default scaling factor
PROGRAM = 'Siril 1.4.1' / Software that created this HDU
DATE = '2026-05-09T12:39:35' / UTC date that FITS file was created
ROWORDER= 'TOP-DOWN' / Order of the rows in image array
FOCALLEN= 271.609 / [mm] Focal length
XBINNING= 1 / Camera binning mode
YBINNING= 1 / Camera binning mode
XPIXSZ = 4.59999990463257 / [um] Pixel X axis size
YPIXSZ = 4.59999990463257 / [um] Pixel Y axis size
STACKCNT= 1 / Stack frames
OBJCTRA = '12 30 25.880' / [H M S] Image center Right Ascension
OBJCTDEC= '+12 59 44.591' / [D M S] Image center Declination
RA = 187.6078322215 / [deg] Image center Right Ascension
DEC = 12.9957196381853 / [deg] Image center Declination
CTYPE1 = 'RA---TAN-SIP' / TAN (gnomic) projection + SIP distortions
CTYPE2 = 'DEC--TAN-SIP' / TAN (gnomic) projection + SIP distortions
CUNIT1 = 'deg ' / Unit of coordinates
CUNIT2 = 'deg ' / Unit of coordinates
EQUINOX = 2000. / Equatorial equinox
CRPIX1 = 1907.5 / Axis1 reference pixel
CRPIX2 = 1195.5 / Axis2 reference pixel
CRVAL1 = 187.6078322215 / [deg] Axis1 reference value
CRVAL2 = 12.9957196381854 / [deg] Axis2 reference value
LONPOLE = 180. / Native longitude of celestial pole
CDELT1 = -0.00097039173640588 / [deg] X pixel size
CDELT2 = 0.000970340658429196 / [deg] Y pixel size
PC1_1 = -0.993730423218991 / Linear transformation matrix (1, 1)
PC1_2 = -0.11180271002532 / Linear transformation matrix (1, 2)
PC2_1 = 0.111482463494496 / Linear transformation matrix (2, 1)
PC2_2 = -0.993766401290161 / Linear transformation matrix (2, 2)
A_ORDER = 3 / SIP polynomial degree, axis 1, pixel-to-sky
A_0_0 = 0.
A_1_0 = 0.
A_0_1 = 0.
A_2_0 = 2.29631973768908E-07
A_1_1 = -3.16661530707206E-07
A_0_2 = 9.99498876885144E-09
A_3_0 = -5.44657606126471E-10
A_2_1 = -2.53037586168604E-11
A_1_2 = -5.0334558735337E-10
A_0_3 = -3.55140391078357E-11
B_ORDER = 3 / SIP polynomial degree, axis 2, pixel-to-sky
B_0_0 = 0.
B_1_0 = 0.
B_0_1 = 0.
B_2_0 = -7.69062004474646E-08
B_1_1 = 1.12818763914739E-07
B_0_2 = -4.79992208398082E-07
B_3_0 = -1.29031272028323E-11
B_2_1 = -5.97540790321906E-10
B_1_2 = -6.18304552636071E-11
B_0_3 = -4.03811484109476E-10
AP_ORDER= 3 / SIP polynomial degree, axis 1, sky-to-pixel
AP_0_0 = 0.00100528008989444
AP_1_0 = -6.14325407732874E-06
AP_0_1 = -1.53987853926689E-06
AP_2_0 = -2.32087746751692E-07
AP_1_1 = 3.19927155817197E-07
AP_0_2 = -1.02113292988582E-08
AP_3_0 = 5.49881340309269E-10
AP_2_1 = 2.61123187096622E-11
AP_1_2 = 5.08933785325102E-10
AP_0_3 = 3.64582533367397E-11
BP_ORDER= 3 / SIP polynomial degree, axis 2, sky-to-pixel
BP_0_0 = -0.00131104366546618
BP_1_0 = -1.23191071629197E-06
BP_0_1 = -3.74680066617117E-06
BP_2_0 = 7.80028593013161E-08
BP_1_1 = -1.13636248118533E-07
BP_0_2 = 4.83056937457889E-07
BP_3_0 = 1.33056871857251E-11
BP_2_1 = 6.02936572667654E-10
BP_1_2 = 6.32735350348065E-11
BP_0_3 = 4.07008778843989E-10
PLTSOLVD= T / Siril internal solver
HISTORY Astrometrie / Plate Solving
HISTORY Photometrische Farbkalibrierung (Algorithmus: PCC)...")