start:astrofotos:m3_pds_585_20260508_160mal60_graxsiril_gimp.jpg
![SIMPLE = T / file does conform to FITS standard
BITPIX = 16 / number of bits per data pixel
NAXIS = 3 / number of data axes
NAXIS1 = 2915 / length of data axis 1
NAXIS2 = 1889 / 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 = '2026-05-09T11:57:02' / UTC date that FITS file was created
ROWORDER= 'TOP-DOWN' / Order of the rows in image array
FOCALLEN= 628.065 / [mm] Focal length
XBINNING= 1 / Camera binning mode
YBINNING= 1 / Camera binning mode
XPIXSZ = 2.9 / [um] Pixel X axis size
YPIXSZ = 2.9 / [um] Pixel Y axis size
STACKCNT= 1 / Stack frames
OBJCTRA = '13 41 19.091' / [H M S] Image center Right Ascension
OBJCTDEC= '+28 22 21.945' / [D M S] Image center Declination
RA = 205.329544402769 / [deg] Image center Right Ascension
DEC = 28.37276239558 / [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 = 1458. / Axis1 reference pixel
CRPIX2 = 945. / Axis2 reference pixel
CRVAL1 = 205.329544402769 / [deg] Axis1 reference value
CRVAL2 = 28.37276239558 / [deg] Axis2 reference value
LONPOLE = 180. / Native longitude of celestial pole
CDELT1 = -0.000264554207781575 / [deg] X pixel size
CDELT2 = 0.000264556257393594 / [deg] Y pixel size
PC1_1 = -0.935506306786633 / Linear transformation matrix (1, 1)
PC1_2 = 0.35330999131419 / Linear transformation matrix (1, 2)
PC2_1 = -0.353414854809899 / Linear transformation matrix (2, 1)
PC2_2 = -0.935466696574334 / 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 = 2.36029914046333E-07
A_1_1 = -1.25826541374622E-07
A_0_2 = 4.68942286444862E-07
A_3_0 = -3.09614255098055E-10
A_2_1 = 2.00399538313748E-10
A_1_2 = -6.38796617775035E-10
A_0_3 = -2.74530336624958E-10
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 = -1.01125176052818E-07
B_1_1 = 2.572381192173E-07
B_0_2 = 1.80288273265436E-07
B_3_0 = 4.96562906615543E-11
B_2_1 = -4.52395737785131E-10
B_1_2 = -1.30688345556544E-10
B_0_3 = -2.8697648720682E-10
AP_ORDER= 3 / SIP polynomial degree, axis 1, sky-to-pixel
AP_0_0 = 0.00060924962662183
AP_1_0 = -8.07178935247066E-07
AP_0_1 = -9.66095599222222E-08
AP_2_0 = -2.3730037040633E-07
AP_1_1 = 1.26709209898822E-07
AP_0_2 = -4.7079830328754E-07
AP_3_0 = 3.10810569553272E-10
AP_2_1 = -2.01303888849744E-10
AP_1_2 = 6.41654931565699E-10
AP_0_3 = 2.75188359220988E-10
BP_ORDER= 3 / SIP polynomial degree, axis 2, sky-to-pixel
BP_0_0 = -7.96787195162728E-05
BP_1_0 = 7.44638342121251E-08
BP_0_1 = -5.90467481687007E-07
BP_2_0 = 1.01500261205451E-07
BP_1_1 = -2.58495257985211E-07
BP_0_2 = -1.80527378330435E-07
BP_3_0 = -4.99345075601809E-11
BP_2_1 = 4.54030025854777E-10
BP_1_2 = 1.30981094750333E-10
BP_0_3 = 2.88088537738887E-10
PLTSOLVD= T / Siril internal solver
HISTORY Astrometrie / Plate Solving
HISTORY SCNR (Typ=Durchschnittlich neutral, St rke=1.00, Erhaltung=true)
HISTORY Photometrische Farbkalibrierung (Algorithmus: PCC)...](/lib/exe/fetch.php?cache=&w=900&h=583&tok=228835&media=start:astrofotos:m3_pds_585_20260508_160mal60_graxsiril_gimp.jpg "SIMPLE = T / file does conform to FITS standard
BITPIX = 16 / number of bits per data pixel
NAXIS = 3 / number of data axes
NAXIS1 = 2915 / length of data axis 1
NAXIS2 = 1889 / 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 = '2026-05-09T11:57:02' / UTC date that FITS file was created
ROWORDER= 'TOP-DOWN' / Order of the rows in image array
FOCALLEN= 628.065 / [mm] Focal length
XBINNING= 1 / Camera binning mode
YBINNING= 1 / Camera binning mode
XPIXSZ = 2.9 / [um] Pixel X axis size
YPIXSZ = 2.9 / [um] Pixel Y axis size
STACKCNT= 1 / Stack frames
OBJCTRA = '13 41 19.091' / [H M S] Image center Right Ascension
OBJCTDEC= '+28 22 21.945' / [D M S] Image center Declination
RA = 205.329544402769 / [deg] Image center Right Ascension
DEC = 28.37276239558 / [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 = 1458. / Axis1 reference pixel
CRPIX2 = 945. / Axis2 reference pixel
CRVAL1 = 205.329544402769 / [deg] Axis1 reference value
CRVAL2 = 28.37276239558 / [deg] Axis2 reference value
LONPOLE = 180. / Native longitude of celestial pole
CDELT1 = -0.000264554207781575 / [deg] X pixel size
CDELT2 = 0.000264556257393594 / [deg] Y pixel size
PC1_1 = -0.935506306786633 / Linear transformation matrix (1, 1)
PC1_2 = 0.35330999131419 / Linear transformation matrix (1, 2)
PC2_1 = -0.353414854809899 / Linear transformation matrix (2, 1)
PC2_2 = -0.935466696574334 / 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 = 2.36029914046333E-07
A_1_1 = -1.25826541374622E-07
A_0_2 = 4.68942286444862E-07
A_3_0 = -3.09614255098055E-10
A_2_1 = 2.00399538313748E-10
A_1_2 = -6.38796617775035E-10
A_0_3 = -2.74530336624958E-10
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 = -1.01125176052818E-07
B_1_1 = 2.572381192173E-07
B_0_2 = 1.80288273265436E-07
B_3_0 = 4.96562906615543E-11
B_2_1 = -4.52395737785131E-10
B_1_2 = -1.30688345556544E-10
B_0_3 = -2.8697648720682E-10
AP_ORDER= 3 / SIP polynomial degree, axis 1, sky-to-pixel
AP_0_0 = 0.00060924962662183
AP_1_0 = -8.07178935247066E-07
AP_0_1 = -9.66095599222222E-08
AP_2_0 = -2.3730037040633E-07
AP_1_1 = 1.26709209898822E-07
AP_0_2 = -4.7079830328754E-07
AP_3_0 = 3.10810569553272E-10
AP_2_1 = -2.01303888849744E-10
AP_1_2 = 6.41654931565699E-10
AP_0_3 = 2.75188359220988E-10
BP_ORDER= 3 / SIP polynomial degree, axis 2, sky-to-pixel
BP_0_0 = -7.96787195162728E-05
BP_1_0 = 7.44638342121251E-08
BP_0_1 = -5.90467481687007E-07
BP_2_0 = 1.01500261205451E-07
BP_1_1 = -2.58495257985211E-07
BP_0_2 = -1.80527378330435E-07
BP_3_0 = -4.99345075601809E-11
BP_2_1 = 4.54030025854777E-10
BP_1_2 = 1.30981094750333E-10
BP_0_3 = 2.88088537738887E-10
PLTSOLVD= T / Siril internal solver
HISTORY Astrometrie / Plate Solving
HISTORY SCNR (Typ=Durchschnittlich neutral, St rke=1.00, Erhaltung=true)
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 = 2915 / length of data axis 1
NAXIS2 = 1889 / 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 = '2026-05-09T11:57:02' / UTC date that FITS file was created
ROWORDER= 'TOP-DOWN' / Order of the rows in image array
FOCALLEN= 628.065 / [mm] Focal length
XBINNING= 1 / Camera binning mode
YBINNING= 1 / Camera binning mode
XPIXSZ = 2.9 / [um] Pixel X axis size
YPIXSZ = 2.9 / [um] Pixel Y axis size
STACKCNT= 1 / Stack frames
OBJCTRA = '13 41 19.091' / [H M S] Image center Right Ascension
OBJCTDEC= '+28 22 21.945' / [D M S] Image center Declination
RA = 205.329544402769 / [deg] Image center Right Ascension
DEC = 28.37276239558 / [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 = 1458. / Axis1 reference pixel
CRPIX2 = 945. / Axis2 reference pixel
CRVAL1 = 205.329544402769 / [deg] Axis1 reference value
CRVAL2 = 28.37276239558 / [deg] Axis2 reference value
LONPOLE = 180. / Native longitude of celestial pole
CDELT1 = -0.000264554207781575 / [deg] X pixel size
CDELT2 = 0.000264556257393594 / [deg] Y pixel size
PC1_1 = -0.935506306786633 / Linear transformation matrix (1, 1)
PC1_2 = 0.35330999131419 / Linear transformation matrix (1, 2)
PC2_1 = -0.353414854809899 / Linear transformation matrix (2, 1)
PC2_2 = -0.935466696574334 / 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 = 2.36029914046333E-07
A_1_1 = -1.25826541374622E-07
A_0_2 = 4.68942286444862E-07
A_3_0 = -3.09614255098055E-10
A_2_1 = 2.00399538313748E-10
A_1_2 = -6.38796617775035E-10
A_0_3 = -2.74530336624958E-10
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 = -1.01125176052818E-07
B_1_1 = 2.572381192173E-07
B_0_2 = 1.80288273265436E-07
B_3_0 = 4.96562906615543E-11
B_2_1 = -4.52395737785131E-10
B_1_2 = -1.30688345556544E-10
B_0_3 = -2.8697648720682E-10
AP_ORDER= 3 / SIP polynomial degree, axis 1, sky-to-pixel
AP_0_0 = 0.00060924962662183
AP_1_0 = -8.07178935247066E-07
AP_0_1 = -9.66095599222222E-08
AP_2_0 = -2.3730037040633E-07
AP_1_1 = 1.26709209898822E-07
AP_0_2 = -4.7079830328754E-07
AP_3_0 = 3.10810569553272E-10
AP_2_1 = -2.01303888849744E-10
AP_1_2 = 6.41654931565699E-10
AP_0_3 = 2.75188359220988E-10
BP_ORDER= 3 / SIP polynomial degree, axis 2, sky-to-pixel
BP_0_0 = -7.96787195162728E-05
BP_1_0 = 7.44638342121251E-08
BP_0_1 = -5.90467481687007E-07
BP_2_0 = 1.01500261205451E-07
BP_1_1 = -2.58495257985211E-07
BP_0_2 = -1.80527378330435E-07
BP_3_0 = -4.99345075601809E-11
BP_2_1 = 4.54030025854777E-10
BP_1_2 = 1.30981094750333E-10
BP_0_3 = 2.88088537738887E-10
PLTSOLVD= T / Siril internal solver
HISTORY Astrometrie / Plate Solving
HISTORY SCNR (Typ=Durchschnittlich neutral, St rke=1.00, Erhaltung=true)
HISTORY Photometrische Farbkalibrierung (Algorithmus: PCC)...
- Date:
- 2026/05/09 14:03
- Filename:
- m3_pds_585_20260508_160mal60_graxsiril_gimp.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 = 2915 / length of data axis 1
NAXIS2 = 1889 / 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 = '2026-05-09T11:57:02' / UTC date that FITS file was created
ROWORDER= 'TOP-DOWN' / Order of the rows in image array
FOCALLEN= 628.065 / [mm] Focal length
XBINNING= 1 / Camera binning mode
YBINNING= 1 / Camera binning mode
XPIXSZ = 2.9 / [um] Pixel X axis size
YPIXSZ = 2.9 / [um] Pixel Y axis size
STACKCNT= 1 / Stack frames
OBJCTRA = '13 41 19.091' / [H M S] Image center Right Ascension
OBJCTDEC= '+28 22 21.945' / [D M S] Image center Declination
RA = 205.329544402769 / [deg] Image center Right Ascension
DEC = 28.37276239558 / [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 = 1458. / Axis1 reference pixel
CRPIX2 = 945. / Axis2 reference pixel
CRVAL1 = 205.329544402769 / [deg] Axis1 reference value
CRVAL2 = 28.37276239558 / [deg] Axis2 reference value
LONPOLE = 180. / Native longitude of celestial pole
CDELT1 = -0.000264554207781575 / [deg] X pixel size
CDELT2 = 0.000264556257393594 / [deg] Y pixel size
PC1_1 = -0.935506306786633 / Linear transformation matrix (1, 1)
PC1_2 = 0.35330999131419 / Linear transformation matrix (1, 2)
PC2_1 = -0.353414854809899 / Linear transformation matrix (2, 1)
PC2_2 = -0.935466696574334 / 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 = 2.36029914046333E-07
A_1_1 = -1.25826541374622E-07
A_0_2 = 4.68942286444862E-07
A_3_0 = -3.09614255098055E-10
A_2_1 = 2.00399538313748E-10
A_1_2 = -6.38796617775035E-10
A_0_3 = -2.74530336624958E-10
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 = -1.01125176052818E-07
B_1_1 = 2.572381192173E-07
B_0_2 = 1.80288273265436E-07
B_3_0 = 4.96562906615543E-11
B_2_1 = -4.52395737785131E-10
B_1_2 = -1.30688345556544E-10
B_0_3 = -2.8697648720682E-10
AP_ORDER= 3 / SIP polynomial degree, axis 1, sky-to-pixel
AP_0_0 = 0.00060924962662183
AP_1_0 = -8.07178935247066E-07
AP_0_1 = -9.66095599222222E-08
AP_2_0 = -2.3730037040633E-07
AP_1_1 = 1.26709209898822E-07
AP_0_2 = -4.7079830328754E-07
AP_3_0 = 3.10810569553272E-10
AP_2_1 = -2.01303888849744E-10
AP_1_2 = 6.41654931565699E-10
AP_0_3 = 2.75188359220988E-10
BP_ORDER= 3 / SIP polynomial degree, axis 2, sky-to-pixel
BP_0_0 = -7.96787195162728E-05
BP_1_0 = 7.44638342121251E-08
BP_0_1 = -5.90467481687007E-07
BP_2_0 = 1.01500261205451E-07
BP_1_1 = -2.58495257985211E-07
BP_0_2 = -1.80527378330435E-07
BP_3_0 = -4.99345075601809E-11
BP_2_1 = 4.54030025854777E-10
BP_1_2 = 1.30981094750333E-10
BP_0_3 = 2.88088537738887E-10
PLTSOLVD= T / Siril internal solver
HISTORY Astrometrie / Plate Solving
HISTORY SCNR (Typ=Durchschnittlich neutral, St rke=1.00, Erhaltung=true)
HISTORY Photometrische Farbkalibrierung (Algorithmus: PCC)
END
- Copyright:
- Siril v1.4.1
- Format:
- JPEG
- Size:
- 1MB
- Width:
- 2915
- Height:
- 1889
← 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 = 2915 / length of data axis 1
NAXIS2 = 1889 / 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 = '2026-05-09T11:57:02' / UTC date that FITS file was created
ROWORDER= 'TOP-DOWN' / Order of the rows in image array
FOCALLEN= 628.065 / [mm] Focal length
XBINNING= 1 / Camera binning mode
YBINNING= 1 / Camera binning mode
XPIXSZ = 2.9 / [um] Pixel X axis size
YPIXSZ = 2.9 / [um] Pixel Y axis size
STACKCNT= 1 / Stack frames
OBJCTRA = '13 41 19.091' / [H M S] Image center Right Ascension
OBJCTDEC= '+28 22 21.945' / [D M S] Image center Declination
RA = 205.329544402769 / [deg] Image center Right Ascension
DEC = 28.37276239558 / [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 = 1458. / Axis1 reference pixel
CRPIX2 = 945. / Axis2 reference pixel
CRVAL1 = 205.329544402769 / [deg] Axis1 reference value
CRVAL2 = 28.37276239558 / [deg] Axis2 reference value
LONPOLE = 180. / Native longitude of celestial pole
CDELT1 = -0.000264554207781575 / [deg] X pixel size
CDELT2 = 0.000264556257393594 / [deg] Y pixel size
PC1_1 = -0.935506306786633 / Linear transformation matrix (1, 1)
PC1_2 = 0.35330999131419 / Linear transformation matrix (1, 2)
PC2_1 = -0.353414854809899 / Linear transformation matrix (2, 1)
PC2_2 = -0.935466696574334 / 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 = 2.36029914046333E-07
A_1_1 = -1.25826541374622E-07
A_0_2 = 4.68942286444862E-07
A_3_0 = -3.09614255098055E-10
A_2_1 = 2.00399538313748E-10
A_1_2 = -6.38796617775035E-10
A_0_3 = -2.74530336624958E-10
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 = -1.01125176052818E-07
B_1_1 = 2.572381192173E-07
B_0_2 = 1.80288273265436E-07
B_3_0 = 4.96562906615543E-11
B_2_1 = -4.52395737785131E-10
B_1_2 = -1.30688345556544E-10
B_0_3 = -2.8697648720682E-10
AP_ORDER= 3 / SIP polynomial degree, axis 1, sky-to-pixel
AP_0_0 = 0.00060924962662183
AP_1_0 = -8.07178935247066E-07
AP_0_1 = -9.66095599222222E-08
AP_2_0 = -2.3730037040633E-07
AP_1_1 = 1.26709209898822E-07
AP_0_2 = -4.7079830328754E-07
AP_3_0 = 3.10810569553272E-10
AP_2_1 = -2.01303888849744E-10
AP_1_2 = 6.41654931565699E-10
AP_0_3 = 2.75188359220988E-10
BP_ORDER= 3 / SIP polynomial degree, axis 2, sky-to-pixel
BP_0_0 = -7.96787195162728E-05
BP_1_0 = 7.44638342121251E-08
BP_0_1 = -5.90467481687007E-07
BP_2_0 = 1.01500261205451E-07
BP_1_1 = -2.58495257985211E-07
BP_0_2 = -1.80527378330435E-07
BP_3_0 = -4.99345075601809E-11
BP_2_1 = 4.54030025854777E-10
BP_1_2 = 1.30981094750333E-10
BP_0_3 = 2.88088537738887E-10
PLTSOLVD= T / Siril internal solver
HISTORY Astrometrie / Plate Solving
HISTORY SCNR (Typ=Durchschnittlich neutral, St rke=1.00, Erhaltung=true)
HISTORY Photometrische Farbkalibrierung (Algorithmus: PCC)...](/lib/exe/fetch.php?cache=&media=start:astrofotos:m3_pds_585_20260508_160mal60_graxsiril_gimp.jpg "SIMPLE = T / file does conform to FITS standard
BITPIX = 16 / number of bits per data pixel
NAXIS = 3 / number of data axes
NAXIS1 = 2915 / length of data axis 1
NAXIS2 = 1889 / 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 = '2026-05-09T11:57:02' / UTC date that FITS file was created
ROWORDER= 'TOP-DOWN' / Order of the rows in image array
FOCALLEN= 628.065 / [mm] Focal length
XBINNING= 1 / Camera binning mode
YBINNING= 1 / Camera binning mode
XPIXSZ = 2.9 / [um] Pixel X axis size
YPIXSZ = 2.9 / [um] Pixel Y axis size
STACKCNT= 1 / Stack frames
OBJCTRA = '13 41 19.091' / [H M S] Image center Right Ascension
OBJCTDEC= '+28 22 21.945' / [D M S] Image center Declination
RA = 205.329544402769 / [deg] Image center Right Ascension
DEC = 28.37276239558 / [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 = 1458. / Axis1 reference pixel
CRPIX2 = 945. / Axis2 reference pixel
CRVAL1 = 205.329544402769 / [deg] Axis1 reference value
CRVAL2 = 28.37276239558 / [deg] Axis2 reference value
LONPOLE = 180. / Native longitude of celestial pole
CDELT1 = -0.000264554207781575 / [deg] X pixel size
CDELT2 = 0.000264556257393594 / [deg] Y pixel size
PC1_1 = -0.935506306786633 / Linear transformation matrix (1, 1)
PC1_2 = 0.35330999131419 / Linear transformation matrix (1, 2)
PC2_1 = -0.353414854809899 / Linear transformation matrix (2, 1)
PC2_2 = -0.935466696574334 / 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 = 2.36029914046333E-07
A_1_1 = -1.25826541374622E-07
A_0_2 = 4.68942286444862E-07
A_3_0 = -3.09614255098055E-10
A_2_1 = 2.00399538313748E-10
A_1_2 = -6.38796617775035E-10
A_0_3 = -2.74530336624958E-10
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 = -1.01125176052818E-07
B_1_1 = 2.572381192173E-07
B_0_2 = 1.80288273265436E-07
B_3_0 = 4.96562906615543E-11
B_2_1 = -4.52395737785131E-10
B_1_2 = -1.30688345556544E-10
B_0_3 = -2.8697648720682E-10
AP_ORDER= 3 / SIP polynomial degree, axis 1, sky-to-pixel
AP_0_0 = 0.00060924962662183
AP_1_0 = -8.07178935247066E-07
AP_0_1 = -9.66095599222222E-08
AP_2_0 = -2.3730037040633E-07
AP_1_1 = 1.26709209898822E-07
AP_0_2 = -4.7079830328754E-07
AP_3_0 = 3.10810569553272E-10
AP_2_1 = -2.01303888849744E-10
AP_1_2 = 6.41654931565699E-10
AP_0_3 = 2.75188359220988E-10
BP_ORDER= 3 / SIP polynomial degree, axis 2, sky-to-pixel
BP_0_0 = -7.96787195162728E-05
BP_1_0 = 7.44638342121251E-08
BP_0_1 = -5.90467481687007E-07
BP_2_0 = 1.01500261205451E-07
BP_1_1 = -2.58495257985211E-07
BP_0_2 = -1.80527378330435E-07
BP_3_0 = -4.99345075601809E-11
BP_2_1 = 4.54030025854777E-10
BP_1_2 = 1.30981094750333E-10
BP_0_3 = 2.88088537738887E-10
PLTSOLVD= T / Siril internal solver
HISTORY Astrometrie / Plate Solving
HISTORY SCNR (Typ=Durchschnittlich neutral, St rke=1.00, Erhaltung=true)
HISTORY Photometrische Farbkalibrierung (Algorithmus: PCC)...")