start:astrofotos:m81_82_ifn_graxsiril_gimp1_starnet_gimp2.jpg
![SIMPLE = T / file does conform to FITS standard
BITPIX = 16 / number of bits per data pixel
NAXIS = 3 / number of data axes
NAXIS1 = 3799 / length of data axis 1
NAXIS2 = 2436 / 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
MIPS-HI = 64447 / Lower visualization cutoff
MIPS-LO = 1842 / Upper visualization cutoff
PROGRAM = 'Siril 1.4.3' / Software that created this HDU
DATE = '2026-05-11T11:47:41' / UTC date that FITS file was created
ROWORDER= 'TOP-DOWN' / Order of the rows in image array
FOCALLEN= 273.044 / [mm] Focal length
XBINNING= 1 / Camera binning mode
YBINNING= 1 / Camera binning mode
XPIXSZ = 4.63000011444092 / [um] Pixel X axis size
YPIXSZ = 4.63000011444092 / [um] Pixel Y axis size
STACKCNT= 1 / Stack frames
OBJCTRA = '09 46 36.108' / [H M S] Image center Right Ascension
OBJCTDEC= '+69 36 38.222' / [D M S] Image center Declination
RA = 146.650448191611 / [deg] Image center Right Ascension
DEC = 69.6106173330097 / [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 = 1900. / Axis1 reference pixel
CRPIX2 = 1218.5 / Axis2 reference pixel
CRVAL1 = 146.650448191611 / [deg] Axis1 reference value
CRVAL2 = 69.6106173330097 / [deg] Axis2 reference value
LONPOLE = 180. / Native longitude of celestial pole
CDELT1 = -0.000971719029549205 / [deg] X pixel size
CDELT2 = 0.000971409899788457 / [deg] Y pixel size
PC1_1 = 0.986851753973847 / Linear transformation matrix (1, 1)
PC1_2 = 0.161628016379405 / Linear transformation matrix (1, 2)
PC2_1 = -0.161701954924858 / Linear transformation matrix (2, 1)
PC2_2 = 0.986839641367066 / 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 = -1.59825229370558E-07
A_1_1 = -2.14143245599892E-08
A_0_2 = -6.89873553200454E-08
A_3_0 = -5.50876206454822E-10
A_2_1 = 5.01868816016477E-11
A_1_2 = -5.46084197832714E-10
A_0_3 = -1.19095358808333E-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 = 2.5592712846576E-08
B_1_1 = -1.34253242427426E-07
B_0_2 = 2.016817292038E-08
B_3_0 = 1.37114142761336E-11
B_2_1 = -5.44852422371355E-10
B_1_2 = 9.49393986671247E-11
B_0_3 = -4.34900621720017E-10
AP_ORDER= 3 / SIP polynomial degree, axis 1, sky-to-pixel
AP_0_0 = -0.000784723184248529
AP_1_0 = -6.17253632784198E-06
AP_0_1 = -4.22642989478062E-08
AP_2_0 = 1.61613897335247E-07
AP_1_1 = 2.13788332640129E-08
AP_0_2 = 6.96573971916025E-08
AP_3_0 = 5.56091038404752E-10
AP_2_1 = -5.07026518656791E-11
AP_1_2 = 5.51747314448879E-10
AP_0_3 = 1.19654404672452E-10
BP_ORDER= 3 / SIP polynomial degree, axis 2, sky-to-pixel
BP_0_0 = 0.000104219902878621
BP_1_0 = 5.3947683222542E-07
BP_0_1 = -3.67433761638836E-06
BP_2_0 = -2.58161548350381E-08
BP_1_1 = 1.35339667996683E-07
BP_0_2 = -2.0306890054154E-08
BP_3_0 = -1.40169835321094E-11
BP_2_1 = 5.49689836654879E-10
BP_1_2 = -9.58432995991201E-11
BP_0_3 = 4.37895896880467E-10
PLTSOLVD= T / Siril internal solver
HISTORY Astrometrie / Plate Solving
HISTORY Photometrische Farbkalibrierung (Algorithmus: PCC)...](/lib/exe/fetch.php?cache=&w=900&h=577&tok=fdd8de&media=start:astrofotos:m81_82_ifn_graxsiril_gimp1_starnet_gimp2.jpg "SIMPLE = T / file does conform to FITS standard
BITPIX = 16 / number of bits per data pixel
NAXIS = 3 / number of data axes
NAXIS1 = 3799 / length of data axis 1
NAXIS2 = 2436 / 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
MIPS-HI = 64447 / Lower visualization cutoff
MIPS-LO = 1842 / Upper visualization cutoff
PROGRAM = 'Siril 1.4.3' / Software that created this HDU
DATE = '2026-05-11T11:47:41' / UTC date that FITS file was created
ROWORDER= 'TOP-DOWN' / Order of the rows in image array
FOCALLEN= 273.044 / [mm] Focal length
XBINNING= 1 / Camera binning mode
YBINNING= 1 / Camera binning mode
XPIXSZ = 4.63000011444092 / [um] Pixel X axis size
YPIXSZ = 4.63000011444092 / [um] Pixel Y axis size
STACKCNT= 1 / Stack frames
OBJCTRA = '09 46 36.108' / [H M S] Image center Right Ascension
OBJCTDEC= '+69 36 38.222' / [D M S] Image center Declination
RA = 146.650448191611 / [deg] Image center Right Ascension
DEC = 69.6106173330097 / [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 = 1900. / Axis1 reference pixel
CRPIX2 = 1218.5 / Axis2 reference pixel
CRVAL1 = 146.650448191611 / [deg] Axis1 reference value
CRVAL2 = 69.6106173330097 / [deg] Axis2 reference value
LONPOLE = 180. / Native longitude of celestial pole
CDELT1 = -0.000971719029549205 / [deg] X pixel size
CDELT2 = 0.000971409899788457 / [deg] Y pixel size
PC1_1 = 0.986851753973847 / Linear transformation matrix (1, 1)
PC1_2 = 0.161628016379405 / Linear transformation matrix (1, 2)
PC2_1 = -0.161701954924858 / Linear transformation matrix (2, 1)
PC2_2 = 0.986839641367066 / 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 = -1.59825229370558E-07
A_1_1 = -2.14143245599892E-08
A_0_2 = -6.89873553200454E-08
A_3_0 = -5.50876206454822E-10
A_2_1 = 5.01868816016477E-11
A_1_2 = -5.46084197832714E-10
A_0_3 = -1.19095358808333E-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 = 2.5592712846576E-08
B_1_1 = -1.34253242427426E-07
B_0_2 = 2.016817292038E-08
B_3_0 = 1.37114142761336E-11
B_2_1 = -5.44852422371355E-10
B_1_2 = 9.49393986671247E-11
B_0_3 = -4.34900621720017E-10
AP_ORDER= 3 / SIP polynomial degree, axis 1, sky-to-pixel
AP_0_0 = -0.000784723184248529
AP_1_0 = -6.17253632784198E-06
AP_0_1 = -4.22642989478062E-08
AP_2_0 = 1.61613897335247E-07
AP_1_1 = 2.13788332640129E-08
AP_0_2 = 6.96573971916025E-08
AP_3_0 = 5.56091038404752E-10
AP_2_1 = -5.07026518656791E-11
AP_1_2 = 5.51747314448879E-10
AP_0_3 = 1.19654404672452E-10
BP_ORDER= 3 / SIP polynomial degree, axis 2, sky-to-pixel
BP_0_0 = 0.000104219902878621
BP_1_0 = 5.3947683222542E-07
BP_0_1 = -3.67433761638836E-06
BP_2_0 = -2.58161548350381E-08
BP_1_1 = 1.35339667996683E-07
BP_0_2 = -2.0306890054154E-08
BP_3_0 = -1.40169835321094E-11
BP_2_1 = 5.49689836654879E-10
BP_1_2 = -9.58432995991201E-11
BP_0_3 = 4.37895896880467E-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 = 3799 / length of data axis 1
NAXIS2 = 2436 / 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
MIPS-HI = 64447 / Lower visualization cutoff
MIPS-LO = 1842 / Upper visualization cutoff
PROGRAM = 'Siril 1.4.3' / Software that created this HDU
DATE = '2026-05-11T11:47:41' / UTC date that FITS file was created
ROWORDER= 'TOP-DOWN' / Order of the rows in image array
FOCALLEN= 273.044 / [mm] Focal length
XBINNING= 1 / Camera binning mode
YBINNING= 1 / Camera binning mode
XPIXSZ = 4.63000011444092 / [um] Pixel X axis size
YPIXSZ = 4.63000011444092 / [um] Pixel Y axis size
STACKCNT= 1 / Stack frames
OBJCTRA = '09 46 36.108' / [H M S] Image center Right Ascension
OBJCTDEC= '+69 36 38.222' / [D M S] Image center Declination
RA = 146.650448191611 / [deg] Image center Right Ascension
DEC = 69.6106173330097 / [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 = 1900. / Axis1 reference pixel
CRPIX2 = 1218.5 / Axis2 reference pixel
CRVAL1 = 146.650448191611 / [deg] Axis1 reference value
CRVAL2 = 69.6106173330097 / [deg] Axis2 reference value
LONPOLE = 180. / Native longitude of celestial pole
CDELT1 = -0.000971719029549205 / [deg] X pixel size
CDELT2 = 0.000971409899788457 / [deg] Y pixel size
PC1_1 = 0.986851753973847 / Linear transformation matrix (1, 1)
PC1_2 = 0.161628016379405 / Linear transformation matrix (1, 2)
PC2_1 = -0.161701954924858 / Linear transformation matrix (2, 1)
PC2_2 = 0.986839641367066 / 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 = -1.59825229370558E-07
A_1_1 = -2.14143245599892E-08
A_0_2 = -6.89873553200454E-08
A_3_0 = -5.50876206454822E-10
A_2_1 = 5.01868816016477E-11
A_1_2 = -5.46084197832714E-10
A_0_3 = -1.19095358808333E-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 = 2.5592712846576E-08
B_1_1 = -1.34253242427426E-07
B_0_2 = 2.016817292038E-08
B_3_0 = 1.37114142761336E-11
B_2_1 = -5.44852422371355E-10
B_1_2 = 9.49393986671247E-11
B_0_3 = -4.34900621720017E-10
AP_ORDER= 3 / SIP polynomial degree, axis 1, sky-to-pixel
AP_0_0 = -0.000784723184248529
AP_1_0 = -6.17253632784198E-06
AP_0_1 = -4.22642989478062E-08
AP_2_0 = 1.61613897335247E-07
AP_1_1 = 2.13788332640129E-08
AP_0_2 = 6.96573971916025E-08
AP_3_0 = 5.56091038404752E-10
AP_2_1 = -5.07026518656791E-11
AP_1_2 = 5.51747314448879E-10
AP_0_3 = 1.19654404672452E-10
BP_ORDER= 3 / SIP polynomial degree, axis 2, sky-to-pixel
BP_0_0 = 0.000104219902878621
BP_1_0 = 5.3947683222542E-07
BP_0_1 = -3.67433761638836E-06
BP_2_0 = -2.58161548350381E-08
BP_1_1 = 1.35339667996683E-07
BP_0_2 = -2.0306890054154E-08
BP_3_0 = -1.40169835321094E-11
BP_2_1 = 5.49689836654879E-10
BP_1_2 = -9.58432995991201E-11
BP_0_3 = 4.37895896880467E-10
PLTSOLVD= T / Siril internal solver
HISTORY Astrometrie / Plate Solving
HISTORY Photometrische Farbkalibrierung (Algorithmus: PCC)...
- Date:
- 2026/05/11 14:01
- Filename:
- m81_82_ifn_graxsiril_gimp1_starnet_gimp2.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 = 3799 / length of data axis 1
NAXIS2 = 2436 / 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
MIPS-HI = 64447 / Lower visualization cutoff
MIPS-LO = 1842 / Upper visualization cutoff
PROGRAM = 'Siril 1.4.3' / Software that created this HDU
DATE = '2026-05-11T11:47:41' / UTC date that FITS file was created
ROWORDER= 'TOP-DOWN' / Order of the rows in image array
FOCALLEN= 273.044 / [mm] Focal length
XBINNING= 1 / Camera binning mode
YBINNING= 1 / Camera binning mode
XPIXSZ = 4.63000011444092 / [um] Pixel X axis size
YPIXSZ = 4.63000011444092 / [um] Pixel Y axis size
STACKCNT= 1 / Stack frames
OBJCTRA = '09 46 36.108' / [H M S] Image center Right Ascension
OBJCTDEC= '+69 36 38.222' / [D M S] Image center Declination
RA = 146.650448191611 / [deg] Image center Right Ascension
DEC = 69.6106173330097 / [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 = 1900. / Axis1 reference pixel
CRPIX2 = 1218.5 / Axis2 reference pixel
CRVAL1 = 146.650448191611 / [deg] Axis1 reference value
CRVAL2 = 69.6106173330097 / [deg] Axis2 reference value
LONPOLE = 180. / Native longitude of celestial pole
CDELT1 = -0.000971719029549205 / [deg] X pixel size
CDELT2 = 0.000971409899788457 / [deg] Y pixel size
PC1_1 = 0.986851753973847 / Linear transformation matrix (1, 1)
PC1_2 = 0.161628016379405 / Linear transformation matrix (1, 2)
PC2_1 = -0.161701954924858 / Linear transformation matrix (2, 1)
PC2_2 = 0.986839641367066 / 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 = -1.59825229370558E-07
A_1_1 = -2.14143245599892E-08
A_0_2 = -6.89873553200454E-08
A_3_0 = -5.50876206454822E-10
A_2_1 = 5.01868816016477E-11
A_1_2 = -5.46084197832714E-10
A_0_3 = -1.19095358808333E-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 = 2.5592712846576E-08
B_1_1 = -1.34253242427426E-07
B_0_2 = 2.016817292038E-08
B_3_0 = 1.37114142761336E-11
B_2_1 = -5.44852422371355E-10
B_1_2 = 9.49393986671247E-11
B_0_3 = -4.34900621720017E-10
AP_ORDER= 3 / SIP polynomial degree, axis 1, sky-to-pixel
AP_0_0 = -0.000784723184248529
AP_1_0 = -6.17253632784198E-06
AP_0_1 = -4.22642989478062E-08
AP_2_0 = 1.61613897335247E-07
AP_1_1 = 2.13788332640129E-08
AP_0_2 = 6.96573971916025E-08
AP_3_0 = 5.56091038404752E-10
AP_2_1 = -5.07026518656791E-11
AP_1_2 = 5.51747314448879E-10
AP_0_3 = 1.19654404672452E-10
BP_ORDER= 3 / SIP polynomial degree, axis 2, sky-to-pixel
BP_0_0 = 0.000104219902878621
BP_1_0 = 5.3947683222542E-07
BP_0_1 = -3.67433761638836E-06
BP_2_0 = -2.58161548350381E-08
BP_1_1 = 1.35339667996683E-07
BP_0_2 = -2.0306890054154E-08
BP_3_0 = -1.40169835321094E-11
BP_2_1 = 5.49689836654879E-10
BP_1_2 = -9.58432995991201E-11
BP_0_3 = 4.37895896880467E-10
PLTSOLVD= T / Siril internal solver
HISTORY Astrometrie / Plate Solving
HISTORY Photometrische Farbkalibrierung (Algorithmus: PCC)
END
- Copyright:
- Siril v1.4.3
- Format:
- JPEG
- Size:
- 3MB
- Width:
- 3799
- Height:
- 2436
← 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 = 3799 / length of data axis 1
NAXIS2 = 2436 / 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
MIPS-HI = 64447 / Lower visualization cutoff
MIPS-LO = 1842 / Upper visualization cutoff
PROGRAM = 'Siril 1.4.3' / Software that created this HDU
DATE = '2026-05-11T11:47:41' / UTC date that FITS file was created
ROWORDER= 'TOP-DOWN' / Order of the rows in image array
FOCALLEN= 273.044 / [mm] Focal length
XBINNING= 1 / Camera binning mode
YBINNING= 1 / Camera binning mode
XPIXSZ = 4.63000011444092 / [um] Pixel X axis size
YPIXSZ = 4.63000011444092 / [um] Pixel Y axis size
STACKCNT= 1 / Stack frames
OBJCTRA = '09 46 36.108' / [H M S] Image center Right Ascension
OBJCTDEC= '+69 36 38.222' / [D M S] Image center Declination
RA = 146.650448191611 / [deg] Image center Right Ascension
DEC = 69.6106173330097 / [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 = 1900. / Axis1 reference pixel
CRPIX2 = 1218.5 / Axis2 reference pixel
CRVAL1 = 146.650448191611 / [deg] Axis1 reference value
CRVAL2 = 69.6106173330097 / [deg] Axis2 reference value
LONPOLE = 180. / Native longitude of celestial pole
CDELT1 = -0.000971719029549205 / [deg] X pixel size
CDELT2 = 0.000971409899788457 / [deg] Y pixel size
PC1_1 = 0.986851753973847 / Linear transformation matrix (1, 1)
PC1_2 = 0.161628016379405 / Linear transformation matrix (1, 2)
PC2_1 = -0.161701954924858 / Linear transformation matrix (2, 1)
PC2_2 = 0.986839641367066 / 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 = -1.59825229370558E-07
A_1_1 = -2.14143245599892E-08
A_0_2 = -6.89873553200454E-08
A_3_0 = -5.50876206454822E-10
A_2_1 = 5.01868816016477E-11
A_1_2 = -5.46084197832714E-10
A_0_3 = -1.19095358808333E-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 = 2.5592712846576E-08
B_1_1 = -1.34253242427426E-07
B_0_2 = 2.016817292038E-08
B_3_0 = 1.37114142761336E-11
B_2_1 = -5.44852422371355E-10
B_1_2 = 9.49393986671247E-11
B_0_3 = -4.34900621720017E-10
AP_ORDER= 3 / SIP polynomial degree, axis 1, sky-to-pixel
AP_0_0 = -0.000784723184248529
AP_1_0 = -6.17253632784198E-06
AP_0_1 = -4.22642989478062E-08
AP_2_0 = 1.61613897335247E-07
AP_1_1 = 2.13788332640129E-08
AP_0_2 = 6.96573971916025E-08
AP_3_0 = 5.56091038404752E-10
AP_2_1 = -5.07026518656791E-11
AP_1_2 = 5.51747314448879E-10
AP_0_3 = 1.19654404672452E-10
BP_ORDER= 3 / SIP polynomial degree, axis 2, sky-to-pixel
BP_0_0 = 0.000104219902878621
BP_1_0 = 5.3947683222542E-07
BP_0_1 = -3.67433761638836E-06
BP_2_0 = -2.58161548350381E-08
BP_1_1 = 1.35339667996683E-07
BP_0_2 = -2.0306890054154E-08
BP_3_0 = -1.40169835321094E-11
BP_2_1 = 5.49689836654879E-10
BP_1_2 = -9.58432995991201E-11
BP_0_3 = 4.37895896880467E-10
PLTSOLVD= T / Siril internal solver
HISTORY Astrometrie / Plate Solving
HISTORY Photometrische Farbkalibrierung (Algorithmus: PCC)...](/lib/exe/fetch.php?cache=&media=start:astrofotos:m81_82_ifn_graxsiril_gimp1_starnet_gimp2.jpg "SIMPLE = T / file does conform to FITS standard
BITPIX = 16 / number of bits per data pixel
NAXIS = 3 / number of data axes
NAXIS1 = 3799 / length of data axis 1
NAXIS2 = 2436 / 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
MIPS-HI = 64447 / Lower visualization cutoff
MIPS-LO = 1842 / Upper visualization cutoff
PROGRAM = 'Siril 1.4.3' / Software that created this HDU
DATE = '2026-05-11T11:47:41' / UTC date that FITS file was created
ROWORDER= 'TOP-DOWN' / Order of the rows in image array
FOCALLEN= 273.044 / [mm] Focal length
XBINNING= 1 / Camera binning mode
YBINNING= 1 / Camera binning mode
XPIXSZ = 4.63000011444092 / [um] Pixel X axis size
YPIXSZ = 4.63000011444092 / [um] Pixel Y axis size
STACKCNT= 1 / Stack frames
OBJCTRA = '09 46 36.108' / [H M S] Image center Right Ascension
OBJCTDEC= '+69 36 38.222' / [D M S] Image center Declination
RA = 146.650448191611 / [deg] Image center Right Ascension
DEC = 69.6106173330097 / [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 = 1900. / Axis1 reference pixel
CRPIX2 = 1218.5 / Axis2 reference pixel
CRVAL1 = 146.650448191611 / [deg] Axis1 reference value
CRVAL2 = 69.6106173330097 / [deg] Axis2 reference value
LONPOLE = 180. / Native longitude of celestial pole
CDELT1 = -0.000971719029549205 / [deg] X pixel size
CDELT2 = 0.000971409899788457 / [deg] Y pixel size
PC1_1 = 0.986851753973847 / Linear transformation matrix (1, 1)
PC1_2 = 0.161628016379405 / Linear transformation matrix (1, 2)
PC2_1 = -0.161701954924858 / Linear transformation matrix (2, 1)
PC2_2 = 0.986839641367066 / 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 = -1.59825229370558E-07
A_1_1 = -2.14143245599892E-08
A_0_2 = -6.89873553200454E-08
A_3_0 = -5.50876206454822E-10
A_2_1 = 5.01868816016477E-11
A_1_2 = -5.46084197832714E-10
A_0_3 = -1.19095358808333E-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 = 2.5592712846576E-08
B_1_1 = -1.34253242427426E-07
B_0_2 = 2.016817292038E-08
B_3_0 = 1.37114142761336E-11
B_2_1 = -5.44852422371355E-10
B_1_2 = 9.49393986671247E-11
B_0_3 = -4.34900621720017E-10
AP_ORDER= 3 / SIP polynomial degree, axis 1, sky-to-pixel
AP_0_0 = -0.000784723184248529
AP_1_0 = -6.17253632784198E-06
AP_0_1 = -4.22642989478062E-08
AP_2_0 = 1.61613897335247E-07
AP_1_1 = 2.13788332640129E-08
AP_0_2 = 6.96573971916025E-08
AP_3_0 = 5.56091038404752E-10
AP_2_1 = -5.07026518656791E-11
AP_1_2 = 5.51747314448879E-10
AP_0_3 = 1.19654404672452E-10
BP_ORDER= 3 / SIP polynomial degree, axis 2, sky-to-pixel
BP_0_0 = 0.000104219902878621
BP_1_0 = 5.3947683222542E-07
BP_0_1 = -3.67433761638836E-06
BP_2_0 = -2.58161548350381E-08
BP_1_1 = 1.35339667996683E-07
BP_0_2 = -2.0306890054154E-08
BP_3_0 = -1.40169835321094E-11
BP_2_1 = 5.49689836654879E-10
BP_1_2 = -9.58432995991201E-11
BP_0_3 = 4.37895896880467E-10
PLTSOLVD= T / Siril internal solver
HISTORY Astrometrie / Plate Solving
HISTORY Photometrische Farbkalibrierung (Algorithmus: PCC)...")