start:astrofotos:barnard-e_sharpstar_405_2060260806_160mal90_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 = 3880 / length of data axis 1
NAXIS2 = 2573 / 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 1.4.4' / Software that created this HDU
DATE = '2026-08-08T08:31:36' / UTC date that FITS file was created
ROWORDER= 'TOP-DOWN' / Order of the rows in image array
FOCALLEN= 273.23 / [mm] Focal length
XBINNING= 1 / Camera binning mode
YBINNING= 1 / Camera binning mode
XPIXSZ = 4.63 / [um] Pixel X axis size
YPIXSZ = 4.63 / [um] Pixel Y axis size
STACKCNT= 1 / Stack frames
OBJCTRA = '19 39 53.182' / [H M S] Image center Right Ascension
OBJCTDEC= '+10 54 52.322' / [D M S] Image center Declination
RA = 294.971591344405 / [deg] Image center Right Ascension
DEC = 10.9145340143125 / [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 = 1940.5 / Axis1 reference pixel
CRPIX2 = 1287. / Axis2 reference pixel
CRVAL1 = 294.971591344405 / [deg] Axis1 reference value
CRVAL2 = 10.9145340143125 / [deg] Axis2 reference value
LONPOLE = 180. / Native longitude of celestial pole
CDELT1 = -0.000970690495631681 / [deg] X pixel size
CDELT2 = 0.000971110001296507 / [deg] Y pixel size
PC1_1 = -0.0979033501182985 / Linear transformation matrix (1, 1)
PC1_2 = 0.995195927461328 / Linear transformation matrix (1, 2)
PC2_1 = -0.995181567842935 / Linear transformation matrix (2, 1)
PC2_2 = -0.0980492071649612 / 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 = -4.796120423433E-08
A_1_1 = 1.4841153337085E-08
A_0_2 = -3.95472633305224E-08
A_3_0 = -5.19864311719626E-10
A_2_1 = -2.4920150988639E-11
A_1_2 = -5.75165560736532E-10
A_0_3 = 1.46851409022095E-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 = 8.36335181972561E-08
B_1_1 = -1.34304584060672E-08
B_0_2 = 8.21044895895501E-08
B_3_0 = -5.42454283507796E-12
B_2_1 = -5.4074117342157E-10
B_1_2 = -4.54509195881747E-11
B_0_3 = -5.44688392028648E-10
AP_ORDER= 3 / SIP polynomial degree, axis 1, sky-to-pixel
AP_0_0 = -0.000422552347696804
AP_1_0 = -6.89174169887785E-06
AP_0_1 = -3.97501179713279E-07
AP_2_0 = 4.85733157292064E-08
AP_1_1 = -1.47103406573758E-08
AP_0_2 = 3.99395180195509E-08
AP_3_0 = 5.24963004571391E-10
AP_2_1 = 2.53884058436903E-11
AP_1_2 = 5.81365560686719E-10
AP_0_3 = -1.45789015033921E-11
BP_ORDER= 3 / SIP polynomial degree, axis 2, sky-to-pixel
BP_0_0 = 9.55480025252055E-06
BP_1_0 = -3.86765876684781E-07
BP_0_1 = -4.7665010346476E-06
BP_2_0 = -8.41102562973785E-08
BP_1_1 = 1.37086055810168E-08
BP_0_2 = -8.23812068674732E-08
BP_3_0 = 5.57250251082633E-12
BP_2_1 = 5.45962680172485E-10
BP_1_2 = 4.60809881287736E-11
BP_0_3 = 5.48836367614934E-10
PLTSOLVD= T / Siril internal solver
HISTORY Astrometrie / Plate Solving
HISTORY Photometrische Farbkalibrierung (Algorithmus: SPCC)
HISTORY VeraLux v1.5.2 Stretch...](/lib/exe/fetch.php?cache=&w=900&h=596&tok=47751c&media=start:astrofotos:barnard-e_sharpstar_405_2060260806_160mal90_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 = 3880 / length of data axis 1
NAXIS2 = 2573 / 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 1.4.4' / Software that created this HDU
DATE = '2026-08-08T08:31:36' / UTC date that FITS file was created
ROWORDER= 'TOP-DOWN' / Order of the rows in image array
FOCALLEN= 273.23 / [mm] Focal length
XBINNING= 1 / Camera binning mode
YBINNING= 1 / Camera binning mode
XPIXSZ = 4.63 / [um] Pixel X axis size
YPIXSZ = 4.63 / [um] Pixel Y axis size
STACKCNT= 1 / Stack frames
OBJCTRA = '19 39 53.182' / [H M S] Image center Right Ascension
OBJCTDEC= '+10 54 52.322' / [D M S] Image center Declination
RA = 294.971591344405 / [deg] Image center Right Ascension
DEC = 10.9145340143125 / [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 = 1940.5 / Axis1 reference pixel
CRPIX2 = 1287. / Axis2 reference pixel
CRVAL1 = 294.971591344405 / [deg] Axis1 reference value
CRVAL2 = 10.9145340143125 / [deg] Axis2 reference value
LONPOLE = 180. / Native longitude of celestial pole
CDELT1 = -0.000970690495631681 / [deg] X pixel size
CDELT2 = 0.000971110001296507 / [deg] Y pixel size
PC1_1 = -0.0979033501182985 / Linear transformation matrix (1, 1)
PC1_2 = 0.995195927461328 / Linear transformation matrix (1, 2)
PC2_1 = -0.995181567842935 / Linear transformation matrix (2, 1)
PC2_2 = -0.0980492071649612 / 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 = -4.796120423433E-08
A_1_1 = 1.4841153337085E-08
A_0_2 = -3.95472633305224E-08
A_3_0 = -5.19864311719626E-10
A_2_1 = -2.4920150988639E-11
A_1_2 = -5.75165560736532E-10
A_0_3 = 1.46851409022095E-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 = 8.36335181972561E-08
B_1_1 = -1.34304584060672E-08
B_0_2 = 8.21044895895501E-08
B_3_0 = -5.42454283507796E-12
B_2_1 = -5.4074117342157E-10
B_1_2 = -4.54509195881747E-11
B_0_3 = -5.44688392028648E-10
AP_ORDER= 3 / SIP polynomial degree, axis 1, sky-to-pixel
AP_0_0 = -0.000422552347696804
AP_1_0 = -6.89174169887785E-06
AP_0_1 = -3.97501179713279E-07
AP_2_0 = 4.85733157292064E-08
AP_1_1 = -1.47103406573758E-08
AP_0_2 = 3.99395180195509E-08
AP_3_0 = 5.24963004571391E-10
AP_2_1 = 2.53884058436903E-11
AP_1_2 = 5.81365560686719E-10
AP_0_3 = -1.45789015033921E-11
BP_ORDER= 3 / SIP polynomial degree, axis 2, sky-to-pixel
BP_0_0 = 9.55480025252055E-06
BP_1_0 = -3.86765876684781E-07
BP_0_1 = -4.7665010346476E-06
BP_2_0 = -8.41102562973785E-08
BP_1_1 = 1.37086055810168E-08
BP_0_2 = -8.23812068674732E-08
BP_3_0 = 5.57250251082633E-12
BP_2_1 = 5.45962680172485E-10
BP_1_2 = 4.60809881287736E-11
BP_0_3 = 5.48836367614934E-10
PLTSOLVD= T / Siril internal solver
HISTORY Astrometrie / Plate Solving
HISTORY Photometrische Farbkalibrierung (Algorithmus: SPCC)
HISTORY VeraLux v1.5.2 Stretch...")
SIMPLE = T / file does conform to FITS standard
BITPIX = 16 / number of bits per data pixel
NAXIS = 3 / number of data axes
NAXIS1 = 3880 / length of data axis 1
NAXIS2 = 2573 / 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 1.4.4' / Software that created this HDU
DATE = '2026-08-08T08:31:36' / UTC date that FITS file was created
ROWORDER= 'TOP-DOWN' / Order of the rows in image array
FOCALLEN= 273.23 / [mm] Focal length
XBINNING= 1 / Camera binning mode
YBINNING= 1 / Camera binning mode
XPIXSZ = 4.63 / [um] Pixel X axis size
YPIXSZ = 4.63 / [um] Pixel Y axis size
STACKCNT= 1 / Stack frames
OBJCTRA = '19 39 53.182' / [H M S] Image center Right Ascension
OBJCTDEC= '+10 54 52.322' / [D M S] Image center Declination
RA = 294.971591344405 / [deg] Image center Right Ascension
DEC = 10.9145340143125 / [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 = 1940.5 / Axis1 reference pixel
CRPIX2 = 1287. / Axis2 reference pixel
CRVAL1 = 294.971591344405 / [deg] Axis1 reference value
CRVAL2 = 10.9145340143125 / [deg] Axis2 reference value
LONPOLE = 180. / Native longitude of celestial pole
CDELT1 = -0.000970690495631681 / [deg] X pixel size
CDELT2 = 0.000971110001296507 / [deg] Y pixel size
PC1_1 = -0.0979033501182985 / Linear transformation matrix (1, 1)
PC1_2 = 0.995195927461328 / Linear transformation matrix (1, 2)
PC2_1 = -0.995181567842935 / Linear transformation matrix (2, 1)
PC2_2 = -0.0980492071649612 / 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 = -4.796120423433E-08
A_1_1 = 1.4841153337085E-08
A_0_2 = -3.95472633305224E-08
A_3_0 = -5.19864311719626E-10
A_2_1 = -2.4920150988639E-11
A_1_2 = -5.75165560736532E-10
A_0_3 = 1.46851409022095E-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 = 8.36335181972561E-08
B_1_1 = -1.34304584060672E-08
B_0_2 = 8.21044895895501E-08
B_3_0 = -5.42454283507796E-12
B_2_1 = -5.4074117342157E-10
B_1_2 = -4.54509195881747E-11
B_0_3 = -5.44688392028648E-10
AP_ORDER= 3 / SIP polynomial degree, axis 1, sky-to-pixel
AP_0_0 = -0.000422552347696804
AP_1_0 = -6.89174169887785E-06
AP_0_1 = -3.97501179713279E-07
AP_2_0 = 4.85733157292064E-08
AP_1_1 = -1.47103406573758E-08
AP_0_2 = 3.99395180195509E-08
AP_3_0 = 5.24963004571391E-10
AP_2_1 = 2.53884058436903E-11
AP_1_2 = 5.81365560686719E-10
AP_0_3 = -1.45789015033921E-11
BP_ORDER= 3 / SIP polynomial degree, axis 2, sky-to-pixel
BP_0_0 = 9.55480025252055E-06
BP_1_0 = -3.86765876684781E-07
BP_0_1 = -4.7665010346476E-06
BP_2_0 = -8.41102562973785E-08
BP_1_1 = 1.37086055810168E-08
BP_0_2 = -8.23812068674732E-08
BP_3_0 = 5.57250251082633E-12
BP_2_1 = 5.45962680172485E-10
BP_1_2 = 4.60809881287736E-11
BP_0_3 = 5.48836367614934E-10
PLTSOLVD= T / Siril internal solver
HISTORY Astrometrie / Plate Solving
HISTORY Photometrische Farbkalibrierung (Algorithmus: SPCC)
HISTORY VeraLux v1.5.2 Stretch...
- Date:
- 2026/08/08 10:34
- Filename:
- barnard-e_sharpstar_405_2060260806_160mal90_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 = 3880 / length of data axis 1
NAXIS2 = 2573 / 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 1.4.4' / Software that created this HDU
DATE = '2026-08-08T08:31:36' / UTC date that FITS file was created
ROWORDER= 'TOP-DOWN' / Order of the rows in image array
FOCALLEN= 273.23 / [mm] Focal length
XBINNING= 1 / Camera binning mode
YBINNING= 1 / Camera binning mode
XPIXSZ = 4.63 / [um] Pixel X axis size
YPIXSZ = 4.63 / [um] Pixel Y axis size
STACKCNT= 1 / Stack frames
OBJCTRA = '19 39 53.182' / [H M S] Image center Right Ascension
OBJCTDEC= '+10 54 52.322' / [D M S] Image center Declination
RA = 294.971591344405 / [deg] Image center Right Ascension
DEC = 10.9145340143125 / [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 = 1940.5 / Axis1 reference pixel
CRPIX2 = 1287. / Axis2 reference pixel
CRVAL1 = 294.971591344405 / [deg] Axis1 reference value
CRVAL2 = 10.9145340143125 / [deg] Axis2 reference value
LONPOLE = 180. / Native longitude of celestial pole
CDELT1 = -0.000970690495631681 / [deg] X pixel size
CDELT2 = 0.000971110001296507 / [deg] Y pixel size
PC1_1 = -0.0979033501182985 / Linear transformation matrix (1, 1)
PC1_2 = 0.995195927461328 / Linear transformation matrix (1, 2)
PC2_1 = -0.995181567842935 / Linear transformation matrix (2, 1)
PC2_2 = -0.0980492071649612 / 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 = -4.796120423433E-08
A_1_1 = 1.4841153337085E-08
A_0_2 = -3.95472633305224E-08
A_3_0 = -5.19864311719626E-10
A_2_1 = -2.4920150988639E-11
A_1_2 = -5.75165560736532E-10
A_0_3 = 1.46851409022095E-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 = 8.36335181972561E-08
B_1_1 = -1.34304584060672E-08
B_0_2 = 8.21044895895501E-08
B_3_0 = -5.42454283507796E-12
B_2_1 = -5.4074117342157E-10
B_1_2 = -4.54509195881747E-11
B_0_3 = -5.44688392028648E-10
AP_ORDER= 3 / SIP polynomial degree, axis 1, sky-to-pixel
AP_0_0 = -0.000422552347696804
AP_1_0 = -6.89174169887785E-06
AP_0_1 = -3.97501179713279E-07
AP_2_0 = 4.85733157292064E-08
AP_1_1 = -1.47103406573758E-08
AP_0_2 = 3.99395180195509E-08
AP_3_0 = 5.24963004571391E-10
AP_2_1 = 2.53884058436903E-11
AP_1_2 = 5.81365560686719E-10
AP_0_3 = -1.45789015033921E-11
BP_ORDER= 3 / SIP polynomial degree, axis 2, sky-to-pixel
BP_0_0 = 9.55480025252055E-06
BP_1_0 = -3.86765876684781E-07
BP_0_1 = -4.7665010346476E-06
BP_2_0 = -8.41102562973785E-08
BP_1_1 = 1.37086055810168E-08
BP_0_2 = -8.23812068674732E-08
BP_3_0 = 5.57250251082633E-12
BP_2_1 = 5.45962680172485E-10
BP_1_2 = 4.60809881287736E-11
BP_0_3 = 5.48836367614934E-10
PLTSOLVD= T / Siril internal solver
HISTORY Astrometrie / Plate Solving
HISTORY Photometrische Farbkalibrierung (Algorithmus: SPCC)
HISTORY VeraLux v1.5.2 Stretch
END
- Copyright:
- Siril v1.4.4
- Format:
- JPEG
- Size:
- 3MB
- Width:
- 3880
- Height:
- 2573
← Back to start:astrofotos:sommer26
![SIMPLE = T / file does conform to FITS standard
BITPIX = 16 / number of bits per data pixel
NAXIS = 3 / number of data axes
NAXIS1 = 3880 / length of data axis 1
NAXIS2 = 2573 / 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 1.4.4' / Software that created this HDU
DATE = '2026-08-08T08:31:36' / UTC date that FITS file was created
ROWORDER= 'TOP-DOWN' / Order of the rows in image array
FOCALLEN= 273.23 / [mm] Focal length
XBINNING= 1 / Camera binning mode
YBINNING= 1 / Camera binning mode
XPIXSZ = 4.63 / [um] Pixel X axis size
YPIXSZ = 4.63 / [um] Pixel Y axis size
STACKCNT= 1 / Stack frames
OBJCTRA = '19 39 53.182' / [H M S] Image center Right Ascension
OBJCTDEC= '+10 54 52.322' / [D M S] Image center Declination
RA = 294.971591344405 / [deg] Image center Right Ascension
DEC = 10.9145340143125 / [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 = 1940.5 / Axis1 reference pixel
CRPIX2 = 1287. / Axis2 reference pixel
CRVAL1 = 294.971591344405 / [deg] Axis1 reference value
CRVAL2 = 10.9145340143125 / [deg] Axis2 reference value
LONPOLE = 180. / Native longitude of celestial pole
CDELT1 = -0.000970690495631681 / [deg] X pixel size
CDELT2 = 0.000971110001296507 / [deg] Y pixel size
PC1_1 = -0.0979033501182985 / Linear transformation matrix (1, 1)
PC1_2 = 0.995195927461328 / Linear transformation matrix (1, 2)
PC2_1 = -0.995181567842935 / Linear transformation matrix (2, 1)
PC2_2 = -0.0980492071649612 / 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 = -4.796120423433E-08
A_1_1 = 1.4841153337085E-08
A_0_2 = -3.95472633305224E-08
A_3_0 = -5.19864311719626E-10
A_2_1 = -2.4920150988639E-11
A_1_2 = -5.75165560736532E-10
A_0_3 = 1.46851409022095E-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 = 8.36335181972561E-08
B_1_1 = -1.34304584060672E-08
B_0_2 = 8.21044895895501E-08
B_3_0 = -5.42454283507796E-12
B_2_1 = -5.4074117342157E-10
B_1_2 = -4.54509195881747E-11
B_0_3 = -5.44688392028648E-10
AP_ORDER= 3 / SIP polynomial degree, axis 1, sky-to-pixel
AP_0_0 = -0.000422552347696804
AP_1_0 = -6.89174169887785E-06
AP_0_1 = -3.97501179713279E-07
AP_2_0 = 4.85733157292064E-08
AP_1_1 = -1.47103406573758E-08
AP_0_2 = 3.99395180195509E-08
AP_3_0 = 5.24963004571391E-10
AP_2_1 = 2.53884058436903E-11
AP_1_2 = 5.81365560686719E-10
AP_0_3 = -1.45789015033921E-11
BP_ORDER= 3 / SIP polynomial degree, axis 2, sky-to-pixel
BP_0_0 = 9.55480025252055E-06
BP_1_0 = -3.86765876684781E-07
BP_0_1 = -4.7665010346476E-06
BP_2_0 = -8.41102562973785E-08
BP_1_1 = 1.37086055810168E-08
BP_0_2 = -8.23812068674732E-08
BP_3_0 = 5.57250251082633E-12
BP_2_1 = 5.45962680172485E-10
BP_1_2 = 4.60809881287736E-11
BP_0_3 = 5.48836367614934E-10
PLTSOLVD= T / Siril internal solver
HISTORY Astrometrie / Plate Solving
HISTORY Photometrische Farbkalibrierung (Algorithmus: SPCC)
HISTORY VeraLux v1.5.2 Stretch...](/lib/exe/fetch.php?cache=&media=start:astrofotos:barnard-e_sharpstar_405_2060260806_160mal90_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 = 3880 / length of data axis 1
NAXIS2 = 2573 / 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 1.4.4' / Software that created this HDU
DATE = '2026-08-08T08:31:36' / UTC date that FITS file was created
ROWORDER= 'TOP-DOWN' / Order of the rows in image array
FOCALLEN= 273.23 / [mm] Focal length
XBINNING= 1 / Camera binning mode
YBINNING= 1 / Camera binning mode
XPIXSZ = 4.63 / [um] Pixel X axis size
YPIXSZ = 4.63 / [um] Pixel Y axis size
STACKCNT= 1 / Stack frames
OBJCTRA = '19 39 53.182' / [H M S] Image center Right Ascension
OBJCTDEC= '+10 54 52.322' / [D M S] Image center Declination
RA = 294.971591344405 / [deg] Image center Right Ascension
DEC = 10.9145340143125 / [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 = 1940.5 / Axis1 reference pixel
CRPIX2 = 1287. / Axis2 reference pixel
CRVAL1 = 294.971591344405 / [deg] Axis1 reference value
CRVAL2 = 10.9145340143125 / [deg] Axis2 reference value
LONPOLE = 180. / Native longitude of celestial pole
CDELT1 = -0.000970690495631681 / [deg] X pixel size
CDELT2 = 0.000971110001296507 / [deg] Y pixel size
PC1_1 = -0.0979033501182985 / Linear transformation matrix (1, 1)
PC1_2 = 0.995195927461328 / Linear transformation matrix (1, 2)
PC2_1 = -0.995181567842935 / Linear transformation matrix (2, 1)
PC2_2 = -0.0980492071649612 / 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 = -4.796120423433E-08
A_1_1 = 1.4841153337085E-08
A_0_2 = -3.95472633305224E-08
A_3_0 = -5.19864311719626E-10
A_2_1 = -2.4920150988639E-11
A_1_2 = -5.75165560736532E-10
A_0_3 = 1.46851409022095E-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 = 8.36335181972561E-08
B_1_1 = -1.34304584060672E-08
B_0_2 = 8.21044895895501E-08
B_3_0 = -5.42454283507796E-12
B_2_1 = -5.4074117342157E-10
B_1_2 = -4.54509195881747E-11
B_0_3 = -5.44688392028648E-10
AP_ORDER= 3 / SIP polynomial degree, axis 1, sky-to-pixel
AP_0_0 = -0.000422552347696804
AP_1_0 = -6.89174169887785E-06
AP_0_1 = -3.97501179713279E-07
AP_2_0 = 4.85733157292064E-08
AP_1_1 = -1.47103406573758E-08
AP_0_2 = 3.99395180195509E-08
AP_3_0 = 5.24963004571391E-10
AP_2_1 = 2.53884058436903E-11
AP_1_2 = 5.81365560686719E-10
AP_0_3 = -1.45789015033921E-11
BP_ORDER= 3 / SIP polynomial degree, axis 2, sky-to-pixel
BP_0_0 = 9.55480025252055E-06
BP_1_0 = -3.86765876684781E-07
BP_0_1 = -4.7665010346476E-06
BP_2_0 = -8.41102562973785E-08
BP_1_1 = 1.37086055810168E-08
BP_0_2 = -8.23812068674732E-08
BP_3_0 = 5.57250251082633E-12
BP_2_1 = 5.45962680172485E-10
BP_1_2 = 4.60809881287736E-11
BP_0_3 = 5.48836367614934E-10
PLTSOLVD= T / Siril internal solver
HISTORY Astrometrie / Plate Solving
HISTORY Photometrische Farbkalibrierung (Algorithmus: SPCC)
HISTORY VeraLux v1.5.2 Stretch...")