Table 3.

Best-fitting parameters derived from the photometric disc–bar–bulge model applied to R-band images of UGC 7899 and UGC 9037. Column 1: the disc position angle. Column 2: the disc inclination. Column 3: the sky-plane bar angle.

|$\phi ^{\prime }_{\rm d, phot}$| ()iphot ()|$\phi ^{\prime }_{\rm b, phot}$| ()
Galaxy(1)(2)(3)
UGC 789942.6 ± 0.776.6 ± 0.736 ± 2
UGC 9037330 ± 648 ± 5112 ± 3
|$\phi ^{\prime }_{\rm d, phot}$| ()iphot ()|$\phi ^{\prime }_{\rm b, phot}$| ()
Galaxy(1)(2)(3)
UGC 789942.6 ± 0.776.6 ± 0.736 ± 2
UGC 9037330 ± 648 ± 5112 ± 3
Table 3.

Best-fitting parameters derived from the photometric disc–bar–bulge model applied to R-band images of UGC 7899 and UGC 9037. Column 1: the disc position angle. Column 2: the disc inclination. Column 3: the sky-plane bar angle.

|$\phi ^{\prime }_{\rm d, phot}$| ()iphot ()|$\phi ^{\prime }_{\rm b, phot}$| ()
Galaxy(1)(2)(3)
UGC 789942.6 ± 0.776.6 ± 0.736 ± 2
UGC 9037330 ± 648 ± 5112 ± 3
|$\phi ^{\prime }_{\rm d, phot}$| ()iphot ()|$\phi ^{\prime }_{\rm b, phot}$| ()
Galaxy(1)(2)(3)
UGC 789942.6 ± 0.776.6 ± 0.736 ± 2
UGC 9037330 ± 648 ± 5112 ± 3
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