Table 3: Corrections for the position angle effect. Columns: 1 - position angle (PA) in degrees; 2 - projected spectrograph entrance apertures in arcsec; 3 - slit position angle (PA) corrections for emission lines (kp); 4 - estimated PA correction error for emission line, e(kp); 5 - position angle (PA) corrections for continuum flux, kp(cnt); 6 - the estimated PA correction error for continuum flux, e (kp(cnt)).
PA Aperture kp(H $\beta$ ) $\pm$ e kp(cnt) $\pm$ e

deg. arcsec

90 2.0 $\times$ 6.0 1 1

90 4.0 $\times$ 20.4 1 1

0 2.0 $\times$ 6.0 0.969 0.035 0.968 0.017

0 4.0 $\times$ 20.4 1.011 0.018 1.019 0.009

45 2.0 $\times$ 6.0 1.062 0.006 1.098 0.024

45 4 $\times$ 20.4 1.048 0.003 1.071 0.006

135 2.0 $\times$ 6.0 0.954 0.018 0.943 0.011

135 4.0 $\times$ 20.4 0.974 0.004 0.981 0.005

**Table 3:** Corrections for the position angle effect. Columns: 1 - position angle (PA) in degrees; 2 - projected spectrograph entrance apertures in arcsec; 3 - slit position angle (PA) corrections for emission lines (kp); 4 - estimated PA correction error for emission line, e(kp); 5 - position angle (PA) corrections for continuum flux, kp(cnt); 6 - the estimated PA correction error for continuum flux, e (kp(cnt)).
PA	Aperture	kp(H $\beta$ )	$\pm$ e	kp(cnt)	$\pm$ e
deg.	arcsec
90	2.0 $\times$ 6.0	1		1
90	4.0 $\times$ 20.4	1		1
0	2.0 $\times$ 6.0	0.969	0.035	0.968	0.017
0	4.0 $\times$ 20.4	1.011	0.018	1.019	0.009
45	2.0 $\times$ 6.0	1.062	0.006	1.098	0.024
45	4 $\times$ 20.4	1.048	0.003	1.071	0.006
135	2.0 $\times$ 6.0	0.954	0.018	0.943	0.011
135	4.0 $\times$ 20.4	0.974	0.004	0.981	0.005

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