**Table 2:** Atmospheric abundances in the Ap star HD 133792 with the error estimates based on n measured lines. Abundances in the solar atmosphere and in the evolved Ap star HD 204411 are given for comparison.
Ion	HD 133792		HD 204411	Sun
	$\log~ (N/N_{\rm tot})$	n	$\log~ (N/N_{\rm tot})$	$\log~ (N/N_{\rm tot})$
Be II	-11.80:	2		-10.66
C I	-4.68 $\pm$ 0.07	2	-4.37	-3.65
N I	-5.16 $\pm$ 0.08	2	-3.93	-4.26
O I	-4.23 $\pm$ 0.42	5	-4.03	-3.38
Na I	-5.35 $\pm$ 0.22	2	-5.28	-5.87
Mg I	-3.91 $\pm$ 0.02	5	-4.34	-4.51
Mg II	-4.18 $\pm$ 0.68	2	-4.62	-4.51
Al II	-6.03:	1	-5.85	-5.67
Si I	-3.69 $\pm$ 0.21	3	-4.13	-4.53
Si II	-5.09 $\pm$ 0.50	5	-4.11	-4.53
Ca I	-5.31 $\pm$ 0.20	2	-5.17	-5.73
Ca II	-7.36 $\pm$ 0.83	3	-4.67	-5.73
Sc II	-9.50 $\pm$ 0.38	2	-9.52	-8.99
Ti II	-6.88 $\pm$ 0.18	50	-6.49	-7.14
V II	-8.14 $\pm$ 0.17	8		-8.04
Cr I	-3.79 $\pm$ 0.20	131	-4.85	-6.40
Cr II	-3.75 $\pm$ 0.22	320	-4.70	-6.40
Mn I	-5.55 $\pm$ 0.17	13	-5.96	-6.65
Mn II	-5.39 $\pm$ 0.10	9	-5.66	-6.65
Fe I	-3.31 $\pm$ 0.20	247	-3.76	-4.59
Fe II	-3.18 $\pm$ 0.25	347	-3.52	-4.59
Co I	-6.49 $\pm$ 0.16	6	-6.19	-7.12
Co II	-5.99 $\pm$ 0.79	6	-6.50	-7.12
Ni I	-6.05 $\pm$ 0.25	15	-5.68	-5.81
Ni II	-5.96 $\pm$ 0.11	2	-5.31	-5.81
Sr I	-5.71 $\pm$ 0.37	8	-7.74	-9.12
Sr II	-6.36 $\pm$ 0.09	3	-8.5	-9.12
Y II	-9.12 $\pm$ 0.46	6	-9.95	-9.83
Zr II	-9.47 $\pm$ 0.10	7	-8.66	-9.45
Ru II	-8.82:	1		-10.20
Pd I	-7.33 $\pm$ 0.10	2		-10.35
Ba II	-8.73 $\pm$ 0.16	4	-9.02	-9.87
La III	$\le$ -9.6	2		-10.46
Ce II	-9.07:	1	-10.26	-10.46
Ce III	-8.41 $\pm$ 0.07	3		-10.46
Pr III	-9.51 $\pm$ 0.17	3	<-10.5	-11.33
Nd II	-9.08 $\pm$ 0.43	3	-9.48	-10.59
Nd III	-9.10 $\pm$ 0.01	2	-10.05	-10.59
Sm II	$\le$ -10.4	1		-11.03
Eu II	-9.80 $\pm$ 0.20	4	-10.95	-11.52
Gd II	-9.60 $\pm$ 0.04	2		-10.92
Dy II	-10.02 $\pm$ 0.38	3		-10.90
Er II	$\le$ -9.4	1		-11.11
$T_{\rm eff}$	9400 K		8400 K	5777 K
$\log g$	3.70		3.50	4.44
$\langle B \rangle$	1.1 kG		$\le$ 0.7 kG

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