Table 3: Sensitivity of the calculated abundances to the changes in the atmospheric parameters.
HD 10132 Adopted parameters $T_{\rm eff}$ = 5000 K log g= 2.5 $\xi=1.0~\rm km~s^{-1}$

Wavelength Species EP $W_\lambda$ mA log $\epsilon$ $\Delta T_{_{\rm eff}}+250~\rm K$ $\Delta \log g +0.5$ $\Delta \xi +0.5$ $\Delta W_\lambda +8\%$

5867.57 CaI 2.93 43.2 6.55 +0.20 -0.20 -0.06 +0.08

6169.04 CaI 2.52 116.5 6.48 +0.27 -0.27 -0.19 +0.13

5441.32 FeI 4.31 52.0 7.47 +0.22 -0.19 -0.12 +0.10

6054.07 FeI 4.37 24.0 7.58 +0.19 -0.18 -0.04 +0.05

4631.48 FeI 4.37 35.3 7.64 +0.19 -0.19 -0.07 +0.06

5294.56 FeI 3.64 32.2 7.56 +0.23 -0.23 -0.06 +0.06

5320.03 FeI 3.64 42.0 7.46 +0.24 -0.23 -0.09 +0.07

6411.66 FeI 3.65 152.0 7.46 +0.30 -0.28 -0.17 +0.10

6084.12 FeII 3.20 42.3 7.41 -0.08 +0.14 -0.11 +0.07

6149.25 FeII 3.89 52.6 7.38 -0.11 +0.18 -0.16 +0.10

6204.64 NiI 4.09 39.6 6.17 +0.19 -0.14 -0.08 +0.07

6175.42 NiI 4.09 66.0 6.18 +0.22 -0.16 -0.19 +0.12

HD 27381 Adopted parameters $T_{\rm eff}$ = 7500 K log g= 1.0 $\xi=4.0~\rm km~s^{-1}$

Wavelength Species EP $W_\lambda$ mA log $\epsilon$ $\Delta T_{_{\rm eff}}+250~\rm K$ $\Delta \log g +0.5$ $\Delta \xi +0.5$ $\Delta W_\lambda +8\%$

6122.23 CaI 1.89 40.2 5.81 +0.44 -0.20 -0.01 +0.04

6162.18 CaI 1.90 56.2 5.78 +0.45 -0.21 -0.02 +0.04

6462.57 CaI 2.52 44.2 5.78 +0.43 -0.21 -0.02 +0.05

5328.04 FeI 0.93 140.2 6.88 +0.40 -0.14 -0.09 +0.12

5569.62 FeI 3.42 34.0 6.80 +0.30 -0.15 -0.01 +0.04

5572.84 FeI 3.40 55.0 6.84 +0.34 -0.15 -0.01 +0.05

5162.27 FeI 4.18 44.0 6.96 +0.32 -0.15 -0.01 +0.05

5415.27 FeI 4.39 63.0 6.91 +0.32 -0.15 -0.02 +0.05

4620.51 FeII 2.83 127.0 6.82 +0.16 +0.08 -0.08 +0.09

4632.68 FeII 2.89 94.0 6.89 +0.17 +0.07 -0.04 +0.06

6419.25 FeII 3.89 105.0 6.89 +0.15 +0.08 -0.04 +0.10

HD 137569 Adopted parameters $T_{\rm eff}$ = 12 000 K log g= 2.5 $\xi=7.0~\rm km~s^{-1}$

Wavelength Species EP $W_\lambda$ mA $\log$ $\epsilon$ $\Delta T_{_{\rm eff}}-500~\rm K$ $\Delta \log g +0.5$ $\Delta \xi +1.0$ $\Delta W_\lambda +16\%$

7423.64 N I 10.33 33.8 6.55 +0.15 +0.33 -0.01 +0.09

7442.29 N I 10.33 50.0 6.49 +0.16 +0.33 -0.02 +0.11

7468.31 N I 10.33 66.4 6.53 +0.16 +0.33 -0.02 +0.12

5330.74 O I 10.74 36.0 6.92 +0.14 +0.32 -0.02 +0.10

6155.99 O I 10.74 39.0 6.89 +0.16 +0.33 -0.02 +0.10

6156.78 O I 10.74 62.0 7.00 +0.15 +0.32 -0.03 +0.11

5014.03 SII 14.07 28.6 6.98 +0.11 +0.25 -0.01 +0.09

5432.80 SII 13.62 23.0 6.51 +0.13 +0.26 -0.03 +0.08

5606.11 SII 13.73 20.0 6.68 +0.13 +0.28 -0.03 +0.10

6578.05 CII 14.45 36.0 4.10 +0.34 +0.69 -0.04 +0.13

6582.88 CII 14.45 19.9 3.92 +0.34 +0.70 -0.02 +0.12

**Table 3:** Sensitivity of the calculated abundances to the changes in the atmospheric parameters.
HD 10132	Adopted	parameters	$T_{\rm eff}$ = 5000 K	log g= 2.5	$\xi=1.0~\rm km~s^{-1}$
Wavelength	Species	EP	$W_\lambda$ mA	log $\epsilon$	$\Delta T_{_{\rm eff}}+250~\rm K$	$\Delta \log g +0.5$	$\Delta \xi +0.5$	$\Delta W_\lambda +8\%$
5867.57	CaI	2.93	43.2	6.55	+0.20	-0.20	-0.06	+0.08
6169.04	CaI	2.52	116.5	6.48	+0.27	-0.27	-0.19	+0.13
5441.32	FeI	4.31	52.0	7.47	+0.22	-0.19	-0.12	+0.10
6054.07	FeI	4.37	24.0	7.58	+0.19	-0.18	-0.04	+0.05
4631.48	FeI	4.37	35.3	7.64	+0.19	-0.19	-0.07	+0.06
5294.56	FeI	3.64	32.2	7.56	+0.23	-0.23	-0.06	+0.06
5320.03	FeI	3.64	42.0	7.46	+0.24	-0.23	-0.09	+0.07
6411.66	FeI	3.65	152.0	7.46	+0.30	-0.28	-0.17	+0.10
6084.12	FeII	3.20	42.3	7.41	-0.08	+0.14	-0.11	+0.07
6149.25	FeII	3.89	52.6	7.38	-0.11	+0.18	-0.16	+0.10
6204.64	NiI	4.09	39.6	6.17	+0.19	-0.14	-0.08	+0.07
6175.42	NiI	4.09	66.0	6.18	+0.22	-0.16	-0.19	+0.12
HD 27381	Adopted	parameters	$T_{\rm eff}$ = 7500 K	log g= 1.0	$\xi=4.0~\rm km~s^{-1}$
Wavelength	Species	EP	$W_\lambda$ mA	log $\epsilon$	$\Delta T_{_{\rm eff}}+250~\rm K$	$\Delta \log g +0.5$	$\Delta \xi +0.5$	$\Delta W_\lambda +8\%$
6122.23	CaI	1.89	40.2	5.81	+0.44	-0.20	-0.01	+0.04
6162.18	CaI	1.90	56.2	5.78	+0.45	-0.21	-0.02	+0.04
6462.57	CaI	2.52	44.2	5.78	+0.43	-0.21	-0.02	+0.05
5328.04	FeI	0.93	140.2	6.88	+0.40	-0.14	-0.09	+0.12
5569.62	FeI	3.42	34.0	6.80	+0.30	-0.15	-0.01	+0.04
5572.84	FeI	3.40	55.0	6.84	+0.34	-0.15	-0.01	+0.05
5162.27	FeI	4.18	44.0	6.96	+0.32	-0.15	-0.01	+0.05
5415.27	FeI	4.39	63.0	6.91	+0.32	-0.15	-0.02	+0.05
4620.51	FeII	2.83	127.0	6.82	+0.16	+0.08	-0.08	+0.09
4632.68	FeII	2.89	94.0	6.89	+0.17	+0.07	-0.04	+0.06
6419.25	FeII	3.89	105.0	6.89	+0.15	+0.08	-0.04	+0.10
HD 137569	Adopted	parameters	$T_{\rm eff}$ = 12 000 K	log g= 2.5	$\xi=7.0~\rm km~s^{-1}$
Wavelength	Species	EP	$W_\lambda$ mA	$\log$ $\epsilon$	$\Delta T_{_{\rm eff}}-500~\rm K$	$\Delta \log g +0.5$	$\Delta \xi +1.0$	$\Delta W_\lambda +16\%$
7423.64	N I	10.33	33.8	6.55	+0.15	+0.33	-0.01	+0.09
7442.29	N I	10.33	50.0	6.49	+0.16	+0.33	-0.02	+0.11
7468.31	N I	10.33	66.4	6.53	+0.16	+0.33	-0.02	+0.12
5330.74	O I	10.74	36.0	6.92	+0.14	+0.32	-0.02	+0.10
6155.99	O I	10.74	39.0	6.89	+0.16	+0.33	-0.02	+0.10
6156.78	O I	10.74	62.0	7.00	+0.15	+0.32	-0.03	+0.11
5014.03	SII	14.07	28.6	6.98	+0.11	+0.25	-0.01	+0.09
5432.80	SII	13.62	23.0	6.51	+0.13	+0.26	-0.03	+0.08
5606.11	SII	13.73	20.0	6.68	+0.13	+0.28	-0.03	+0.10
6578.05	CII	14.45	36.0	4.10	+0.34	+0.69	-0.04	+0.13
6582.88	CII	14.45	19.9	3.92	+0.34	+0.70	-0.02	+0.12

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observations and data reduction
	3 Derived elemental abundances
	4 Conclusions
	References