\begin{table}%t12
%\centering
\par
\caption {\label {Tableofdata03}Table summarizing orbital elements of all 42~meteors. alp geo and del geo are respectively geocentric right ascension and declination 
at the epoch J2000.0. TJ is Tisserand parameter with respect to Jupiter. PEKI20 is the case of meteors which crossed the entire field of view making it difficult to compute any 
trajectory solution.}
{\tiny\begin{tabular} {lcccccccccc}
\hline\hline
Name & \multicolumn{2}{c}{Radiant} &\multicolumn{7}{c}{Orbital elements}& TJ\\
\hline
 & $\alpha_{g}$ ($\degr$) & $\delta_{g}$ ($\degr$) & $a$ (AU) & $e$ & $i$ ($\degr$) & $\omega$ ($\degr$) & $\Omega$ ($\degr$) & q per (AU) & q aph (AU)&  \\
\par
\hline
\par
{\bf ELSL01}	&	214.5 $\pm$ 0.4	&	1.5 $\pm$ 1.3	&	1.06 $\pm$ 0.04	&	0.1 $\pm$ 0.2	&	1.2 $\pm$ 0.8	&	47.9 $\pm$ 0.8 	&	236.6 $\pm$ 0.1	&	0.99 $\pm$ 0.01	&	1.14 $\pm$ 0.08	&	5.804\\
ELSL02	&	257.8 $\pm$ 1.1	&	--22.1$\pm$1.1	&	1.3 $\pm$ 0.1 	&	0.84 $\pm$ 0.01 	&	1.4 $\pm$ 1.7	&	317.5 $\pm$ 1.9	&	56.66 $\pm$ 0.03	&	0.21 $\pm$ 0.02	&	2.4 $\pm$ 0.2	&	4.542\\
ELSL03	&	215.0 $\pm$ 1.4	&	32.4 $\pm$ 1.1	&	2.9 $\pm$  0.8	&	0.7 $\pm$  0.1 	&	14.7 $\pm$  1.5	&	207.9 $\pm$  1.2 	&	59.5 $\pm$  0.1	&	0.965 $\pm$  0.005	&	4.8 $\pm$  1.5	&	2.825\\
ELSL04	&	239.5 $\pm$ 1.4	&	--43.3 $\pm$ 1.1	&	4.2 $\pm$  1.3	&	0.88 $\pm$  0.04	&	23.5 $\pm$  1.2 	&	94.9 $\pm$  2.3	&	239.6 $\pm$  0.1	&	 0.5 $\pm$  0.1 	&	7.9 $\pm$  2.6	&	2.021\\
ELSL05	&	179.5 $\pm$ 2.9	&	25.25 $\pm$ 2.02	&	2.6 $\pm$ 1.3	&	0.6 $\pm$  0.2	&	1.9 $\pm$  1.5 	&	181.8 $\pm$  1.9	&	66.2 $\pm$  0.1	&	1.0 $\pm$  0.3	&	 4.1 $\pm$  2.7	&	3.131\\
ELSL06	&	260.3 $\pm$ 1.1	&	--13.3 $\pm$ 1.1	&	3.6 $\pm$  0.9	&	0.92 $\pm$  0.02	&	15.2 $\pm$  1.7	&	299.2 $\pm$  2.4	&	66.2 $\pm$  0.1 	&	0.29 $\pm$  0.02	&	6.8 $\pm$  1.7	&	2.074\\
ELSL07	&	82.76 $\pm$ 2.8	&	64.8 $\pm$ 4.1	&	1.3 $\pm$  0.1	&	0.32 $\pm$  0.07	&	10.9 $\pm$  3.0	&	127.4 $\pm$  4.3	&	66.241 $\pm$  0.001	&	0.918 $\pm$  0.006	&	1.8 $\pm$  0.3	&	4.930\\
ELSL08	&	201.3 $\pm$ 3.5	&	61.8 $\pm$ 1.2	&	1.7 $\pm$  0.2	&	0.42 $\pm$  0.06	&	14.2 $\pm$  1.6	&	178.5 $\pm$  1.4	&	66.3 $\pm$  0.1	&	1.01 $\pm$  0.01	&	2.5 $\pm$  0.3	&	4.064\\
{\bf ELSL09}	&	259.6 $\pm$ 1.1	&	--6.3 $\pm$ 1.1	&	1.9 $\pm$  0.2	&	0.80 $\pm$  0.02 	&	19.2 $\pm$  1.4	&	292.4 $\pm$  2.4 	&	 66.3 $\pm$  0.1 	&	0.39 $\pm$  0.02 	&	3.5 $\pm$  0.4	&	3.422\\
ELSL10	&	304.3 $\pm$ 1.1	&	14.9 $\pm$ 1.1	&	0.644 $\pm$ 0.007 	&	0.65 $\pm$  0.02 	&	41.9 $\pm$  4.1	&	346.7 $\pm$  1.1	&	66.31 $\pm$  0.01	&	0.22 $\pm$  0.01 	&	1.07 $\pm$  0.01 	&	8.472\\
{\bf ELSL11}	&	272.8 $\pm$ 1.4	&	41.9 $\pm$1.1	&	2.1 $\pm$  0.2	&	0.57 $\pm$  0.05	&	47.5 $\pm$  1.2 	&	225.1 $\pm$  3.1 	&	66.33 $\pm$  0.01	&	0.91 $\pm$  0.01 	&	3.3 $\pm$  0.5	&	3.182\\
{\bf ELSL12}	&	307.9 $\pm$ 1.5	&	44.7 $\pm$ 1.1	&	1.01 $\pm$  0.05 	&	0.03 $\pm$  0.02	&	59.9 $\pm$  1.7	&	 272.4 $\pm$ 3.1 	&	66.34 $\pm$  0.01 	&	0.99 $\pm$  0.05 	&	1.04 $\pm$  0.05	&	5.590\\
ELSL13	&	318.1 $\pm$ 1.1	&	8.6 $\pm$ 1.1	&	0.56 $\pm$  0.06	&	0.84 $\pm$  0.02 	&	72.7 $\pm$  1.4	&	354.7 $\pm$  0.7 	&	66.34 $\pm$  0.01 	&	0.09 $\pm$  0.01	&	1.04 $\pm$  0.01	&	9.392\\
PEKI01	&	84.6 $\pm$ 1.1	&	--3.02 $\pm$ 1.1	&	8.8 $\pm$ 0.1	&	0.9 $\pm$ 0.1	&	129.1 $\pm$ 1.8	&	55.3 $\pm$ 5.3	&	12.3 $\pm$ 0.1	&	0.79 $\pm$ 0.03	&	16.8 $\pm$ 0.4	&	--0.124\\
PEKI02	&	326.1 $\pm$ 1.2	&	--6.3 $\pm$ 2.8	&	2.6 $\pm$  0.6	&	 0.64 $\pm$  0.09 	&	1.8 $\pm$  0.9	&	207.5 $\pm$  1.3	&	195.1 $\pm$  0.5 	&	 0.9 $\pm$  0.1 	&	4.3 $\pm$  1.2 	&	3.086\\
PEKI03	&	22.9 $\pm$ 1.1	&	2.3 $\pm$ 1.1	&	2.6 $\pm$  0.3	&	0.83 $\pm$  0.02	&	6.67 $\pm$  1.04	&	103.2 $\pm$  2.2	&	15.148 $\pm$ 0.001	&	0.44 $\pm$ 0.01	&	4.8 $\pm$ 0.6	&	--0.287\\
PEKI04	&	156.7 $\pm$ 2.1	&	61.5 $\pm$ 1.1	&	0.99 $\pm$ 0.06	&	0.35 $\pm$ 0.02	&	74.9 $\pm$ 2.2	&	67.9 $\pm$ 9.4	&	194.4 $\pm$ 0.1	&	0.64 $\pm$ 0.04	&	1.33 $\pm$ 0.08	&	5.466\\
PEKI05	&	80.6 $\pm$ 1.1	&	8.7 $\pm$ 1.1	&	1.8 $\pm$ 0.3	&	0.75 $\pm$  0.03	&	145.9 $\pm$  2.4	&	108.3 $\pm$  6.7 	&	15.3 $\pm$  0.1	&	 0.44 $\pm$  0.04 	&	 3.1 $\pm$  0.6 	&	2.244\\
PEKI06	&	77.2 $\pm$ 1.2	&	34.6 $\pm$ 1.1	&	 0.88 $\pm$  0.04	&	0.79 $\pm$  0.02 	&	144.2 $\pm$  2.9	&	328.3 $\pm$  2.9	&	195.3 $\pm$  0.1 	&	 0.2 $\pm$  0.1	&	 1.6 $\pm$  0.1	&	5.499\\
PEKI07	&	175.7 $\pm$ 2.1	&	61.01 $\pm$ 1.04	&	1.1 $\pm$  0.1	&	0.4 $\pm$  0.1	&	61.6 $\pm$ 2.4	&	81.7 $\pm$  4.5	&	195.3 $\pm$  0.1 	&	 0.69 $\pm$  0.03	&	 1.5 $\pm$  0.1 	&	5.128\\
{\bf PEKI08}	&	77.98 $\pm$ 1.52	&	48.43 $\pm$ 0.06	&	0.85 $\pm$  0.04	&	0.65 $\pm$  0.02	&	111.7 $\pm$  2.2 	&	321.1 $\pm$  3.5 	&	195.3 $\pm$ 0.1	&	0.30 $\pm$  0.02 	&	1.41 $\pm$  0.06	&	5.890\\
{\bf PEKI09}	&	82.5 $\pm$ 1.8	&	57.2 $\pm$ 1.1	&	--1.8 $\pm$  0.3	&	1.49 $\pm$  0.09 	&	120.8 $\pm$  1.5	&	220.4 $\pm$  2.6 	&	195.3 $\pm$  0.1 	&	0.86 $\pm$  0.02 	&	--	&	--3.554\\
PEKI10	&	85.9 $\pm$ 1.1	&	4.59 $\pm$ 1.01	&	1.9 $\pm$  0.4	&	 0.67 $\pm$  0.05 	&	140.6 $\pm$  2.1	&	 86.9 $\pm$  7.3	&	15.3 $\pm$  0.1 	&	0.62 $\pm$  0.04	&	3.1 $\pm$  0.7	&	2.043\\
PEKI11	&	91.5 $\pm$ 1.4	&	43.7 $\pm$ 1.1	&	1.19 $\pm$  0.09	&	0.45 $\pm$  0.03 	&	137.6 $\pm$ 1.9 	&	275.6 $\pm$  7.9	&	196.3 $\pm$  0.1 	&	0.66 $\pm$  0.04	&	1.7 $\pm$  0.2 	&	3.739\\
PEKI12	&	0.1 $\pm$ 1.4	&	41.6 $\pm$ 1.1	&	2.5 $\pm$  0.3	&	 0.73 $\pm$  0.03 	&	27.3 $\pm$  1.1 	&	 257.8 $\pm$  2.3	&	196.3 $\pm$  0.1 	&	 0.66 $\pm$  0.01	&	4.3 $\pm$  0.6	&	2.922\\
PEKI13	&	351.9 $\pm$ 3.4	&	72.45 $\pm$ 1.03	&	2.0 $\pm$  0.4	&	0.6 $\pm$  0.1  	&	48.9 $\pm$  2.3 	&	232.6 $\pm$  4.2	&	196.3 $\pm$  0.1 	&	 0.86 $\pm$  0.01	&	 3.15 $\pm$  0.71 	&	3.252\\
PEKI14	&	30.6 $\pm$ 1.3	&	37.9 $\pm$ 1.1	&	4.4 $\pm$  1.4 	&	0.94 $\pm$  0.01	&	47.8 $\pm$  1.9	&	300.4 $\pm$  2.7	&	197.09 $\pm$  0.01	&	0.27 $\pm$  0.02	&	 8.6 $\pm$  2.7	&	1.603\\
PEKI15	&	156.3 $\pm$ 2.2	&	62.16 $\pm$ 1.03	&	0.96 $\pm$  0.05	&	0.30 $\pm$  0.02	&	75.7 $\pm$  1.7	&	65.8 $\pm$  9.2 	&	197.1 $\pm$  0.1 	&	 0.67 $\pm$  0.04	&	 1.26 $\pm$  0.06 	&	5.619\\
PEKI16	&	162.5 $\pm$ 1.3	&	40.07 $\pm$ 1.01	&	--2.1 $\pm$  0.6	&	1.2 $\pm$  0.1	&	109.4 $\pm$  1.9	&	98.4 $\pm$  3.7	&	197.1 $\pm$  0.1 	&	0.52 $\pm$  0.03	&	-- 	&	--2.756\\
PEKI17	&	213.1 $\pm$ 3.2	&	71.35 $\pm$ 1.03	&	2.8 $\pm$  0.5	&	0.6 $\pm$  0.1  	&	57.7 $\pm$  1.1 	&	156.8 $\pm$  2.6	&	197.1 $\pm$  0.1 	&	0.97 $\pm$  0.01 	&	4.5 $\pm$  0.9	&	2.484\\
PEKI18	&	262.89 $\pm$ 2.4	&	63.9 $\pm$ 1.1	&	2.1 $\pm$  0.3	&	 0.5 $\pm$  0.1	&	34.4 $\pm$  1.8	&	176.1 $\pm$  1.8 	&	197.1 $\pm$  0.1 	&	0.9 $\pm$  0.1	&	3.2 $\pm$  0.6 	&	3.384\\
PEKI19	&	19.02 $\pm$ 1.06	&	14.76 $\pm$ 1.05	&	3.2 $\pm$ 0.5	&	0.86 $\pm$ 0.02	&	6.28 $\pm$ 1.08	&	281.4 $\pm$ 2.2	&	197.150 $\pm$ 0.001	&	0.45 $\pm$ 0.02	&	5.9 $\pm$ 0.9	&	--0.814\\
PEKI20	&	--	&	--	&	--	&	--	&	--	&	--	&	--	&	--	&	--	& --	\\
PEKI21	&	200.2 $\pm$ 4.4	&	76.54 $\pm$ 1.02	&	5.0 $\pm$  2.5	&	0.8 $\pm$  0.1	&	67.3 $\pm$  1.5	&	166.8 $\pm$  2.4	&	197.3 $\pm$  0.1	&	0.9 $\pm$  0.1 	&	 9.1 $\pm$  4.9	&	1.494\\
PEKI22	&	309.9 $\pm$ 2.0	&	58.6 $\pm$ 1.1	&	2.5 $\pm$  0.3	&	0.62 $\pm$  0.05	&	 29.7 $\pm$  1.4	&	206.3 $\pm$  1.6	&	197.3 $\pm$  0.1 	&	 0.9 $\pm$  0.1 	&	4.1 $\pm$  0.7	&	3.025\\
PEKI23	&	99.6 $\pm$ 1.1	&	23.1 $\pm$ 1.1	&	--1.3 $\pm$  0.3	&	1.7 $\pm$  0.2 	&	179.9 $\pm$  0.5	&	203.9 $\pm$ 5.2	&	198.1 $\pm$ 5.1	&	0.95 $\pm$  0.01	&	--	&	--5.374\\
PEKI24	&	127.6 $\pm$ 1.1	&	25.34 $\pm$ 1.01	&	1.5 $\pm$  0.2	&	0.6 $\pm$  0.1  	&	167.2 $\pm$  2.1	&	93.5 $\pm$  8.0	&	197.3 $\pm$  0.1	&	0.6 $\pm$  0.4	&	2.5 $\pm$  0.4	&	2.629\\
PEKI25	&	176.7 $\pm$ 3.6	&	73.33 $\pm$ 1.03	&	1.2 $\pm$  0.1	&	0.21 $\pm$  0.04	&	62.8 $\pm$  1.4 	&	134.4 $\pm$  9.7	&	198.01 $\pm$  0.01	&	0.94 $\pm$  0.02	&	1.4 $\pm$  0.1	&	4.763\\
PEKI26	&	31.88 $\pm$ 1.05	&	8.6 $\pm$ 1.1	&	1.4 $\pm$  0.1	&	 0.72 $\pm$  0.02	&	3.9 $\pm$  1.1 	&	117.5 $\pm$  2.1	&	19.01 $\pm$  0.01 	&	0.39 $\pm$  0.02	&	2.4 $\pm$  0.2	&	4.433\\
PEKI27	&	133.9 $\pm$ 2.8	&	68.70 $\pm$ 1.02	&	2.5 $\pm$  0.7	&	0.6 $\pm$  0.1	&	94.8 $\pm$  1.7	&	174.0 $\pm$  3.6	&	199.02 $\pm$  0.01	&	 0.9 $\pm$  0.3 	&	 4.1 $\pm$  1.4	&	1.987\\
PEKI28	&	71.9 $\pm$ 1.5	&	48.38 $\pm$ 1.01	&	--3.1 $\pm$  1.2	&	1.2 $\pm$  0.1 	&	123.7 $\pm$ 1.9	&	 258.4 $\pm$  3.9 	&	199.2 $\pm$  0.1	&	0.6 $\pm$  0.3	&	--	&	--2.245\\
PEKI29	&	35.09 $\pm$ 1.03	&	6.9 $\pm$ 1.05	&	1.8 $\pm$  0.2	&	 0.8 $\pm$  0.2 	&	8.9 $\pm$  1.4 	&	122.3 $\pm$  2.2	&	19.2 $\pm$  0.1 	&	0.3 $\pm$  0.2 	&	3.4 $\pm$  0.4	&	3.586\\
\par
\hline
\end{tabular}}
\end{table}