The UV resonance transitions of neutral argon, Ar I j1066, and of singly ionized phosphorus, P II j963, originated in the damped Lya system (DLA) at toward QSO 0000[2620, have been z abs 3.3901 detected by means of the Ultraviolet-Visual Echelle Spectrograph (UVES) spectrograph at the 8.2 m ESO KUEYEN telescope. So far, this is the —rst measurement of Ar I and the second of P II ever performed in damped galaxies and in high-redshift objects. This DLA is well known for having one of the lowest metal abundances and dust content and the lowest fractional abundance of molecular hydrogen The measured Ar abundance is [Ar/H] \[ 1.91 ^ 0.09, which is equal to the abundances of the H 2 . other a-chain elements (O, S, and Si). The similarity of the Ar abundance with the other a-chain elements implies the absence of signi—cant photoionization by either UV background or stellar sources along the sight line throughout the damped Lya system. Both log (Ar/O) and log (Ar/S) ratios are found close to those measured in the extragalactic H II regions and in blue compact galaxies where O is more abundant by at least 1 order of magnitude. This strengthens the universality of the Ar/O and Ar/S ratios and lends support to the existence of a universal IMF. The abundance of the nonrefractory element phosphorus [P/H] \[ 2.31 ^ 0.10 con—rms the low amount of chemical evolution in the DLA. This is the measurement of P in the most metal-poor material and shows a subsolar [P/Fe] \[ 0.27 value. The measured ratios [P/Si] \[ 0.40 ^ 0.13 and [P/S] \[ 0.40 ^ 0.13 provide evidence for a mild odd-even eUect. Finally, a stringent upper limit to the population of the level in the ground state of O I is 3P 1 derived, which provides a lower limit to the physical dimensions of the system of L [ 7p c. z abs 3.3901
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