<?xml version="1.0" encoding="UTF-8"?><xml><records><record><source-app name="Biblio" version="7.x">Drupal-Biblio</source-app><ref-type>10</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Imen, Chairat</style></author><author><style face="normal" font="default" size="100%">Fouad, DJAIZ</style></author><author><style face="normal" font="default" size="100%">Mabrouk, Boughdiri</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Reconsideration of the Cenomanian-Turonian stratigraphics units in the Tebessa region (Algero-TunisienConfines): Petroleum implications</style></title><secondary-title><style face="normal" font="default" size="100%">The 1st National Seminar in Geosciences and Environment (SGSE 2019)</style></secondary-title></titles><dates><year><style  face="normal" font="default" size="100%">2019</style></year><pub-dates><date><style  face="normal" font="default" size="100%">2019</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">https://www.researchgate.net/publication/337011266_Reconsideration_of_the_Cenomanian-Turonian_stratigraphic_units_in_the_Tebessa_region_Algero-Tunisian_Confines_Petroleum_implications</style></url></web-urls></urls><pub-location><style face="normal" font="default" size="100%">Tamanrasset, Algeria</style></pub-location><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">&lt;p style=&quot;text-align: justify;&quot;&gt;
	The Algero-Tunisian confines (Tebessa region) is partially composed of Cenomano- Turonian carbonate outcrops; therefore, it presents a good example to highlight the black shale levels reported over a short period, around the Cenomanian-Turonian boundary. The lithostratigraphic study made it possible to specify the paleoenvironment during the Cenomano-Turonian in the Tebessa region. At that time, the depositional environment emphasized a relatively deep, calm and often confined ocean environment that was significantly shalloweron the north part of the study area. The lithology and the distribution of the facies in the Constantine domain allow us to underline the pelagic influences during the Upper Cretaceous and neritic during the lower Cretaceous period. We note a maximum thickness of the Cenomano- Turonian in the southern zones and a minimum (100m) appears further north. This Palaeogeographic organization continue laterally in Tunisia on the extension of the Constantine mole.
&lt;/p&gt;
</style></abstract></record></records></xml>