PoS(ICRC2017)776 Monitoring at TeV Energies with M@TE Ruben Alfaro a* , Abel Bernal b , Thomas Bretz c , Simone Dichiara b , Daniela Dorner d , Fernando Garfias b , María Magdalena González b , David Hiriart b , Arturo Iriarte b , Elena Jimenez b , Luis Artemio Martínez b , Lukas Nellen e , Ibrahim Torres f , Gagik Tovmasian b , a Instituto de Física, Universidad Nacional Autónoma de México, México D.F., México b Instituto de Astronomía, Universidad Nacional Autónoma de México, México D.F., México c RWTH Aachen University, Physics Institute III A, Aachen, Germany d Universität Würzburg, Institute for Theoretical Physics and Astrophysics, Würzburg, Germany e Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, México D.F., México f Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, México E-mail: ruben@fisica.unam.mx Blazars are extremely variable objects emitting radiation across the electromagnetic spectrum and showing variability on time scales from minutes to years. Simultaneous multi-wavelength obser- vations are crucial for understanding the emission mechanisms. In particular the study of their TeV emission is relevant to test the dominant radiative process at such energies (e.g. leptonic models predict a correlation between X-ray and TeV emission). As well, the correlation with the bump at low energy or the possible common detection with a neutrino signal can be relevant to constrain the physical model. From radio via optical and from X-ray to gamma rays, a variety of instruments, as OVRO and Fermi, are already monitoring blazars. At TeV energies, long-term monitoring is currently carried out by HAWC and FACT. Towards 24/7 continuous observations, the goal is to have similar monitoring telescopes at locations around the globe in order to close temporal gaps and compile light curves with homogeneous sensitivity. With the M@TE (Moni- toring at TeV energies) project, we are planning to install an Imaging Air Cherenkov Telescope equipped with an improved version of the FACT camera and the mechanical structure of one of the mounts of the HEGRA experiment at the site of San Pedro Mártir in Mexico. Featuring excellent observation conditions, this location provides a variety of instruments from radio to op- tical wavelength allowing for coordinated multi-wavelength blazar studies. In this work, we will present the status of the project. 35th International Cosmic Ray Conference — ICRC2017 10–20 July, 2017 Bexco, Busan, Korea * Speaker. c  Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0). http://pos.sissa.it/