Active Galactic Nuclei are the dominant sources of gamma rays outside our Galaxy and also candidates for being the source of ultra-high energy cosmic rays. In addition to being emitters of broad-band non-thermal radiation throughout the electromagnetic spectrum, their emission is highly variable on timescales from years to minutes. Hence, high-cadence monitoring observations are needed to understand their emission mechanisms. The Africa Millimetre Telescope is planned to be the first mm-wave radio telescope on the African continent and one of few in the Southern hemisphere. Further to contributing to the global mm-VLBI observations with the Event Horizon Telescope, substantial amounts of observation time will be available for monitoring observations of Active Galactic Nuclei. Here we review the scientific scope of the Africa Millimetre Telescope for monitoring of Active Galactic Nuclei at mm-wavelengths. PACS: 95.85.Bh; 98.54.Cm; 98.54.Gr; 98.62.Nx
IntroductionActive Galactic Nuclei (AGN) and more particularly the subclass of blazars have been a major topic of research throughout the electromagnetic spectrum for the past fifty years. Despite significant progress in understanding the blazar phenomenon [1], many open questions remain. Several apparent differences could be attributed to their non-spherical structure and the orientation of the highly relativistic jets relative to the line of sight [2]. Still, the underlying particle acceleration and emission processes remain a matter of current research. Connected to the more than one hundred years of quest for the sources of the highest-energetic cosmic rays, hadronic emission scenarios are tested, e.g. [3,4], and recent coincident gamma-ray and neutrino detections point in that direction [5]. Even though, hadronic emission scenarios are not uncontested, as also the leptonic Synchrotron Self-Compton (SSC) model [6] is highly successful in explaining the broad-band spectral energy distribution (SED) for blazars, see e.g. [7]. AGN are variable on all time scales: from optical quasi-periods of several years [8] down to gamma-ray flares lasting only minutes [9] and even limiting the size of the emission region to be smaller than 20% of the gravitational radius of the central black hole [10]. This motivates intensive efforts for monitoring the variability of AGN across the electromagnetic spectrum.Following recent positive developments of astronomy in Africa in general [11] and Namibia in particular [12], the Africa Millimetre Telescope (AMT) project aims to build a mm-wave radio telescope in Namibia [13]. It will be the first telescope of its kind on the African continent and one of only few in the Southern hemisphere. The proposed site for the AMT is Mt. Gamsberg (23.34 • S, 16.23 • E) in the Khomas Highlands of Namibia, at a height of 2,347 m a.s.l. At very similar latitude to ALMA, this