Strong-field ionization is central to intense laser-matter interactions. However, standard ionization measurements have been limited to extremely low density gas samples, ignoring potential high density effects. Here, we measure strong-field ionization in atmospheric pressure range air, N2 and Ar over 14 decades of absolute yield, using mid-IR picosecond avalanche multiplication of single electrons. Our results are consistent with theoretical rates for isolated atoms and molecules and quantify the ubiquitous presence of ultra-low concentration gas contaminants that can significantly affect laser-gas interactions.The unification of tunneling ionization and multiphoton ionization (MPI) of atoms in intense laser fields by Keldysh in 1965 [1] provided an analytic foundation for strong field laser physics [2-6], but measurements of the transition from MPI to tunneling had to await later advances in short pulse lasers [7][8][9][10]. This transition is characterized in atomic units by the dimensionless Keldysh parameter = 2 ⁄ / , where is the atom's ionization potential, is the peak laser field, and is the laser frequency. At moderate intensity ( ≫ 1, MPI regime), the yield is proportional to (∝ ), while at higher intensities or longer wavelengths ( < 1), the transition to tunneling and barrier suppression ionization [7,9] is characterized by ∝ , where is the integer number of photons needed to exceed . These early measurements were conducted in extremely low density gases (typically ~10 8 −10 12 cm −3 ) in order to prevent ionization products interacting with background gas or experiencing space charge effects in transit to high voltage detectors [7,9,11]. However, many applications of strong-field ionization, such as high harmonic