This paper describes the algorithms for the reconstruction and identification of electrons in the central region of the ATLAS detector at the Large Hadron Collider (LHC). These algorithms were used for all ATLAS results with electrons in the final state that are based on the 2012 pp collision data produced by the LHC at  = 8 TeV. The efficiency of these algorithms, together with the charge misidentification rate, is measured in data and evaluated in simulated samples using electrons from Z → ee, Z → eeγ and J/ψ → eedecays.
For these efficiency measurements, the full recorded data set, corresponding to an integrated luminosity of 20.3 fb-1, is used. Based on a new reconstruction algorithm used in 2012, the electron reconstruction efficiency is 97% for electrons with ET = 15 GeV and 99% at ET = 50 GeV. Combining this with the efficiency of additional selection criteria to reject electrons from background processes or misidentified hadrons, the efficiency to reconstruct and identify electrons at the ATLAS experiment varies from 65 to 95%, depending on the transverse momentum of the electron and the background rejection.
Electron isolation
In order to further reject hadronic jets misidentified as electrons, most analyses require electrons to pass some isolation requirement in addition to the identification requirements described above. The two main isolation variables are:
Calorimeter-based isolation: The calorimetric isolation variable EconeΔRT is defined as the sum of the transverse energy deposited in the calorimeter cells in a cone of size ΔR around the electron, excluding the contribution within Δη × Δϕ= 0.125 × 0.175 around the electron cluster barycentre. It is corrected for energy leakage from the electron shower into the isolation cone and for the effect of pile-up using a correction parameterized as a function of the number of reconstructed primary vertices.
Track-based isolation: The track isolation variable pconeΔRT is the scalar sum of the transverse momentum of the tracks with pT > 0.4 GeV in a cone of ΔR around the electron, excluding the track of the electron itself. The tracks considered in the sum must originate from the primary vertex associated with the electron track and be of good quality; i.e. they must have at least nine silicon hits, one of which must be in the innermost pixel layer.
Both types of isolation are used in the tag-and-probe measurements, mainly in order to tighten the selection criteria of the tag.
Whenever isolation is applied to the probe electron candidate in this work, this only happens in the J/ψ analysis, the criteria are chosen such that the effect on the measured identification efficiency is estimated to be small.
Max The efficiency εID of the algorithms used by ATLAS to identify photons during the LHC Run 1 has been measured from pp collision data using three independent methods in different photon ET ranges. The three measurements agree within their uncertainties in the overlapping ET ranges, and are combined.
For the data taken in 2011, 4.9 fb-1 at s√=7 TeV, the efficiency of the cut-based identification algorithm increases from 60– 70% at ET = 20 GeV up to 87–95% (90–99%) at ET > 100 GeV for unconverted (converted) photons. With an optimised neural network this efficiency increases from 85–90% at ET = 20 GeV to about 97% (99%) at ET > 100 GeV for unconverted (converted) photon candidates for a similar background rejection. For the data taken in 2012, 20.3 fb-1 at s√=8 TeV, the efficiency of a re-optimised cut-based photon identification algorithm increases from 50–65% (45–55%) for unconverted (converted) photons at ET = 10 GeV to 95–100% at ET > 100 GeV, being larger than ≈ 90% for ET > 40 GeV.
The nominal MC simulation of prompt photons in ATLAS predicts significantly higher identification efficiency values than those measured in some regions of the phase space, particularly at low ET. A simulation with shower shapes corrected forthe average shifts observed with respect to the data describes the values of εID better in the entire ET and η range accessible by the data-driven methods. The residual difference between the efficiencies in data and in the corrected simulation are taken into account by computing data-to-MC efficiency scale factors. These factors differ from one by up to 10% at ET = 10 GeV and by only a few percents above ET = 40 GeV, with an uncertainty decreasing from 1.4–4.5% (1.7– 5.6%) at ET = 10 GeV for unconverted (converted) photons to 0.2–0.8% (0.2–0.5%) at high ET for s√=8 TeV. The uncertainties are slightly larger for s√=7 TeV data due to the smaller size of the control samples.