Anatomy of an eyeris Object
In eyeris: Flexible, Extensible, & Reproducible Pupillometry Preprocessing

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📦 Key Components

When preprocessing .asc EyeLink files with eyeris, returned objects will be of the class eyeris, and will contain key components used throughout the package's backend.

The key components are:

file: the original file path of the source .asc file
timeseries: a list of data frames (1 df per identified recording block per file) which contains the following columns:
block: block number
time_orig: raw tracker time (ms)
time_secs: normalized tracker time, starting at 0 (seconds)
eye_x: eye position x-coordinate
eye_y: eye position y-coordinate
eye: which eye (Left or Right) the recorded data are sourced from
hz: tracker sampling rate (hz)
type: whether source data were recorded using the diameter or area method
pupil_raw: raw recorded pupil source data in arbitrary units (a.u.)
is_resampled: logical flag marking rows that resample() inserted for dropped samples (present only when the sampling grid had to be repaired -- see the glassbox() steps below)

You'll notice that for each preprocessing step run, a new column will be added after the pupil_raw column; these new columns follow a structure where each subsequent step is appended to the previous columns name (i.e., pupil_raw_{previous steps}_{current_step}). To illustrate:

pupil_raw -> pupil_raw_deblink -> pupil_raw_deblink_detransient -> and so on...
events: a list of data frames containing trial event messages and timestamps
blinks: a list of data frames containing start/stop/durations for blinks
info: EyeLink EDF header data parsed into a data frame
latest: internal tracker used for assessing which steps have been run so far
confounds: a list of data frames containing confounding variables for each preprocessing step (see: 📊 summarize_confounds())
params: detailed list of steps run and parameters passed to each step
epoch_{name}: list of data frames for any given epoched timeseries

💡 Note: This vignette describes the structure of an `eyeris` object as returned by the main preprocessing pipeline. 1. Understanding these components will help you interpret results, debug issues, and extend the pipeline for your own research needs. 2. Furthermore, binocular data will have a `left` and `right` component to the `eyeris` object, which will contain the same components as the main `eyeris` object. 3. There is also a phantom `raw_binocular_object` component to the `eyeris` object, which contains the raw binocular data used internally to perform the binocular correlation analysis and plotting.

Now that we've explained what you can expect to see after running the eyeris glassbox() function, we'll demonstrate what the glassbox() wrapper is generally comprised of in terms of the steps and defaults that are implemented.

🧱 Building Blocks Under the Hood

While we strongly recommend against manually constructing the pipeline as will be shown below (given that using the glassbox() will provide maximum opportunities for reproducibility and reduction of accidental errors), more advanced users may want to see how the individual steps can be used like building blocks to iteratively test out parameters, switch steps around / remove steps (again, we strongly recommend against doing this unless you know what you're doing), etc.

The Default `glassbox()` Steps and Parameters, Deconstructed:

The chunk below is the complete, end-to-end reference pipeline. It reproduces the default glassbox() recipe step-by-step, with every eyeris preprocessing function chained together exactly as the wrapper calls them internally. Use it as a copy-paste template whenever you need to inspect, reorder, or swap out individual steps (e.g., during parameter optimization):

system.file("extdata", "memory.asc", package = "eyeris") |>
  eyeris::load_asc(block = "auto") |>
  eyeris::resample() |>  # repair the sampling grid (no-op on uniform data)
  eyeris::deblink(extend = 50) |>
  eyeris::detransient(n = 16) |>
  eyeris::interpolate() |>
  eyeris::lpfilt(wp = 4, ws = 8, rp = 1, rs = 35, plot_freqz = TRUE) |>
  # eyeris::downsample(target_fs = 100) |>  # optional (read docs before enabling)
  # eyeris::bin(bins_per_second = 10) |>  # optional (read docs before enabling)
  # eyeris::detrend() |>  # optional (read docs before enabling)
  eyeris::zscore() |>
  eyeris::summarize_confounds()

Each line above maps directly to one exported preprocessing function. Click any function below to jump to its help page, where you'll find its parameters and a worked example:

| Step | Function | What it does | |------|----------|--------------| | 1. Load | eyeris::load_asc() | Parse the raw .asc file into an eyeris object | | 2. Resample | eyeris::resample() | Place each block on the expected uniform sampling grid (repair dropped samples; no-op if already uniform) | | 3. Deblink | eyeris::deblink() | NA-pad samples surrounding blink artifacts | | 4. Detransient | eyeris::detransient() | Remove physiologically implausible jumps | | 5. Interpolate | eyeris::interpolate() | Linearly fill in missing samples | | 6. Lowpass filter | eyeris::lpfilt() | Smooth the pupil time series | | (optional) Downsample | eyeris::downsample() | Decimate to a lower sampling rate (anti-aliased) | | (optional) Bin | eyeris::bin() | Average samples within fixed time bins | | (optional) Detrend | eyeris::detrend() | Remove a linear or spline trend from the time series | | 7. Z-score | eyeris::zscore() | Standardize to mean 0 and SD 1 | | (summary) Confounds | eyeris::summarize_confounds() | Tabulate per-step data-quality metrics |

💡 Note: downsample() and bin() are mutually exclusive (enable at most one), and detrend() is disabled in the default glassbox() recipe. See each function's help page for guidance before enabling these optional steps.

💡 **For more detailed information on the implementation of functions within** **the `glassbox()` and thus how to create your own custom pipeline** **extensions that conform to the `eyeris` protocol, see the:** [🧩 Building your own Custom Pipeline Extensions vignette](custom-extensions.html).