ASTR 472 · Lecture 07

Lecture 07: Calibration I: Complex Gains and Bandpass

Radio Astronomy

Calibration solves for antenna-based complex gains by comparing measured correlations with a source model.

Objectives and route

  1. Write the interferometric measurement equation for antenna gains.
  2. Distinguish flux-scale, phase, delay, bandpass, and polarization calibration.
  3. Estimate coherence loss from random residual phase.

Route: identify what the receiver measures, derive the physical/instrument relation, calculate a scale, then test its assumptions against a diagnostic.

Terms for This Lecture

Complex gain

Definition: Antenna-based amplitude and phase response that multiplies the true electric-field correlation.

Why it matters here: It is needed to answer If residual phase rms doubles from 10 degrees to 20 degrees, does coherence loss double? Compute or reason from the exponential form. and to interpret A baseline visibility is multiplied by one antenna gain and the complex conjugate of the other.

Relationships: Use it with Phase calibrator and Bandpass; the lecture model is \(V_{pq}^{\rm obs}(\nu,t)=g_p(\nu,t)g_q^*(\nu,t)V_{pq}^{\rm true}(\nu,t)+n_{pq}\).

Boundary or common confusion: A wrong calibrator model can transfer systematic error to every target. The phase-coherence approximation assumes zero-mean Gaussian residual phase and does not model direction-dependent structure.

Observation before interpretation

Calibration solves for antenna-based complex gains by comparing measured correlations with a source model.

Keep four layers distinct in your notebook: raw correlation or spectrum, calibrated product, model parameter, and physical claim.

Physical model

For antennas p and q, V_pq^obs=g_p g_q* V_pq^true+n_pq. With g=a exp(i phi), phase differences and amplitude products are coupled across baselines, so solve a connected antenna graph against a calibrator model. Bandpass calibration estimates frequency dependence; delay is the phase slope dphi/dnu divided by 2 pi.

\(V_{pq}^{\rm obs}(\nu,t)=g_p(\nu,t)g_q^*(\nu,t)V_{pq}^{\rm true}(\nu,t)+n_{pq}\)

Define each quantity and convention before substitution. A relation is useful only inside its stated regime.

Worked calculation

Inputs: Gaussian residual phase rms=10 deg.

coherence = 0.9849

A wrong calibrator model can transfer systematic error to every target. The phase-coherence approximation assumes zero-mean Gaussian residual phase and does not model direction-dependent structure.

Independent audit: carry SI units through the derivation, then check the limiting direction and scale.

Read the geometry or data relation

observed phasemodel-corrected phasegain amplitude and phase are solved together
A baseline visibility is multiplied by one antenna gain and the complex conjugate of the other.

Identify what is directly encoded in the figure and which inference requires an instrument model or physical assumption.

Where the inference can fail

A wrong calibrator model can transfer systematic error to every target. The phase-coherence approximation assumes zero-mean Gaussian residual phase and does not model direction-dependent structure.

Reasoning prompt

If residual phase rms doubles from 10 degrees to 20 degrees, does coherence loss double? Compute or reason from the exponential form.

Write the predicted scaling first; then identify which measurement would falsify it.

Connection to the observing workflow

This lecture feeds into the paired lab: Complex Gain Calibration and Error Propagation. Preserve the raw-to-calibrated-to-inferred chain and carry the same units and assumptions into the analysis.

For a real observation, archive the project identifier, correlator setup, antenna configuration, calibration version, flags, beam, and data-release citation.

Synthesis

Calibration I: Complex Gains and Bandpass is one stage in a measurement chain: celestial signal → antenna and receiver → sampled data → calibration → image/spectrum → uncertainty-aware inference.

Next: connect this result to Calibration II: Error Budgets and Imaging Systematics.

References and scope

NRAO VLA calibration-pipeline documentation and ALMA data-processing documentation; OpenStax §6.4 does not cover calibration equations.

Primary/authoritative material and provenance levels are recorded in ../reference-log.md. Numeric examples are reproducibly calculated by ../src/generate_astr472_package.py; figure geometry is original and lecture-specific.