Gain-Only Calibration Skill

Calibrate radio astronomy mosaic tiles by reusing bandpass solutions with GPU-accelerated sky model prediction.

Updated Aug 27, 2026
One-click install
npx skills add https://github.com/dsa110/dsa110-contimg --skill gain-only-calibration-skill
Or copy as Structured Prompt for Agent
Please help me install this Agent Skill.
Skill: Gain-Only Calibration Skill
Source: https://github.com/dsa110/dsa110-contimg/tree/main/backend/.github/skills/gain-only-calibration
Command: npx skills add https://github.com/dsa110/dsa110-contimg --skill gain-only-calibration-skill

SYSTEM DOCUMENTATION & REQUIREMENTS

💡 This Skill includes scripts (resource) and references (resource) components.

What problem does it solve?

This Skill streamlines the calibration process for radio astronomy mosaic observations by reusing existing bandpass solutions, significantly reducing computation time for subsequent tiles.

Core Features & Use Cases

  • Reuses Bandpass Solutions: Leverages pre-existing bandpass calibration tables, avoiding redundant calculations.
  • Multi-Source Sky Model Prediction: Builds and populates a sky model using efficient GPU-accelerated prediction with fallbacks.
  • Optimized for Mosaics: Designed specifically for scenarios where bandpass calibration is stable across multiple observations.

Quick Start

Use the gain-only calibration skill to calibrate a science field using an existing bandpass solution.

Frequently Asked Questions about Gain-Only Calibration Skill

High-intent search queries and answers about installing and using this skill.

FAQPage Schema
How do I perform gain-only calibration for radio astronomy mosaic observations?

Gain-only calibration for radio astronomy mosaic observations is performed by reusing existing bandpass solutions and employing GPU-accelerated sky model prediction to calibrate sequential mosaic tiles efficiently.

Why does gain-only calibration reduce processing time for sequential mosaic tiles?

Gain-only calibration reduces processing time for sequential mosaic tiles by assuming bandpass stability and avoiding redundant bandpass solves, which significantly cuts down required computation time and resources.

Can I use an existing bandpass solution to calibrate a science field?

Yes, you can use an existing bandpass solution to calibrate a science field. The Skill leverages pre-existing bandpass calibration tables for mosaics where bandpass calibration is stable across observations.

How does sky model prediction work in radio astronomy data processing?

Sky model prediction in radio astronomy data processing works by building and populating a sky model using GPU-accelerated prediction, which includes fallback mechanisms to ensure efficient and reliable calibration.

What are the limitations of assuming bandpass stability for mosaic imaging?

The limitation of assuming bandpass stability for mosaic imaging is that it restricts calibration to scenarios where the bandpass is stable across multiple observations, making it unsuitable for data with significant bandpass variations.

Do I need GPU acceleration for radio astronomy mosaic calibration?

GPU acceleration is not strictly required as the sky model prediction includes fallbacks, but utilizing GPU-accelerated prediction provides optimized performance and reduced processing time for radio astronomy mosaic calibration.