Photometry Skill
OfficialMeasure astronomical source fluxes.
Data & Analytics#astronomy#photometry#radio astronomy#ESE detection#flux measurement#variability detection
Authordsa110
Version1.0.0
Installs0
System Documentation
What problem does it solve?
This Skill automates the measurement of astronomical source fluxes and the detection of their variability, crucial for identifying transient astronomical events.
Core Features & Use Cases
- Adaptive Binning: Dynamically adjusts frequency channels for optimal signal-to-noise ratio (SNR) in flux measurements.
- Variability Analysis: Calculates metrics like Eta (η), V, and sigma-deviation to identify sources with changing brightness.
- Use Case: Automatically process daily radio astronomy data to detect and flag newly appearing or flaring celestial objects by analyzing their flux variations over time.
Quick Start
Run the photometry skill to process a measurement set and detect variable sources.
Dependency Matrix
Required Modules
None requiredComponents
scriptsreferences
💻 Claude Code Installation
Recommended: Let Claude install automatically. Simply copy and paste the text below to Claude Code.
Please help me install this Skill: Name: Photometry Skill Download link: https://github.com/dsa110/dsa110-contimg/archive/main.zip#photometry-skill Please download this .zip file, extract it, and install it in the .claude/skills/ directory.
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