ir_excess
Computes NEOWISE infrared excess relative to a baseline photosphere epoch, reporting per-band excess flux fractions and the excess blackbody temperature from the W1/W2 ratio.
Instructions
Infrared excess in NEOWISE over a baseline (photosphere) epoch: excess flux in each band as a fraction of the star, and the blackbody temperature of the excess from its W1/W2 ratio.
Tool call template
Replace each placeholder with a value matching the input schema. Only required parameters are included; add optional parameters as needed.
{
"id": 1,
"jsonrpc": "2.0",
"method": "tools/call",
"params": {
"arguments": {
"case": "<case>",
"baseline_start": "<baseline_start>",
"baseline_end": "<baseline_end>",
"start": "<start>",
"end": "<end>"
},
"name": "ir_excess"
}
}Input Schema
| Name | Required | Description | Default |
|---|---|---|---|
| end | Yes | ||
| case | Yes | ||
| start | Yes | ||
| baseline_end | Yes | ||
| baseline_start | Yes |