beam_and_brightness
Convert between Jy/beam and brightness temperature (K) for a Gaussian beam, optionally using Planck inversion, and report beam areas for ALMA data.
Instructions
Convert between Jy/beam and brightness temperature (K) for a Gaussian beam, and report beam areas.
Rayleigh-Jeans: T = S c^2 / (2 k nu^2 Omega) = 1.222e6 S(Jy/beam) / (nu_GHz^2 bmaj bmin) with FWHMs in arcsec. planck=True uses the full Planck inversion T = (h nu / k) / ln(1 + 2 h nu^3 / (c^2 I_nu)) (no CMB term). direction: 'jy_to_k' (value in Jy/beam) or 'k_to_jy' (value in K). Limits: T_B equals the gas or dust temperature only for optically thick emission that fills the beam.
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": {
"value": "<value>",
"freq_ghz": "<freq_ghz>",
"bmaj_arcsec": "<bmaj_arcsec>",
"bmin_arcsec": "<bmin_arcsec>"
},
"name": "beam_and_brightness"
}
}Input Schema
| Name | Required | Description | Default |
|---|---|---|---|
| value | Yes | ||
| planck | No | ||
| freq_ghz | Yes | ||
| direction | No | jy_to_k | |
| bmaj_arcsec | Yes | ||
| bmin_arcsec | Yes | ||
| pixel_arcsec | No |