largest_angular_scale
Compute maximum recoverable angular scale and resolution from baseline lengths or visibility data, using ALMA Handbook formulas for both legacy and current conventions.
Instructions
Maximum recoverable scale (MRS) and angular resolution from baseline lengths.
Gives both conventions: the older ALMA Technical Handbook / Wilner and Welch (1994) form theta_MRS ~ 0.6 lambda / B_min, and the current Handbook form theta_MRS ~ 0.983 lambda / L05 with L05 the 5th percentile baseline; resolution ~ 0.574 lambda / L80 (80th percentile). The Handbook percentiles are over unique antenna pairs. Input: baselines_m (one projected length in metres per antenna pair), or a visibility file (u, v; with antenna id columns ant1/ant2 the percentiles use each pair's mean length, otherwise they are over visibility rows and say so), or just b_min_m (then only the 0.6 form). Limits: these are rules of thumb for smooth structure; flux on scales near the MRS is already partly lost (use flux_recovery for a model estimate) and the actual MRS depends on uv coverage and imaging.
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": {
"freq_ghz": "<freq_ghz>"
},
"name": "largest_angular_scale"
}
}Input Schema
| Name | Required | Description | Default |
|---|---|---|---|
| b_min_m | No | ||
| uv_unit | No | lambda | |
| freq_ghz | Yes | ||
| vis_path | No | ||
| baselines_m | No |