Spec

Codefragmenten

curl "https://api.oanor.com/telescope-api/v1/meta" \
  -H "x-oanor-key: oanor_test_..."

await fetch("https://api.oanor.com/telescope-api/v1/meta", {
  headers: { "x-oanor-key": "oanor_test_..." }
});

$ch = curl_init("https://api.oanor.com/telescope-api/v1/meta");
curl_setopt($ch, CURLOPT_HTTPHEADER, ["x-oanor-key: oanor_test_..."]);
curl_setopt($ch, CURLOPT_RETURNTRANSFER, true);
$out = curl_exec($ch);

import requests
requests.get(
    "https://api.oanor.com/telescope-api/v1/meta",
    headers={"x-oanor-key": "oanor_test_..."}
)

Voorbeeldrespons

Een echte respons van dit endpoint, vastgelegd bij de laatste health check.

{
    "data": {
        "notes": "mm, degrees, arcseconds. mag = scope FL ÷ eyepiece FL; exit pupil = aperture ÷ mag; Dawes = 116/aperture, Rayleigh = 138/aperture; limiting mag = 2.7 + 5·log10(aperture mm). For camera/thin-lens imaging use a lens API; for stellar magnitudes a star-magnitude API.",
        "service": "telescope-api",
        "endpoints": {
            "GET /v1/meta": "This document.",
            "GET /v1/exit-pupil": "Exit pupil from aperture and magnification.",
            "GET /v1/resolution": "Dawes/Rayleigh resolution and limiting magnitude from aperture.",
            "GET /v1/magnification": "Magnification, focal ratio, useful range and true field of view."
        },
        "description": "Telescope optics maths: magnification and useful range, exit pupil, and resolving power / limiting magnitude."
    },
    "meta": {
        "timestamp": "2026-06-07T08:18:03.953Z",
        "request_id": "112e00f1-f88e-44d2-ac48-7a177e1bbf4b"
    },
    "status": "ok",
    "message": "Meta",
    "success": true
}