The archive's default-parameter rows leave sy_dist blank for 100 planets, TRAPPIST-1's seven among them, so the matcher could not place a host the catalogue had drawn since the Gaia nearby query (Gaia DR3 2635476908753563008, 12.47 pc). fetchExoplanets now also reads the Planetary Systems Composite table (pscomppars) and fills a default row's blank host cells from it. Only host columns: a composite row takes each column from its own reference, so orbits still come from the default row alone, one fit per planet. Where both tables give a distance or a position they agree on all 6 225 and 6 352 rows. Three hosts the catalogue holds by name failed the distance ratio test because the archive's sy_dist, from TICv8, contradicts its own parallax: Lalande 21185 (GJ 411) 5.68 pc against 392 mas, Luyten's Star (GJ 273) 5.92 against 263 mas, Struve 2398 B (Gl 725 B) 6.84 against 285 mas. resolveHostStarId now takes the archive's parallax (sy_plx) as a second distance the ratio test accepts. It is a second chance, not a replacement: 47 of 5 959 systems disagree past the tolerance, and for faint far hosts the inverse parallax is the worse figure (K2-238: 538 pc by sy_dist, 6 779 by parallax). Planets on a catalogue star: 2 071 -> 2 090 of 6 354. The 19 gained are TRAPPIST-1 (7), GJ 273 (2), GJ 411 (2), Gl 725 B, HD 62509 (Pollux), K2-65, TOI-2267 A and B, and two brown-dwarf hosts, 2MASS J02192210-3925225 and DENIS-P J082303.1-491201. No planet lost or changed its host. A matched host whose catalogue name is a bare Gaia designation now takes the archive's host name, so search finds TRAPPIST-1, Teegarden's Star, TOI-700, LP 791-18 and K2-18: 575 stars renamed. validateExoplanets refuses a host that is still only a designation, and the star assets are rewritten after the exoplanets for that reason; stars.bin and stars-meta.bin are unchanged. TOI-2267 A and B both land on one Gaia entry, which takes the name TOI-2267 A. Each planet also carries its host's radius, effective temperature and luminosity (10^st_lum), and a mass for 6 344 planets instead of 5 474, from the default row where it gives one and the composite table otherwise, for the star-physics step. Co-Authored-By: Claude Opus 5.5 (1M context) <noreply@anthropic.com>
210 lines
8.9 KiB
TypeScript
210 lines
8.9 KiB
TypeScript
import { writeFileSync } from 'node:fs';
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import { mergeStarCatalogues, placementDistancePc } from '../../src/app/shared/astro/star-merge';
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import { encodeStarCatalog } from '../../src/app/shared/models/star-catalog';
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import { StarRecord, SUN_STAR_ID } from '../../src/app/shared/models/star.model';
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import { fetchGaiaDistancesByHip, GaiaAnswerError } from './sources/gaia';
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import { positionalSources } from './sources/registry';
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import { PARALLAX_PRECISION_MAS } from './sources/star-sources';
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import { parseCsvObjects, parseOptionalNumber } from './lib/csv';
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import { fetchTextCached } from './lib/http';
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import { dataPath, ensureDataDir } from './lib/paths';
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const HYG_CSV_URL = 'https://raw.githubusercontent.com/astronexus/HYG-Database/main/hyg/CURRENT/hygdata_v41.csv';
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const HYG_UNKNOWN_DISTANCE_PC = 100000; // HYG's placeholder for unmeasured/unreliable parallax
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/**
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* Stand-in magnitude for a star with no photometry. Faint rather than 0, because 0 would mean
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* "as bright as Vega" and render it as one of the largest points on the map.
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*/
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const UNKNOWN_MAGNITUDE = 15;
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/**
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* Stars either survey places within this distance (parsecs) of the Sun are kept for the galaxy
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* view, and every naked-eye star wherever it is; `placementDistancePc` decides which distance a
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* kept star is drawn at.
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*
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* Set at the range Hipparcos's own measurements reach rather than at a round number: its
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* parallaxes are good to roughly a milliarcsecond, so at 250 pc (4 mas) a distance is uncertain
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* by some tens of per cent. That is why it is not applied to the Hipparcos distance alone:
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* Gaia puts 6 833 of the stars Hipparcos places inside it outside, and 3 666 the other way
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* round. Only the *radial* placement blurs; a star's direction on the sky stays exact.
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*
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* The catalogue is also magnitude-limited, so this is not a volume-complete sample beyond about
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* 50 pc: it thins to the intrinsically bright, which is the same selection the naked eye makes.
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*/
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const DISTANCE_CUTOFF_PC = Number(process.env['ETL_STAR_DISTANCE_PC'] ?? 250);
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function resolveName(row: Record<string, string>): string {
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if (row['proper']) {
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return row['proper'];
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}
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if (row['bayer'] && row['con']) {
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return `${row['bayer']} ${row['con']}`;
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}
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if (row['flam'] && row['con']) {
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return `${row['flam']} ${row['con']}`;
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}
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if (row['hd']) {
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return `HD ${row['hd']}`;
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}
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if (row['gl']) {
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// Already a complete designation ("Gl 581", "GJ 3512"), unlike the bare numbers in `hd`
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// and `hip` — prefixing it again produced 2331 stars named "Gl GJ 1076", which broke
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// search, the on-screen labels, and exoplanet host-star name matching alike.
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return row['gl'];
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}
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if (row['hip']) {
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return `HIP ${row['hip']}`;
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}
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return `HYG ${row['id']}`;
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}
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/**
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* Downloads the HYG (Hipparcos/Yale/Gliese) stellar database, places each star along its
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* equatorial direction (epoch J2000.0) at the better of its Hipparcos and Gaia distances, keeps
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* the ones either survey puts within range, unions the other positional sources, and writes
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* `stars.bin` (packed positions) + `stars-index.json` (everything else).
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*/
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export async function fetchStars(): Promise<StarRecord[]> {
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console.log(`Fetching HYG star catalog (distance cutoff: ${DISTANCE_CUTOFF_PC} pc)...`);
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const csv = await fetchTextCached(HYG_CSV_URL, 'hygdata_v41.csv');
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const rows = parseCsvObjects(csv);
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// Not skipped when unreachable, unlike the positional sources below; see its own comment.
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const gaiaPcByHip = await fetchGaiaDistancesByHip();
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const stars: StarRecord[] = [];
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let atGaiaDistance = 0;
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let pastCutoff = 0;
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for (const row of rows) {
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const id = Number(row['id']);
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if (id === SUN_STAR_ID) {
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stars.push({ id, name: 'Sol', x: 0, y: 0, z: 0, magnitude: parseOptionalNumber(row['mag']) ?? UNKNOWN_MAGNITUDE, spectralType: row['spect'] || 'G2V', colorIndex: parseOptionalNumber(row['ci']) ?? null });
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continue;
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}
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const hygPc = Number(row['dist']);
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const hipparcosPc = Number.isFinite(hygPc) && hygPc > 0 && hygPc < HYG_UNKNOWN_DISTANCE_PC ? hygPc : undefined;
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const gaiaPc = row['hip'] ? gaiaPcByHip.get(Number(row['hip'])) : undefined;
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const magnitude = parseOptionalNumber(row['mag']) ?? UNKNOWN_MAGNITUDE;
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const distancePc = placementDistancePc(hipparcosPc, gaiaPc, magnitude, DISTANCE_CUTOFF_PC);
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if (distancePc === null) {
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continue;
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}
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// HYG's own Cartesian columns rather than its `ra`/`dec`, which are in the same frame as
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// `raDecDistanceToXyz` and would be redundant if the two agreed. They do not, for the stars
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// that move: the right ascension was carried from the Hipparcos epoch to 2000.0 without the
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// cos δ its motion needs, which puts Proxima 17.9″ from where HYG's own x/y/z — and Gaia,
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// once brought to the same epoch — have it. 1813 stars differ by over an arcsecond, and the
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// Cartesian columns are the ones Gaia agrees with for 1155 of them against 156 (one of those,
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// HIP 57146, has x/y/z 161″ from its own ra/dec and stays double).
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//
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// Only their direction is used. They sit at HYG's own distance, or at its 100 000 pc
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// placeholder where it has none, and are carried along that direction to the one chosen above.
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const x = Number(row['x']);
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const y = Number(row['y']);
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const z = Number(row['z']);
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const length = Math.hypot(x, y, z);
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if (![x, y, z].every(Number.isFinite) || length === 0) {
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continue;
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}
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const scale = distancePc / length;
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if (gaiaPc !== undefined) {
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atGaiaDistance++;
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}
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if (distancePc > DISTANCE_CUTOFF_PC) {
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pastCutoff++;
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}
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stars.push({
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id,
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name: resolveName(row),
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x: x * scale,
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y: y * scale,
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z: z * scale,
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magnitude,
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spectralType: row['spect'] || 'Unknown',
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colorIndex: parseOptionalNumber(row['ci']) ?? null,
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// Only for the Gliese-only rows, whose positions are what the merge needs the motion to see
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// past. A Hipparcos position is good to under an arcsecond; given its motion too, 15 stars
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// took their co-moving companion's Gaia entry, and the companion was kept twice.
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...(row['hip'] ? {} : { pmRaMasYr: parseOptionalNumber(row['pmra']), pmDecMasYr: parseOptionalNumber(row['pmdec']) })
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});
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}
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console.log(` kept ${stars.length} stars (of ${rows.length} in the catalog): ${atGaiaDistance} at Gaia's distance, ${pastCutoff} of them past ${DISTANCE_CUTOFF_PC} pc.`);
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const merged = await mergeWithOtherSources(stars);
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merged.sort((a, b) => a.id - b.id);
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writeStarAssets(merged);
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return merged;
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}
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/**
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* Unions HYG with every other positional source that is wired in and reachable.
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*
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* A source that cannot be reached is reported and skipped here rather than thrown, so a run still
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* gets as far as validation and says what it has. Whether that may be published is decided
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* there: `validateMerge` in build.ts refuses a catalogue Gaia contributed nothing to. A source
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* that answered with something unusable ({@link GaiaAnswerError}) is a different matter, and stops
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* the run where it happened rather than being reported later as an outage.
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*/
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async function mergeWithOtherSources(hygStars: StarRecord[]): Promise<StarRecord[]> {
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const others = positionalSources().filter((source) => source.id !== 'hyg');
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if (others.length === 0) {
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return hygStars;
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}
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const candidates = [{ sourceId: 'hyg', parallaxPrecisionMas: PARALLAX_PRECISION_MAS['hyg'], stars: hygStars }];
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for (const source of others) {
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try {
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candidates.push({
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sourceId: source.id,
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parallaxPrecisionMas: PARALLAX_PRECISION_MAS[source.id] ?? 1,
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stars: await source.fetch!()
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});
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} catch (error) {
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// An answer that cannot be worked with is not an outage: skipping it would write a
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// half-catalogue over the published assets before the merge gate got to say so.
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if (error instanceof GaiaAnswerError) {
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throw error;
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}
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console.log(` skipping ${source.name}: ${error instanceof Error ? error.message : error}`);
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}
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}
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if (candidates.length === 1) {
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return hygStars;
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}
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const { stars, summary } = mergeStarCatalogues(candidates);
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console.log(` merged ${summary.total} stars from ${candidates.length} catalogues (${summary.duplicates} entries folded into a better-measured one):`);
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for (const [sourceId, count] of Object.entries(summary.bySource)) {
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console.log(` ${sourceId}: ${count}`);
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}
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return stars;
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}
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export function writeStarAssets(stars: StarRecord[]): void {
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ensureDataDir();
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// The layout lives in `star-catalog.ts`, which the app decodes with — one definition, so the
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// writer and the reader cannot drift.
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const { index, positions, meta } = encodeStarCatalog(stars);
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writeFileSync(dataPath('stars.bin'), Buffer.from(positions.buffer));
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writeFileSync(dataPath('stars-meta.bin'), Buffer.from(meta));
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writeFileSync(dataPath('stars-index.json'), JSON.stringify(index));
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}
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if (require.main === module) {
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fetchStars().catch((error) => {
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console.error(error);
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process.exitCode = 1;
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});
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}
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