Tint a star measured in Gaia's BP−RP as the B−V of the dwarf of that colour
colorIndexToRgb maps a B−V onto the star field's tint ramp, and its one caller passed it every star's colour index, whatever colorSystem said. BP−RP is the larger of the two for the same star — 0.823 against 0.65 for a G2 dwarf, 1.84 against 1.42 for an M0 (Pecaut & Mamajek) — so the 376 703 stars measured in it, 83 % of the catalogue, were tinted as later types than they are, and redder than HYG's stars of the same type, and than their own disc in the system view. A BP−RP is now carried to the B−V of the dwarf sequence at that colour (the table's own B−V column, which DwarfSequencePoint now returns, clamped at its ends), then tinted as before. The median Gaia colour, BP−RP 0.883, a G7 dwarf, read as a K2: its tint goes from (1, 0.972, 0.955) to (0.975, 0.982, 1), the same as HYG's G7 stars. Controls, each failing its named test: BP−RP read as B−V (2 of 792 failed), the star field not passing the colour system (1 of 792), and the B−V taken from the wrong column (3 of 792). Co-Authored-By: Claude Opus 5.5 (1M context) <noreply@anthropic.com>
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@@ -168,8 +168,8 @@ describe('dwarfSequenceAtColor', () => {
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});
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it('reads the row at the end a colour is past, when asked to', () => {
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expect(dwarfSequenceAtColor(2.2, 'B-V', true)).toEqual({ temperatureK: 2420, bolometricCorrectionV: -5.78, gMinusV: -3.09 });
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expect(dwarfSequenceAtColor(-0.15, 'BP-RP', true)).toEqual({ temperatureK: 10700, bolometricCorrectionV: -0.42, gMinusV: 0.018 });
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expect(dwarfSequenceAtColor(2.2, 'B-V', true)).toEqual({ bMinusV: 2.16, temperatureK: 2420, bolometricCorrectionV: -5.78, gMinusV: -3.09 });
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expect(dwarfSequenceAtColor(-0.15, 'BP-RP', true)).toEqual({ bMinusV: -0.07, temperatureK: 10700, bolometricCorrectionV: -0.42, gMinusV: 0.018 });
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expect(dwarfSequenceAtColor(null, 'B-V', true)).toBeNull();
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});
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});
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