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1 Trigonometric Parallaxes William van Altena Yale University Basic Astrometric Methods Yale University July 18-22, 2005
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2 The Geometry
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3 More Geometry
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4 Yes, the Earth moves around the Sun!
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5 Parallactic motion in Ecliptic Coords
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6 The Parallactic Ellipse
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7 Parallax in RA and Dec
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8 Parallax in RA and Dec (cont.)
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9 Observational Techniques
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10 Maximum Parallax Factor
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11 Ecliptic Latitude Dependence
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12 Determination of π & µ
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13 Typical analysis “pipeline”
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14 Typical analysis “pipeline” (cont.)
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15 Solving for a single π
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16 Errors and weights
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17 Errors and weights (cont.)
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18 Errors and weights (cont.)
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19 Reference stars
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20 Atmospheric Refraction
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21 Effective wavelength of each star
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22 Refraction versus star color
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23 Correction to Absolute π
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24 Systematic errors
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25 External error sources
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26 Deriving external errors
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27 Parallax Programs CatalogDate#stars mas) Comments YPC19958112±15 masCat. of all π through 1995 USNO pgTo 1992~1000±2.5 masPhotographic parallaxes USNO ccdFrom ‘92~150±0.5 masCCD parallaxes Nstars & GBCurrent100?± 2 masSouthern π programs Hipparcos199710 5 ±1 masFirst modern survey HST FGS1995-2010?100?±0.5 masA few important stars SIM2016?10 3 ±4 µasCritical targets & exoplanets Gaia2016?10 9 ±10µas“Ultimate” modern survey
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28 References for Parallax Programs CatalogCommentsReferences YPCCat. of all π through 1995van Altena, Lee & Hoffleit 1995 USNO pgPhotographic parallaxesDahn, Harrington, et al USNO ccdCCD parallaxesMonet, Dahn, et al. AJ,103,638,1992 Nstars & GBSouthern π programsHenry, Jao, Ianna, Costa, Mendez, … HipparcosFirst modern surveyESO HST FGSA few important starsBenedict & HST FGS Team SIMCritical targets & Exo-planetsNASA/JPL Gaia“Ultimate” modern surveyESO
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