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HSC Year 1 cosmology results with the minimal bias method: <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>HSC</mml:mi><mml:mo stretchy="false">×</mml:mo><mml:mi>BOSS</mml:mi><mml:mrow /></mml:mrow></mml:math> galaxy-galaxy weak lensing and BOSS galaxy clustering

HSC Year 1 cosmology results with the minimal bias method: <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>HSC</mml:mi><mml:mo stretchy="false">×</mml:mo><mml:mi>BOSS</mml:mi><mml:mrow /></mml:mrow></mml:math> galaxy-galaxy weak lensing and BOSS galaxy clustering

We present cosmological parameter constraints from a blinded joint analysis of galaxy-galaxy weak lensing, $\mathrm{\ensuremath{\Delta}}\mathrm{\ensuremath{\Sigma}}(R)$, and the projected correlation function, ${w}_{\mathrm{p}}(R)$, measured from the first-year HSC (HSC-Y1) data and SDSS spectroscopic galaxies over $0.15<z<0.7$. We use luminosity-limited samples as lens samples for $\mathrm{\ensuremath{\Delta}}\mathrm{\ensuremath{\Sigma}}$ and as large-scale structure tracers for ${w}_{\mathrm{p}}$ …