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xyc_2025_5_30

 

BTOF comparison between BFC production vs. BFC+Afterburner (MuDst->picoDst) production

 Currently in STAR, there are two ways of producing picoDst data used for physics analysis.

Run XXIII AuAu200GeV dE/dx calibration with P24iy_calib sample

 

Update: C(k*) and sideband correlations, effect of merged tracks with Run 16 Au+Au, 200 GeV data

hypernuclei analysis status

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Supporting-materials

Run XXI OO200GeV dE/dx recalibration with P24iy_calib sample

 

Directed flows of light nuclei across large rapidities (from mid-rapidity to beam rapidity) in FXT and COL Au Au Collisions

 

V0(pT) in Au+Au collisions at 3 GeV

 

v0_pt_at_11p5_GeV

 

Paper proposal: Observation of Strong ϕ meson Directed Flow at High Baryon Density Region