Tracking Efficiency Uncertainty meeting

2024-11-05 10:00
2024-11-05 11:00
America/New York
Tuesday, 5 November 2024
https://bnl.zoomgov.com/j/1607035037?pwd=WDVqaEdwa0RtTEM5a1VvZ24yU2gwdz09, at 15:00 (GMT), duration : 01:00

Tracking Efficiency Uncertainty meeting

2024-11-19 10:00
2024-11-19 11:00
America/New York
Tuesday, 19 November 2024
https://bnl.zoomgov.com/j/1607035037?pwd=WDVqaEdwa0RtTEM5a1VvZ24yU2gwdz09, at 15:00 (GMT), duration : 01:00
TimeTalkPresenter
10:00Final results from 2019 19GeV AuAu SL23f ( 00:20 ) 1 file

Tracking Efficiency Uncertainty meeting

2024-11-12 10:00
2024-11-12 11:00
America/New York
Tuesday, 12 November 2024
https://bnl.zoomgov.com/j/1607035037?pwd=WDVqaEdwa0RtTEM5a1VvZ24yU2gwdz09, at 15:00 (GMT), duration : 01:00

Tracking Efficiency Uncertainty meeting

2024-10-29 10:00
2024-10-29 11:00
America/New York
Tuesday, 29 October 2024
https://bnl.zoomgov.com/j/1607035037?pwd=WDVqaEdwa0RtTEM5a1VvZ24yU2gwdz09, at 14:00 (GMT), duration : 01:00

Tracking Efficiency Uncertainty meeting

2024-10-22 10:00
2024-10-22 11:00
America/New York
Tuesday, 22 October 2024
https://bnl.zoomgov.com/j/1607035037?pwd=WDVqaEdwa0RtTEM5a1VvZ24yU2gwdz09, at 14:00 (GMT), duration : 01:00

Tracking Efficiency Uncertainty meeting

2024-10-15 10:00
2024-10-15 11:00
America/New York
Tuesday, 15 October 2024
https://bnl.zoomgov.com/j/1607035037?pwd=WDVqaEdwa0RtTEM5a1VvZ24yU2gwdz09, at 14:00 (GMT), duration : 01:00

Tracking Efficiency Uncertainty meeting

2024-10-08 10:00
2024-10-08 11:00
America/New York
Tuesday, 8 October 2024
https://bnl.zoomgov.com/j/1607035037?pwd=WDVqaEdwa0RtTEM5a1VvZ24yU2gwdz09, at 14:00 (GMT), duration : 01:00

Tracking Efficiency Uncertainty meeting

2024-10-01 10:00
2024-10-01 11:00
America/New York
Tuesday, 1 October 2024
https://bnl.zoomgov.com/j/1607035037?pwd=WDVqaEdwa0RtTEM5a1VvZ24yU2gwdz09, at 14:00 (GMT), duration : 01:00

Isolating continuum $\gamma\gamma \rightarrow \pi^+\pi^-$ production via entanglement enabled spin interference effects

 In ultra-peripheral heavy ion collisions,  the highly Lorentz-contracted electromagnetic fields of the nuclei can be quantized as a flux of quasi-real phot

LBNL_seminar

 

Production of K*0 and K*± in Au+Au Collisions at BES-II energies (3-19.6 GeV)

Speaker : Aswini Kumar Sahoo


Talk time : 10:40, Duration : 00:20

 

K0s production at 5.2, 6.2, and 7.2 GeV

Speaker : Li'Ang Zhang


Talk time : 10:20, Duration : 00:20

 

K+/K- production in Au+Au collosions at √S_NN=3.2GeV

Speaker : Ziyue Xiang


Talk time : 11:20, Duration : 00:20

 

K^{*0} production in Run21 Au+Au collisions at √sNN=3 GeV

Speaker : Tingbao Liu


Talk time : 10:00, Duration : 00:20

 

neutral and charged K* in O+O collisions

Speaker : Subhash Singha


Talk time : 11:00, Duration : 00:20

 

Run-by-Run phi distribution at 9.2 GeV

 

QM2025_LaLa_CF_3GeV

 

test blog 2024-10-06

test page

Quark Matter 2025

 

EPD Gate Timing Scan - transition from pp running to AuAu running

Since Mike's drupal code doesn't work for some reason, Maria has logged in and let Mike produce this drupal page under her name.


Executive Summary