ALPHA ``tracks'' are stored in the internal ALPHA bank QVEC.
If the FRF0 card is present in the ALPHA cards file, the NR=0 version of the FRFT bank (track parameters determined without vertex detector coordinates) will be used. Otherwise, the NR=2 version of FRFT (TPC + ITC + VDET tracks) will be used. Only FRFT NR=2 tracks are available on the MiniDST.
For physics analysis with optimised energy resolution, one should better use the Energy Flow objects (see below).
Calorimeter objects can be any of the following:
``REconstructed'' objects are:
See Section 7.5.1 for comments on the daughters of standard V0s.
Charged tracks outgoing from reconstructed DeCay vertices. The momenta for these tracks are calculated relative to the secondary vertex position.
Caution: this section includes only the daughter tracks from reconstructed standard V0s from YV0V, and not from the ``Long V0s'' coming from the new tracking with JULIA version 302 and after (see below).
``Long V0s'' (coming from the new tracking with JULIA version 302 and after). One gets the loop limits for them through the following subroutine call:
CALL QLV0T(KFLVT,KLLVT)
This section includes selected charged tracks and ECAL and HCAL clusters remaining after subtracting track energies. These objects may also be accessed with their particle name `EFLW' using the functions KPDIR and KFOLLO (described in 7.4). This section is not filled unless the EFLW card is included in the card file (see Ch. 11).
Energy Flow objects made with the ENFLW package (see Chapter 11) should be used for all analyses which need an optimised calorimeter energy resolution.
Neutral objects derived from the PCPA bank. These objects may also be accessed with their particle name `NEOB' using the functions KPDIR and KFOLLO (described in 7.4). To be used only by experts.
These objects may also be accessed with their particle name `GAMP' using the functions KPDIR and KFOLLO (described in 7.4).
Jets based on EFLW objects using QJMMCL with YCUT = 0.003. These objects may also be accessed with their particle name `EJET' using the functions KPDIR and KFOLLO (described in 7.4). They may be used as input for jet finding with a higher YCUT (see 10.11.1 and 11.1).