NINJA2 data set stored in Virgo clusters:

Lyon:
cchpssvirgo:/hpss/in2p3.fr/group/virgo/NINJA2/H1_NINJA2_G1000176_EARLY_GAUSSIAN/
cchpssvirgo:/hpss/in2p3.fr/group/virgo/NINJA2/L1_NINJA2_G1000176_EARLY_GAUSSIAN/
cchpssvirgo:/hpss/in2p3.fr/group/virgo/NINJA2/V1_NINJA2_G1000176_EARLY_GAUSSIAN/
cchpssvirgo:/hpss/in2p3.fr/group/virgo/NINJA2/V1_NINJA2_G1000176_EARLY_RESCALED_GAUSSIAN/

Bologna:
/storage/gpfs_virgo4/virgo/virgoD0T1/NINJA2/H1_NINJA2_G1000176_EARLY_GAUSSIAN/
/storage/gpfs_virgo4/virgo/virgoD0T1/NINJA2/L1_NINJA2_G1000176_EARLY_GAUSSIAN/
/storage/gpfs_virgo4/virgo/virgoD0T1/NINJA2/V1_NINJA2_G1000176_EARLY_GAUSSIAN/
/storage/gpfs_virgo4/virgo/virgoD0T1/NINJA2/V1_NINJA2_G1000176_EARLY_RESCALED_GAUSSIAN/

Comments (from Ian Harry):
V1_NINJA2_G1000176_EARLY_GAUSSIAN is coloured to reflect the predicted early advanced Virgo PSD as given by document G1000176 in the DCC. This predicted early advanced Virgo PSD is about 50% more sensitive than the predicted early advanced LIGO PSD. The parameter estimation group argued that it would be useful to have 3 data sets from 3 sites with equal sensitivity. Therefore it was decided to also distribute the Virgo data, using the same *shape* PSD, but rescaled to have the same horizon distance as the early aLIGO PSD. This data is distributed as: V1_NINJA2_G1000176_EARLY_RESCALED_GAUSSIAN

More information here

Wavforms catalogue:
The tarball is:
https://ldas-jobs.ligo.caltech.edu/~ninja/120509_catalogue.tar.gz
or from here on CIT:
/home/ninja/public_html/120509_catalogue.tar.gz

The tarball needs to be untared in:
<root_path>/ninja2_injection_catalogue
where the root path must be changed according to the final destination

the file ninja2catalog.xml will also need to be edited so that the paths point to the correct locations.