Chiquita data: iterative fit - Jan. 29

The goal here is to compare the various data sets taken from the chiquita data. It is probably most interesting to first compare the original set of 500 showers with the set of showers found by analysiscut2 during the same time period.

The aperture histogram for the first set is the most recent one, (using analysiscut2) and takes into account a cutoff of theta <= 45 degrees.

Aperture from simulations:

aperture
acceptance
rhist

Iterative fits:

Results:

Data histogram:

Data x E^3 histogram:

Data x E^3, iterated:

The aperture histogram for the second set is taken from the set of simulations used for the spectrum in the ICRC paper, but in order to be consistent with the above, I have added a cutoff of theta <= 45 degrees. I wouldn't trust the low end of rhist because the simulated energies only extend down to 10^16.4.

Aperture from simulations:

aperture
acceptance
rhist

Iterative fits:

Results:

Data histogram:

Data x E^3 histogram:

Data x E^3, iterated:

Previous versions for comparison:

One possible problem is that chiquita showers are being filtered into the chicos list... I looked through part of the analysiscut2 list and found quite a few that would qualify as chiquita showers (most are not very high energy, though).

shower 1
shower 2
shower 3
shower 4
shower 5
shower 6
shower 7
shower 8
shower 9
shower 10