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No calibration errors. All measurements of the anisotropy.

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Presentation on theme: "No calibration errors. All measurements of the anisotropy."— Presentation transcript:

1 No calibration errors. All measurements of the anisotropy.
“right out of the box” if you will. For a book With Jim Peebles.

2 Note that if the experiments had targeted the l=200 region they would have detected something! There were a couple of false detections of the quad. MASBAL first presentation of a map..Fixsen et al.

3 Earry days for the detections. Started with DMR in 1992
Earry days for the detections. Started with DMR in The first two cosmological parameters to be fit were n_s and the amplitude.

4 Earry days for the detections. Started with DMR.

5 Discovery and detections at larger scales. Indications for a rise.

6 Discovery and detections at larger scales. Indications for a rise
Discovery and detections at larger scales. Indications for a rise. ARGO was deBernardis

7 Fleshing out the first peak.

8 The new milennium along with its great jump in sensitivity
The new milennium along with its great jump in sensitivity. Part of the core Boomerang team.

9 Start to see higher order structure, but B and DASI also fit flat lines.

10 Just before WMAP. Second peak now in good shape and we see damping scale.

11 WMAP plus all of the others with prior bins
WMAP plus all of the others with prior bins.This is a testament to the field.


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