ICRC2015: TALK , EBL studies with 1ES 1011+496

[david.paneque]

Posted on behalf of Priya


First version of slides intended to be presented at the ICRC2015.
Comments welcome until Friday July 31h.

1ES1011_ICRC2015_.pdf

ICRC2015: TALK , EBL studies with 1ES 1011+496. Version ready for review.

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[elisa.prandini]

Dear Priya,
thanks for the nice presentation! The main concern that I have is on its length, maybe you have to cut some details.
Please find below a few additional comments (all minor).
Cheers,
Elisa

slide 3 - the image quality is very bad
slide 4: "...higher than predicted by " -> higher than THAT predicted by
slide 4: universe -> Universe
slide 5: a opportunity -> an opportunity
slide 5: impact of the (EBL) -> impact of the EBL
slide 6: cradit Abelardo -> Credits: A. Moralejo
slide 7: extra ( after Integral sensitivity
slide 8: 10 times than -> 10 times the
slide 8: Crab flux -> Crab nebula flux
slide 8: Fermi and Swift should be written in italics
slide 8: X-ray flux is -> was
slide 9: you can mention the EBL model assumed
slide 11: could you add a ref to the plot?
slide 18: maybe you can skip the second point (too technical)
slide 21: Fermi, Swift in italics
slide 21: This was the first time to observe flare with such high flux from such a distant source around 1TeV. Thus presented an opportunity to perform measurements of the EBL.->
I suggest to rephrase in two points:
- Fist time that we see a strong flare from this distant source
- Spectrum up to TeV energies -> opportunity to test EBL models