22 Apr
2013
22 Apr
'13
5:22 p.m.
Looks right to me.
So...average looks like around 5%, with significant parts of the field
higher than that but not > 10%.
Can you overlay the same on slide 5 (I_353)?
Reward offered: for the first to construct 353 p*I in our field from
"public" Planck data.
On 4/22/13 5:11 PM, Chris Sheehy wrote:
Hi,
I started doing the b2 overlay earlier, so I've got it now. Does this
look right to people? I don't have a good sense for where the B2 field
should be.
-Chris
On Mon, Apr 22, 2013 at 3:37 PM, John Kovac <jmkovac(a)cfa.harvard.edu
<mailto:jmkovac@cfa.harvard.edu>> wrote:
I second this request. I've been squinting trying to work out our field
boundary, and if I've got it right it looks like p for our field is
around average...
Jamie, would you be able to overlay our field boundary on these various
maps for a clear illustration, and estimate our mean p?
Of course p*I would be even better.
John
On 4/22/13 3:22 PM, Denis Barkats wrote:
--
___________________________________________________________________
John Kovac jmkovac(a)cfa.harvard.edu
Assistant Professor, Astronomy and Physics, Harvard University
160 Concord Ave rm 310, Cambridge MA 02138, 617-496-0611
Wow,
can you take the slide and derive a mean polarization fraction
from the 2%
bicep region in that full sky ?
*******************************************************************
Denis Barkats Phone: +56 2 467 6273
Commissioning Scientist Fax: +56 2 467 6101
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On Apr 22, 2013, at 15:15, jamie tolan wrote:
> Slide 6 in this talk is also interesting:
>
>
http://www.rssd.esa.int/SA/PLANCK/docs/eslab47/Session07_Galactic_Science/4…
>
> Dust polarization fraction at 353 GHz.
>
> -Jamie
>
>
> On Sun, Apr 21, 2013 at 12:54 PM, Randol Aikin <rwa(a)caltech.edu
<mailto:rwa@caltech.edu>> wrote:
> Hi All,
>
> For those of you not on the Caltech obscos list, please see the
note below
from Olivier - this presentation in particular:
>
http://www.rssd.esa.int/SA/PLANCK/docs/eslab47/Session09_Data_Processing/47…
>
>> Randol
>
>> Begin forwarded
message:
>
>>> From: "Dore,
Olivier P (3267)" <Olivier.P.Dore(a)jpl.nasa.gov
<mailto:Olivier.P.Dore@jpl.nasa.gov>>
>> Subject: [Obscos] Planck ESLAB slides
>> Date: April 21, 2013 12:38:57 PM PDT
>> To: ObsCos group <obscos(a)astro.caltech.edu
<mailto:obscos@astro.caltech.edu>>
>>
>> Hey all,
>> Just wanted to point you to the presentations from the very
good
Planck meeting from two weeks ago in The Netherlands.
>>
http://www.rssd.esa.int/index.php?project=PLANCK&page=47_ESLAB
>> A lot of good stuff in there. Besides Planck results, I
particularly
enjoyed the presentations by Zaldarriaga, Mukhanov,
Freedman and Page.
>> Also, if you are interested in dust
polarization (if not, you
should!), I recommend the presentations of Bernard
and Aumont.
>>> Definitely worth a look.
>>> Olivier
>>>
>>> ----------------
>>> Olivier Doré
>>> olivier.p.dore(a)jpl.nasa.gov <mailto:olivier.p.dore@jpl.nasa.gov>
>>> +(1) 626 375 6347 <tel:%2B%281%29%20626%20375%206347>
>>>
>>>
>>>
>>>
>>>
>>>
>>>
>>>
>>>
>>>
>>>
>>> _______________________________________________
>>> Obscos mailing list
>>> Obscos(a)astro.caltech.edu <mailto:Obscos@astro.caltech.edu>
>>> http://astro.caltech.edu:88/mailman/listinfo/obscos
>
>
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Christopher Sheehy - Ph.D. candidate - University of Chicago
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Tel: 612-625-1802 Fax: 612-624-4578 email: csheehy(a)uchicago.edu
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