I wonder ...

JoeB
JoeB
Joined: 24 Feb 05
Posts: 124
Credit: 88165178
RAC: 15031
Topic 193189

I believe the data for the S5 run was taken with the detectors running at their design sensitivity. At this sensitivity current theory says gravity waves should be detectable. Also we haven't heard from Ben at all, or Bruce much lately. And Bruces's computers seem to be otherwise occupied. Bruces's Computers

I wonder if we have identified a signal and they are now doing refined analysis on it and getting their publications ready? (I hope so!)

Joe B

Annika
Annika
Joined: 8 Aug 06
Posts: 720
Credit: 494410
RAC: 0

I wonder ...

Interesting theory. I'd tend to put it down to Bruce being in Germany atm, but maybe you do have a point... exciting idea indeed!

rbpeake
rbpeake
Joined: 18 Jan 05
Posts: 266
Credit: 1089551140
RAC: 705596

RE: ..I wonder if we have

Quote:
..I wonder if we have identified a signal and they are now doing refined analysis on it and getting their publications ready? (I hope so!)


I hope so, too! :)

And on a side note, with the publicity if that is true, it might bring in a lot more people to the project (hopefully!) to make additional discoveries!

Bikeman (Heinz-Bernd Eggenstein)
Bikeman (Heinz-...
Moderator
Joined: 28 Aug 06
Posts: 3522
Credit: 692305997
RAC: 1539

At the pan galactic BOINC

At the pan galactic BOINC meeting (I think this was the official title), the status of the data analysis was given as :

S3 data: analysis finished, nothing found, see link on the homepage
S4 data: analysis finished, under internal review
S5 data: post-processing not finished yet

So don't hold your breath, as the most sensitive S5 data isn't yet fully processed.

(This is from the top of my head as the boinc.berkeley.edu site where the presentation was linked is currently offline.)

CU
H-BE

rbpeake
rbpeake
Joined: 18 Jan 05
Posts: 266
Credit: 1089551140
RAC: 705596

RE: At the pan galactic

Message 73619 in response to message 73618

Quote:

At the pan galactic BOINC meeting (I think this was the official title), the status of the data analysis was given as :

S3 data: analysis finished, nothing found, see link on the homepage
S4 data: analysis finished, under internal review
S5 data: post-processing not finished yet

So don't hold your breath, as the most sensitive S5 data isn't yet fully processed.

(This is from the top of my head as the boinc.berkeley.edu site where the presentation was linked is currently offline.)

CU
H-BE


Thinking about it some more, I also recall from the recent paper that there are other post-processing analyses they do as well, so Bruce's computers may just be working on another aspect of the post-data analysis.

Donald A. Tevault
Donald A. Tevault
Joined: 17 Feb 06
Posts: 439
Credit: 73516529
RAC: 0

RE: RE: At the pan

Message 73620 in response to message 73619

Quote:
Quote:

At the pan galactic BOINC meeting (I think this was the official title), the status of the data analysis was given as :

S3 data: analysis finished, nothing found, see link on the homepage
S4 data: analysis finished, under internal review
S5 data: post-processing not finished yet

So don't hold your breath, as the most sensitive S5 data isn't yet fully processed.

(This is from the top of my head as the boinc.berkeley.edu site where the presentation was linked is currently offline.)

CU
H-BE


Thinking about it some more, I also recall from the recent paper that there are other post-processing analyses they do as well, so Bruce's computers may just be working on another aspect of the post-data analysis.

Or, perhaps Bruce is giving the rest of us a chance to catch up with him.

Annika
Annika
Joined: 8 Aug 06
Posts: 720
Credit: 494410
RAC: 0

Yeah, if I get a couple of

Yeah, if I get a couple of hundred additional computers, I might :-D anyone volunteer as a sponsor?

peanut
peanut
Joined: 4 May 07
Posts: 162
Credit: 9644812
RAC: 0

I'm still in awe that we can

I'm still in awe that we can even try to detect something on the order of the size of a proton with an instrument contected to the surface of a geologically active planet like our Earth. The space based instrument may have some advantages there.

I'm hoping for a positive signal though. That would be great.

rbpeake
rbpeake
Joined: 18 Jan 05
Posts: 266
Credit: 1089551140
RAC: 705596

RE: Yeah, if I get a couple

Message 73623 in response to message 73621

Quote:
Yeah, if I get a couple of hundred additional computers, I might :-D anyone volunteer as a sponsor?


Better make sure they pay your electric bill, too! ;)

Bernd Machenschalk
Bernd Machenschalk
Moderator
Administrator
Joined: 15 Oct 04
Posts: 4305
Credit: 248553143
RAC: 31527

RE: At the pan galactic

Message 73624 in response to message 73618

Quote:

At the pan galactic BOINC meeting (I think this was the official title), the status of the data analysis was given as :

S3 data: analysis finished, nothing found, see link on the homepage
S4 data: analysis finished, under internal review
S5 data: post-processing not finished yet

So don't hold your breath, as the most sensitive S5 data isn't yet fully processed.


I can confirm that (apart from the title actually being "3rd Pangalactic BOINC Workshop").

Some things to add:

* The sensitivity of the search is not only limited by the sensitivity of the detectors, but also by that of the search (algorithm, parameters). This is one of the reasons why we changed that algorithm for S5R2 (see Reinhard's post).

* The sensitivity of a search for continuous gravitational waves (from sources we call pulsars) increases with the "observation time", i.e. the amount of data analyzed. So far we are only analyzing roughly the first half of S5 data (S5 officially ended on 1 Oct 2007). We plan to do a search of the full S5 data for S5R4, but there are still some technical problems to overcome.

* In S5 the LIGO detectors run at their "design sensitivity", i.e. the highest sensitivity achievable with their design. Still we are not sure that there is a source of (continuous) gravitational waves near enough that we can actually detect it with the current instruments. Advanced LIGO is designed to extend the distance by a factor of ten (see "Figure 8" on Reinhard's poster).

* There are other possible sources of gravitational waves than gravitational pulsars, requiring other methods to search for their signals in the detector data than the one we use on Einstein@home. The clusters of the LSC (including "Nemo") are usually running other searches, and do help Einstein@home only when they would be idle otherwise.

BM

BM

Annika
Annika
Joined: 8 Aug 06
Posts: 720
Credit: 494410
RAC: 0

Thanks, Bernd, that was

Thanks, Bernd, that was really a very interesting statement. Always exciting to learn about the science behind the crunching. Don't worry, we'll be there, no matter how long it takes to finally find sth ;-)
Btw, "Nemo" is a really cool name (should have though of it when I assigned my last hostname), reminds me of both the story and the Nightwish song...

Comment viewing options

Select your preferred way to display the comments and click "Save settings" to activate your changes.