Sanjay Padhi kindly reminded me that there is already an arXiv whitepaper
on the event generation, so citations of this can be used to gauge the
impact of the data. From Sanjay:
1) Methods and Results for Standard Model Event Generation at
$\sqrt{s}$ = 14 TeV, 33 TeV and 100 TeV Proton Colliders (A Snowmass
Whitepaper), arXiv:1308.1636, Aug. 2013
2) Snowmass Energy Frontier Simulations using the Open Science Grid (A
Snowmass 2013 whitepaper), arXiv:1308.0843, Aug. 2013
The detector part, we are currently getting comments from the
spokesperson of the experiments. So one can cite
3) "Snowmass Energy Frontier Simulations" A. Avetisyan et. al,
arXiv:1308.xxxx, Aug. 2013
Markus Luty
============================================
Physics Department
University of California, Davis
One Shields Avenue
Davis, CA 95616
Phone: +1 530 554 1280
Skype: markus_luty
On Mon, Aug 19, 2013 at 11:39 AM, Markus A. Luty
<[log in to unmask]>wrote:
> I cannot agree more with what Chip says. Let's find a way to keep this
> valuable resource accessible. In fact, the way should be kept open to *add*
> to it or improve it.
>
> I also suggest that the people who generated the data write a brief ArXiv
> note on it so that people who use it in their research can cite it. We
> should cite it in the Snowmass report as well. This is a very important
> contribution, and should be recognized.
>
> Markus Luty
>
> ============================================
> Physics Department
> University of California, Davis
> One Shields Avenue
> Davis, CA 95616
>
> Phone: +1 530 554 1280
> Skype: markus_luty
>
>
>
> On Sun, Aug 18, 2013 at 10:44 PM, JoAnne L. Hewett <
> [log in to unmask]> wrote:
>
>> Hi All,
>>
>> I think this set of backgrounds is an extremely valuable resoure that our
>> community could greatly use. Every LHC theory paper would be better off
>> using it. Surely we can find a good home for it somewhere....
>>
>> -JoAnne
>>
>>
>> On Mon, 19 Aug 2013, Raymond Brock wrote:
>>
>> Hi folks,
>>>
>>> Look. These data constitute a unique resource, created at considerable
>>> expense and time. There is nothing else like it anywhere: full-statistics
>>> in tails for small signal comparison, in a tool that's easy to use and
>>> mated to standard matrix element generators, and with pileup conditions
>>> that not even the LHC collaborations have simulated in all respects.
>>>
>>> It would be a tangible gift provided to the community by their DPF.
>>>
>>> Can I promise that it will be used immediately? No. But if the DPF EC
>>> can get over what I'm sure are a few loud voices and make the nominal funds
>>> available from its embarrassingly large bank roll, it can then advertise to
>>> its membership that these tools were built for the community and that they
>>> remain available for use.
>>>
>>> The theory community has nothing like this and neither, frankly, does
>>> the LHC community.
>>>
>>> I can't believe that we're actually considering getting rid of it or
>>> hiding it.
>>>
>>> I've cc'd the EF conveners to this thread (read it all from the bottom!)
>>> as apparently I need help or a straightjacket.
>>>
>>> best
>>> Chip
>>>
>>>
>>> On Aug 18, 2013, at 11:47 AM, LATBauerdick <[log in to unmask]<mailto:
>>> bau**[log in to unmask] <[log in to unmask]>>>
>>> wrote:
>>>
>>>
>>> I?d say, people should make the case if they think this data should be
>>> an actively available dataset long-term, that people continue to run on and
>>> thus should be available on disk (and there?s much more at Fermilab and
>>> Brookhaven).
>>>
>>>
>>> Otherwise it can be archived and brought back when it is needed.
>>>
>>> I heard some people would like to continue in the next weeks to run for
>>> some additional studies for the ECFA meeting, which is fine, but also has a
>>> finite time scale.
>>>
>>> Beyond that, keeping data on disk just in case somebody later might want
>>> it is generally not a good way to go. And, yes, USCMS would like to
>>> eventually get that space back at Lincoln and at the LPC/Fermilab.
>>>
>>> Cheers, LatB
>>>
>>> --
>>> LATBauerdick
>>>
>>>
>>> On Sunday, August 18, 2013 at 11:34 AM, Raymond L Brock wrote:
>>>
>>> Hi Steve,
>>>
>>> There's more. Here's a reply that I made to the EC after it was turned
>>> down after what Jon called "considerable resistance."
>>>
>>> The storage I spoke of is for a snowmass product. It's not a lot of
>>> money and we have to somehow relieve Ken Bloom of the violation of his MOU
>>> that he's done to host the root tuples that are of all of the backgrounds
>>> generated within the snowmass detector tool. The madgraph and pythia source
>>> still lives at FNAL and I've not heard of any threat to delete that stuff.
>>> He's also created an http download ability and I think he'd continue to
>>> support that. So it's a one-stop shopping center for backgrounds that
>>> include a fancy weighting scheme to populate tails of SM background
>>> distributions for rare signal comparisons. It's quick. It's simple and it's
>>> got a lot of use to it. For theorists, students, and yes, EF people who
>>> venture outside of their collaborations' straightjackets.
>>>
>>> I'm shocked that the EC would put up "considerable resistance" to this
>>> request. It has utility if we might ever - in the next few years - do any
>>> other community-wide simulation jamboree. I think at least some of the good
>>> feelings you got from Marcelle and Bjoern reflect that non-tribal benefits
>>> of working together. The Italians do something like this between CMS and
>>> ATLAS and I'd like to explore that in the US and those background samples
>>> are a great way for people to work on simulations for fun (or profit) and
>>> not worry about the onerous CMS and ATLAS rules. And as I said, they're
>>> available for theorists as well.
>>>
>>> Here's the tally: http://snowmass2013.org/tiki-**index.php?page=**
>>> NPBackgroundSamplesTwiki<http://snowmass2013.org/tiki-index.php?page=NPBackgroundSamplesTwiki>
>>>
>>> The context is that the DPF always has way more money in its account
>>> than I felt comfortable with as chair. It's _down_ to $100k now.
>>>
>>> So if the goal was just to archive the stuff, then sure. Tape would be a
>>> portable, permanent way to do that. But I have in mind that people might
>>> continue to use it. So the ability to get at the files easily would be a
>>> premium, as it has been for snowmass. I then offered to buy back the disks
>>> from DPF for our tier 2 if nobody used it for a couple of years.
>>>
>>> best
>>> Chip
>>>
>>>
>>> On Aug 18, 2013, at 2:29 AM, Steven Gottlieb <
>>> [log in to unmask]**<mailto:[log in to unmask]**indiana.edu<[log in to unmask]>
>>> >>
>>>
>>> wrote:
>>>
>>> Why not write them to tape? That would be much less expensive.
>>>
>>> Steve
>>>
>>> On Sun, 2013-08-18 at 01:15 -0500, Jonathan L. Rosner wrote:
>>> See the third thing. Opinions welcome. Is this a Snowmass resource
>>> that DPF should pay to preserve?
>>>
>>> Regards,
>>> Jon
>>> -- Jonathan L. Rosner
>>> Enrico Fermi Inst., U. Chicago Phone: 773-702-7694
>>> 5620 S. Ellis Avenue Fax: 773-702-8038
>>> Chicago, IL 60637 USA [log in to unmask]<**mailto:
>>> [log in to unmask]**>
>>> ==============================**==============================**====
>>>
>>>
>>> On Aug 14, 2013, at 11:40 AM, Chip Brock <[log in to unmask]<mailto:brock*
>>> *@pa.msu.edu <[log in to unmask]>>> wrote:
>>>
>>> hi Chair Line,
>>> Two things have come up which I think I should alert you to.
>>>
>>> ...
>>>
>>> 3. I know. I lied. This is a third thing. The snowmass background
>>> samples have been stored at the Nebraska T2. Ken supplied the resources
>>> - disk shelves - out of his T2 resources and he'll need them back. I
>>> think that this stuff should be preserved so people can continue to use
>>> them and so the easiest way to do that would be to buy disks for Ken to
>>> replace his loan. He's thinking about whether he can justify the
>>> support, but I suspect he can. The top end of storage would be about
>>> 100TB, so that's a $10k or so expense which I suggest DPF spend.
>>>
>>> That is all.
>>> Thanks
>>> Chip
>>>
>>> ------------------------------**------------------------------**---
>>> Raymond Brock * University Distinguished Professor
>>> Department of Physics and Astronomy
>>> Michigan State University
>>> Biomedical Physical Sciences
>>> 567 WIlson Road, Room 3210
>>> East Lansing, MI 48824
>>> sent from: [log in to unmask]<mailto:brock@**pa.msu.edu <[log in to unmask]>
>>> >
>>>
>>>
>>> cell: (517)927-5447
>>> MSU office: (517)353-1693/884-5579
>>> open fax: (517)355-6661
>>> secure fax: (517)351-0688
>>> Fermilab office: (630)840-2286
>>> CERN Office: 32 2-B03 * 76-71756
>>>
>>> Twitter: @chipbrock
>>> Home: http://www.pa.msu.edu/~brock/
>>> ISP220: http://www.pa.msu.edu/courses/**ISP220/<http://www.pa.msu.edu/courses/ISP220/>
>>> ISP213H: http://www.pa.msu.edu/courses/**2007spring/ISP213H/<http://www.pa.msu.edu/courses/2007spring/ISP213H/>
>>> Facebook: http://msu.facebook.com/**profile.php?id=2312233<http://msu.facebook.com/profile.php?id=2312233>
>>>
>>>
>>>
>>>
>>>
>>>
>>>
>>>
>>>
>>>
>>> ------------------------------**------------------------------**---
>>> Raymond Brock * University Distinguished Professor
>>> Department of Physics and Astronomy
>>> Michigan State University
>>> Biomedical Physical Sciences
>>> 567 WIlson Road, Room 3210
>>> East Lansing, MI 48824
>>> sent from: [log in to unmask]<mailto:brock@**pa.msu.edu <[log in to unmask]>
>>> >
>>>
>>>
>>> cell: (517)927-5447
>>> MSU office: (517)353-1693/884-5579
>>> open fax: (517)355-6661
>>> secure fax: (517)351-0688
>>> Fermilab office: (630)840-2286
>>> CERN Office: 32 2-B03 * 76-71756
>>>
>>> Twitter: @chipbrock
>>> Home: http://www.pa.msu.edu/~brock/
>>> ISP220: http://www.pa.msu.edu/courses/**ISP220/<http://www.pa.msu.edu/courses/ISP220/>
>>> ISP213H: http://www.pa.msu.edu/courses/**2007spring/ISP213H/<http://www.pa.msu.edu/courses/2007spring/ISP213H/>
>>> Facebook: http://msu.facebook.com/**profile.php?id=2312233<http://msu.facebook.com/profile.php?id=2312233>
>>>
>>>
>>>
>>>
>>>
>>>
>>>
>>>
>>>
>>>
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