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SSH connection stability

Updated on Sat, 2007-04-07 08:16. Originally created by jeromel on 2006-12-19 16:58. Under:
IF
  • Your SSH connections are closed from home
  • You get disconnected from any nodes without any reasons?
  • ... and you are a PuTTY user
  • ... or an Uglix SSH client user
This page is for you. If you are another user, use different clients and so on, this page may still be informative and help you stabalize your connection (the same principles apply).

PuTTY users

PuTTY to connect to gateway (from a home connection), you have to

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SSH Keys and login to the SDCC

Updated on Fri, 2021-01-15 12:58 by starweb. Originally created by jeromel on 2006-12-19 16:32. Under:

How to generate keys for about every platform ...

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Facility Access

Updated on Tue, 2006-12-19 16:50. Originally created by jeromel on 2006-12-19 16:30. Under:

A selection of tips on how to log to the RCF
facility. We hope to augment those pages and add
information as user request or need.

Run VII preparation, meeting #9

Updated on Fri, 2006-12-15 12:30. Originally created by jeromel on 2006-12-15 12:23. Under:
-00-00
Thursday, 1 January 1970
, at 00:00 (GMT), duration : 00:00
TimeTalkPresenter
14:00Follow-ups ( 00:20 ) 0 filesAll (All)
14:30SDAS, requirements, current model, path forward ( 00:20 ) 0 filesAll (All)
14:50AOB ( 00:10 ) 0 filesAll (All)
15:00Offline and online QA ( 00:10 ) 0 filesGene Van Buren & Jerome Lauret (BNL, BNL)

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chain tricks

Updated on Thu, 2008-05-15 11:05. Originally created by balewski on 2006-12-13 22:04. Under:

 

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Preview of the 2006/12 review findings

Updated on Thu, 2007-01-11 11:14. Originally created by jeromel on 2006-12-13 18:57. Under:

The panel recommends simulation
and optimization of the following possible configuration, one of which should
be chosen; either

  • Two layers of active pixel sensors followed
    radially outward by a layer of ALICE
    style pixels (the HPD) located at a slightly larger radius than its present
    location, followed by the existing STAR SSD.
  • Two layers of active pixel sensors followed
    radially outward by the IST1 and IST2 layers both at somewhat smaller radii
    than presently proposed, followed by the existing STAR SSD.

In the event the existing SSD can
not be counted on as part of the future mid-rapidity tracking system, the panel
recommends the following configuration be optimized:

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P06ib

Updated on Tue, 2007-02-27 12:45. Originally created by starembed on 2006-12-08 13:56. Under:

Time Stamps

Updated on Tue, 2009-06-30 09:59 by testadmin. Originally created by deph on 2006-12-08 11:36. Under:
STAR  
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Load Balancer

Updated on Tue, 2009-05-05 13:23 by testadmin. Originally created by deph on 2006-12-08 11:31. Under:

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Online API

Updated on Tue, 2009-05-05 13:23 by testadmin. Originally created by deph on 2006-12-08 11:30. Under:

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IRMIS

Updated on Tue, 2009-05-05 13:22 by testadmin. Originally created by deph on 2006-12-08 11:00. Under:

Irmis

Instalation Recipe

  1. install MySQL & setup (set admin password, set user, set user password, set database called irmis, etc)
  2. download and install Jav
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Development

Updated on Tue, 2009-08-18 17:02 by testadmin. Originally created by deph on 2006-12-08 10:29.

The links below lead to projects being worked on for the ongoing delevopment of the STAR database system.

 

Run VII preparation, meeting #8

Updated on Fri, 2006-12-08 13:54. Originally created by jeromel on 2006-12-07 17:01. Under:
-00-00
Thursday, 1 January 1970
, at 00:00 (GMT), duration : 00:00
TimeTalkPresenter
14:00Follow-ups ( 00:10 ) 1 fileAll (All)
14:10IRMIS progress ( 00:20 ) 0 filesJiro Fujita (Creighton)
14:30Offline QA and online ( 00:10 ) 0 filesJerome Lauret / Gene Van Buren (BNL)
14:40Electronic Elog ( 00:10 ) 0 filesLevente Hajdu (BNL)
14:50AOB ( 00:10 ) 0 filesAll (All)

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P bar

Updated on Fri, 2007-02-16 17:55. Originally created by starembed on 2006-12-07 16:31.
P06ib: Plots_Nfit-Pbar-nfit_0.20pT0.30_0nch1000
P06ib: Pbar 0.20pT0.30_0nch1000

      

Proton

Updated on Thu, 2006-12-28 16:17. Originally created by starembed on 2006-12-07 16:28.
P06ib: Plots_Nfit-Proton-nfit_0.20pT0.30_0nch1000
P06ib: Proton 0.20pT0.30_0nch1000

      

K Plus

Updated on Fri, 2007-02-16 17:36. Originally created by starembed on 2006-12-07 16:25.
P06ib: Plots_Nfit-KPlusMinus-nfit_0.20pT0.30_0nch1000
P06ib: K plus 0.20pT0.30_0nch1000

      

K Minus

Updated on Fri, 2007-02-16 17:30. Originally created by starembed on 2006-12-07 16:22.
P06ib: Plots_Nfit-KMinus-nfit_0.20pT0.30_0nch1000
P06ib: K minus 0.20pT0.30_0nch1000

      

Pi Plus

Updated on Fri, 2007-02-16 17:54. Originally created by starembed on 2006-12-07 16:18.
P06ib: Plots_Nfit-PiPlusMinus-nfit_0.20pT0.30_0nch1000
P06ib: Pi plus 0.20pT0.30_0nch1000

      

Pi Minus

Updated on Fri, 2007-02-16 17:53. Originally created by starembed on 2006-12-07 16:14.
P06ib: Plots_Nfit-PiMinus-nfit_0.20pT0.30_0nch1000
P06ib: Pi minus 0.20pT0.30_0nch1000

      

Plots - Number of Fitted Points

Updated on Fri, 2007-03-02 12:08. Originally created by starembed on 2006-12-07 16:10.
The Following are the results for dca distributions for different pT bins in Pi Minus. The results of dca agrees reasonable for the cut-off of 2 cm and above. These plots were done using the macro plot_dca.C