Generated by ARS on 6/1/2004 5:46:56 PM ACTION ITEMS LIST FOR SUPPORT TEAMS AND LOGISTIC Telescope : RITZ Create-date : 1/27/2004 3:26:59 PM Problem Short Description : The control area of the 220 telescope should be rearranged. Action : The control area should be rearranged according to the requirements from J Pritchard, adding dual screen terminals as required. Cables should also be put in order. Action Log : 3/16/2004 2:44:39 PM blopez MPA and RSO re-arranged the monitors and set up the dual screen. The required layout could not be fit exactly due to a limit for the USB cable length of keyboard and mouses (note: to solve this HW has to be purchased). 3/26/2004 8:38:15 AM gandreon GIH:It was done but, it does not fulfill the specifications. Problems with cabling length. To be discussed with JPR. 3/30/2004 2:41:06 PM gandreon USB hub to be ordered. 4/20/2004 4:41:11 PM gandreon Hub ordered. 5/11/2004 3:39:57 PM gandreon Hubs arrived. New deadline. 5/18/2004 4:34:45 PM gandreon USB Hubs are not compatible with HP B2000. More investigation is required. 5/25/2004 2:56:38 PM gandreon There will be a last attempt with "Active cables", already ordered. Responsible : Software&Commun.Supp.T. Status : Assigned Deadline : 3/23/2004 12:00:00 AM Deadline Status : Pending ________________________________________________________________________________ Telescope : RITZ Create-date : 5/17/2004 5:57:56 PM Problem Short Description : Bar value of FF lamps in the control panel does not reflect the real status of lamps if apply is not pressed. Action : Add to the 360 and NTT Dome FF panel a ON/OFF command and state for the variable lamps. OFF state should be obvious when cero volts are applied Action Log : 5/18/2004 4:36:58 PM gandreon During VLT upgrade. Responsible : Software&Commun.Supp.T. Status : Assigned Deadline : 8/31/2004 12:00:00 AM Deadline Status : Pending ________________________________________________________________________________ Telescope : ESO NTT Create-date : 6/13/2003 4:38:07 PM Problem Short Description : Az temp monitoring: replace Pulpo by Adams Action : The 4 temp. monitoring points on the NTT Az motors are currently read by a Pulpo which is one of the only spares available. Pls replace this Pulpo by Adams module. The software aspects of this action point should be developed having in mind that it is very likely that similar systems will be integrated on 3p6 and Feros. Action Log : 7/8/2003 3:58:31 PM gandreon Type has been selected (6 channels, RS-232). 8/26/2003 2:51:02 PM gandreon Adams modules have been ordered. 9/23/2003 2:39:26 PM gandreon Adams are in Vitacura 10/21/2003 3:14:42 PM gandreon The Adam modules are on the mountain. Please proceed to next step. 11/4/2003 2:45:23 PM gandreon Modules delivered to SWC. Under test because of differences with other modules. 11/18/2003 9:22:51 AM ikastine Software ready and tested at lab. Adam could be installed 04 - 08 Dec technical time. Help for electronics is needed for that. 11/30/2003 3:15:28 PM ikastine RPA said they will not have time to install adam during technical time of 4-8 Dec due encoder business. Thus, we have to wait next oportunity. 12/9/2003 3:58:24 PM gandreon New deadline. 12/16/2003 2:47:02 PM gandreon Waiting for the cabling. 1/27/2004 12:07:18 PM gandreon GIH:Electronics mentioned that they have no time for the cabling. To be postponed until March 2004. 3/2/2004 2:39:28 PM gandreon Cabling ready. SWC should now install the Adams. 3/9/2004 2:54:56 PM gandreon Wrong module was purchased (6 2-wires channels). Four single channel-4 wires modules needed. 4/13/2004 3:33:17 PM gandreon New modules ordered. Responsible : Software&Commun.Supp.T. Status : Assigned Deadline : 3/16/2004 12:00:00 AM Deadline Status : Pending ________________________________________________________________________________ Telescope : ESO NTT Create-date : 5/9/2004 2:25:09 PM Problem Short Description : replace J' by Js in SOFI configuration Action : Necessary modification: (1) J' has t be renamed Js for consystency with ISAAC (2) the Js filter has to be added as a valid filte choice in the configuration files. Action Log : 5/11/2004 3:40:39 PM gandreon Could this be posponed until the VLT Update? 5/18/2004 4:37:29 PM gandreon During VLT upgrade Responsible : Software&Commun.Supp.T. Status : Assigned Deadline : 8/31/2004 12:00:00 AM Deadline Status : Pending ________________________________________________________________________________ Telescope : ESO NTT Create-date : 5/11/2004 4:34:18 AM Problem Short Description : INSTRUM keyword on SUSI-2 images Action : we got a request from B.Pirenne @ archive to modify the INSTRUME keyword of the SuSI2 frames from "SUSI" to "SUSI2", for archive consistency. Action Log : 5/11/2004 3:46:47 PM gandreon To be verified with Pirenne if this really what he wants. 5/25/2004 2:57:09 PM gandreon Waiting for Anton, due back by June 6th. Responsible : Software&Commun.Supp.T. Status : New Deadline : Deadline Status : Not Assigned ________________________________________________________________________________ Telescope : ESO NTT Create-date : 5/18/2004 3:08:09 PM Problem Short Description : The current maintenance plan for EMMI is insufficient. Action : A maintenance plan for the 29 optomechanic functions should be prepared and put into Remedy. Action Log : 5/30/2004 5:35:28 PM psinclai Waiting for input from main provider: AGI Responsible : Engineering Dep.(Instrum.) Status : Assigned Deadline : Deadline Status : Not Assigned ________________________________________________________________________________ Telescope : ESO 360 Create-date : 1/27/2004 3:28:09 PM Problem Short Description : Image analysis software not readily usable. Action : The package should be porperly implemented. Action Log : 2/1/2004 11:36:47 AM ebarrios Properly implemented for me is to be included in the M2 proyect as it was requested sometime ago. Yes is not readily to any user because is not fully automatic. I´ll explain here what are the current procedure and tools used for measurements. Method: The idea is to take intra/extra focal images using the combination of center field mirror (CFM), center field focus function (CFF) and the image technical CCD (imgTEC). As the intra/extra focal images have to be taken with the same focal distance, telescope focus have to be done with the center field focus function set to 30000 enc-units. Then for intra/extra focal images, it has to be moved to 0 and 60000 enc-units. Image Analysis is done by a remote application currently installed on optics@kila:$HOME/curvature Procedure: 1.- On TCS control panel select the image quality catalog and do a Telescope Preset around Zenith (check not hatch viggneting). Stars magnitud have to be bigger than 12 to avoid pupil saturation after 30sec. exposure without neutral density(ND). Using the current ND installed in the curvature sensing carriage (CVS), stars magnitud bigger than 8 will be ok. 2.- Open a xterm on cam@w3p6tcs and type e3p6opsIqMes. This scrip will open a panel, logFile xterm and midas console to run the images sequence and its analysis. From panel user can do: - define both the imgTCCD and Image Analysis - Start imgTCCD infinite loop - Do imgTCCD setup - Start the image sequence - Run the image batch analysis - Run image analysis software for manual checks - Print results - See the imgTCCD status and the image analysis results Buttons Telescope focus and M2 correction don´t have an associated action yet 3.- Move Center Field Mirror (CFM) in 4.- Move Center Field Focus (CFF) to 30000 enc-units 5.- Do Telescope focus sequence (Moving M2). This is a manual procedure to be optimized because could take easily 15 minutes. Focus function is not precise enouht to just set M2 without check. The expectation with the new M2 is to have a better focus and collimation function modeling. To avoid this step, it was suggested by Alan to move CFF to 0 enc-units and move M2 until the pupil reach the reference diameter. But as the M2 movement also move the pupil image, automatic procedure is not an easy cake, for the moment this is also a manual procedure. 6.- On e3p6opsIqMes panel press StartSeq button. This procedure do the following: - check and moves center field mirror in - moves center field focus function - take by each CFF posistion a 30sec. exposure of pupil, do 90" telescope offset to take a 30sec. exposure of skybackground, do the skybackground substraction and send it to optics@kila:$HOME/curvature/data/eso_3m60_f8/yy_mm_dd 7.- On e3p6opsIqMes press Run EFbatch button to get the IQ results. If the results are not in the range, e.i. Total IQ < 0.5" this means either the M2 was re-installed in a wrong position or collimations screws were moved or M1 moves. M1 reset is the only action that can be done on-spot. M2 corrections need one morning to re-install it + one night for measurement and collimation corrections, so two setup nights after TIMMI2 run are a must. I´m still around for questioning Thanks 2/10/2004 9:05:29 AM ikastine The image analysis panels and scripts were copied to e3p6gui module. Some minor changes were made to IA sequence. After talking with Alain, it is clear that focusing of telescope is the main time consuming task of IA sequence. The focus circle shall be implemented to E3P6 RTD. With this circle user can fast check if telescope is at focus or not. This is not totally automatic operation due user interaction is needed, but will save time 10-15 min. Also Alain asked that long time statistics are saved to log file. He will send email to me defining those. The EF program can be problem. Currently it runs at kila and we have only installation disks to linux. So if something happens to kila or network, IA cannot be executed. To make things evem worst the company which made EF program has disappeared, so we will have no support for that program. I think we should see possibility to port image analysis EF part to midas procedures. Alain knows theory behing, but we do not know midas programming, so somebody (Emilio?) at SCI should do this. 2/10/2004 3:20:11 PM gandreon The point is limited in scope to the provision of a command for taking a sequence of images. The rest will be delt in the Image Analysis project later this year. 2/23/2004 9:35:30 AM ikastine The SW is ready to test. I shall make premilinary tests 15 of March if (Efos setup night) sciop gives time to me. Possible comissioning of software can be 28 of Abril (Efos setup night) or 12-14 of May (Harps setup nights). So I request to move deadline at end of May. If it possible, Alain should be here during comissioning due he will be one of major users of system. Additonal note about EF-program: I could not install EF program to redhat 7.3 linux, so we have only binaries at kila. 3/26/2004 8:39:54 AM gandreon GIH:To be tested by E.Barrios 4/20/2004 4:42:52 PM gandreon To be commissioned the night of 12 May Responsible : Software&Commun.Supp.T. Status : Closed Deadline : 4/26/2004 12:00:00 AM Deadline Status : Closed on Time ________________________________________________________________________________ Telescope : ESO 360 Create-date : 2/8/2004 2:00:39 PM Problem Short Description : Generate throu focus template for HARPS Action : A throu focus template is needed for HARPS. It should use the counts from the exposure meter. Action Log : 4/20/2004 11:03:58 AM jguzman First draft implemented in haotsf 1.26.1.1 haoseq 1.36.1.1 Not tested yet. Responsible : Software&Commun.Supp.T. Status : Closed Deadline : 5/11/2004 12:00:00 AM Deadline Status : Closed on Time ________________________________________________________________________________ Telescope : ESO 360 Create-date : 3/23/2004 10:27:54 AM Problem Short Description : CCD40 Left Amplier e/adu and Mode Updates Action : Include in the OS panel the left Amplifier speed options: normal Left fast Left Update conversion factor and readout noise values in the data base as follow: Fast left binining 1x1 CF = 1.2 RON = 8.19 Fast left bining 2x2 CF = 1.15 RON = 10.54 Normal left bining 1x1 CF = 1.21 RON = 7.59 Normal left bining 2x2 CF = 1.17 RON = 8.72 Please confirm thie above values with Linda Schmidtobreick Action Log : 3/30/2004 2:43:37 PM gandreon Values have been confirmed. Pls proceed. 4/7/2004 12:16:15 PM blopez New readout modes have been included at the OS panel (efouif 3.12). Installed and tested successfully at telescope. Please test. Note: chip parameters (CF, RON) to be configured by LIN. 5/11/2004 3:49:00 PM gandreon Peter pls put final comment. No automatic update allowed. Responsible : Engineering Dep.(Instrum.) Status : Closed Deadline : 4/27/2004 12:00:00 AM Deadline Status : Closed on Time ________________________________________________________________________________ Telescope : ESO 360 Create-date : 3/23/2004 10:34:22 AM Problem Short Description : Current Dome FF lamps Replacement Action : Provide a new support for 8 dome flat field lamps (like the NTT ones). Action Log : 4/13/2004 8:18:40 AM gandreon WEC:The design of the new arrangement will be finished next week. 4/26/2004 9:39:27 PM ebarrios I got the first design and for me is OK. 4/27/2004 3:20:27 PM gandreon New deadline. 5/25/2004 2:58:06 PM gandreon There is a problem with the deadline due to additional work for 360 M2. Responsible : Engineering Dep.(Mechanics) Status : Assigned Deadline : 5/30/2004 12:00:00 AM Deadline Status : Pending ________________________________________________________________________________ Telescope : ESO 360 Create-date : 4/12/2004 6:11:18 AM Problem Short Description : Upgrade autoguider functionality for HARPS Action : a) save the partial integrated image in a temporary file for online viewing b) add keywords to the fits header (list already submitted to SWC). Action Log : 5/10/2004 12:38:35 PM rsoto Software ready to be tested during HARPS technical night (May, 12) Responsible : Software&Commun.Supp.T. Status : Closed Deadline : 5/12/2004 12:00:00 AM Deadline Status : Closed on Time ________________________________________________________________________________ Telescope : ESO 360 Create-date : 4/14/2004 9:40:14 AM Problem Short Description : Hacth Control Panel for Night Operation Action : Sorry about this point, but, User Requirements were reviewed on Abril 2003 and the action was to wait till October 2003 for its implimentation. Requirements, comments+from+reviewers actions+points docs and the hatch control commands/status tables were given to Ismo. Hatch Commands and status were tested by me and Jorge Vilaza using the VLT inducer tool, so system is working. Hatch control is part of the 360 to RITZ User requirements document: http://docs.ls.eso.org/LSO-URS-ESO-90400-0001/LSO-URS-ESO-90400-0001.pd f Here are the Reviewer comments: http://www.ls.eso.org/lasilla/sciops/3p6/pub/userReq/sciopReqComm.ps Here the assigned Actions points after review: http://www.ls.eso.org/lasilla/sciops/3p6/pub/userReq/reviewActions.ps And the User requirements for 360 Auxiliary Functions use by J. Fluxa and Jorge Vilaza for the electronic implementation: http://www.ls.eso.org/lasilla/sciops/3p6/pub/userReq/360_Aux_Functions3 6400-1b.ps Requirements for HATCH panel control are done ... Action Log : 4/27/2004 3:21:11 PM gandreon This point requires a safety review to be conducted asap. 5/10/2004 4:41:05 PM gandreon Today this point has been reviewed by O Hainaut, G Andreoni, R Aguilar, and G Ihle. The point has been approved with the following conditions: - The remote closing of the hatches should be implemented. - An emergency remote stop should also be implemented. - The use of this feature shoud be logged and occurrencies should appear in the outrep report. - The Lock-pins insertion and the Hatches opening will only be possible locally. The remote operation should be done only in emergency, after closing the main mirror protection, and with great care to unusual noise. 6/1/2004 5:25:35 PM gandreon Implementation was more difficult than foreseen. Deadline extended. 6/1/2004 5:27:00 PM gandreon A cable carrying the mirror cover status to the auxiliary LCU will have to be installed by Telma. Responsible : Software&Commun.Supp.T. Status : Assigned Deadline : 6/15/2004 12:00:00 AM Deadline Status : Pending ________________________________________________________________________________ Telescope : ESO 360 Create-date : 4/27/2004 4:10:49 PM Problem Short Description : Due to disappeared key, a new lock is needed on Timmi 2 Laboratory main gate (instrument gate) Action : Please provide the new keys to SCI-Ops (E. Barrios) LIN (PSinclaire/JValenzuela) Action Log : Responsible : Infrastructure Support Group Status : Closed Deadline : 5/18/2004 12:00:00 AM Deadline Status : Closed on Time ________________________________________________________________________________ Telescope : ESO 360 Create-date : 5/17/2004 4:45:59 PM Problem Short Description : The focus formula is now computed by each applications separately. Action : Create new tcs data base points to implement the F8 and F35 M2 focus formula: F8_M2(enc-units) = A + B*Tsesurier + C*ZD : Computed value A: Focus Offset by instrumnet points efoscOff = 1996 harpsOff = 2081 cesOff = 2100 Coefficients B; SerTmperatureCoeff = -5.90646 C: zenithdistanceCoeff = -0.142615 ____________________________________________________ F35_M2(enc-units) = AA + BB*Tserurier +CC*ZD ; Computed value AA: timmi2Offset = 4.0226 Coefficients BB: SerTempCoeff = -0.0957 CC: zenithDisCoeff = -0.0046 _____________________________________________________ Center field and guid-probe focus variation factors as M2 movement function GPF(M2) = 0 (To be measured)) CFF(M2) = 0 (To be measured) Action Log : 5/17/2004 8:34:10 PM ebarrios Sorry I forgot to add for F8 offset the iqMesOff = 1883. Responsible : Software&Commun.Supp.T. Status : Assigned Deadline : 8/31/2004 12:00:00 AM Deadline Status : Pending ________________________________________________________________________________ Telescope : ESO 360 Create-date : 5/17/2004 7:25:56 PM Problem Short Description : A ND filter is needed to balance the flux between the two fibers after the fiber change. Action : Install a 0.1ND and a 0.2ND filter in the HARPS tungsten lamp, test them and select the adequate for the purpose (in collaboration with SciOps) Action Log : 5/18/2004 12:37:27 PM glocurto The filter is needed to balance the flux between the two fibers after the fiber change. 5/19/2004 7:45:34 AM gandreon Francesco Pepe wrote: Dear Gaetano, Indeed we already discussed the necessity to install/replace the fixed ND filter and the technical aspects with Gaspare and Alain. We authorize to proceed with the action. Many thanks and best regards, Francesco > -----Message d'origine----- > De : Gaetano Andreoni [mailto:gandreon@eso.org] > Envoye : mardi, 18. mai 2004 22:58 > A : Francesco Pepe > Cc : psinclai@eso.org > Objet : HARPS action item request. > > > Dear Francesco, > I would be most obliged if could authorize the opening of the > technical action item listed in the following, that I understand has > been already discussed with you by Gaspare. > Kind regards > Gaetano 5/25/2004 2:58:59 PM gandreon To be executed when Gaspare is back, on June 20. Responsible : Engineering Dep.(Instrum.) Status : Assigned Deadline : 6/20/2004 12:00:00 AM Deadline Status : Pending ________________________________________________________________________________ Telescope : ESO 360 Create-date : 5/18/2004 3:06:39 PM Problem Short Description : Low pressure in M1 compress air can be detected only by image distorsion. Also low flux in TCCD cooling cannot be detected. Action : Install two sensors for low air pressure (M1) and low water pressure (TCCD cooling). Alarms to be sent to Ritz. Action Log : 5/25/2004 2:59:33 PM gandreon Sensors ordered. 6/1/2004 5:28:56 PM gandreon Current deadline is for installation of the water sensor, already received. Responsible : Engineering Dep.(Mechanics) Status : Assigned Deadline : 6/15/2004 12:00:00 AM Deadline Status : Pending ________________________________________________________________________________ Telescope : ESO 360 Create-date : 5/29/2004 12:40:27 AM Problem Short Description : Tune HARPS PMT safety interlock Action : Current;y the HARPS Photo Multiplier Tube i(PMTs) nterlock cuts the power to the PMTs when the number of 10M counts per second is reached. This value however is too high and risks to jeopardize the safety of the PMTs. According to the company specifications the PMT stops to be linear at 2.5M counts per second. I am asking to lower the maximum number of obtainable counts to 3M counts per second. The possibility to discharge the PMT to ground in such cases would increase safety. It is critical that the interlock maintains the present capability to be reset via software, *without* having to go to the telescope. Action Log : 6/1/2004 5:33:28 PM gandreon Approval requested to ODG. Responsible : Engineering Dep.(Instrum.) Status : New Deadline : Deadline Status : Not Assigned ________________________________________________________________________________ Telescope : ESO 360 Create-date : 6/1/2004 5:23:48 PM Problem Short Description : Internal cone/sky baffle is in bad shape. Action : Refurbish or better rebuild the cone. Action Log : Responsible : Engineering Dep.(Mechanics) Status : Assigned Deadline : 8/31/2004 12:00:00 AM Deadline Status : Pending ________________________________________________________________________________ Telescope : ESO/MPI 220 Create-date : 8/11/2003 5:59:56 PM Problem Short Description : Sometimes the WFI filter wheel control stays in moving status for ever Action : To study the possibility to provide an abort button in the control panel of the instrument in order to generate an init situation Action Log : 9/19/2003 2:25:26 PM blopez The movement of the filter wheel is being controlled by low-level software, i.e., at electronics. The available listings show that commands are executed sequentially, meaning that during filter wheel movements no other commands can be sent to interrupt that action. This explains why it needs a power-cycle of the electronics to solve this problem. Due to this low-level limitation an abort button as requested is not feasible. Note: in order to improve the diagnostic of this problem tests can be carried out during the next technical time (30/09 - 04/10) to adjust the respective timeout settings. 9/23/2003 2:46:53 PM gandreon Electronic will investigate if a reset contact can be made available or if the power cycle will have to be used. 11/18/2003 2:57:17 PM gandreon The microprocessor has a reset pin. An Adam module (TCP/IP) will be used for remote resetting it. Responsible : Engineering Dep.(Electronics) Status : Closed Deadline : 10/28/2003 12:00:00 AM Deadline Status : Closed with Delay ________________________________________________________________________________ Telescope : ESO/MPI 220 Create-date : 3/1/2004 3:27:24 PM Problem Short Description : Move ESO-1.52m Flatfield screen to ESO-2.20m Telescope Action : Please install the SORIC flatfield screen from the ESO-1.52m telescope at the ESO-2.20m telescope. The simplist is probably to install over the top of the old small flatfield screenThe reason for this action is that the SORIC screen is a high UV reflectivity material and we thus hope to be able to get sufficiently blue light into FEROS using this screen to properly flatfield the full FEROS spectrum. If this proves successful, a new FEROS-FF screen position will need to be implemented within the 2.20m TCS control panel, but that should probably be a separate Action point when the screen has been demonstrated to provide the required BLUE flux. Action Log : 3/30/2004 2:44:59 PM gandreon Small project to be reviewed together with the ADC and new shutter. 5/25/2004 3:00:36 PM gandreon Waiting for A Gilliotte, due back on June 14th 5/25/2004 5:39:08 PM jpritcha I am UNBELIEVABLY DISAPPOINTED that such a simple request is taking SO long to complete. With a delay at least until mid June, this will mean at least 3.5 months from the date of creation of this Action Point. 6/1/2004 5:40:51 PM gandreon This action point was assigned on May 11th after being reviewed in the frame of the Feros project, part III. It had been rejected on March 30th because it was part of a larger project as mentioned dabove. Due to AGI illness, E Araya will supervise the delicate task of the reinstallation. Responsible : Infrastructure Support Group Status : Assigned Deadline : 6/15/2004 12:00:00 AM Deadline Status : Pending ________________________________________________________________________________ Telescope : ESO/MPI 220 Create-date : 3/6/2004 12:06:29 AM Problem Short Description : New functionality for HARPS/FEROS TCCD GRAB command Action : In order to remove the rcp command from HARPS and FEROS acquisition templates which can cause templates to fail if the target computer (for HARPS whaldrs and for FEROS drl2p2) is down, add the following functionality to the GRAB command (which will be used by a script running on the remote computers to determine which images need copying): **) After creating the TCCD image in $insroot/.../DETDATA/ create a softlink in $insroot/.../DETDATA/links pointing back at the actual image file. The copy script on the remote computer will then copy the TCCD image via the link, and when successfully completed remove the link (so as to avoid attempting to copy the image one than once). Action Log : 4/12/2004 3:31:11 PM tshen The asked functionality was added to the GRAB command, the new version of e3p6agws (3.6.1.4) was installed (2004-Apr-10) and is under observation. Now we are waiting for the commission, and it should be installed at 2004-Apr-28 or 2004-05-04 during the technical time. 4/13/2004 3:41:40 PM gandreon Deadline changed because it will be tested first at 360 during test time. 5/11/2004 2:53:04 AM rsoto New version of e2p2agws installed and commissioned during FEROS technical night (May 10). For HARPS, it will be commissioned during HARPS technical night (May 12). 5/11/2004 3:50:39 PM gandreon Feros done and commissioned by JPR. Responsible : Software&Commun.Supp.T. Status : Closed Deadline : 5/16/2004 12:00:00 AM Deadline Status : Closed on Time ________________________________________________________________________________ Telescope : ESO/MPI 220 Create-date : 4/20/2004 4:40:34 PM Problem Short Description : Reduced light arrive throught the calibration fiber of Feros. Action : Locate the source of the loss (fiber or optics at its ends) and eventually replace the fiber. Action Log : 4/27/2004 3:22:12 PM gandreon Waiting for the spare fiber 5/18/2004 4:42:17 PM gandreon The PO has been issued in Garching. Responsible : Engineering Dep.(Instrum.) Status : Assigned Deadline : 5/31/2004 12:00:00 AM Deadline Status : Pending ________________________________________________________________________________ Telescope : ESO/MPI 220 Create-date : 5/13/2004 2:00:07 AM Problem Short Description : The version of some modules in the integration module of FEROS INS is not correct. Action : Please note the current module versions for the following FEROS instrument modules: feotsf 1.17 feoseq 1.21 femtsf 0.4 femseq 1.6 Please insure the integration module (or whatever it is called) is updated appropriately. Action Log : 5/25/2004 11:43:42 AM rsoto feins integration module (2.10) updated according to the new version of the modules. Responsible : Software&Commun.Supp.T. Status : Closed Deadline : 5/25/2004 12:00:00 AM Deadline Status : Closed on Time ________________________________________________________________________________ Telescope : ESO/MPI 220 Create-date : 5/13/2004 2:06:47 AM Problem Short Description : The pecs configurations is not updated. Action : Please make the following updates to the pecs configurations for 2.20m machines. 1) Archive the current version of feros@wferos:.pecs/misc-all.env This includes the definition of the PERLLIB environment variable. After discussion with JCGT + RSo it was agreed this variable was NOT necessary for the ferosmgr account. 2) Archive the current versions of .rhosts for the astro accounts on w2p2off, w2p2dhs, wferos and w2p2tcs. This action is necessary to allow access to these machines from the drl PCs currently providing the FEROS data backup. Action Log : 5/25/2004 3:02:35 PM gandreon A change in the Pecs configuration has to be propagated to all telescopes. Therefore it should be done in occasion of VLT software updates. The 360 wil be updated first, at the current deadline. 5/27/2004 3:17:22 PM jpritcha PECS is configured so that it is specific to each telescope... so I do't quite understand this comment... In any case, I spoke to Juan Carlos Guzman yesterday about this item. He plans to make the changes for the 2.20m during the technical time tomorrow (Friday May 28th). Furthermore, as discussed with him there is an additional request: The e2p2ops .rhosts configuration should be updated. A new version of .rhosts file has been configured in e2p2ops on w2p2tcs. the file is .rhosts.new. This version should be instegrated into PECs and then installed for all 2.20m machines. Testing will be carried out during the technical night of 28/5/2004 by Ivo Saviane. 5/30/2004 3:51:50 PM jguzman The following version of the pecs module for 2p2 were installed in 2p2 machines: 2p2 WS pecslse2p2 version -------------------------------------------------- w2p2tcs 3.21 w2p2ins 3.21 wferos 3.22 w2p2oh 3.21 w2p2dhs 3.21 w2p2off 3.21 New image tape of wferos made. A complete verification of the 2p2 systems were performed on 28/05/2004 => succesfull. Responsible : Software&Commun.Supp.T. Status : Completed Deadline : 6/30/2004 12:00:00 AM Deadline Status : Pending ________________________________________________________________________________ Telescope : GENERAL Create-date : 9/30/2003 12:34:55 AM Problem Short Description : Finalize implementation of RITZ subnets. Action : The original users requirements and implementation plan of the network at RITZ considered a separate subnet for "visitors" and another one for "general purpose" use, in addition to the telescope subnets. The cabling is ready, but this was never implemented. Pls complete this implementation, so that, for instance, critical functions don't have to share subnet with visitor's laptop. Action Log : 4/13/2004 3:43:48 PM gandreon A conceptual design document has been prepared by Flavio 5/25/2004 3:03:32 PM gandreon An updated map of La Silla network (Rolando style) should be prepared for the review of the plan. Responsible : LS Management Status : Assigned Deadline : 6/11/2004 12:00:00 AM Deadline Status : Pending ________________________________________________________________________________ Telescope : GENERAL Create-date : 11/11/2003 2:57:20 PM Problem Short Description : Vapors from solvent used in PLS maintenance are not properly evacuated. Action : Improve the working area and the exaust pipe. Action Log : 1/27/2004 3:35:27 PM gandreon The solvent has been changed. 3/30/2004 2:45:45 PM gandreon ... but vapors are flamable and this make urgent a good gas evacuation. 4/13/2004 8:19:21 AM gandreon WEC:O.Lavin and L.Wendegass started and L.Gonzales will do the work in the near future. 4/27/2004 3:22:56 PM gandreon New deadline (it was 16/March) 5/25/2004 3:04:58 PM gandreon A more powerful extractor has been installed in the meantime. Responsible : Engineering Dep.(Mechanics) Status : Assigned Deadline : 6/1/2004 12:00:00 AM Deadline Status : Pending ________________________________________________________________________________ Telescope : GENERAL Create-date : 3/15/2004 6:58:17 PM Problem Short Description : Web filter page http://filters is esoonly accessible Action : Make it accessible from outside world. Action Log : 4/13/2004 8:19:52 AM gandreon WEC: Software (Percy) will study the problem 4/18/2004 8:47:26 AM agilliot It is a so old problem requested by opticians since long time ago. I am glad to see how formal has been requested by the Users Sciop 4/27/2004 3:24:02 PM gandreon Waiting for a report on the problem with our WEB maintenance to be forwarded to Director. 5/7/2004 8:07:16 AM gandreon Michael Naumann - ESO Garching +49 89 3200 6430 wrote: Dear Olivier, I sent the attached message 2 weeks ago to Elena telling her that I haven't received any response regarding the La Silla filter database setup and configuration; no response from Alain or his student who built the system. cheers>