... HST . ... Data . ... HST Overview . Overview . ... Cycle 24 Announcement . ... Changing Programs & Resolving Problems . ... Program Information . ... Hubble Observation Problem Reports (HOPRs) provide a mechanism for you to inform STScI when a problem has occurred with the implementation, scheduling, execution, or data processing of your observations. ... If one or more of your HST observations appears to have a problem, go to the Program Information Page and retrieve the program information. ...

Next: Mission Operations Data Transfer . ... VLBI Tape Management . VLBI Tapes . ... When: As soon as the correlator is satisfied with the correlator output. back to top . ... What: Each correlator will maintain a data base including the status of all VLBI tapes under its control. ... The correlators will distribute tapes to mission elements based on the Observation Summary File produced by the RSOG ( Observation Summary File ) to ensure each element has enough tapes to support SVLBI observations. ...

ATNF Home . About ATNF . ... About ATNF overview . ... Governance overview . Australia Telescope Steering Committee . ... Our people overview . ... Staff list | ... Parkes radio telescope . ... Australia Telescope Online Archive (ATOA) . ... VLBI . ... CSIRO ATNF Data Archives . ... Visiting Parkes radio telescope . ... Parkes radio telescope webcam . ... This message : [ Message body ] [ More options ( top , bottom ) ] . ... like elevation of the sources during the observations, slew times, . ...

The run progress pages document the execution of Service Mode and Visitor Mode observing runs carried out at the Paranal Observatory. A summary of the run's characteristics is given, as well as a time-stamped list of all Observation Blocks (OB) that were executed until now. ... If reduced data for the given run exist, those are also reported in both the OB Summary table and in the details. ... Reduced : information shown only if pipeline-processed reduced data exist for the OB . ... OB ID . ...

... mar05: filter bank installed but left in wide band mode. 05apr05: 10db amps placed in pixel 2a,2b path in front of the filter bank. 08apr05: 10db amps placed in front of filter bank for all alfa pixels. 12apr05: 6db attenuators placed before 10db amps. 25apr05: 10db amps are now only in the OH filter bath. ... This allowed the search of the data taken by P2030 (100Mhz bandwidth, cfr 1420Mhz, 64usec samples) between 01feb05 and 01may05 for signals of the aerostat radar. ...

How do I report problems I've encountered using NEdit ? ... If you have a problem which is not covered in the on-line help, in this FAQ, or in the README file specific to your system, you can report it to discuss@nedit.org (usage questions) or, develop@nedit.org (error reports). ... Below are some suggestions for information you can provide to help in diagnosing your problem. ... As of version 5.2 a summary with build information is present under 'Version' in the Help menu. ...

... There are still a few items on a punch list of things to be completed. ... Sometimes recovery is quick and other times the instrument self corrects itself just by sitting idle. ... As of August 30, 2013, the 3.5-m has implemented a TAI time standard in all the instrument headers. ... ARCES . ... 2015-11-30: The slitviewer computer problems appear to be intermittent but are quickly resolved by the observing specialist. ... The instrument is available again . ... 2015-10-26: Vacuum not soft. ...

... Help . ... Before you report a problem you should check if it has already been reported in the help desk's SAS archive . If you decide to report a problem, then you can do so via the Observation Report (OR) form. Shortly thereafter you will be contacted by the XMM-Newton help desk . ... In most cases you'll be asked to send the following information, so you may consider enclosing it right away in your report (not all items apply in all cases): . ... Information about the CCF in use . ...

multi-rsh is a perl script which runs the same command on multiple machines, in parallel, and provides reasonable, adjustable timeouts for those machines which fail to answer. Both standard output and standard error are returned through the same channel, and all output has the hostname prepended to each line. Multi-rsh must be run as root (remote jobs can be set to run as any user, see Options below). ... Neither form allows you to directly pass input to the remote programs. ...

... Stellar Evolution is driven entirely by the never ending battle between Pressure and Gravity . As imbalances are reached, the star is driven to find a new Energy source. ... Pressure and gravitational forces are equal, the star is stable and its core is sufficiently hot to fuse Hydrogen into Helium More about main sequence stars . ... The luminosity generated by the core fusion of Helium into Carbon is far greater than the shell luminosity associated with the fusion of Hydrogen into Helium. ...

Next: Reduction procedure Up: Extinction and transformation Previous: Strategy . Standard stars can be included in the extinction solution, if one is careful. The problem is that there are usually appreciable ``conformity errors'' due to mismatch between the instrumental and the standard passbands [ 16 ]. ... Thus, it is wrong to assume that the transformation between the instrumental system and the standard system is exact, even if there were no measurement error in either system [ 1 ]. ...

... 12:20 S.V. Chervon. ... 15:00-17:30 Workshops (section VI: Modern Extensions of General Relativity ): (Chair: M.V. Sazhin) V.D. Ivashchuk, V.N. Melnikov. Black Hole P-Brane Solutions for General Intersections . ... M. Pomazanov, S.O. Alexeyev. Numerical Analytical Methods for Investigation of the Black Hole Solutions in Low Energy String Gravity . A.Toporensky, V. Ustiansky, S.O. Alexeyev. ...

... We summarize the discussions that took place during the FITS Birds of a Feather (BoF) session, which was held Monday, September 23, 1996 at 16:00. For completeness we also include a summary of the 1995 FITS BoF, which was never published. ... Oral papers by Clarke, Allen, Mink, Mandel, and Wells were presented in a special FITS afternoon session, and posters were presented by Pence, Farris, Tripicco, and Stobie; see the papers by these authors elsewhere in this volume. ... CFITSIO (Pence) . ...

PRESS-RELEASE . ... At S.P.Korolev Rocket and Space Corporation Energia under the chairmanship of N.N. Sevastyanov, Corporation President, General Designer, took place the next session of the General Designer’s Review Board on the Russian Segment of the International Space Station (ISS). ... The Report on the status of Soyuz TMA-9 manned transport spacecraft launch processing (reporter: Yu.I.Grigoriev, RSC Energia Deputy General Designer, Director of Orbital Complex Programs); . ...

... Astrophysics Group . ... Optical Interferometry . BSMEM Software . ... OIFITS: A Data Exchange Standard for Optical (Visible/IR) Interferometry . ... The Cambridge software package for image reconstruction from optical interferometry data has been dubbed BSMEM, to stand for BiSpectrum Maximum Entropy Method. It was first written in Fortran and completed by David Buscher in 1992 to demonstrate direct maximum entropy reconstruction from optical aperture synthesis data (Buscher 1994). ...

Note: there are 3 CIS id's for reporting problems listed at the end of this file. ... Can you recreate the problem? ... CSD Level: _______ OS/2 Version 2.0 GRE.. ... Port Used : ________________ Printer is attached to: Local _ LAN Server _ Host _ COMMUNICATIONS MANAGER - If this is a problem with Communications Manager, please provide answers in this section: OS/2 Extended Services .. ... CSD Level: ________ OS/2 LAN Server 2.0 Advanced: _ CSD Level: ________ LAN REQUESTER: LAN Server 2.0 Requester.. ...

As it proposed by the Statutes/Regulations of the International Astronomy Olympiad, the first part of preparing application to participate in the coming IAO is presenting of a short report of National Astronomy Olympiad of the current year for the Advisory Committee. ... Date of receiving report from the country . ... July 18 - August 7 . ... August 31 . ... Date of receiving draft report (or not full report) . ... Date of receiving official application . ... Done after receiving ANRAO application) . ...

... R.A. = 00h55m04s.86, Decl. = -37 41'43".7 . ... Variable star in NGC 1511 . ... Variable star near Pegasus 2001bn IAUC 8624 BV anon 2001bh 7622 K star ugc11635 2001dh 7482 M star ic5374 1999db 7227 QSO anon 1999dc 7227 AGN anon 1999cx 7210 AGN anon 1999cu 7210 AGN anon 1999bs 7141 cat var ugc11093 1998di 6982 dwarf nova anon 1993U 5818 QSO anon 1993V 5818 QSO anon 1992W 5517 M star mcg 8-23-96 1992X 5517 M star mcg 6-32-24 1991ap 5327 QSO anon 1989Z 5162 var ngc4013 1985J 4059 CV ugc6274 ? ...

... The 1997 conference of the Astronomical Data Analysis Software and Systems Conference series was organized by ST-ECF/ESO during 14 to 17 September, 1997. It was the first time this conference was held in Europe. ... Key topics of the conference were Computational Astrophysics, Computational Infrastructure, Future Technologies, Data Analysis Applications, Education and Public Outreach, Data Flow and Scheduling , Archives Information Services, and Astrostatistics/Data Bases. ...

The CHIANTI database consists of 4 primary ASCII files for each ion in the database. contains the energy levels in cm^(-1) It includes both experimental data and theoretical values of the levels energies. ... 1997, ADNDT, 67, 225. %comment: energies have been corrected (Sep 2003). ... Wavelengths are based on experimental level energies where available; wavelengths calculated from theoretical energies are less accurate and are given as negative values. ...