... Recalibration / 26-10 . ... DPERSC-CP34SE: ...and 0 packets were found to have segments without Reed Solomon corrections CPEEND- DATA EDITING ENDED 31-AUG-94 16:23:20 FOR U28S0303P . CPE0EN--------------------------------------------- DATA EDITING COMPLETED ----------------------------------------------------- CPG0VS--------------------------------------------- DATA EVALUATION STARTED ----------------------------------------------- DPVSTR- DATA EVALUATION STARTED 31-AUG-94 16:23:39 FOR ...

... This guide will provide the basic procedure for a "standard" wview install. ... If a package requires installation, you should use the package management utility appropriate for your OS and distribution. ... If they are, you should install the devel version in order to get the development libraries that radlib/wview needs. libz - compression library - normally included in OS distribution . ... libgd2 - graphics drawing library - may require installation - http://www.boutell.com/gd/ . ...

... The J, H and K bands are characterized by a bright background, such a background is mainly due to the emission of atmospheric lines and of thermal radiation. ... If the source cover a large fraction of the slit, spectra off-source must be observed to adequately sample the sky background. ... The on chip integration time (time spent in each position of the slit) must not exceed 40 seconds in J and H bands and 60 seconds in K band. ... We suggest a sequence of 10 for each elementary integration time. ...

... 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. ...

... There are compelling reasons for the pulsar community to utilise a standard data storage format. For example, standardisation of file formats significantly decreases the amount of effort required to integrate new instruments into the analysis chain. ... Accordingly, we have defined PSRFITS as a standard FITS-based format for pulsar data files. ... For example, the first line of Processing History HDU contains information about the data acquisition program and the initial structure of the file. ...

Using the free source form it is not permitted to have comments starting with a C or a * in column 1. This would be a violation of the free format. ... An advantage compared with earlier Fortran standards is that the standard now requires that the compiler can signal if the user deviates from the permitted standard. It is required that a Fortran 90 compiler can signal . ... It has to be possible to ask the program to signal for any extensions outside the Fortran 90 standard. ...

... The SIRTF Science Center is developing two Web-based tools that will be used during operations. One tool is for Quality Analysis. ... The basic design requirements for the QA tool are (1) that it provide an easy way of looking at all the data, observation by observation, and (2) that it provide an easy way to specify status and comments for each observation. ... The data accessed by this tool consists of meta-data in the central database as well as the actual data files in the archive. ...

... New Mexico State University is seeking a technical and computer-oriented person as a Support Astronomer for nighttime astronomical observing at Apache Point Observatory (APO) with the Astrophysical Research Consortium (ARC) 3.5m Telescope. б  . ... Paper/email documents will not be accepted. ... TELESCOPE OPERATIONS SPECIALIST . ... Responsibilities include nightly operation of the 3.5m telescope and instruments, Quality monitoring the data streams and system performance and observing efficiency. ...

... For these observations night-time is required. Begin ­ End Interval­Interval ­ ­ ­ ­ 2 Days Needed at This Interval Time Constraints (Must Be Justified in the Prop osal Text) LST 0700 0700 0930 1715 Range - 1145 - 1300 - 1300 - 2000 Nights Notes 19 NGC 2577/UGC 4375 + Leo I Group 6 NGC 2577/UGC 4375 + Leo I Group + Abell 1367 51 Leo I Group + Abell 1367 89 Local Void (complete in second semester ) Constraints on scheduling: The Turn On Galfa Survey ( TOGS ) operates commensally with ...

... ORIGIN = 'ASC ' / Source of FITS file CREATOR = 'cxc - Version CIAO 2.2' / tool that created this output CHECKSUM = '78aM87YM77aM77YM' / HDU checksum updated 2003-01-07T20:23:55 DATASUM = ' ' DATE = '2003-01-07T20:23:25' / Date and time of file creation DATE-OBS= '2002-12-29T23:20:17' / Date and time of observation start DATE- END = '2002-12-30T10:13:33' / Date and time of observation stop TIMESYS = 'TT ' / ... DSVAL1 = 'TABLE ' / DM Keyword: Descriptor value. ...

Largely automated science processing (working title: phoenix) Reinhard Hanuschik, 2012-05-10 Pre-conditions · · · all associations ( ABs ) already done, by standard QC workflow all associations point to certified and archived master calibrations (the ones to virtual calibrations can't be processed so they need to be filtered) we use only selected ... Issues: · which products do we select for ingestion? ... VM, standard vs. non-standard setups no processing: o o ECHELLE, SLICER (why not?) ...