Next: Summary of reduction Up: Echelle Reduction Previous: Saving the Data . In the present version we will be concerned with the standard configuration of CASPEC, the Cassegrain Echelle Spectrograph which is in operation at the Cassegrain focus of the ESO 3.6 m telescope. ... In its standard configuration CASPEC uses a a 31.6 lines/mm echelle grating together with a 300 lines/mm grating cross disperser. ... The table shows the change in resolution with the order number. Table: Resolution . ...

... unpriV - filter to unpack ri data (ao) unpriV [ -b bits ] [ -i numInputFifos ] [ -f fifoToOutput ] [ -d dataFormat ] [- t type] . unpriV is a program to unpack a single channel of RADAR INTERFACE (RI) binary data to the specified output format type. ... The radar interface has 2 channels of 2 digitizers each. ... numFifos 1 or 2 to specify the number of channels in the input data. ... fifoToOutput If the input data has two channels then this specifies which of the two to output (1 or 2). ...

Russian . Main . News . ... Minutes of the Telecon on January 17, 2012. ... News of the RadioAstron mission on the Lavochkin Association site up to September 15, 2011 (in Russian). News of the RadioAstron mission up to September 3, 2011. News of the RadioAstron mission on the Lavochkin Association site (in Russian). News of the RadioAstron mission up to August 18, 2011. ... Second version of the RadioAstron Mission Operations Handbook ( in Russian )is placed on the project site . ...

. User must specify the main plane and equinox of coordinate system by marking corresponding radio buttons, first in the left column Main plane and then in the right one Equinox . Paid attention to the fact that previously made choice of coordinate type (spherical or rectangular) and that of the type of positions (astrometric or geometric or apparent) constrains the choice in present item (see III.1. Basic concepts ).

... distributed/updated files; VCAL directory managed . ... export to qcweb: all files (ex hdr/fits) in $DFO_LOG_DIR/<date>; all files (ex hdr/fits, ex ps) in $DFO_PLT_DIR/<date> . ... The final directories on the DFOS systems are: $DFO_CAL_DIR/$DATE for calib data, $DFO_SCI_DIR/$DATE for science data, $DFO_PLT_DIR/$DATE for graphical information, and $DFO_LOG_DIR/$DATA for pipeline logs, association logs, trending logs, and ABs. ... 2.14 move the ABs, AB logs and processing logs to $DFO_LOG_DIR/<DATE> ...

New RRC variables with an additional non-radial pulsation . PZ, vol. ... We present a new study of 14 known RR Lyrae variable stars from the Catalina surveys periodic variable star catalog. ... New Double-Mode RR Lyrae Variables III . ... We present a new study of 123 known RR Lyrae variable stars from the Catalina surveys periodic variable star catalog. ... According to these data, the stars are double-mode RR Lyrae variables, pulsating in the first-overtone and fundamental modes. ...

... Exposure Time Calculator (ETC) . ... ESO - Public Surveys . ... the recommended values to use for DIT, . ... Detector on-chip integration (DIT): seconds. to your chosen value - a separate page gives recommended values to use for DIT - for modes 1 and 2 below you may wish to start with the maximum recommended values as these will minimize the effect of read noise (a total object exposure of Y secs with DIT=X secs will produce Y/X lots of read noise) and give you a lower limit on the time needed. ...

Comedi Documentation . ... Next . comedi_get_timer -- timer information (deprecated) . ... int comedi_get_timer (comedi_t * device, unsigned int subdevice, double frequency, unsigned int * trigvar, double * actual_frequency); . deprecated The function comedi_get_timer converts the frequency frequency to a number suitable to send to the driver in a comedi_trig structure. ... comedi_get_buffer_offset . ... comedi_timed_1chan ...

... We present requirements for a standardized 1-dimensional spectral data model for use in the Virtual Observatory. ... Our model separates metadata needed by applications using the idealized, generalized spectrum (pixel values, coordinates, errors, units, resolution) from metadata describing the idealized observation (sky region, observation date) and from metadata which are needed by specialized applications which deal with particular observational strategies (e.g. spectral extraction details). ...

... Recent Topics . ... Forum . MAO main . Flame . The "Flame" description . ... The English description is not quite correct, I suggest something like: . ... Just testing forum . The administrator has disabled public write access. sekanato . ... Description changed. ... The administrator has disabled public write access. Board Categories MAO main - Info - MAO - news - Flame Technical - Technical Support(Forum)(Техподдержка(Форум)) . ... Powered by Kunena Forum . ...

Next: Roche lobe overflow (stage Up: Principal Evolutionary States of Previous: Main-sequence stars (stage I) . ... The duration of this stage for a binary component is no longer a function of the stellar mass alone (as in the case of single stars), but also depends on the initial binary type (A, B or C) (Iben and Tutukov, 1985, 1987[ 74 , 75 ]): . The radius of the post-MS star rapidly increases (on a thermal time-scale)   and reaches characteristic giant values. ...

... Государственного Астрономического Института им. П.К.Штернберга . Московского Государственного Университета им. М.В.Ломоносова . ... zharov @ sai.msu.ru . ... Россия, 119992, Москва, Университетский проспект, д.13, ГАИШ . ... Телефон: (095)939-50-24, . 939-37-64 . Факс: (095)932-88-41 . ...

XPA supports host-based access control for each XPA access point. You can enable/disable access control using the XPA_ACL environment variable. ... See XPA Access Points and Templates for more information about xpa templates. ... For example: xpaset -p xpa1 -acl "somehost -" will turn off all access control for somehost to the xpa1 access point, while: xpaset -p XPA:xpa1 -acl "beberly gs" will give beberly xpaget and xpaset access to the access point whose class is XPA and whose name is xpa1. ...

SAO is Russia's main centre for ground-based space research. ... The basic instruments of the Observatory are the optical telescope BTA (Big Alt-azimuth Telescope) with a main mirror diameter of 6 m and the radio telescope RATAN-600 with the antenna diameter 600 m. Study of the Universe as a whole, analysis of non-stationary energy release in galactic and extragalactic objects of various types, investigation of evolution and chemical composition of our Galaxy and the nature of solar activity. ...

... About meteorites . ... Meteoritic data . Meteorite Encyclopedia . ... About laboratory . ... In addition, meteorites are divided into falls and finds depending on how they were collected. ... In other words, by far most meteorites falling on Earth are chondrites. Finds are meteorites that were not seen to fall but were subsequently discovered on the ground, often long after they landed. ... The vast majority of meteorites in museum and private collections around the world are finds, not falls. ...

The results of the 2008 Research Assessment Exercise (RAE), published on 18th December, show that the Armagh Observatory has significantly improved its research performance since the last RAE in 2001. ... In 2008, as in previous RAEs, the Observatory submitted 100% of its eligible research staff for assessment. ... The Armagh Observatory is a modern astronomical research institute supported by grant-in-aid from the Northern Ireland Department of Culture, Arts and Leisure. ...

The data that comprise the figures on the previous page can now be directly retrived as formatted text files. Click on any of the links below to download the data. The links are sorted by spectral type. If you want to try something difficult, see if you can combine various classes of stars to produce a galaxy spectrum. ... The data stars at wavelength 3505 angstroms and each point represents an additional 5 angstroms. ... wavelength = 3505 + 5*(bin) ; bin = 1,1084 . ...

NAME apxs - APache eXtenSion tool SYNOPSIS apxs - g [ - S variable = value ] - n name apxs - q [ - S variable = value ] query ... apxs - c [ - S variable = value ] [ - o dsofile ] [ - I incdir ] [ - D variable [= value ] ] [ - L libdir ] [ - l libname ] [ - Wc, compiler - flags ] [ - Wl, linker - flags ] files ... apxs - i [ - S variable = value ] [ - n name ] [ - a ] [ - A ] dso- file ... apxs - e [ - S variable = value ] [ - n name ] [ - a ] [ - A ] dso- file .. ...

... Comments, Opinions Publications Dnepr Program . Dnepr launch record 17 August 2011. Cluster Launch of Dnepr LV 22 August 2013 KOMPSAT-5 Launch 21 November 2013. Dnepr Cluster Mission 2013 19 June 2014. ... Mission profile SHM configuration Reliability Dnepr LV Performance Launch Sites . ... Description and main specifications . Dnepr launch vehicle (LV) is based on the SS-18 liquid-fuelled ICBM and has a three-stage plus Space Head Module (SHM) in-line configuration. ... Dnepr LV . ...