... The LI or list item element is used for items in both ordered and unordered lists. ... An SGML identifier used as the target for hypertext links or for naming particular elements in associated style sheets. ... CLASS . This a space separated list of SGML NAME tokens and is used to subclass tag names. ... CLEAR . This attribute is common to all block-like elements. ... The CLEAR attribute allows you to move down unconditionally: . clear=left . move down until left margin is clear . ...

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• Definition Lists
• Overview of Character-Level Elements
• The Body Element and Related Elements

The overall efficiency (including atmospheric transmission, reflectivity of the telescope mirrors and overall efficiency of the optics and of the detector) for broad-band imaging should be about 25% in H and K, and about 15% in J. The main noise source for both broad- and narrow-band imaging should be the photon noise associated to the background+source flux. ... Flat fielding (and possibly background subtraction) might increase the noise by a factor 2 ? ...

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• Appendix B - The K-T Event
• Home - Fractionation of isotopes in space: from the solar system to galaxies
• CHIANTI: A Database for Astrophysical Emission Line Spectroscopy

... There is one record per exposure. ... Field dataset_ name date_obs dec_targ dec_v1 equinox expend expflag expstart exptime fgslock instrume linenum monangl mtflag npdectrg npratrg observtn ... progrmid proposid ra_targ ra_v1 seqline seqname short_pep_expo sun_alt sunangle surfaltd surflatd surflong targname time_obs tuple_id Contents Name of the dataset UT date of the start of the observation (dd/mm/yy) Declination of target ( degrees ) Declination of telescope's V1 axis ( ...

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• Spectral Element [Sp_Element]
• CSPICE Routines: ORDD_C
• CSPICE Routines: ORDI_C

... The collecting area is increased by nesting concentric mirror pairs, all having the same focal length. ... Figure shows the largest optical element being ground at HDOS. ... X-ray testing demonstrated that the CXO mirrors are indeed the largest high-resolution X-ray optics ever made; the nominal effective area (based on the ground calibrations) is shown as a function of energy in the left panel of Figure , along with those of their Einstein and ROSAT predecessors. ...

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• Be/X-ray binaries and candidates
• AXAF-Chandra

... J102815: A Star That Should Not Exist . ... Stars born in the generation before our Sun, Population II stars , the stars that created most of the heavy elements around us today, are seen to have some, although less, elements heavier than H and He. Furthermore, even the elusive never-seen first stars in the universe, so-called Population III stars, are predicted to have a large mass and a small but set amount of heavy elements. ... Publications with keywords: star - lithium - Population III . ...

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• Journal "Peremennye Zvezdy"
• XWare > APOD

... Driver ID: IRIG-AUDIO . ... This driver supports the Inter-Range Instrumentation Group standard time-distribution signal IRIG-B using the audio codec native to the Sun SPARCstation. ... The driver gadget uses a modified BSD audio driver for the Sun SPARCstation which provides a timestamp, raw binary timecode, status byte and decoded ASCII timecode. ... The 100 elements of the IRIG-B timecode are numbered from 0 through 99. ... This driver presently does not use the CF elements. ...

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• APOD: 2011 September 7 - J102815: A Star That Should Not Exist
• Cidadao Atlas
• APOD: 2013 November 12 - The Unexpected Tails of Asteroid P5

... Bojan Nikolic web pages home . ... For some numerical experiments with CASA , I have recently been recompiling some parts of this package. ... That is before even touching the code! ... I used the SCons build system to build the CASACORE libraries. ... Apparently missing include for strlen: --- a/code/display/Display/Options.cc +++ b/code/display/Display/Options.cc @@ -30,6 +30,7 @@ #include <sys/stat.h> #include <iostream> #include <dirent.h> +#include <string.h> namespace casa { namespace viewer {...

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• _element struct Reference
• OptInt PmWiki : Include Other Pages | Attach
• OptInt PmWiki : Include Other Pages | History

EUNAWE Project Manager Europ ean Universe Awareness A two-year fixed-term position of EUNAWE Pro ject Manager is available at the Armagh Observatory funded by the Seventh Framework Programme of the European Union (EU). ... There will be regular meetings between the EUNAWE Pro ject Manager and the Grant PI at the Armagh Observatory, several per month during the initial phases of the pro ject and a minimum of one per month thereafter. ... The Armagh Observatory is an equal opportunities employer. ...

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• Definition of Scientific Misconduct
• Armagh Observatory Press Release
• Atomic data for Stellar Atmospheres: lte_lines

... SciSim release covered by this note . ... Data-Analysis-with-SAS in a simple and standardised way, and should allow calibration experts to re-assess the reliability of the different elements of XMM-Newton simulations. ... Also, a release of all calibration files to be used in the reduction, through the SAS, of SciSim generated data, is coordinated with this release. ... Furthermore, two SAS tasks (odffix and epicproc) had to be updated to make possible a proper SAS data reduction of simulated data. ...

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• Selection of observations of empty RGS files
• Input
• Generation from In-Orbit Data

Underdetermined sets is a new type of data structures (terms) developed in Actor Prolog . ... The point is that an underdetermined set can include some indefinite rest (a tail) like a list in usual Prolog . At the same time, the order of elements of an underdetermined set can be arbitrary one and it does not affect results of unification of underdetermined sets. Moreover, Actor Prolog guarantees that a rest of an underdetermined set never contains elements that are explicitly given in the set. ...

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... ALMA . ... ARC Staff at ESO . ... The European ALMA Regional Centre (ARC) provides the interface between the ALMA project and the European science community. ... Below you can read the latest Announcements from the European ARC Network.. ... The call for 1-mm Very Long Baseline Interferometry (VLBI) proposals to use phased ALMA at Band 6 in Cycle 4, in collaboration with the Event Horizon Telescope Consortium (EHTC), will be released to coincide with the ALMA Cycle 4 Call for Proposals in March 2016...

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• BL Lacs
• pyQC: Python 2.6.2
• The Very Large Telescope Project

... Any elements created after this call will be placed in the container. ... After such a shell container has been created, it is not visible yet. ... Main program: /* example9.c -XT */ # include stddef.h # include gipsyc.h # include cmain.h # include init.h # include finis.h # include userfio.h # include ggi.h /* * Button keyword handler for quitting. */ static void quit(ident id, char * key , int code, void *arg) { bool button =toflog(FALSE); ( void )userflog( , 1, 2, ...

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• Graphical User Interface Example (2)
• casacore: casa::Link< t > Class Template Reference
• Synth Workshop

The Russian Parliament will soon consider a bill that would restructure the Russian space program, 35 years after the launch оf Sputnik. ... But the legislation's most striking and controversial feature is a provision that would ban testing and deployment оf space weapons ? including anti-satellite weapons and space-based missile interceptors. ... A draft bill was written by a group of experts within the Moscow Space Club, several of whom now work on space issues with the Russian Parliament. ...

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XmCCD ----- The programs provided here offer a Linux graphical user interface to astronomical and scientific CCD cameras. ... It is the latest one they offer and the files included allow support for Android and Mac OS X. This distribution of XmCCD includes source code to utilize the SBIG shared library libsbigudrv.so with a Motif-based graphical user interface. ... The XmCCD source package includes and will install: SAOimage ds9 xpa cfitsio SAOimage is the primary image display for XmCCD. ...

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• http://www.astro.louisville.edu/software/sbig/archive/xmccd-4.2.2/README
• http://www.astro.louisville.edu/software/xmtel/archive/xmtel-3.1/TODO
• http://www.astro.louisville.edu/software/sbig/xmccd-5.1/README

... , for reviews and suggestions ================================================================ * Play Information * Episode and Level # : E1M1 Single Player : Yes Cooperative 2-4 Player : Yes Deathmatch 2-4 Player : Yes , although not recommended Difficulty Settings : Yes New demos : No New Sounds : No New Graphics : No * Construction * Base : New ... You were assigned to the base on Mars, before any of this horrible Hell broke loose. ... Now finally, a taste of freedom! ...

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• SGML reference information for HTML
• Conformance: requirements and recommendations
• Explanations for solar physics computing page

This page is devoted to information on Supernova 1999dq in NGC 976 Basic information on this SN, including the last reported brightness, on this Supernova can be found on the main supernova page. Information on the original web pages for many of these images can be found on the Supernova links web page. Supernova 1999dq is the 24th LOSS discovery this year. ... VSNET Light curve (requires JAVA). ... vsnet-alert 3442 ] SNe 1999dp and 1999dq . vsnet-chat 2285 ] Host galaxy of SN1999dq . ...

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• Supernova 1999ee and 1999ex in IC 5179
• Supernova 1999ev in NGC 4274
• Supernova 2001C in PGC 19975

.

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• Rainfall in Eugene Oregon
• Low Surface Brightness Galaxy Gallery
• Astronomy HyperText Book: Fusion Sequences in Stars

Boris I. Rabinovich . Magnetohydrodynamical element in the problems of RC and SC stabilization . ... The use of the control system including the MGD elements for stabilization of the dynamically non stable objects as been considered. ... The possibilities of the control system with MHD elements are presented: RC non stable in the longitudinal direction (POGO) and the non stable rotating SC with the flexible spike antenna located along the rotation axis (like Auroral probe of INTERBALL project). ...

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• Units and elements of flight and airborne systems
• Elements of Algebra
• A Math Refresher

Stellarium 0.12.3 . ... Classes . ... FileљStructure . FileљList . FileљMembers . core . ... StelSkyLayerMgr.hpp File Reference . Define the classes needed for managing layers of sky elements display. More... #include <QString> . include <QStringList> . include <QMap> . include "StelModule.hpp" . ... Go to the source code of this file. class љ . ... Manage the sky background images, including DSS and deep sky objects images. ... Definition in file StelSkyLayerMgr.hpp . ...

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• Stellarium: CLIProcessor Class Reference
• Stellarium: core/planetsephems/calc_interpolated_elements.h Source File
• Stellarium: MultiLevelJsonBase Class Reference

... A # # [defs] CREG_DEC_F 0 CREG_ROUND_EN 1 CREG_TUNE_L 2 CREG_TUNE_M 3 CREG_D1_COUNT_L 4 CREG_D1_COUNT_M 5 CREG_S2_COUNT_L 6 CREG_S2_COUNT_M 7 CREG_D2_COUNT_L 8 CREG_D2_COUNT_M 9 CREG_S3_COUNT_L 10 CREG_S3_COUNT_M 11 CREG_D3_COUNT_L 12 CREG_D3_COUNT_M 13 CREG_SHIFT_FIR 14 CREG_GP_SEL 15 CREG_ADC1_SEL 16 CREG_ADC2_SEL 17 [dump] packet 0x0200000 # Size of each data packet name sasdr_world filesize 20000000 # in 1kbyte blocks byteswap 1 # 0-7 adcclk ...

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• Pulsars
• Frontiers of Astronomy with the World's Largest Radio Telescope Frontiers of
• University of Bristol: Lecturer/Reader in Astrophysics (Two posts) - jobs.ac.uk