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... Science Users Information > Data Handling and Products > Data Reduction FAQ > Where do I find reference data (e.g. line catalogs, configuration tables, etc.) ... Observing with ESO Telescopes . ... ESO-MIDAS . ... Data Handling and Products . Quality Control and Data Processing . Data Pipelines and Calibrations . ... Data Packages . Science Data Products Forum . Data Reduction FAQ . ... Data Portal . ESO Data . Hubble Space Telescope Data . ... ESO Data Access Policy . ...

... We present ultraviolet and optical spectra of the bright (V=16.5), high-redshift ( ) QSO HE1122 - 1649 (Reimers et al. 1995a,1995b). ... Keywords: absorption lines . ... The combined data are shown in Figure 1. ... The Ly profile reveals an absorbing subcomponent at in agreement with results from heavy element absorption lines detected in the high resolution optical data. ... Figure: Velocity profiles of heavy element absorption lines arising in the damped Ly system as seen in the optical data. ...

. Back to the Oxygen Page . Electron configuration: 1s 2 2s 2 2p . Electron impact Excitation . Blum R.D. "Rate coefficients for the excitation of infrared and ultraviolet lines in CII, NIII ans OIV", Ap.J. Suppl, 80 , 425-452 (1992)

... Many extragalactic objects for which radial velocities are desired display strong emission lines. ... EMSAO, a companion to the cross-correlation task XCSAO (Kurtz et al. 1992), was written to find emission lines automatically, compute redshifts for each identified line, and combine them into a single radial velocity. ... Figure: This EMSAO Summary page shows line centers and fit information for a night sky spectrum. ... To test EMSAO adequately, a lot of emission line spectra were needed. ...

... List of all members. static Quantum < Double > . ... HI line. static Quantum < Double > . ... vel of light static Quantum Double c; // Gravitational constant static Quantum Double G ; // Planck static Quantum Double h ; // HI line static Quantum Double HI ; // Gas constant static Quantum Double R ; // Avogadro static Quantum Double NA ; // electron charge static Quantum Double e ; // proton mass ... Quantum < Double > casa::QC::a0 [static] . ...

The Arcetri Spectral Code (Landi and Landini 1998) allows to evaluate the spectrum of continuum and line radiation emitted by hot and optically thin plasmas in the spectral range 1-2000 Angstrom. The Code is composed by a large database of atomic data and transition probabilities for calculating spectral line emissivities and a suite of fortran programs able to evaluate free-free, free-bound and two-photon continuum radiation. ... To get he Arcetri Spectral Code related publications . ...

... Files . ... tcc.msg.formatObjFields Namespace Reference . ... Definition at line 36 of file formatObjFields.py . ... Definition at line 107 of file formatObjFields.py . ... Definition at line 115 of file formatObjFields.py . ... Definition at line 129 of file formatObjFields.py . ... Definition at line 122 of file formatObjFields.py . ... Definition at line 213 of file formatObjFields.py . ... Definition at line 139 of file formatObjFields.py . ... Definition at line 247 of file formatObjFields.py ....

spaceweb@oulu.fi - last update: 5 January 1999, 1730 UT (RR) . According to ideal MHD wave theory, a plasma can support two basic wave types, i.e., the magnetosonic wave and the AlfvИn wave. In the theory, standing AlfvИn waves can be excited on geomagnetic field lines , forming so called field line resonances (FLR). ... 1996). ... Bellan, P. M., Mode conversion into non-MHD waves at the AlfvИn layer: The case against the field line resonance concept, J. Geophys. Res. ...

... The spectrum of the Sgr B2 molecular cloud has been surveyed between 215 and 265 GHz towards 3 positions, the dense cores Sgr B2(N)and Sgr B2(M), and the quiescent core Sgr B2(NW). ... The Sgr B2 molecular cloud, located approximately 100 pc from the Galactic Centre and with a mass of , is one of the most extreme cases among star formation sites ( Lis & Goldsmith (1991) ). ... Of the 3 observed positions Sgr B2(N) has the strongest line emission in most molecular species with a few exceptions. ...

Next: References Up: No Title Previous: Observational data and reduction . ... A minor loss of information is due to the overestimation of the scattered light in the region of and to the broad emission lines and . On the diagrams are shown the blue-shifted absorption lines and the interstellar diffusion bands. ... In Table 1 are given only emission lines. Questionable features and the lines that fell within the gaps are not included in it, question-marks are for unreliable identification. ...

Stellarium 0.12.3 . ... Classes . ... FileљStructure . ... StelLocation Class Reference . Store the informations for a location on a planet. More... #include < StelLocation.hpp > . QStringљ . ... Output the location as a string ready to be stored in the user_location file. ... createFromLine (const QString &line) . ... Definition at line 26 of file StelLocation.hpp . ... line . ... Output the location as a string ready to be stored in the user_location file. int StelLocation::altitude . ...

For calculating model spectra of early-type helium stars in LTE, we maintain a database of atomic data for, mostly, blue-visual absorption lines of light elements. The data is sorted with one file for each ion. ... III = ++ . ... It will work on both complete linelists (including the atomic data at the start and references at the end) or raw ion files (such as Ni2.d). ... A Fortran utility to convert linelists downloaded from the Vienna Atomic Line Database into the new QUB format. synspec_qub . ...

... In some cases where memory space is at a premium, it is possible to tailor the configuration to remove such features as reference clock driver support, debugging support, and so forth. ... The following lines are used in this file: . ... The DEFS_LOCAL line defines global flags that apply to all machines. Ordinarily, the only flags included are the -DDEBUG , which includes the debugging code, and -DREFCLOCK , which includes basic reference clock support. ... D_INCLUDE_BSD_SOURCE . ...

Next: Determination of the Up: Getting the Dispersion Previous: Line Detection in . In order to compute the dispersion relation, lines stored in table line.tbl have to be cross-identified with a reference catalogue . For the first few spectral lines in the central row, this has to be done interactively, the rest is automatic. ... Midas.. ... IDENTIFY/LONG . ... which plots the central row of the comparison spectrum and the interactive line identifications. ...

This section contains information of how user agents should treat control characters and other special characters. ... There are 256 character positions in the Latin-1 encoding. ... It consists of the space character, 186 characters that form a subset of the graphic characters in ISO 6937/2 (1983), and four additional characters that are intended for inclusion in ISO 6937/2. ... Certain characters are taken to have special meaning within the context of an HTML document. ...

... 22.Reference Frames . ... To derive the motion of a penny dropped inside an airliner moving at 600 miles/hr (about 1000 km/hr)--should we calculate it with respect to the interior of the airliner, or with respect to the ground? ... And if a similar penny is let go inside an orbiting spaceship--should its motion be calculated relative to the interior of the spaceship, or relative to the Earth outside? ... How do observations differ in the two frames--the airliner cabin and the Earth? ...

... We will consider the rms, (K), for observations with a receiver of system temperature, T , frequency resolution, per polarization, and total integration time per observing cycle, . ... For ``in-band'' frequency switching, the line under investigation is always in the observing band. ... Position Switching or ``Out-of-Band'' Frequency Switching: Here the line is only observed for one half of the time, with noise being present all of the time. ...

... This file table3 82 660 Observed wavelengths, laboratory values and identifications -------------------------------------------------------------------------------- Byte-by-byte Description ... Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- SpOrd Spectrum order 5- 12 F8.3 0.1nm SolLam Wavelength determination of all solar and telluric lines measurable on the ... Note (6): J: Junkes et al., ...

Emission Line -- Continuum Correlations in Low­Redshift Quasars Belinda Wilkes , Smita Mathur, Jonathan McDowell (SAO) and Ari Laor (Caltech) We investigate the relation between the observed optical emission line strengths, widths and ratios and the observed continuum properties for two samples of quasars: 43 Einstein observed quasars for which we have obtained IR--soft­X­ 1994). ... 1) Contrary to PG sample and Shastri et al. ...