... Abstract Bracket a number. That is, given a number and an acceptable interval, make sure that the number is contained in the interval. ... Brief_I/O VARIABLE I/O DESCRIPTION -------- --- -------------------------------------------------- number I Number to be bracketed. end1 I One of the bracketing endpoints for number. end2 I The other bracketing endpoint for number. ... Particulars This routine provides a shorthand notation for code fragments like the following #include "SpiceUsr.h" . ...

... V.G. Kurt, V.V. Sokolov, S.V. Zharikov, G.G. Pavlov, B.V. Komberg: "BVRI observations of PSR0656+14 with the 6-meter telescope" (astro-ph/9706076), 1998, A&A, 333, 547 . ... A. Shibanov, A. B. Koptsevich, V.V. Sokolov, S.V. Zharikov, G.G. Pavlov, V.G. Kurt, V.N. Komarova: "Optical photometry of the PSR B0656+14 and its neigbourhood", 2000, Abstracts of JENAM-2001, 99 . ... A. Shibanov, V.V. Sokolov, V.G. Kurt: "Optical photometry of PSR B0656+14 and its neigbourhood", 2001, A&A, 370 , 1004 . ...

EURONEAR - recovery, follow-up and discovery of NEAs and MBAs using large field 1-2 m telescopes . ... Using these data, we present the incidental survey work which includes 558 known MBAs and 628 unknown moving objects mostly consistent with MBAs from which 58 objects became official discoveries. ... Based on three evaluation methods, most of our unknown objects are consistent with MBAs, while up to 16 unknown objects could represent NEO candidates and four represent our best NEO candidates. ...

... From the uvby photometry and proper motions for about 5500 nearby F stars we have found the following: (i) F stars , taken in narrow ranges of metallicity , show at [fe/H] 0 rather distinct cut-off in their distribution along the Main Sequence (MS) at the blue side, which is suggested to be an indication for the MS turn-off in stellar groups of fixed metallicity ; (ii) the corresponding turn-off age from theoretical isohrones strongly correlates with the ...

... The size of a regular paper should not exceed 12 pages in the journal format. ... Keywords: journal, composites, nanostructures, abstract, illustrations. ... The main text The main text should be in Microsoft Word format. ... Illustration and Tables All illustrations and tables should be submitted as separate files. ... Examples of the graph formats in linear and log scales are given in Fig. 1 and Fig. 2, respectively. ... Formulas, to which there are references in the text, are to be numbered. ...

This diagram illustrates the effects of floating a box ("inner") and how its "sibling" is forced below it due to the 'clear' property. A document window is shown, with 8 lines (numbered 1 to 8), each 24px high. Text before the "inner" box flows on lines 1 and halfway on line 2. The "inner" box has been floated to the right and occupies the second half of lines 3 and 4. ... The lines, as they appear in the image, contain: 1 Beginning of body contents. ... Inner contents" is blue. ...

... OOF software . ... Memos . ... Raw data . ... We present a Bayesian approach to calculating the coefficients that convert the outputs of ALMA 183 GHz water-vapour radiometers into estimates of path fluctuations that can be used to correct the observed interferometric visibilities. ... Please note that the files"COPYING" in each of the distribution packages have GPL listed but it is in fact LGPL which applies. ... This is the raw data from the SMA used in the analysis shown in Section 4 of the memo. ...

Next: Introduction Up: Old neutron star distribution Previous: Old neutron star distribution . The population of old galactic neutron stars is computed for model galactic potential and initial neutron star velocity distribution following from binary system evolution scenario. ... Statistical tests appropriate to the problem of gamma-ray burst space distributions are carried out for the obtained distribution. Key words: pulsars - old neutron stars - space distribution - gamma-ray bursts . ...

. Abstract can be submitted from April 1 to July 31, 2013. To submit your abstract: . Download the LaTeX templates here . Insert your abstract to the file "sample_en.tex" following the given sample. Control the result (applying LaTeX to the file "book_sample_en.tex"). Please, keep your abstract within one page, if possible. Rename the edited file "sample_en.tex" using for the filename your last name and e-mail it to ffk@gao.spb.ru , marking the message by the word "Abstract" in the field "Subject".

... 2 Preamble Please follow this sample (see LaTeX file). If your contribution is submitted by less than 3 co-authors, please use \markboth{A.B.\,Author A and A.B.\,Author B}{Title of Contribution} otherwise please use \markboth{A.B.\,Author A et al.} ... See, for example, \cite{ref1}. ... 6.2 Reference list Please follow the examples: [1] shows the ref. for a journal article, [3] shows the ref. for a monograph, [4] shows the ref. for an article in proceedings, [5] shows the ref. for a preprint. ...

... Author(s) (name or initials are given before family name); . ... Every entry in the list should give full list of authors (initials are printed after names) (for collections editor(s)), full title of book, collection and paper. ... Type - Times New Roman 12 pt (for the exceptions indicated below: title, list of authors, names of Institutions, names of sections should be printed in bold). ... Title of paper, list of authors, names of Institutions, formula, tables and pictures are centered. ... Name ....

Call For Abstracts . We welcome abstract submissions for oral presentations at the workshop, Concept Development for an Upper Atmospheric Research Facility at the Arecibo Magnetic Conjugate Point in Argentina to take place in April 17 - 19, 2006 , at the Arecibo Observatory, Puerto Rico . ... This section of the meeting includes talks on the instruments that are required at the facility to satisfy the science requirements discussed in Part I of the meeting. ... Part I~50% meeting time . ...

... 30, 2006 . ... If you retrieve these files via a Web browser, please note that you need to use the browser's "Save As..." facility. ... Figures must be provided as Encapsulated PostScript files and should be incorporated in your contribution using the standard Latex2e "graphicx" package as demonstrated in the demo file author.tex. ... Please submit the LaTeX source file of your contribution, and PostScript/PDF files of any figures, via email (!!!) to Iris Bronnert ( ibronner@eso.org ). ...

... This paper ( Burke et al. 2003 ) describes the creation of one such catalogue - the Southern Serendipitous High-redshift Archival ROSAT Cluster (SHARC) survey - which covers an area of 17.7 deg 2 and consists of 32 clusters with redshifts between 0.05 and 0.7 and X-ray luminosities between 7 x 10 42 and 4 x 10 44 erg/s: the high-redshift subsample contains 16 clusters with = 0.3 and X-ray luminosities greater than 2 x 10 43 erg/s (luminosities are quoted for the 0.5 - 2.0 keV energy band). ... 1997 ...

... Accurate positions of 404 compact radio sources used as calibrators by the VLA are presented. In addition, the structure and polarization of each source at both 4885 and 1465 MHz are given. ... Amplitude calibration was based on 3C286, whose fluxes at 4885 and 1465 MHz were assumed to be 7.41 and 14.41 Jy, respectively, in accord with the scale of Baars et al. (1977). short description of columns, as taken from the publication: . 1 source name . ... 8 Polarized flux at 4885 MHz (mJy) . ...

... Study of Mg-Fe-silicate glasses of variable composition. ... With the new data, the astrophysical discussion started in Paper I was continued and focussed on the comparison of the olivine glass data with IRAS LRS spectra of O-rich circumstellar envelopes around Mira stars. ... The new olivine glasses point to the interesting consequence that the temperature for silicate dust grains at the inner edge of circumstellar envelopes must be considerably higher than the values often given in the literature....

Pairs, groups and filaments of dwarf galaxies in the nearby Lynx-Cancer void as a reflection of void Dark Matter distribution Tepliakova A.L.1 , Pustilnik S.A. 1 1 Special Astrophysical Observatory, SAO RAS; Abstract The web of the three-dimensional matter distribution in the Universe is well repro duced in the N-b o dy simulations of Dark Matter in voids, alb eit scaled-down (Gottlo eb er et al. ... The total numb er of the void galaxies also app ears larger than exp ected in simulations. ...

IAU Commission 31 (Time) Circular 8, 4 April 2003 Dear colleagues, Here are some informations or events related to our Commission 1)Election of officers for the triennium 2003-2006 For 2003-2006, the present vice-president D.N. Matsakis will be president of Commission 31. ... 2)IAU GA and related deadlines The XXV IAU General Assembly takes place in Sydney, Australia, July 13-26 2003 (see http://www.astronomy2003.com). Please note the following deadlines: *30 April 2003: Early registration to GA. ...

... List of SAS threads . This thread contains a (very!) simple standard XSPEC session for fitting data from the X-ray cameras. ... Start XSPEC . ... Load spectrum data: . ... response 1 PN.rmf . ... plot data . Fig.1: XSPEC data plot . Ignore bad channels in data: . ... The latter, the maximum number of channels to bu summed. plot data with model adjustment and e.g. the residuals (alternatives, ratio data/model, absolute chi-squared, etc) . ... Fig.2: XSPEC data, model and residual plot . ...

... Up: Algorithms . ... Non-linear and non-parametric algorithms for data averaging, smoothing and clipping in the RATAN-600 flexible astronomical data processing system are proposed. Algorithms are based on robust methods and non-linear filters using an iterative approach to smoothing and clipping. ... The history of algorithms, based on the robust methods and non-linear filters using an iterative approach to smoothing and clipping, began twelve years ago in the data reduction at the RATAN-600. ...