... filename list . ... Names of input EPIC fits images or event lists (if useevents = true; not yet implemented) . ... Name of eboxdetect source list . ... float . ... 1.0 param 50.0] . ... XID band energy conversion factors, given in units of counts cm erg . ... false . ... Array of six integer numbers specifiying the upper and lower energy band for each of three hardness ratios (PN) . ... Array of six integer numbers specifiying the upper and lower energy band for each of three hardness ratios (MOS1)...

The HyperNews Linux KHG Discussion Pages . Forum: The Linux Kernel Hackers' Guide . Date: Thu, 22 May 1997 19:29:43 GMT . From: < castejon@kbw350.chem.yale.edu > . How the resources limits (filesize, cpu,etc) can be changed? . Messages . 1. Setting resource limits by Jukka Santala .

... 389Voges+ IX/29 ROSAT All-Sky Survey Faint Source Catalog (Voges+ 2000) ============================================================================= ROSAT All-Sky Survey Faint source Catalogue (RASS-FSC) Voges W., Aschenbach B., Boller Th., ... The sources have a detection likelihood of at least 7 and contain at least 6 source photons. ... 0 Extraction radius 141-146 A6 --- PrioFlags [01] priority flags (8) 147 A1 --- PHA [ABCDb] PHA range of best detection (9) 149-152 F4.2 --- VigFactor ?= ...

... BEHR is a standalone command-line C program designed to quickly estimate the hardness ratios and their uncertainties for astrophysical sources. It is especially useful in the Poisson regime of low counts, and computes the proper uncertainty regardless of whether the source is detected in both passbands or not. ... src are the counts within the source region, and *bkg are counts within the background region. ... soft-band counts in source region . hard-band counts in source region . ...

... CentralProcessor 0.11 documentation . ... Only continuum source-finding is done at this point - spectral-line source-finding will be added in the future. The source-finding applies a spatially-varying signal-to-noise threshold, and fits 2D Gaussians to detected islands to create a component catalogue. At this point, only a limited set of Selavy?s possible parameters are made available through these scripts. ... nsubx ( Selavy Basics ) . ... User Parameters - Mosaicking Continuum images . ...

... In this section we list important STScI sources of documentation for the HSP and its various types of output data. The final version of the HSP Instrument Handbook (version 3.0) is a useful description of the technical capabilities of the instrument and practical information for its use. Although many figures are not currently included, the text of the final version is available in electronic form from the STScI HSP WWW pages. ... The STScI home page is at: . ...

OPTICAL IDENTIFICATIONS OF INTEGRAL / RXTE SOURCES WITH 1.5-METER OPTICAL TELESCOPE RTT150 I.Bikmaev (1,2), M.Revnivtsev (3,4) , R.Burenin (3) R.Sunyaev (3,4) , N.Sakhibullin (1,2) (1) Kazan State University, Kremlevskaya Str., ... 1, D-85741, Garching bei MЭnchen , Germany (3 (4) ABSTRACT We present the first results of our project on optical identifications of INTEGRAL / RXTE hard X-ray sources by using scientific instrumentations of the 1.5meter joint Russian-Turkish optical telescope RTT150. ...

... A modern driver for a device will find out the bus-resource configuration without you having to tell it anything. ... In the worst case you must hard-code the bus-resources into the kernel (or a module) and recompile. In the middle are cases such as where you run a program to give the bus-resource info to the driver or put the info in a configuration file. ... You give such bus-resources as a parameter to the kernel or to a loadable module. ... Setserial is often run from a start-up file. ...

11 august 2014/Monday: Arriving, Registration . ... The variation of solar flare coronal X-ray source spatial properties. ... Melnikov V.F., Charikov Yu.E., Kudriavtsev I.V. Directivity of X-ray and gamma-ray emission from different parts of flaring magnetic loops. ... E., Melnikov V.F. Angular characteristics of polarization degree of hard X-ray emission from different parts of flaring magnetic loops. ... The thick target model and analytical calculations of the hard X-ray emission from solar flares. ...

The AstroGuide . ... AstroGuide Listing . ... See many more Astronomy Listings by: Category or Alphabet . Located in the middle of Hard Labor Creek State Park in Rutledge, Georgia (~50 miles east of downtown Atlanta), the observatory is a resource for professional and amateur astronomers. However, an additional service of HLCO has been to the public - bringing the wonders of the Universe to Georgia residents. ... Web Site . ... Web . ... dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

These pages collect together references to many pictures of the solar system that can be found on the Net. ... Since I originally compiled this list the number of relevant images has grown tremendously. ... http://www.jpl.nasa.gov/pictures/ . ... ftp://dftnic.gsfc.nasa.gov/images/gifs/ . ... http://www.jpl.nasa.gov/galileo/images.html . http://www.jpl.nasa.gov/magellan/images.html . ... http://nssdc.gsfc.nasa.gov/image/planetary/ . ... NASA Image Access Homepage (Planetary Photojournal) . ...

... The Nine Planets Shop . Posters, T-shirts, mouse pads, coffee mugs with a planetary theme. ... These pages collect together references to many pictures of the solar system that can be found on the Net. ... Since I originally compiled this list the number of relevant images has grown tremendously. ... Earth . ... Planet Earth . Amazing pictures of Earth from space combine useful science and artistic beauty. http://oposite.stsci.edu/pubinfo/ . ... ftp://dftnic.gsfc.nasa.gov/images/gifs/ . ...

... RC0133+0459 . ... RC0154+0459 . ... Radio source parameters . R.A.(J2000) Dec.( J2000) R.A.(B1950) Dec.( B1950) Freq. Comp. ... Parameters of optical candidates for identification . ... B1950) Magn. ... Crosses mark radio source components ps . Last updated 19 Dec 2000 ...

... 314, 2004 F. Ochsenbein, M. Al len, and D. Egret, eds. Efficient data mining in the X-ray sky background John Cunniffe, Evert J.A. Meurs Dunsink Observatory, Castleknock, Dublin 15, Ireland Aaron Golden IT Centre, NUI Galway, University Road, Galway, Ireland Abstract. Abstract: The calculation of flux upper limits in the sourcefree ("background") regions of photon-limited images is complicated by instrumental and statistical modeling and requires non-trivial computational effort. ... 2004). ...

The Ryle Telescope was used for some years for monitoring variable sources (in addition to its role in source-surveys related to the Sunyaev-Zeldovitch studies). The instrument is now transformed into the "AMI large array": see the AMI pages for details. ... The rebuild took place between 2006 June and mid-2008; between these dates there is no useful data available. ... For some sources there are many plots, organised by date: . ...

... Chandra Resolves the Hard X Ray Background . ... 14.01.2000 . ... Chandra , NASA Explanation: It is everywhere but nobody knew why. ... The above photograph shows that about 80 percent of the apparently diffuse hard X-ray background can be resolved into very many very faint sources. ... January 2000 . ... Publications with keywords: Chandra - x-ray background - cosmic microwave background radiation . Publications with words: Chandra - x-ray background - cosmic microwave background radiation . ...

... This flare was observed simultaneously in H alpha, ratio (at microwave and millime­ ter wavelenghts), and soft and hard X­rays (by the Yohkoh spacecraft) with high spatial and moderate spectral resolution. ... Analysis of the microwave/hard X­ray/soft X­ray emission from individual sources provides information on the radio emission mechanisms, the energetic electron population, the magnetic field strenght, and plasma den­ sity. ...

... All the parameters provided in this database have been obtained using the the MIRIAD ( Sault et al. 1995 ) task MBSPECT . MBSPECT makes a spectrum of the velocity (or frequency) axis of a cube. The spectrum is beam-weighted, over the width specified, for the other image axes. ... Robust parameters are calculated by using an algorithm which minimises the mean absolute deviation of the flux-weighted velocities. mask= This specifies the x-axis ranges to be excluded from any continuum fit. ...

... a) As source material for the high-school or college curriculum, especially in physics. astronomy and their history. (b) As a source of supplemental projects by high school students or by undergraduates. (c) As material for independent studies, In particular by motivated students who seek to know more about space . ... Those wishing to look up specific topics are advised to use the index file, accessible from the end of any "Exploration" file. ... files not listed and at other resource material. ...

... Exposure Time . ... 2000 May 27 . ... 2000 Jun 03 . ... 2000 Dec 10 . ... log N -log S in the soft (0.5 2 keV), hard (2 10 keV), and very hard (5 10 keV) bands from the 1 Ms observations of the CDF-S. The shaded areas indicate uncertainties due to the Poisson statistics (1 ) and the choice of the conversion factor (corresponding to a power law spectrum with = 1.4 0.3). ... Soft [0.5-2 keV] . ... Soft band [0.5-2] keV .. ... Hard band [2-10] keV .. ... Exposure maps . ... Exposure map [0.5-2] keV .. ...