... Thu, 21 Nov 2002 11:10:06 +0100 . Previous message: [sas-uploads] ccftools-1.29.tgz . Next message: [sas-uploads] saslib-1.76.tgz . Messages sorted by: [ date ] [ thread ] [ subject ] [ author ] . Package: omsource-1.1.4.tgz - 1098037 B MD5: c600bff0b87ce65636fbdaf953818944 Uploaded by: cb1@mssl.ucl.ac.uk Accepted on: Thu Nov 21 10:10:06 2002 UTC The most recent ChangeLog entry says: Version 1.1.4 - 2002-11-21 (CB) ------------- corrected DEPEND file for build failure. ...

Next: Fringe correction Up: Special Processing Options Previous: Sky Illumination Corrected . A third method to account for illumination problems in the flat fields is to remove the large scale pattern from the flat field itself. This is useful if there are no reasonable blank sky calibration frames and the astronomical exposures are evenly illuminated but the flat fields are not. This is done by smoothing the flat field frames instead of blank sky frames. ...

... Gallery . ... The sculpture is accepted . Sidebar Left . Sidebar Top . No Sidebar . Sidebar Bottom . Sidebar Right . ... Title: The sculpture is accepted . Description: Image: Bob Cooper . NOTE: All images are copyright and must not be reproduced or mirrored in any form without written permission. ... The sculpture is accepted Image: Bob Cooper . ... Powered by Gallery 3.0.9 (Chartres) . ...

STScI . Staff Research . Summer Students . After You're Accepted . ... Hubble Heritage Project . ... Hubble Fellowships . ... Students that are non-U.S. citizens will need a visa to work in the U.S. regardless of where their school is located. ... Some will be on topics related to careers, some on our missions at STScI, some on the practices of professional astronomers and other professionals on our staff, and some on the research done by our scientific staff. ... Working at STScI . ...

We would like to announce the release of Version 3.03 of the CHIANTI database for astrophysical spectroscopy. This now extends the database to include the 1 - 50 wavelength region. The additions to the database are described in a paper `CHIANTI - an atomic database for emission lines, IV - Extension to X-ray Wavelengths' by K.P. Dere, E. Landi, G. Del Zanna, and P.R. Young and accepted for publication by the Astrophysical Journal Supplement Series. ... Atomic Data Updates (April 30, 2001) . ...

... Authors: Spyros Basilakos (Imperial College London) . ... Title: Populating a cluster of galaxies - I. Results at z=0 . ... Title: The Merger Rate to Redshift One from Kinematic Pairs: Caltech Faint Galaxy Redshift Survey XI . ... Title: Multi-wavelength observations of an evolved galaxy group: An endpoint of galaxy merging? ... 23 matches for the search pattern galaxy merging . The URL for this page is: http://xxx.itep.ru/find/astro-ph/1/galaxy+merging/0/1/0/past,all/0/0 www-admin@xxx.lanl.gov ...

... Thus the FTE described below must be added to the AOF FTE budget. ... Activity Scientist overview of changes (R7M) Observing preparation tool ( section 15.1) Instrument Control Panel ( section 15.2) Modification of AOF / Hawk-I acquisition template ( section 15.3) Site quality monitoring and display ( section 15.5) Exposure Time Calculator ( section 15.6) Modification Observing Tool (OT3) ( section 15.8) TOTAL FTE effort 1 0.1 0.3 0.3 0.3 0.2 0.3 2.5 ...

MATERIAL SAFETY DATA SHEET WOMAN CHEMICAL ANALYSIS . ELEMENT: WOMAN SYMBOL: WO2 DISCOVERER: ADAM ATOMIC MASS: Accepted as 118lb, but know to vary from 100 to 550lb. ... Found in various states ranging from virgin metal to common ore. ... CHEMICAL PROPERTIES 1. Has a great affinity for Gold, Silver, Platinum and most precious stones. ... May explode spontaneously without prior warning, and for no known reason. ... COMMON USES 1. Highly ornamental, especially in sports cars. ...

... FIX: Download corrected routines line_chianti.pro , popsol.pro , and nenh.pro and regenerate the CHIANTI database (or download) . NOTE: all tar files in the distribution have been updated. ... Updated all .pro files, include many enhancements and some minor bug fixes. ... 2001 Dec 07: . ... FIX: the files have been updated to correct for this. download new versions of rd_line.pro , fold_ioneq.pro , and rd_ioneq.pro . ... FIX: Copy corrected routine and replace . ... Fixed in all tar files. ...

... Step 1: The magnetic field line tracing from the satellite position up to magnetic equatorial plane using IGRF magnetic field model. Step 2: Tracing back from the point (produced on the Step 1) to the Ionosphere (by using only dipole magnetic field) . ... The magnetic field line tracing from the satellite position up to the Ionosphere (the stop trace altitude 110 km) using Main (dipole) + Extraterrestrial magnetic field model (for example, Tsyganenko [1987], or [1989], or [1990] ) . ...

Peremennye Zvezdy", . ... Period: . 12.4 d; . ... We report photometric monitoring of the pre-main sequence binary AK Sco covering about 45 days in 2003. ... Nowadays we recognize AK Sco as a double-lined spectroscopic binary with large eccentricity (e=0.47) and spectroscopic orbital period of 13.6 days (Andersen et al. ... The light curve shows brightness variation with an amplitude of about 0.3 magnitude and changes reaching 0.2 magnitude from night to night. ... Light curve of AK Sco. ...

Next: Commands Up: SPC (formerly S) A Previous: Introduction Contents . ... Control of SPC commands is via questions and answers. ... If you type a dash (-) as a file name (in D IRECTORY , L OAD , or W RITE ) you return to the command prompt. ... SPC does not alter SPECTRA ( .SPC ) files; it is even safe to load data from an open SPC file at Parkes, i.e. during the observation. Use the command D IRECTORY to list available sequence numbers in a data file to check what's there. loading spectra . ...

... Step 1: The Footprint position calculation by the magnetic field line tracing from the satellite position up to the Ionosphere by using IGRF + Tsyganenko [1987] magnetic field model (the stop trace altitude 110 km). Step 2: Tracing back from the Footprint (produced on the Step 1) to the dipole equatorial plane (by using only IGRF magnetic field model up to the geocentric distance 8 RE and dipole field model after this distance). ... Back to the description . ...

To compile a working copy of Apache under UnixWare, there are several other steps you may need to take. ... Make sure that USE_FCNTL_SERIALIZE_ACCEPT is defined (if not defined by Apache autoconfiguration). If using the UnixWare cc compiler, and you still see accept() errors, don't use compiler optimization, or get gcc . SCO patch tf2163 is required in order for Apache to work correctly on UnixWare 2.0.x. See http://www.sco.com for UnixWare patch information. ...

Stellarium 0.12.3 . ... Classes . ... FileљStructure . ClassљList . ClassљIndex . ClassљHierarchy . ... TuiNodeResponse Struct Reference . A TuiNodeResponse contains a flag, "accepted" if a keystroke was accepted And a link to a node, should the key action have prompted a change in the current node used by the menu system. More... #include < TuiNode.hpp > . ... Definition at line 30 of file TuiNode.hpp . The documentation for this struct was generated from the following file: . ...

... Telescopes . ... The time requests are accepted in an electronic version with on-line form in Russian or English. ... Unregistered request will be disregarded by the Large Telescopes Programm Committee. In exclusive cases the secreatry of the Committee is entitled to accept an observational time request given permission of the Chairman of the Committee or the director of the SAO RAS. The Program Committee considers generally one time request submitted by the principal applicant. ...

... A. M. M. Scaife, E. I. Curtis , M. L. Davies and 15 others. ... MNRAS , 2010, accepted . PDF | ADS | astro-ph . ... A submillimetre survey of the kinematics of the Perseus molecular cloud - III. ... MNRAS , 2010, in press . ... Citations 1 | ... MNRAS , 2010, 408, 1516 . ... The JCMT legacy survey of the Gould Belt: a first look at Serpens with HARP . ... MNRAS , 2010, 405, 759 . ... MNRAS , 2010, 402, 603 . ... PDF Star Formation in Perseus Observed with HARP . ... 2010 Emily Curtis | ...

... In brief: the frequency-dependent radiative transfer equation is solved for a dust under assumption of spherically-symmetric geometry for its distribution taking into account particle size distribution and quantum heating effects for the very small dust particles. ... Table: Model parameters for IRAS04296+3429. ... parameter . ... hot dust shell) . ... The best fit to the spectral energy distribution of IRAS04296 is shown by heavy solid line (see Table2 for details concerning parameters of the model...

... Track quality = nHits 999 BBbar events Nevents 999 Accepted by ZPD DecMod in bit 0, pT > 0.8, no cut on Z0 bit 1, pT > 0.2, |z 0| 15 L3OutDch accepted 997 best tick wrong tick 877 10 997 0 L3 rejected 0 best tick wrong tick 0 0 0 0 MC efficiency is as expected Zp d p erformance O.Igonkina 5 Events selected in wrong tick , Track quality = nHits wrong tick - best tick delta Nhit vs nHits nHits ( wrong ) - nHits ( ... Zp d p erformance O.Igonkina 8 ...

A2500 is doing 300 sec on,off position switching with the xband receiver. ... average multiple on/offs for a given source . average pols . ... most sources were taken with vlsr=0 (accept the first which had the correct vlsr velocity). The difference between the flagged and measured lines will be the vlsr velocity of the source . I flagged alfa,beta,gamma transitions for H,He,C. 21oct11 (.ps) ( .pdf ) . processing: x101/111021/a2500.pro .. and other dates. home_~phil ...