XMM-Newton Calibration - intro · Briefly review the ground calibration · Highlight the unique calibration issues of XMMNewton · Review the life-cycle of calibration observations, analysis, and ingestion into SAS · The publication of calibration data and ensuring correct sets used in SAS XMM-Newton David Lumb -- No need to calibrate XMM on-ground ­ AXAF will be calibrated to 1% so just calibrate to them!" ... XMM-Newton David Lumb --XMM-SOC 8 ...

... Data . ... In general, Dolphin finds good agreement with the Whitmore, Heyer, and Casertano results, and the longer baseline and more extensive data set used by Dolphin result in less scatter in the residuals. ... In these case the Dolphin corrections are larger than the Whitmore et al. corrections. ... Figure 1 shows the ratio of counts from a 14 second exposure of Omega Cen in August, 2000 to the counts in a 100 second exposure, vs. the Y position on the chip (WF2 in this case with gain=15). ...

... Primordial theory review : Dick Bond . Defects and the CMB review : Andy Albrecht . ... Gravitational wave contribution to CMB anisotropies : V.B. Lukash and E.V. Mikheeva . C_l from cosmic strings : Lloyd Knox . Some aspects of CMB anisotropies induced from topological defects : Mairi Sakellariadou . ... CMB anisotropies from scaling sources : Ruth Durrer . ... SZ observations I : Sarah Church . ... Holes in the microwave sky? ... Detecting cosmic strings in the CMB : James Robinson . ...

CHIANTI - an atomic database for emission lines. ... K.P.Dere, E.Landi, H.E.Mason, B.C.Monsignori-Fossi, P.R.Young, 1997, A , 125, 149 . Article: Available from ADS . The Arcetri Spectral Code for thin plasmas . E.Landi M.Landini 1998, A , 133, 1 . ... E.Landi, M.Landini K.P.Dere, P.R.Young, H.E.Mason, 1999, A , 135, 339 . ... K.P.Dere, E.Landi, P.R.Young, G.Del Zanna, 2001, ApJS, 134, 331 . ... G.Del Zanna, B.J.I.Bromage, E.Landi, M.Landini, 2001, A , 379, 708 . ...

This module allows "anonymous" user access to authenticated areas. ... Source File: mod_auth_anon.c . ... This module does access control in a manner similar to anonymous-ftp sites; i.e. have a 'magic' user id 'anonymous' and the email address as a password. ... Anonymous_VerifyEmail The example below (when combined with the Auth directives of a htpasswd-file based (or GDM, mSQL etc. ) base access control system allows users in as 'guests' with the following properties: . ... Default: none . ...

. First page Back Continue Last page Summary Graphics . First cut, cross calibrate to Leiden-Dwingeloo (0.5 ) . This tends to smooth out total column changes on small scales, but preserves velocity features .

... Observatory . ... Science . ... Science Users Information > Science Publications > Science Announcements > MUSE Pipeline Version 1.0 available . ... Observing Facilities . ... Observing with ESO Telescopes . ... Data Handling and Products . ... Data Pipelines and Calibrations . ... Science Data Products Forum . ... Science Archive Facility . ... ESO Data . ... ESO Data Access Policy . ... ESO Science Newsletter . ... The MUSE pipeline recipes version 1.0 are available and can be obtained here . ...

Next: Data analysis and Spatial Up: Spatial Corrections of ROSAT Previous: Spatial Corrections of ROSAT . ... We start with an observation for which the PRF is much worse than it should be; caused by residual wobble errors or other causes. ... Spatial analysis of ROSAT HRI observations are often plagued by poor aspect solutions, precluding the attainment of the potential resolution of about 5''. ... A recent example showed one obi for which the source was 10 north of its position in the other 17 obis. ...

Next: NICMOS Science Up: NICMOS Data Calibration and Previous: NICMOS Software at the . ... Reference File Tools . Image Analysis and Reduction . ... These include the tasks used in the STScI pipeline, tools to generate the reference files used by the calibration pipeline tasks, and general image analysis, manipulation, and arithmetic tasks. ... Calnica is used to apply instrumental calibrations to individual datasets, while calnicb is used to process associated sets of NICMOS images. ...

... As input, OFFAXIS takes a visibility dataset and a model of the source total intensity (Stokes I). Given this, it computes the expected off-axis effects (given its internal models of the effects), subtracts this from the data, and produces an output (nominally) corrected dataset. Key: vis Input visibility dataset. ... Key: out The name of the output, corrected, visibility dataset. ... The default is to apply these if they are available. nopol Do not apply any polarization leakage correction. ...

Next: Other People's Software . ... Quality system management of computer workstations for astronomy can be achieved with relatively small manpower requirements, if the right cost-effective administrative design decisions are made. ... This is all done with essentially one system manager. ... The system is designed so that one doesn't depend on four or more hosts, (such as a software server, cpu server, data file server, font server, etc.) to get work done. ...

... Obviously, the size of the cavern is of the order of the Schwartzman radius. ... Thus, consideration of the inverse effect of pulsar radiation on the properties of accreting plasma makes the ejection possible even when the Schwartzman radius is smaller than the capture radius. ... If the cavern radius , the condition at its boundary can be written as . ... Apart from magnetic dipole radiation, the cavern may also contain relativistic particles (which are also reflected from the cavern boundary). ...

Peremennye Zvezdy", . ... Max . Min . ... USNO-A2.0 0900-11355573 . ... Comm. ... USNO-A2.0 0900-11358267 . ... USNO-A2.0 0900-11400726 . ... USNO-A2.0 0900-11423464 . ... USNO-A2.0 0900-11451497 . ... Period 0 d .2948 is also possible. ... Primary minimum: HJD(TT) 2455502.1597 0.0008. ... A close pair of two stars: USNO-A2.0 0900-11502589 and a faint star, not presented in any catalogues. ... The comparison star was USNO-A2.0 0900-11460273 = USNO-B1.0 0950-0327798 (?=18 h 04 m 33 s .51, ?= ...

This page gives the name and meaning of the various parameters which can be queried in HyperLeda through SQL requests . ... real . ... actual error on t . ... log 10 of apparent major axis diameter d25 at 25 mag.arcsec -2 (d25 in 0.1') . ... actual error on logd25 . ... Apparent maximum rotation velocity of gas . ... log 10 of apparent corrected diameter (dc in 0.1') . ... total apparent corrected B-magnitude . ... total apparent corrected U-B color . ... Questions: leda@univ-lyon1.fr ...

Please enter the lightcurve file name and period search parameters: . Lightcurve file: . ... Apply the Heliocentric correction and convert all dates to Terrestrial Time (TT)? ... Also, the Heliocentric correction cannot be applied to such lightcurves. ... This period search service is also available at the mirror sites: Mirror 1 , Mirror 2 , Mirror 3 , Mirror 4 . You may download the latest source code distribution and install the period search service at your own web server. ...

... Ширина: 225 мм . Шины . ... Артикул 3386432 . ...

... HD144941 is a B type hydrogen-deficient star. ... However, its H/He ratio puts it between the classifications of an extreme and an intermediate helium star, and its low C and N abundances make it unique amongst known H-deficient stars. ... Keywords. stars: helium stars -- stars: individual stars (HD144941) -- stars: atmospheres -- stars: abundances -- stars: oscillations -- stars: evolution . ... The iron abundance in the helium star HD144941 has been measured from ultraviolet Fe III lines. ...

Results of analysis . ... IAA EOP Service . ... EOP series are regularly submitted to the IERS, and also are available at the IAA EOP Service page. EPN coordinate time series . EUREF Permanent GPS Network (EPN) coordinate time series is computed from analysis of available EUREF weekly solutions. ... Second solution is based on independent combination of individual EPN Analysis Centers' solutions . ... USNO GPS Timing Operations . ... GPS Time Series . ... EPN : European Permanent GPS Network . ...

... Abstract . ... Special Astrophysical Observatory of the Russian Academy of Sciences (SAO RAS), Russia . ... Mingaliev M.G. Special Astrophysical Observatory of the Russian Academy of Sciences (SAO RAS), Russia . ... Moiseev A.V. Special Astrophysical Observatory of the Russian Academy of Sciences (SAO RAS), Russia . Scanning FPI for Galactic and Extragalactic Observations in SAO RAS . ... Semenova T.A. Special Astrophysical Observatory of the Russian Academy of Sciences (SAO RAS), Russia . ...

LEP Energy WG Report October 13th, 2001 WWMMI Cetraro , Italy Eric Torrence University of Oregon Eric Torrence WWMMI Cetraro October 2001 Overview Work Continues in several areas · Flux Loop analysis · Qs vs. fRF analysis · Spectrometer magnet mapping · Spectrometer BPM analysis More general overview available here: http://www.cern.ch/LEPECAL/talks/CERN_01Apr Eric Torrence WWMMI Cetraro ... Eric Torrence WWMMI Cetraro October 2001 Bunch Length? ...