... 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 . ...

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Mitigation of CTE Losses in ACS/WFC: ! ... CTE) of the ACS/WFC CCD dete! ors is declining with time due to the ct ! ... These include post-observation corrections, adjusting the ze CTE losses, and the use of a short post-flash to increase the The photometric CTE correction formula of Chiaberge (2012) is compared with the pixel-based CTE correction in CALACS in Fig. ... The charge transfer efficiency cumulative effects of radiation to mitigate CTE losses are observing strategy to minimi background.! ...

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• New CTE Correction Formula Available from Dolphin (2000)
• CTE in the WFC3 UVIS
• Correcting ETC Calculations of CCD Spectral Observations for CTE Effects

XMM-Newton CCF Release Note XMM-CCF-REL-314 The RGS effective area: up date of the contamination correction R. GonzЄlez-Riestra a April 11, 2014 1 CCF comp onents Name of CCF RGS1 EFFAREACORR 0009 RGS2 EFFAREACORR 0009 VALDATE 2001-01-01T00:00:00 2001-01-01T00:00:00 List of Blocks changed EFFAREACORR EFFAREACORR XSCS flag NO NO 2 Changes A correction to the RGS effective area for contamination on the detectors was first implemented in SAS in 2007 [1]. ...

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• From 0 to <tt>Xspec</tt> in a few clicks
• XMM-Newton OM Response Files Page
• XMM-Newton Calibration Documentation

... Using a simple 2-D Gaussian Point Spread Function (PSF) on a constant (flat) sky background, I derive a theoretical photometric and astrometric performance model for analytical and digital PSF-fitting stellar photometry. ... The photometric performance is maximized when either the effective background area or the effective-background-level measurement error is minimized. ... An important, but frequently ignored, noise source is the uncertainty of the measurement of the effective background level ( )...

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• A New PROS Task for Calculating HRI Source Intensities or Upper Limits
• Simulation of HST PSFs using Tiny Tim
• Towards Optimal Analysis of HST Crowded Stellar Fields

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 . ...

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• Procedures for Observations
• Fasti Noise in the Lab
• Radioastronomy reduction procedures

Hamburg/SAO Survey (HSS) for Emission-Line Galaxies - New Wide-Angle Search for Blue Compact Galaxies (BCG) . ... New project named Hamburg/SAO Survey extends study of blue compact galaxies to new large wide-angle sample based on digitized objective-prism photoplates of the Hamburg Quasar Survey (HQS). ... 60%) of observed emission-line objects in accordance to the idea of use objective-prism wide-field surveys as favorable technique to search for narrow emission-line galaxies . ...

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• The SNR X-rays Catalog
• Extinction and transformation models
• Source Positions

Peremennye Zvezdy", . ... Star Name: . GSC 3710-00312, USNO-A2.0 1425-04252279 . ... Variability type: . ... USNO-A2.0 1425-04252279 is located at the distance of 15?.7 from the X-ray source 1RXS J031707.9+572942, which is larger than the position error of the source (12?), but its hardness ratio HR1 = 0.03 0.29, typical of chromospherically active stars, and its character of variability allow us to assume that the star is related to the X-ray source. ... Eclipsing variability . Sine wave 1 . ...

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... Staff list | ... Murchison Radio-astronomy Observatory . ... Australia Telescope Online Archive (ATOA) . ... VLBI . ... The successful applicant will pursue a range of challenges related to low-frequency, wide-field, and astrometric radio observations at high angular resolution, with substantial scope for personal research direction. ... ASTRON operates the LOFAR and Westerbork radio telescopes and hosts the Joint Institute for VLBI in Europe (JIVE), which operates the European VLBI Network (EVN). ...

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• tac_info
• Pulsar Group Main/ANDSATNF

... Einstein data for SNR are available as images on magnetic tape or diskette and as tables of counting rates. ... In seven cases, with coverage from 35% to 90%, we have calculated an HRI rate for the entire SNR by using the observed IPC data and assuming the ratio of HRI to IPC rates was the same for the observed and the unobserved parts of the remnant. ... Positions of the bright bulge sources and remnants in the galactic plane are known and the rates in table 2 are free of the effects of these. ...

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• Introduction
• Filtering ROSAT HRI data on the basis of background level
• The Diffuse X-Ray Background

SAI 175 anniversary . ... Moscow University . Search for in SAI Moscow University Search for in Russian astronomical resources . ... SAI Astronomical Databases . ... Browse SAI Software archive(ftp.sai.msu.su) . ASTRONET.RU - Russian Astronomical Network (available in translit also) . ... SAI Supernovae Research Group . ... Department of the Galaxy and Variable Stars (in Russian) . Sternberg Astronomical Institute Seminars . ... All-Russian Astronomical Olympiad (in Russian) . ...

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• Frozen Text Tutorial
• Creating a watermark effect
• CoolType - Dripping Text

... They were determined as a result of orbit improving on the base of all kinds of optical observations available in the catalog of observations of the Minor Planet Center on March 16, 2014 (radar observations have not been used at this stage). ... As the MPC orbits do not all were improved simultaneously with EMP orbits, only 383866 sets of elements were used for data comparison (for selected sets of elements process of improvement had started with the use of the same observations). ...

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• Keywords_99

Title: A New Model of the Gravitational Lens 0957+561 and a Limit on the Hubble Constant . Authors: Norman A. Grogin , Ramesh Narayan (Harvard Univ.) ... Title: ROSAT/PSPC observation of the distant cluster CL0939+472 . ... Title: Interaction in the Bimodal Galaxy Cluster A3528 . ... Title: Cosmological Implications of Galaxy Cluster Evolution . ... Title: Galaxy Cluster Virial Masses and Omega . ... Matches 201 to 222 from a total of 222 matches for the search pattern galaxy cluster . ...

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... We present new progress in our extensive pro ject mCPod (Onґline database of photometric observations of magnetic CP stars), which was initiated five and a half years ago (MikulЄ et. al, 2007). ... The database consists of two parts, the Data and the References. In the References one finds the sources of data, the bibcodes including links to the corresponding papers, names of comparison and check stars (if available), the number of observations in individual filters (see Fig. ...

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• Solar system sector, archive 2006
• The GLORIA Project makes available to internet users 13 robotic telescopes in
• Hardware sector, archive 2009

The NAIC-NRAO School on Single-Dish Radio Astronomy Techniques and Applications -- July 2005 Writing Effective Telescope Proposals Chris Salter (NAIC) Chris Salter's credent ials to present a talk on writ ing telescope proposals: 1. ... Service as a member of the Arecibo Scheduling Advisory Co mmittee. ... 1 The Arecibo Telescope Proposal System Components that make up an Arecibo proposal; Ї The Cover Sheet (web-based) containing technical details and an abstract (not more than 150 words). ...

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• http://www.naic.edu/vscience/schedule/tpfiles/FreudlingtagA2133tp.pdf
• http://www.naic.edu/vscience/schedule/tpfiles/FreudlingtagA1956tp.pdf
• The Mock Spectrometer

... 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 . ...

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• Cosmological Gene project
• harak_e
• Vitaly Goranskij, SAI/Moscow Univ.

... Exposure Time Calculator (ETC) . ... ESO - Public Surveys . ... the recommended values to use for DIT, . ... Detector on-chip integration (DIT): seconds. to your chosen value - a separate page gives recommended values to use for DIT - for modes 1 and 2 below you may wish to start with the maximum recommended values as these will minimize the effect of read noise (a total object exposure of Y secs with DIT=X secs will produce Y/X lots of read noise) and give you a lower limit on the time needed. ...

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• VISTA - Visible and Infrared Survey Telescope for Astronomy

... This class is designed to be an up to date summary of the last 10-20 years of observations relevant to Cosmology. ... Theory today is bombarded by a vast array of observational data but there remains no clear and preferred model for the origin and evolution of structure in the Universe. ... The inflationary paradigm and the nature of the Dark Matter - Inflation solves a lot of problems that are inherent in the standard Big Bang Model. ... Kinds of Dark Matter and Observational Constraints . ...

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• Astronomy HyperText Book: Interstellar Medium
• Thermal History of the Universe

Disastrous earthquakes happen 100 to 200 times a year. ... There is a chance that the data of ionospheric plasma observations hold an answer to the latter question. Satellites and ground-based facilities may detect earthquake precursors in the ionosphere a few hours or days before the main shock. ... ULF "Hz"-oscillations have been recorded several hours before the main shock in a narrow magnetic field tube (40...100 km along the satellite trajectory) conjugated with epicenter of the earthquake. ...

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• Practical Astrophysics
• Vasyl M. Ivchenko

Next: J.E. Chambers, Research Astronomer Up: Research Previous: Research Contents . ... Solar Variability and Climate . Other Activities . ... Applied to data of flares on Gliese866 he was able to estimate the area of hydrogen emitting flare regions as 1-13% of the stellar surface. ... As partners in the project, Armagh Observatory has been asked to contribute to the selection process in exchange for priority access to the data which will eventually flow from the satellite. ...

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• Background
• Armagh Observatory
• An Overview of the Coupled Earth-Sun System PPARC Introductory Solar System

To main of Laboratory . The research work and design of optical and optical-electronic devices are carries out by laboratory staff: . ... Lens: . ... In the layout 1 prism systems perform functions of dispersive element, corrector of aberrations, optical reducer. ... Spectral range 200 - 400 nm; . ... Back Forward . ... The main corrector's function are compensation of field aberrations of the main spherical mirror of a telescope (diameter of 600 mm, f'=1200 mm) and increase aperture ratio. ...

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• MAO NASU :: Topic: Open access submissions and content now available (1/1)