ASC-FITS-2.0.1: ASC FITS File Designers' Guide (Rots and McDowell) (1999 Jun) . ASC-FITS-REGION-1.0: FITS region document (McDowell and Rots) (1998 Mar) . ... CXC-DM-001 Introduction: Data Analysis with the Chandra Data Model (2001 Oct) . ... 1998 Feb 26: SDS-1.0: Data Product List: obsolete . ... 1998 Mar 09: SDS-10.0: (ASC-FITS-REGION-1.0) FITS region document: see ASC-FITS-REGION-1.0 . 1998 Feb 09: SDS-11.0: FITS function document (superseded by ASC-FITS-FUNCTION-1.2) . ...

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• Jonathan's ASC documents
• The AstroStat Slog virtual observatory
• The AstroStat Slog Blog Archive model vs model

... Science Activities > PhD Thesis Topics offered by ESO Faculty Members > Thesis Topic: Dynamical models of multiple globular cluster populations around massive galaxies . ... Different techniques have been devised to separate multiple GC populations and perform dynamical analyses. ... Within this project, the PhD candidate will examine mock models of multiple GC populations around massive galaxies, devising `blinded' functional tests and comparing the possible sources of bias in different techniques....

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• Data Quality Control and Instrument Modeling
• Astroclimatology, Forecast Models
• ESO - Thesis Topic: The interplay of massive stars, gas and dust in very nearby

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... To view them, you must have access to Ghostview , or another suitable viewer. ... A. Fludra, J.G. Doyle, T. Metcalf, J.R. Lemon, K.J.H. Phillips, J.L. Culhane and T. Kosugi . ... View Abstract . ... E.R. Houdebine and J.G. Doyle . ... E.R. Houdebine, J.G. Doyle and M. Koscielecki . ... A.G. Gunn, J.G. Doyle, M. Mathioudakis, E.R. Houdebine, S. Avgoloupis . ... J.G. Doyle, E.R. Houdebine, M. Mathioudakis, P.M. Panagi . ...

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• Armagh Observatory Preprint No. 308
• The Armagh Observatory Human Orrery

Next: Introduction . ... 1]Also with Beijing Astronomical Observatory, CAS, Beijing 100080, China. The model updating technique used in the Maximum Entropy Method (MEM) task for image restoration in IRAF/STSDAS is described in detail. ... Keywords: entropy, Maximum Entropy Method, image restoration, IRAF, photometry . Introduction . Model Updating . ... Tests Using a Simulated Image . ...

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• Evolutionary Models of Extra-Solar Giant Planets and Brown Dwarfs
• HST Focus Model
• Tiny Tim HST PSF Modeling

... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Parkes radio telescope . ... Parkes | ... Atmospheric Modelling of the Companion Star in . GRO J1655-40 . ... We have measured the rotational velocity of the companion star to be = 80 10 kms -1 (1 ) by fitting Kurucz model spectra to our observed spectrum of the black-hole candidate GRO J1655-40. ... binaries: spectroscopic, stars: individual (GRO J1655-40), stars: rotation . ... Companion Star in GRO J1655-40 . ...

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• Probing ISM Models with H observations
• Observational Tests of a Double Loop Model for Solar Flares
• The Structure of Dark Halos: Model-Independent Information from HI Rotation

... Previous: Model Based Corrections to Data from Radiation Damaged Detectors. ... Pound, M. W., Wolfire, M. G., & Amarnath, N. S. 2003, in ASP Conf. ... A large set of physical parameters and dust types are included in the model database, which contains over 500,000 models. ... The model outputs are averaged over the instrument bands using the same weighting ( constant) as the SIRTF data pipeline which allows the SIRTF data products to be compared directly with the model database. ... 2003). ...

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• Calibration and Performance Control for the VLT Instrumentation
• Fitting and Modeling of AXAF Data with the ASC Fitting Application
• Spatial Structure of NGC 6822: An Example for Statistical Modeling of

... Towards a Truly Unified Model of AGN . ... The Unified Model holds that the aspect-dependent effects primarily determine the nature of the active galactic nucleus that we observe. ... The full postscript file can be obtained here: . The PASA Latex file can be obtained here: . The postscript file of Fig 1 can be obtained here: . ...

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• Giant Galaxy String Defies Models of How Universe Evolved
• research
• Lesson 3: Residual Plots and Chi-Squared Fitting of Models to Data

Astronomy Picture of the Day . ... The Sudbury Neutrino Observatory Institute Explanation: The Sudbury Neutrino Observatory (SNO) has been detecting so few neutrinos from the Sun that the Standard Model of fundamental particles in the universe may have to be revised. Pictured above is the SNO as it was being built. ... The most popular model for fundamental particles , known as the Standard Model , did not predict such schizophrenic neutrinos . ... The Sudbury Neutrino Detector . ...

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• Астронет > Sudbury Indicates Nonstandard Particle Model
• Journal "Peremennye Zvezdy"
• Vesta Trek: A Digital Model of Asteroid Vesta

... 2001 July 10 . Sudbury Indicates Nonstandard Particle Model . ... The Sudbury Neutrino Observatory Institute . Explanation: The Sudbury Neutrino Observatory (SNO) has been detecting so few neutrinos from the Sun that the Standard Model of fundamental particles in the universe may have to be revised. Pictured above is the SNO as it was being built. ... The most popular model for fundamental particles , known as the Standard Model , did not predict such schizophrenic neutrinos . ...

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• Modelling of light curve of SN87A
• A Kernel Model for Precision Timekeeping
• APOD: 2015 April 21 - Vesta Trek: A Digital Model of Asteroid Vesta

Chandra X-Ray Observatory CXC 1. ... BI CCD CTI Correction for ACIS Paul Plucinsky, Dan Dewey, & Joseph DePasquale 1 Paul Plucinsky EPIC Cal October 2006 Chandra X-Ray Observatory Gratuitous Pretty Pictures of E0102 S3 Summed Data ~100 ks CXC RGS Spectrum (Pollock 2006) Objective: develop a spectral model which can be used by RGS, HETG, EPIC & ACIS, etc. Paul Plucinsky 2 EPIC Cal October 2006 Chandra X-Ray Observatory What's New Since the Iceland 2006 Meeting? ...

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• http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200704/Plucinsky.pdf
• XMM Radiation Environment Models and Monitor
• Abstract API

... Abstract: We present an extensive study of the radiative transfer in dusty galaxies based on Monte Carlo simulations. ... We have explored the dependence of A_l on a conspicuous set of quantities (Hubble type, inclination, dust optical thickness, dust distribution and extinction properties) for a large wavelength interval, ranging from 1250A to the K band, thus finally providing a comprehensive atlas of dust extinction in galaxies, which is electronically available. ... S04_MD20[ att , abs ] . ...

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• Clumpy dust disks
• Abstract
• serplines (Abstract)

... We find a transition of LBV star from the LBV instability strip to the region of classical WN for the first time. ... Numerical modeling of the atmospheres of these objects are very important for understanding the evolutionary relationship WR and LBV stars, as well as of the physical causes of LBVs variability. We studied spectra of two very luminous stars in the M33 galaxy - LBV V