Next: Analysis Tools for Nebular Emission Lines . ... Extracting spectra from a large number of NICMOS grism images requires a convenient interactive tool which allows a user to manipulate direct/grism image pairs. ... The direct image is used to locate objects of interest, to find the position of the appropriate spectra in the grism image, to determine the optimal extraction technique to use, and to calibrate the wavelength range of the extracted spectra. ... Figure 1: The NICMOSlook User Interface . ...

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• A Technique for Determining Proper Motions from Schmidt Plate Scans at ST ScI
• Refining the Guide Star Catalog: Plate Evaluations
• Determination of the Permissible Solutions Area by Image Reconstruction from a

... The metal abundance gradient in the disk of the Galaxy is found from stars with abundance determination from detailed analysis: d[Fe/H]/dR=(-0.05?0.01) kpc -1 . It is shown that the gradient can be explained by the fact that the disk is constituted of two metallicity groups of stars with an abundance jump between the groups. ... По звездам с определениями [Fe/H] из детального анализа найден градиент металличности в диске Галактики: d[Fe/H]/dR=(-0.05?0.01) кпс -1 . ...

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... Comparative study of Tl-2201 single crystals with T c =30 and 110 K by means of X-ray structural analysis and NMR. Abstract: . The crystal structure of a tetragonal single crystal of Tl-2201 with T c =30 K has been determined by the X-ray diffraction technique ( a = 3.8717(3), c = 23.224(3) Angstrom, space group I4/mmm, Z = 2). The chemical composition is found to be Tl 1.90(1) Cu 0.10(1) Ba 2 CuO 6.18(4) . ... Structural parameters of Tl-2201 cuprates with various T c have been compared. ...

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• LPCBC: Abstract, 1_5
• LPCBC: Abstract 2_4

Workshop on geometric analysis and spectral theory . ... On a class of random walks on groups with infinite number of generators". ... Optimal transportation, weak flows and very degenerate elliptic PDE's". ... Singular solutions to fully nonlinear elliptic equations". ... I will give some hints on how this conjecture is related to minimal surface theory and I will describe some flatness results for non local equations on one hand and on elliptic equations on riemannian manifolds on the other hand. ...

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• Workshop on geometric analysis and spectral theory. Schedule

Next: NICMOS/HST H-band (F160W) Images Up: NICMOS Science Previous: HST NICMOS Observations of . ... Observations of P . ... The NICMOS team has devised a comprehensive program of observations of the Galactic Center. ... Data in hand give a first look at variability and a detailed look at the search for the tip of the main sequence will be discussed where NICMOS has demonstrated adequate sensitivity and photometric precision to identify likely O8-B1 stars at the Galactic Center. ...

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• ST-ECF Grism Spectrum Software for NICMOS Grism Data
• The ``stecf" IRAF Layered Package
• STScI NICMOS Software

We present an extinction analysis of sight lines selected from all public FUSE observations of Galactic O and B stars. Over 90% of Milky Way extinction curves sampled from IR through UV wavelengths (UV coverage provided by IUE) conform to the CCM family of curves based on R(V), a single parameter linked to grain size (Cardelli, Clayton, Mathis 1989, ApJ, 345, 245; Valencic, Clayton, Gordon 2004, ApJ, 616, 912). ... ADS ] . ADS Citation Query . ...

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• WFPC2 ISR Abstract
• Abstract
• Is the Crab Pulsar Showing A 60-second Periodic Modulation?

... Suspected G36.6-0.7 has the spectral index -0.8, it seems to be a background extragalactic source because the spectral index is too steep for SNR. ... During the last years the RATAN-600 has been used to carry out a new survey of the Galactic plane at 960 and 3900 MHz from l=342^o to l=19^o, |b| < 5.5^o, to search for new SNRs and to study the SNRs that have just been detected. Column (1) lists Galactic notation names of the new and well--known SNRs from Green's catalog; . ...

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• Auxiliary utilities
• Spectra of 300 sources
• Radio patrol survey by Gregory and Taylor

... Abstract (txt) . ... Xiao-li Meng (Harvard U) . ... presentation (pdf) . ... web page: astrostatistics.psu.edu/stat05.html . ... H. Kang (Department of Statistics, Harvard University), D. van Dyk (Department of Statistics, University of California at Irvine), V. Kashyap (Harvard-Smithsonian Center for Astrophysics), A. Connors (Eureka Scientific) . ... Poster (ps) . Poster (pdf) . ... Y. Yu, X.L. Meng (Dept. of Statistics, Harvard Univ.) ... Y. Yu (Dept. of Statistics, Harvard Univ.) ...

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• Statistics 310 2005-2006
• Wendy Roberts - Bibliography, Harvard-Smithsonian Center for Astrophysics
• Watching the Stars go `Round and `Round

... Determination of Black Hole Masses via Correlations between their X-Ray Spectral and Timing Properties " . ... This fact strongly support our theoretically motivated idea that low frequency QPO for a particular BH state is inversely proportional to BH mass.Based on our scaling technique, we determine BH masses in H1743-322, GX 339-4, XTE J1650-500, XTE J1859-226, 4U 1543-47, 4U 1630-47, using independently known masses of XTE J1550-564, GRO J1655-40 and GRS 1915+105 as references. ...

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... 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. ...

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• Armagh Observatory
• Abstract 200
• Abstract 218

... The large body of near infrared observations presented in Testi et al. (1997; 1998) are analysed with the aim of characterizing the young stellar clusters surrounding Herbig Ae/Be stars. The results confirm the tendency of early Be stars to be surrounded by dense clusters of lower mass "companions", while Ae stars are never found to be associated with conspicuous groups. ... Only the most massive stars (10-20Msun) are found to be associated with dense (10^3 pc^-3) stellar clusters. ...

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• rho-Oph BD disks (Abstract)
• serplines (Abstract)
• cephe (Abstract)

... 3.2 CTI correction In CCDs part of the charge released by an absorbed photon is lost during transfer to the readout node. This loss depends on several parameters, in particular on the position where the photon was detected, its energy, the temperature of the CCD, and the saturation of traps by charges preceding along the readout direction. ... The model accounts for the e ects of incomplete charge collection close to the detector surface. ...

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• http://xmm.vilspa.esa.es/sas/7.0.0/doc/calpnalgo.ps.gz
• http://xmm.vilspa.esa.es/sas/6.0.0/doc/calpnalgo.ps.gz
• http://xmm.vilspa.esa.es/sas/7.1.0/doc/calpnalgo.ps.gz

Trudy GAISH, vol. LXV, 1996 . Abstracts . The global distribution of average (5 O x 5 O ) depths . of Mohorovicic discontinuity on the Earth . ... Such analysis allows detecting whether the sources of the largest anomalies reside within the Earth's core. This is possible if the limit depths of the sources exceed the depths of the core-mantle boundary. ... by Pasinok S.L. Influence of the Earth’s cover on the polar free oscillation of the Earth’s inner core is considered. ...

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Find Similar Abstracts . ... Determination of the component masses and inclination of a binary system containing a pulsar from relativistic effects . ... BINARY STARS, ORBITAL ELEMENTS, PULSARS, RELATIVISTIC EFFECTS, STELLAR MASS, APSIDES, DOPPLER EFFECT, FREQUENCY SHIFT, INCLINATION . ... Use: Authors Title Abstract Text Text Query with Keywords Return: Query Results Query Form Database: Astronomy Instrumentation Physics and Geophysics ABSTRACT QUERY USER FEEDBACK HELP ...

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• No Title

. Invited Paper AIAA-94-2281, 1994. Jacques Lewalle, jlewalle@syr.edu

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• Boundary layer transition
• Unsteady boundary layer transition
• The Chirplet Transform: Physical Considerations

... The effective temperature Te = 13700+ 500 and the surface gravity log g = 3.75 ± 0.25 were determined. ... It is shown that the ionization equilibrium for Fe I - Fe II and Mn I Hn II lines is maintained only for the second, more cool model. Out of 10 considered elements the largest overabundance was found for Mn (2.0 dex ), Ga (4.5 dex) and Hg (5.5 dex) . ... Hence it follows also that Y and Ce overabundance cannot exceed 2.5 dex. ...

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• The ROSAT Bright Survey: II. Catalogue of all high-galactic latitude RASS
• sostav
• Оптический спектр инфракрасного источника IRAS 23304+6147

Proceedings of the Particle Physics and Early Universe Conference (PPEUC). For this paper: postscript PPEUC CMB index 1 Introduction.. ... Nuffield Radio Astronomy Laboratories , University of Manchester, Jodrell Bank, Cheshire SK11 9DL, U.K. We use radiation emitted by the galaxy to probe the amplitude and spatial distribution of galactic free-free radiation. ... 2 Using to Trace Free--free Emission . ... Acknowledgements . ... PPEUC Proceedings . Fri Jul 25 11:50:21 BST 1997 ...

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• Paper II: Spinning dust in galaxies Bojan Nikolic web pages (r. 329)
• Scaling relations for molecular gas in the Large Magellanic Cloud
• A 215 to 265 GHz spectral line survey of the Sgr B2 molecular cloud

... Proposal Type: General Category: Observation Category: Total Time Requested: Minimum Useful Time: Prop osal Title: Regular Pulsars Galactic 12 Hours 3 hours Timing J1913+1102: A compact, possibly asymmetric double neutron star sys- tem ABSTRACT: J1913+1102, a 27.3-ms pulsar, was discovered by the PALFA Survey in 2012. ... This proposal requires coordination with Punta Salinas radar within the band 1222-1381 MHz.. This proposal requires coordination with GPS L3 at 1381 MHz. ...

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• http://www.naic.edu/vscience/schedule/tpfiles/ChampiontagP2068tp.pdf
• Galactic Spiral Structure in H I Emission and Self-Absorption

... Several attempts to discover the FICN signal in VLBI nutation series made during last years failed. ... We investigated several VLBI CPO series by means of spectral and wavelet analysis. It has been shown that there are several periodic signals with close amplitude around the expected FICN period without any prevailing one that can be reliably associated with the FICN. ... DATA ANALYSIS We analyzed several CPO series obtained in IVS analysis centers by means of spectral and wavelet analysis. ...

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• http://www.gao.spb.ru/english/personal/malkin/publ/zm12e.pdf
• http://www.gao.spb.ru/english/personal/malkin/publ/zm10c.pdf
• http://www.gao.spb.ru/english/as/j2014/presentations/mosenkov.pdf

... Science Users Information > Science Activities > PhD Thesis Topics offered by ESO Faculty Members > Thesis Topic: Planetary Nebulae and HII regions in the Elliptical Galaxy NGC 5128 . ... NGC 5128 is the closest example of a giant early type (elliptical or S0) galaxy. Although often dubbed as a peculiar elliptical galaxy since it has a dust lane with recent star formation and an active galactic nucleus, the majority of early type galaxies have similar structures as revealed by recent surveys. ...

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• ESO - Thesis Topic: ALMACAL: the evolution of the molecular gas in galaxies
• Towards a better understanding of AGN
• ESO - star07