Microsymposium 34, MS058, 2001 ANOMALIES OF THE MOON'S THERMAL EMISSION IN THE IR SPECTRAL RANGE (10.5 - 12.5 micron). ... Sternberg State Astronomical Institute, Moscow, 119899, Russia, pugach@sai.msu.ru Summary: New satellite measurements of the lunar-surface radiation temperature were used to construct the spatial angular function of thermal radiation of the Moon in the infrared (10.5-12.5 micron) spectral range. ... These thermal anomalies are observed only in the limited range of phase angles. ...

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• http://selena.sai.msu.ru/Symposium/ir_luna_e.pdf

... About ISSP . RAS members working in ISSP . Laboratories . ... Tel: 2-82-55, e-mail molotkov@issp.ac.ru . ... Investigation of electron and atomic crystalline structure, transport properties of semiconductor and superconductor compounds, ultrathin metal layers on semiconductor surface using photoelectron spectroscopy, low-energy electron diffractometry, tunneling microscopy and spectroscopy. ... 8(496)52 219-82 . ... Fax: +7(496) 522 8160 . ... ISSP RAS 2004 - 2010 All rights reserved. ...

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• Laboratory of spectroscopy of defect structures ISSP RAS
• Laboratory of materials for electrochemical technologies ISSP RAS
• LSSS - About

AGN dust model of 3CR sources Frank Heymann (PhD), Martin Haas, Endrik Krgel, Christian Leipski MIR imaging spectroscopy ISM dust model PAH SED of a clumpy AGN torus CenA (ESO) Crete 2010 vectorized Monte Carlo model Ralf Siebenmorgen 1) Ground based MIR imaging Nuclear activity in nearby galaxies Surface brightness AGN viz. starbursts Ralf Siebenmorgen 10m telescopes ... Ralf Siebenmorgen Crete 2010 PAH in a mono-energetic heating bath if | ... Crete 2010 ...

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• Gaitee Hussain @ ESO
• GOODS
• ESO - Newsletter January 2016

... The optical spectrum of the infrared source IRAS04296+3429 (optical counterpart - G0Ia star, V=14.2) was obtained with the echelle spectrometer PFES at the prime focus of the 6m telescope. ... 1995, Szczerba et al. 1996), our detailed modelling of its spectral energy distribution suggested that this source also should show the 30 m band. ... Stars: abundances - Stars: atmospheres - Stars: AGB and post-AGB - Stars: individual: IRAS04296+3429 . ... Spectral energy distribution . ...

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... THz spectra of polypeptide powder of glycine, (Gly)n (n = 1 ­ 4). ... Method : (i) gas phase spectroscopy (ii) ice sample transmission spectroscopy (iii) reflection spectroscopy on selective adsorption filter Sensitivity ­ ppm level in raw ice sample Wavelengths: (i) 7-12 m (ii) 15-25 m (iii) 70-90 m - search for simple organic volatiles (gas phase transmission) - search for condensed organics in filter (solid-state reflection) - search for condensed organics in ice ; trapper ions...

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• PhSRM
• Microwave Scanning Radiometer-Polarimeter (MSRP)
• Space Research Institute (IKI) Seminar

... It?s needs solution satellite?s orientation problem for defining location of sources of ionospheric emissions above Earth?s surface with necessary accuracy. There is possibility to define orientation of photometric devices by using TV images of star background. The CCD TV camera is designed for recording of images of star sky, Earth? limb and adjoining part of Earth? surface to fix the orbit point coordinates during the measurements by FAGOT and SICH-F devices. ...

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• INFRARED FOURIER-SPECTROMETER SICH-F
• Optical static Fourier spectrometer

... VOLUME**, **PUBLICATION YEAR** **EDITORS** Time-resolved spectral analysis of the pulsating helium star V652 Her C.S. Je ery, V.M.Woolf Armagh Observatory, College Hill, Armagh BT61 9DG, N. Ireland D.L.Pollacco School of Physical Sciences, Queen's University Belfast, Belfast BT7 9NN, N. Ireland Abstract. We present a summary of a new time-dependent spectro- scopic analysis of the pulsating helium star V652 Her. ... The rst direct evidence of a supersonic shock at minimum radius is also obtained. ...

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• M.D. Smith, Research Astronomer
• V652HER AND MERGED BINARY WHITE DWARF MODELS
• Anatomy of a decline

... Astrophysics Group . ... COAST . COAST Astronomical Results . ... Surface Imaging of Betelgeuse . ... This page highlights some astronomical results obtained with COAST over the years. These are listed in chronological order (most recent first). ... Measurements of cyclic variations in the angular diameter of Chi Cygni . ... The first infrared image from an aperture synthesis array . ... The images of Betelgeuse below were reconstructed from COAST data taken in early 2004. ...

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• Astrophysics Group Surface Imaging of Betelgeuse
• Understanding Infrared emission from galaxies Bojan Nikolic web pages (r. 329)
• Understanding Infrared emission from galaxies

When: Tuesdays at lunch time (12:30 - 13:30). ... Tue, Aug 11: .. ... 070306: "Low Surface Brightness Galaxies" by Ralf-Juergen Dettmar . 140306: "Galactic Chimneys" by Naomi McClure-Griffiths . ... 090506: "Active Galaxies at high redshift" by Ilana Klamer . ... 050606: "Molecular Loops in the Galactic Center: Evidence for magnetic floatation to accelerate molecular gas" by Prof. Fukui . 130606: "Kinematical Studies of Ionized Gas in Nearby Dwarf Galaxies" by Janine van Eymeren . ...

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• Spectroscopy
• Astronomical Acronymns
• MNRF Surface extension project

Proposal Identi cation No.: A1511 Date Received: 2001-Feb-01 17:39:36 Technical Page Proposal Type: Regular General Category: Astronomy Sub-Category: Spectroscopy Observation Category: Extragalactic Total Time Requested: 20 Hours Proposal Title: Low Surface Brightness Galaxies in X-ray Emitting Clusters ABSTRACT: Successful surveys for the detection of low surface brightness disk galaxies have been primarily undertaken in spiral rich clusters with little or no X-ray emission. ...

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• http://www.naic.edu/vscience/schedule/tpfiles/LeetagA2644tp.pdf
• http://www.naic.edu/vscience/schedule/tpfiles/Monnier-RagaignetagA1439tp.ps
• http://www.naic.edu/vscience/schedule/tpfiles/LeetagA2644tp.ps

Near-infrared images of star forming regions containing masers ( Figure 1 ) . L. Testi, M. Felli, P. Persi, M. Roth . 1997, A&AS, in press . ... C. Kramer, J. Alves, C. Lada, E. Lada, A. Sievers, H. Ungerechts, M. Walmsley . ... 1997, "Star Formation with ISO", Lisboa, June 24-26, ASP Conference Series, eds. J. Yun and R. Liseau . ... R. Cesaroni, M. Felli, L. Testi, C.M. Walmsley, L. Olmi . ... Click to examine publications from other years . ... Star Formation Group . ... Arcetri Home Page . ...

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• NGC1068 (Abstract)
• High-resolution Herschel spectroscopy reveals the proto-planetary disk around
• Saturn's Moon Titan

Astronomy Picture of the Day . The Spotty Surface of Betelgeuse . ... Explanation: Betelgeuse really is a big star. ... But like all stars except the Sun, Betelgeuse is so distant it usually appears as a single point of light, even in large telescopes. Still, astronomers using interferometry at infrared wavelengths can resolve the surface of Betelgeuse and reconstructed this image of the red supergiant . ... January . ... January 2010 . ... NASA Web Site Statements, Warnings, and Disclaimers . ...

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• The Surface of Titan
• Mercury's Surface in Exaggerated Color
• Астронет > The Surface of Titan

Mal Ruderman (KIPAC, Stanford) . What do we see when we look at the surface of a neutron star from a great distance? ... The new point that is made is a consequence of near-relativistic electron-positron flows expected in the near-magnetosphere's of "young" (not older than about a million years) neutron stars. Because of cyclotron resonance scattering by these pair-flows on surface X-ray and UV emission, we do not see unprocessed suface emission. ...

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... Max-Planck Institute for Solar System Research, Katlenburg-Lindau , Germany ; Институт космических исследований . ... In particular, a systematic and long-term survey of the atmosphere was missing, and most aspects of atmospheric behaviour remained puzzling. After the Magellan radar mapping mission ended in 1994, there followed a hiatus of more than a decade in Venus research, until the European Space Agency (ESA) took up the challenge and sent its own spacecraft to our planetary neighbour . ...

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• Gamma Ray Spectrometer GRS of 2001 MARS ODYSSEY
• REMOTE SENSING OF OCEAN SURFACE STATE
• Venera 15 & 16

In calculating the NIFS sensitivity, we adopt a read noise of 5 e - , a dark current of 0.01 e - s -1 pix -1 , and a maximum exposure time of 3600 s. Grating . ... e/pix) . ... OH Cont. (e/pix) . ... NIFS should achieve signal-to-noise ratios of ~ 10 per spectral pixel in a 0.1" 0.1" aperture for single 1800 s exposures on uniform, extended, continuum sources with surface brightnesses of J = 15.4, J = 15.0, H = 14.8, and K = 13.5 mag arcsec -2 using the Z , J , H , and K gratings, respectively. ...

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• Gemini Near-Infrared Integral-Field Spectrograph (NIFS) Science.
• Gemini Near-Infrared Integral-Field Spectrograph (NIFS) Spectrograph.
• Gemini Near-Infrared Integral-Field Spectrograph (NIFS) IFU.

Next: Colophon Up: Contents Previous: Software Systems . Spectroscopic reduction and analysis programs at the DAO (invited talk) . ... H.-M. Adorf . Interpolation of Irregularly Sampled Data Series---A Survey . ... Robust Data Analysis Methods for Spectroscopy . ... Application of the Linear Quadtree to Astronomical Databases . ... Automated Globular Cluster Photometry with DASHA . ... A. W. Jones, J. Bland-Hawthorn, and P. L. Shopbell . ... J. Bland-Hawthorn, S. Serjeant, and P. L. Shopbell . ...

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• An Optimal Data Loss Compression Technique for Remote Surface Multiwavelength
• The New JCMT Holographic Surface Mapping System - Implementation
• Modelling Spectro-photometric Characteristics of Eclipsing Binaries

... More than 300 surface reconstructions are already known for pure Si surface and Si surface with adsorbate. Study of their properties by the methods of surface physics reveal numerous interesting phenomena including various phase transitions accompanied by changes of Fermi-surface topology, development of the charge-density wave, etc . ... The charge-density wave (CDW) develops in materials with a chain-like crystal structure at temperatures below the Peierls transition temperature. ...

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• Project 6 - RFBR - Multilayer epitaxial heterostructures of high-temperature

... All portable ladders will meet ANSI standards. The use of step or platform ladders longer than 12 feet, extension ladders longer than 17 feet working length, or straight ladders longer than 20 feet is discouraged. ... Users are responsible for inspecting every ladder they use prior to each use. ... Ladders used to access a walking surface or roof must extend at least 36 inches above the landing. ... Users must face the ladder when ascending or descending, taking one step at a time. ...

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• Weather Summary
• GRIM II Spectroscopy
• SDSS Engineering Papers

... Moon . ... What can astronomers tell us about the different colors on the surface of Jupiter's moon Europa? ... We can use the colors of Europa s surface to tell us about the chemical compounds that make up the surface and subsurface of the jovian moon. Even before the first spacecraft made a close visit to Europa, astronomers on Earth used telescopes to study the moon and were able to use a technique called spectroscopy to determine that Europa s surface is composed mostly of water ice. ...

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• Surface features on Titan form like Earth's, but with a frigid twist |
• Would I be able to see Saturn from the foggy surface of Titan? | Astronomy.com
• The Lunar Reconnaissance Orbiter's Lyman Alpha Mapping Project reveals lunar

... The history of star formation was successfully analyzed for the first time based on the spectra of the stellar population of dwarf galaxies of low surface brightness outside the Local Group. We have investigated the stellar population of two dwarf spheroidal galaxies KDG61 and KDG64 in the central part of a close group of galaxies M81. ... These galaxies are dominated by the old stellar population (12-14 billion years) of low metallicity ([Fe/H] ~ -1.5). ... KDG61 . ... KDG64 ...

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• Discovery of enrichment of the envelopes of post-AGB stars with heavy metals
• articles_lebedev_en
• Galaxy sector, archive 1996