ATM Forum Message . Forums: . ... Post . ... Resolution . Forum List | ... Post Message | ... Posted by Rick Crockett on April 25, 2007 08:46:54 UTC . ... resolution - aschilli - April 30, 2007 - 00:08 UTC . Indoor resolution - rick_crockett - June 2, 2007 - 07:04 UTC . ... www.astronomy.net . About Astronomy Net | Advertise on Astronomy Net | ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

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• Indoor Resolution - an Astronomy Net ATM Forum Message
• Resolution - an Astronomy Net Astrophotography Forum Message
• Measuring Resolution - an Astronomy Net ATM Forum Message

FLAMES is the multi-object, intermediate and high resolution spectrograph of the VLT. Mounted at UT2, FLAMES can access targets over a field of view 25 arcmin in diameter. ... GIRAFFE allows the observation of up to 130 targets at a time or to do integral field spectroscopy, with intermediate resolution (either R ~ 25000 or R ~ 10000). ... Questions related to service mode observations and proposal preparation should be addressed to the User Support Department. ... Instrument Operation Team . ...

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• ESO - Thesis Topic: High-mass Star Formation at High-Angular Resolution
• High Resolution HST Images of Pluto and Charon (ESO Press Release 09/94)
• ESO - Improvement to FLAMES Spectral Resolution and Sensitivity

DIGITAL WDC EXCHANGE FORMAT . FOR OBSERVATORY 1.0 MINUTE VALUES 1. ... DATA-1 .. DATA-60 are 1-minute values of the given element for that hour. ... Typically, digital 1-minute values received by WDCs from organizations operating automatic magnetic observatory instruments are averages of more frequendy sampled values, e.g. 10-second point samples. ... If the method used to obtain 1-minute average values is important to a user, the WDC will assist in determining the exact procedure applied. ...

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• INTERBALL/ELECTRON EXPERIMENT
• Elements of Algebra

... Polish scientists at the Space Research Centre, Polish Academy of Sciences, in Wroclaw, south-west Poland, have constructed an instrument called SphinX (short for Solar PHotometer In X-rays), which is an X-ray spectrophotometer, that will obtain spectra in the energy range 0.5--15 keV in 256 energy channels with frequency of up to 100 times a second. ... SphinX is part of a package of instruments known as TESIS (PI Prof. Sergei Kuzin, Lebedev Institute, Moscow). ... Space Research Centre, . ...

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• TESIS

An Ancient Universe: How Astronomers Know the Vast Scale of Cosmic Time . ... d) The Age of the Chemical Elements . ... Some isotopes (forms of the element with different numbers of neutrons in the nucleus) of these elements are radioactive; they change into other isotopes at a rate that can be measured accurately in the laboratory. ... The Ancient Universe - The Age of the Expanding Universe - The Age of the Oldest Stars - The Age of Light From Distant Galaxies - The Age of the Chemical Elements | ...

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• ASP: Cooking Up Heavy Elements in the Cosmos

What if we could determine if a given star is likely to host a planetary system like our own by breaking down its light into a single high-resolution spectrum and analyzing it? ... The dark bands result from specific chemical elements in the star s outer layer, like hydrogen or iron, absorbing specific frequencies of light. By carefully measuring the width of each dark band, astronomers can determine just how much hydrogen, iron, calcium, and other elements are present in a distant star. ...

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• elements | Astronomy.com
• What is the heaviest element that astronomers can detect? | Astronomy.com
• We are made up of elements forged in stars. But with the vast distances between

... Plots of the 4 wapps (.ps) ( .pdf ) : . ... top plot: this is how many seconds off the wapp clocks were measured to be from the ntp servers on the network. The colors are for the 4 wapps. 2nd plot: This is the offset (in seconds) that the ntpd pll time loop was using. ... Notice that there are no changes from 9.06 till 9.31 when the loop parmeters were reset. 2nd plot: The frequency offset used in the wapp4 pll loop. 3rd plot: The time offset of wapp4 time relative to the 3 primary ntp servers. ...

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• http://www.naic.edu/~phil/lbw/lowfreq/1100mhz_feb07.html
• The AO Optical Laboratories National Astronomy and Ionosphere Center (Arecibo
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... This file table3 82 660 Observed wavelengths, laboratory values and identifications -------------------------------------------------------------------------------- Byte-by-byte Description ... Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- SpOrd Spectrum order 5- 12 F8.3 0.1nm SolLam Wavelength determination of all solar and telluric lines measurable on the ... Note (6): J: Junkes et al., ...

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• Astronomical Catalogues

... SSAU History . SSAU roadmap . ... Engineers of SSAU laboratory of additive technologies started to carry out experiments in the field of 3D-printing of metal parts, components and assemblies. The research of Samara scientists will allow producing highly complex and non-standard elements of spatial forms required for design and creation of advanced aviation and space technology. ... SSAU Laboratory of Additive Technologies is established in 2011. ... e-mail: ssau@ssau.ru . ...

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• In SSAU established Russian-Chinese laboratory "Space Cable Systems"
• Scientific Research Laboratory of automated systems of scientific research

... AMPLE (Adaptable Minor Planet Ephemerides) is integrated software package to deal with a number of problems concerning minor planets with the aid of IBM-type personal computer. ... compiling a list of all numbered minor planets which can be seen at certain moment within specified sky region and visualization of their mutual positions; . ... As AMPLE is able to reproduce virtually any table of "the Ephemerides of Minor Planets" , it may be considered as computer version of the EMP. ...

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• AY2008 (preface)
• (Untitled)
• AY2007 (preface)

Note: An equivalent list, with Statistics terms described for Astronomers, is available at www.ics.uci.edu/~dvd/Astro/stat-jargon-for-astro.pdf . ... X-ray wavelengths geneally range from O(1) to O(100) ?. The equivalent unit of photon energy is [keV], where 1 eV = 1.609 10 -12 ergs, and [?]=12.3985/[keV]. ... Includes the combined telescope/filter/detector areas and efficiencies as a function of energy averaged over time. ... Emission Measure . ... Event . ... Photons v/s Counts . ...

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• The AstroStat Slog low-resolution
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• The AstroStat Slog Line Response Function

... The database on experiments of light (441.6 and 632.8 nm) scattering by small mineral particles performed in the laboratory of Univ. of Amsterdam contains figures and tables of scattering matrix elements as functions of the scattering angle (theta = 5-173) at both wavelengths, figures and tables of the size distributions measured with the laser diffraction method, electron microscope images of the particles, information ...

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• Database of Optical Constants -- Level: welcome
• Statist.htm: Add elements
• AddElem.htm: Add elements

All stars derive their energy through the thermonuclear fusion of light elements in to heavy elements. High temperatures are required so that the mutual electrostatic repulsion of the protons in each fusing atomic nucleus is overcome. ... Elements with more protons in their nuclei require higher temperatures. ... This sequence is now shown in the animation below. ... First Step of the Proton-Proton Chain Narration . Second Step of the Proton-Proton Chain Narration . ...

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• Formation of the Elements
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... Content Model: %Body.Content . ... Note that the ID, LANG and CLASS attributes can be used with virtually all of the elements permitted in the document body. ... CLASS . ... The CLASS attribute is most commonly used to attach a different style to some element, but it is recommended that where practical class names should be picked on the basis of the element's semantics, as this will permit other uses, such as restricting search through documents by matching on element class names. ...

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• The IMG (Image) Element
• The Head Element and Related Elements
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... 2001 September 27 . Elements of Nearby Spiral M33 . ... Explanation: Spiral galaxy M33 is a mid-sized member of our Local Group of Galaxies . ... M33 's proximity to M31 causes it to be thought by some to be a satellite galaxy of this more massive galaxy. M33 's proximity to our Milky Way Galaxy causes it to appear more than twice the angular size of the Full Moon , and be visible with a good pair of binoculars. ... About APOD | ...

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• APOD: 2002 July 25 - NGC 1569: Heavy Elements from a Small Galaxy
• APOD: May 9, 1996 - Supernova Remnant: Cooking Elements In The LMC
• APOD: 2001 October 26 - Elements in the Aftermath

... Elements of Nearby Spiral M33 . ... 27.09.2001 . ... Mayall Telescope , KPNO , NOAO , NSF Explanation: Spiral galaxy M33 is a mid-sized member of our Local Group of Galaxies . M33 is also called the Triangulum Galaxy for the constellation in which it resides. ... It was taken to help separate stars from emission nebulae, and therefore help study how galaxies form stars. ... September 2001 . ... Publications with keywords: M 33 - spiral galaxy . Publications with words: M 33 - spiral galaxy . ...

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• XWare > APOD
• Астронет > Elements of Nearby Spiral M33
• NGC 1569: Heavy Elements from a Small Galaxy

A&A manuscript no. (will be inserted by hand later) Your thesaurus codes are: 06 (08.01.1; 08.03.2; 08.09.2 HD 144941; ASTRONOMY AND ASTROPHYSICS 9.10.1996 The iron abundance in helium star HD144941 ? ... The iron abundance in the helium star HD144941 has been measured from ultraviolet Fe iii lines. ... Pulsations in helium stars The improved iron abundance indicates a fractional heavy element abundance (by mass) of Z = 0:00024 and that the iron­group abundances follow the CNO abundances. ...

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• Simon Jeffery's Software Store: TAP library
• C.S. Jeffery, Research Astronomer
• Armagh Observatory

Stellarium 0.12.3 . ... FileљStructure . FileљList . FileљMembers . core . planetsephems . calc_interpolated_elements.h . ... 6 љ copy of this software and associated documentation files (the "Software"), . ... 26 љ void CalcInterpolatedElements( const double t, double elem[], . ... 36 љ The cache consists of 3 sets of values: . 37 љ e0[0..dim-1] are the cached values at time *t0, . ... 41 љ (*calc_func)(t,elem) calculates the values elem[0..dim-1] at time t, . ...

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... Made with Swarovski Elements - известный бренд, специализирующийся на производстве одежды и аксессуаров, украшенных кристаллами Swarovski. ... В нашей акции представлена богатая коллекция кожаных женских сумок, инкрустированных кристаллами.Артикул: 00_92_BLUE_JEANЦвет: синийСостав: 100% натуральная кожаОсобенности: кожаная сумка с двумя ручками на молнии, украшенная кристаллами Swarovski. ... Тип: Сумка . ... Сумки . ... Тип гриля: Электрический . ... Полезный объем духового шкафа: 66 . ...

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• Lua - Roccat - Roccat Соковыжималка Element
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• Жакет - Shoreline by Violana - Shoreline by Violana Паяльник Element 878

makeprfcorr -- Compute the pixel response function for an image created with asncombine makeprfcorr association . association . ... Interactive program to compute relative shifts of images in an association file. ... After computing the relative shifts of the direct images, alignasn searches for corresponding grism images for each of the direct images. ... The grism association is then updated with the same relative shift measurements as determined from the direct images. ...

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• Footnotes
• Imaging Polarimetry with NICMOS
• CONICA: The high resolution near-infrared camera for the ESO VLT