... Fermi Epicyles: The Vela Pulsar s Path . ... Credit Copyright: NASA , DOE , International Fermi LAT Collaboration Explanation: Exploring the cosmos at extreme energies, the Fermi Gamma-ray Space Telescope orbits planet Earth every 95 minutes. ... Centered on the LAT instrument's field of view, the plot spans 180 degrees and follows Vela's position from August 2008 through August 2010. ... August . ... 2007 2008 . ... NASA Web Site Statements, Warnings, and Disclaimers . NASA Official: Jay Norris. ...

... 2012 May 4 . Fermi Epicycles: The Vela Pulsar's Path . Credit: NASA , DOE , International Fermi LAT Collaboration . Explanation: Exploring the cosmos at extreme energies, the Fermi Gamma-ray Space Telescope orbits planet Earth every 95 minutes. ... As a result of these multiple cycles the paths of gamma-ray sources trace out complex patterns from the spacecraft's perspective, like this mesmerising plot of the path of the Vela Pulsar. ... About APOD | ... A service of: ASD at NASA / GSFC . ...

FCAL Collaboration Meeting , September 18-18, 2005 . LSC Meeting , August 14-17, 2005 . ILC Workshops at Snowmass , August 14-27, 2005 . HEP 2005 , July 21-27, 2005 . SUSY 2005 , July 18-23, 2005 . ILC European Regional Meeting , June 20-23, 2005 . Ligo Scientific Collaboration Meeting , June 4-5, 2005 . Public Lecture Celebrating the World Year of Physics 2005 , May 19, 2005 . ... Exp Talks - Prior Years . ... Energy and Luminosity Spectrum , Eric Torrence . ...

. " The Arecibo Observatory is sponsored by the National Science Foundation. Any opinions, findings and conclusions or recommendations . expressed in this publication are those of the author(s) and do not necessarily reflect the views of the National Science Foundation."

ATMoB 2017 Solar Eclipse Expedition August 21, 2017 ­ Columbia , MO Participant Registration Form Primary Participant: Organized by Mario Motta / Bernie Volz _________________________________ ... _________________________________ (Cell/Work) ______________________________________________________ NO YES (Non-binding, Extra cost ~$60.00/ person ) Eclipse Day Chartered Coach Option (Circle) I understand this package includes only pre- and post- ... Pre-eclipse meeting at the hotel @ 8PM. ...

... 2000 August 30 . The Brown Dwarfs of Orion's Trapezium . ... NICMOS IDT , NASA . ... Explanation: The bright stars above are well known as heart of the Trapezium , an open cluster of stars in the center of the Orion Nebula . ... Although many more brown dwarfs than hot stars have now been found in Orion, their very low masses make them inadequate to compose much of the dark matter expected in galaxies and the Universe . ... About APOD | ... NASA Technical Rep.: ...

... This calibration approach is recommended when dealing with high frequency data from the old ATCA correlator, especially at 3mm wavelengths. ... The approach described here exploits the dual frequency bands that were available with the old correlator. ... Rather the current approach assumes that you have a single Miriad dataset containing bandpass calibrator, phase calibrator, flux density calibrator and program source. ... MFCAL . ... Input multi-source, dual-band dataset. select=source(1921-293) . ...

Blackholes Forum Message . Forums: . ... Alternative Idea . ... With the proposal of exotic super dense entities like quark stars and others including black holes, matter on the atomic level can, and most likely does, break down to its most simplist building blocks (photons, leptons, quarks, etc). ... www.astronomy.net . About Astronomy Net | ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

... There are some generalizations of the classical Eisenbud-Levine-Khimshiashvili formula for the index of a singular point of an analytic vector field on $R^n$ to vector fields on singular varieties. ... For a variety with an isolated singularity, we define an index of a (real) 1-form on it. In the complex setting we define an index of a holomorphic 1-form on a complex isolated complete intersection singularity (icis) and express it as the dimension of a certain algebra. ...

EIGHTH CREW REQUIRED RESOURCES FIFTH RUSSIAN VISITING CREW SERVANTES SSM PROJECT IMAGE VIDEO . ... From May to October 1994 he trained for a 30-day flight to Mir under EC-17 program and Euromir 94 mission within a backup crew together with Russian cosmonauts Yu.P. Gidzenko and S.V. Avdeev. ... From October 2002 to February 2003 he was in training at Yu.A. Gagarin CTC as a flight engineer-1 of the Soyuz TMA TSC of expedition crew-5, visiting crew (VC-5) of the International Space Station. ...

Scott's Little Corner of the Web . Welcome to my alternative page.. ... You might know me as Szyzyg, my net-pseudonym which I've adopted to avoid those nasty 'name already taken' messages. ... The Music Collection Page , in hte past this used to update automatically to tell you what I was listening to - but it only worked for CD's played on my computer :-( - Instead I've been hacking around with myplay.com and you can now use their servers to listen to some of my selections . ... Szyzyg FAQ . ...

... This is a personal project collecting and documenting early images of Harvard College Observatory, focusing on the site at Observatory Hill (previously Summer House Hill). ... This page shows a list of all images related pictures in the same group. [link] 1887 . ... link] 1887/07 . Earliest source: "[Building in Cambridge under construction]." ... link] 1887/07/13ish . ... Earliest source: "[Telescope dome in Cambridge under construction]." ... Creator: Harvard College Observatory, Cambridge . ...

Astronotes Armagh Planetarium's Stellar Blog! ... Space Flight . ... 1976:NASA?s Space Shuttle climbs to orbit . ... 1972:The first American space station, Skylab 1, is placed into orbit and inhabited by a series of three man crews. ... 1973:NASA sends the first two probes in the Voyager program to Mars, more follow every other year throughout the 1970тАЩs preparing the way for the manned Mars missions to follow. ... 14 August 1983 The first Mars mission arrives back in orbit around Earth. ...

Target Acquisition Reference Information . Figure 7.1 on page 88 shows mean predicted count rates as a function of (B - V) 0 color for the four acquisition mirrors. Also shown are the fits to the predicted count rates for different amounts of reddening. ... You can estimate target acquisition count rates using the plots instead of Table 7.1 on page 92 : . ... Read from the Figures (depending on the mirror used) the predicted count rate. ...

... 739C As one part of a program to detect complete samples of active extragalactic objects, the 3.36x10^-3 sr field centered on alpha=12h04min, delta=+11deg30' (1950.0) was mapped with the Very Large Array at 1411MHz. Sixty-seven maps cover this field so that no point is more than 15arcmin from the nearest map center. ... The rms map noise is 0.030 + 0.001 mJy, and the resulting source list is complete to a map peak flux density S_p = 0.2 mJy within 25 arcmin of the field center. ...

... Институт прикладной математики им. М.В.Келдыша . БАЛЛИСТИЧЕСКИЙ ЦЕНТР . О Центре . ... Баллистический Центр Института прикладной математики им. М.В.Келдыша РАН . Баллистический центр (БЦ) ИПМ им. М.В. Келдыша создан по предложению С.П. Королева и М.В. Келдыша в 1965 году. На него были возложены работы по баллистико-навигационному обеспечению (БНО) управления полетом пилотируемых кораблей и автоматических космических аппаратов научного и народно-хозяйственного назначения. ...

. The sharply-defined crater just above the center of this Cassini image shows layers of alternating bright and dark material. Cassini was 8,314 miles (13,377 kilometers) from Phoebe when this image was taken. NASA / JPL / CICLOPS

... The parameter pgdev allows the user to specify a pgplot device, but, in contrast to the pgplot standard, the file name should not be included, but instead supplied via the parameter plotfile . ... To write a colour postscript file called op.ps: pgdev=/cps plotfile=op.ps . However note that at present, if a colour postscript device ( pgdev = `/cps'), a fits file ( pgdev = `/fits') or a ppm file ( pgdev = `/ppm') are selected, the task in fact bypasses pgplot and writes the postscript file directly. ...