... Posts tagged ?EGRET? ... Despite no statistic related discussion, a paper comparing XSPEC and ISIS, spectral analysis open source applications might bring high energy astrophysicists? interests this week. ... ArXiv] 1st week, June 2008? ... Category: arXiv , Data Processing , gamma-ray , High-Energy , Methods , Stat | ... 2007? ... This week, instead of only filtering AstroStatistics related papers from arxiv, I chose additional arxiv/astro-ph papers related to CHASC folks? astrophysical projects. ...

The AstroGuide . ... AstroGuide | ... AstroGuide Listing . ... See many more Astronomy Listings by: Category or Alphabet . Directory of astronomy web sites. ... Listed Since October 25, 2004 . ... Web Site . http://123world.com/astronomy/index.html . ... Web . www.astronomy.net . ... Unless otherwise specified, web site content Copyright 1994-2016 John Huggins All Rights Reserved . dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . are trademarks of John Huggins ...

... The hot pixel finding algorithm has some difficulty dealing with on-board split-event reconstruction (SER). Multi-pixel telemetered events (items in the PIXELS table with SHAPE greater than zero, GRADE greater than one) cannot be compared directly to the thresholds set by the noise limit parameters. ... If a telemetered event passes this aggregate cut, each of its comprising pixels must be taken to pass as well, despite that the reality might be otherwise. ...

The silicates that produce the 10 and 18 micron features appear to be broadly similar to terrestrial minerals such as Forsterite and Enstatite. ... Where pre-solar silicate dust grains can be isolated from meteorite material, these also tend to be Mg-rich silicates rather than Fe-rich silicates. ... It has been suggested that the interstellar silicate grains have a different 10 micron feature profile than what is observed for the silicates around evolved stars. ...

. Comment on J1842+7946 . Comparing the brightnesses of the two main features seen in our 5 GHz image with higher frequency VLBI images available in the literature (at 8.4 GHz from the USNO database and at 15 GHz by Kellermann et al. (1998)), one can conclude that the NW component has a steeper spectrum since the SE one becomes relatively stronger as the observing frequency increases. VLBApls home page . Last modified: 16 Oct 2000

... Submitted by Paul Benni on 11/27/2013 18:38:14 . Comet C/2013 R1 Lovejoy (November 8) . Morning image (Nov. 8) of Comet Lovejoy. ... C8 EdgeHD SCT with Hyperstar (f/2.1) and ST-8300C ccd. Image is uncropped from the Hyperstar setup. Compare to my Comet ISON image with the same image scaling. Interesting how much brighter and larger Comet Lovejoy is now compared to ISON. ... Copyright (c) Amateur Telescope Makers of Boston, Inc. ...

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... Science User Portal . ... ESO, the European Southern Observatory . ... Travel and Contacts . Travel to ESO Headquarters . ... Travel to E-ELT Armazones . ... Green ESO . ... Survey Telescopes . ... Star Clusters . ... Stars@ESO . ... ESO Science Newsletter . ... ESO 3.6-metre telescope . ... MPG/ESO 2.2-metre telescope . ... These publication statistics give an idea of how much scientific work gets done with data from the individual observatories, but does not address the impact of this science. ...

... P1827 Date Received: 2003-Jun-02 18:18:57 Technical Page Proposal Type: Regular General Category: Pulsars Observation Category: Total Time Requested: 24 Hours Proposal Title: Ultra-High Time Resolution Measurements of the Crab Giant Radio Pulses: Phase 2 { Subnanosecond Structure. ... Yes Queue Observing Instrument Setup C X-high Atmospheric Observation Instruments: Description of Observer Equipment: We will use the New Mexico Tech voltage recording system currently installed at Arecibo Observatory....