. This supernova is really magnitude 17.2. In addition, it is the most distant I have ever found. The radial velocity of UGC 5608 is about 15,100 km/sec. It is type IIn . Mike Schwartz , Director . Tenagra Observatories, Ltd. Cottage Grove, OR 97424 . VSNet data on this SN: . [ vsnet-chart 135 ] Chart of SN1999Z . [ vsnet-chat 1637 ] Host galaxy of SN1999Z . Back to Bright Supernovae . Back to Supernova 1999Z in UGC 5608 . David Bishop Last modified: Fri Jul 2 12:15:26 EDT 1999

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• Bright Supernova Bright Supernova
• Supernova 1999an in IC 755
• Supernova 1998es in NGC 632

... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Murchison Radio-astronomy Observatory . ... Parkes radio telescope . ... Mopra radio telescope . ... Visiting Parkes radio telescope . ... Parkes radio telescope webcam . ... For example, modified Newtonian dynamics (MOND) has no relativistic extension, and so makes no firm lensing predictions, but galaxy-galaxy lensing data can be used to empirically constrain the deflection law of a MONDian point-mass. ...

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• lbaops:tidnotes:fileprep [ATNF VLBI Wiki]
• VLBI Wiki | TidNotes / FilePrep

The Astronomical Society of Australia has been asked by STANDARDS AUSTRALIA to compile a list of "designated" optical observatories that are valuable resources for (i) research, (ii) education and (iii) community use. The ASA is the final arbiter of whether any particular observatory is so designated. ... Upon receipt of your application form, your observatory will be entered on a list of "Pending Designated Observatories" on the ASA Home Page. ... It will be emailed for you. ... Email . ...

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• Designated Observatory Registry
• IAU Commission #34 (Interstellar Matter)
• MikeDopita's Homepage

On January 23, 1998 the space probe NEAR was on its way to its closest approach to Earth. Shortly before this, a so-called sunglint event was scheduled: by re-orienting its solar panels in order to reflect sunlight onto Earth's surface, the probe would shine for a few minutes brighter than any star in the sky. ... However, we were able to record a series of images of the space probe shortly before the sunglint event, and we have assembled them into a movie. ...

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• NEAR recorded on 23 January 1998(frame 1)
• Aldebaran Occultations
• IRC+10216/CW Leo Occultation

... His early works dealt with statistical methods especially in atmospheric, geomagnetic and ionospheric tides. In 1928, Bartels became professor in Eberswalde; in 1936, he became director of the Potsdam Geophysical Institute and full professor at Berlin university. ... With these statistical methods, he was able to disprove many widely accepted geophysical models on the one hand and develop some very useful and easy to apply geophysical indices on the other. ...

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• Geomagnetic Kp Index
• Related Solar-Terrestrial Physics Servers
• Geomagnetic Indices Kp, ap, Ap, Cp and C9

Next: The Quasi--Newton Method. Up: Outline of the Previous: The Newton--Raphson Method. ... At each iteration, one computes . ... Neglecting the second derivatives matrix , we obtain the ``normal equations'' and the Gauss--Newton direction . This so--called Gauss--Newton method is intended for problems where is small. ... The algorithm implemented here is a modification of that Gauss--Newton method, that allows convergence even for rank deficient Jacobians or for large residuals. ...

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• Modification of Tables
• NVSS radio survey
• Software Modifications

XMM-Newton Science Analysis System . ... CORR_RATE - The count rate after the following corrections have been applied; . 1) A further point-spread function correction may be applied, to extrapolate the counts from 12 to 35 pixels (presently only done for UV observations) 2) Correction for dead-time. 3) Correction for the OM sensitivity-degradation. A key-word TDS_CORR is added to the table to record the correction value. ... XMM-Newton SOC/SSC -- 2008-07-02 ...

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GrIm II . ... The MC has been modified to change the way GRIM images are stored to disk when FITS format is selected. ... The solution the Grim team has come up with is to internally add a constant of 10000 to every pixel of the 'bias subtracted' grim image which makes it conform to the unsigned 16-bit number standard, in that all pixel values after this addition of 10000 are in the range 0-65535. ... We have now implemented this for storage of GRIM files in FITS format. ... filetype fits . ...

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• APO Home Page
• default
• SDSS M1 Mechanical Collimation

The AstroGuide . ... AstroGuide | ... AstroGuide Listing . ... See many more Astronomy Listings by: Category or Alphabet . Low cost beginner eyepieces. Send SASE for price list. ... Listed Since October 26, 2004 . ... www.astronomy.net . About Astronomy Net | Advertise on Astronomy Net | ... dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

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... Eclipse Moon Trail . ... Cassini Spacecraft Approaches Jupiter . ... Most galaxies have a single nucleus -- does this galaxy have four? ... A Polar Martian Dust Storm . ... Sputnik: Traveling Companion . ... Sputnik means "traveling companion". ... Part of a binary star system only 8 light-years away, it was known in modern times to have a small companion star, Sirius B. N81: Star Cradle in the SMC . ... A huge bar that spans over 150,000 light-years across the galaxy center dominates its appearance...

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Alonso de Cordova 3107 . Casilla 19001 . Santiago 19 . Chile . +56 2 463 3078 (Santiago) +56 55 43 5303 (Paranal) +56 2 464 4203 (La Silla) . +56 2 463 3001 (Santiago) +56 55 43 5995 (Paranal) +56 2 464 4101 (La Silla) . akaufer at eso.org . Private Webpage . akaufer at eso.org Last modified: November 29, 2011

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• World Map of Astronomical Observatory Sites
• The Very Large Telescope Project
• Index of /~lchriste/trans/mahdi22

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . This telescope by George Calver , which was extensively modified in the mid 20th century to a Schmidt design was returned to its original Newtonian configuration, fitted with a new drive, and rehoused in a new dome. ... Tupman spent бе800 on the telescope, and a further sum on a suitable dome. ... Colonel Tupman was so disgusted that he dismantled the telescope and pulled down the dome. ... Schmidt Configuration . ...

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• Armagh Observatory Virtual Visit
• Index of /archives/collections M41
• Index of /archives/ArmaghObservatory/collections M41

... GOODS unites extremely deep observations from NASA's Great Observatories, Spitzer , Hubble , and Chandra , ESA's Herschel and XMM-Newton , and from the most powerful ground-based facilities, to survey the distant universe to the faintest flux limits across the electromagnetic spectrum. ... The space-based observations are complemented by ground-based imaging and spectroscopy, including extensive commitments of ESO and NOAO observing time. ... 2010-04-10: Deep VLA 1.4 GHz data for GOODS-North . ...

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• Modifying a USC
• Index of /ftp/instruments/observatory
• Goals and Purpose of SMOV

... 18sep08: bias for 3a/3b changed. Look at p2030 data (polA,polB summed) . 21sep08: bias for all beams changed. ... The wapps in 3 level mode take 100 MHz bw with 64usec sampling and 256 lags. alfa is centred at 1440 Mhz with the 100 Mhz 1390-1490 filter int. The total power was computed and then averaged to .1 seconds. ... Beam 6b is dead and p2030 is adding polA + polB. ... The a2010 data taken on 21sep08 was analyzed to check the stability of all the beams after the bias changes in alfa. ...

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• National Astronomy and Ionosphere Center (Arecibo Observatory)
• The Evolution of Galaxies Seen Through The Neutral Hydrogen Line The Evolution
• amp_compbrd_settings

. Trace: newsarchive . start : saivo : newsarchive . navigation . Main . SAI VO Projects . CAS . Web Services . TODO . AstroSearch . AstroDB . AstroKeywords . VOLinks . Our People . User Space . Sandbox . Help on Wiki search . toolbox . Index Recent changes Backlinks Login . Show pagesource Old revisions . saivo/newsarchive.txt Last modified: 2007/03/23 21:28 by karpov Back to top . SAI VO | Astronet | SAI MSU | Legal Information .

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• volinks [SAI Virtual Observatory - Wiki]
• google_wheel [SAI Virtual Observatory - Wiki]
• navigation [SAI Virtual Observatory - Wiki]

. May 22, 1996 . Fig. 1. An example of the EUV and soft X-ray large-scale chain of bright point revealed by the modified SOHO/EIT and Yohkoh/SXT images. A coinciding straight-line chain of the bright points extends between very distant points 1 and 2 on the SOHO/EIT (a) and Yohkoh/SXT (b) images of May 22, 1996. Back to the page of the SOHO/EIT and Yohkoh/SXT chains . Back to the parent page . Last update: 9 August 1998 .

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• http://www.izmiran.rssi.ru/~ichertok/CHAINS/ANNOUNC/980407.htm
• http://www.izmiran.rssi.ru/~ichertok/CHAINS/ANNOUNC/980601.htm
• http://www.izmiran.rssi.ru/~ichertok/CHAINS/ANNOUNC/921030.htm

... Our Java and Python software runs anywhere on Windows, Mac, and Linux . ... Alsvid - Algorithms for visualization and processing of image data with Python . Our observatory software . PyDome - Astronomical dome control in Python . ... Software archive . ... XEphem for visual access to astronomical data and remote telescope operation (Linux and Mac OS X) . ... SAOImage DS9 for astronomical data visualization (Linux, Mac OS X, and Windows) . ... G ttingen ImageJ astronomical resources . ...

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• ImageJ for Astronomy
• University of Louisville Wide Field and Planetary Telescopes

. Pulkovo Observatory of Russian Academy of Sciences is situated . near Saint-Petersburg. It was founded in 1839. 196140, Saint-Petersburg, Pulkovskoye chaussee 65/1 . English version . Russian version . This page has been accessed times since May 1, 1999.

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... Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer. 2000 October 12 . HETE-2 Rides Pegasus . Credit: Courtesy MIT , NASA . ... Dropped from its mother ship, the Pegasus then successfully flew HETE-2 into orbit. HETE-2's mission is to hunt gamma-ray bursts, brief, random flashes of high energy photons from the distant cosmos. ... About APOD | ... NASA Technical Rep.: ...

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• Supernova 1994I in M51
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• Supernova 1993J in M81

. Copyright (c) Astro Space Center . Send mail to webmaster with questions or comments about this web site . Last modified on September 2006

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