. This is the confirmation image of SN 1998ey as referenced in IAUC 7065 . Mike Schwartz , Director . Tenagra Observatories, Ltd. Cottage Grove, OR 97424 . Back to Bright Supernovae . Back to 1998ey . Back to 1998 Supernovae . David Bishop Last modified: Wed Jul 18 12:48:00 EDT 2001

... 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. ...

This service contributes to the International Service of Geomagnetic Indices (ISGI) of the IAGA . ... The Kp numbers of the previous month are available in tabular format . ... There are available also historical and current Kp and derived indices per anonoymos FTP (see below). ... U.S.A. FTP server: ftp://ftp.ngdc.noaa.gov/STP/GEOMAGNETIC_DATA/INDICES/KP_AP/ . monthly update) . ... contains the monthly Kp / ap tables in a simple text format readable for both humans and computers (*.tab). ...

The grot masks are located on the NICMOS page here. File . ... INFLIGHT . ... May 04 2009 03:31:56 GMT . ... Bad pixel mask modified using inflight data, grot pixels added to DQ Data quality mask for calibrating pre-NCS NIC1 data. ... Bad pixel mask modified using inflight data, grot pixels added to DQ Data quality mask for calibrating pre-NCS NIC2 data. ... Bad pixel mask modified using inflight data, grot pixels added to DQ Data quality mask for calibrating pre-NCS NIC3 data. ...

... Current APO Weather . ... Search Site . ... Information for New Users . ... Technical Staff pages . Night Logs and Mailing Lists (maintained by APO) . ... Technical Documents and Database Search . ... Observer's Documentation and Procedures . ... Problem Reporting and APO Technical Documents Database Search . ... APO Drawing/Document Management Procedures . ... APO Technical Documents Database Search . Home Astrophysical Research Consortium . ... Mail Lists (maintained by APO) . ...

Stellarium 0.12.3 . ... Classes . ... ClassљList . ... SatellitesListModel Class Reference . A model encapsulating a satellite list. ... Tell the model that its internal data structure is about to be modified. ... Tell the model that its internal data has been modified. ... The model keeps a pointer to the satellite list, not a copy, so every time that list is modified outside the model (i.e. satellites are added or removed), you need to call beginSatellitesChange() and endSatellitesChange() . ...

... We demonstrate through numerical simulations that model parameters estimated with our technique are essentially bias-free, even when the average number of counts per bin is 1. ... The IW technique avoids such biases by estimating through successive iterations, where for each iteration, j, , and the best-fit parameters are determined by minimization of . ... In our sample, we find that the minimum values and best-fit parameters converge after about 6 iterations. ...

Supernova 1994I was one of the brighter Sn from the recent past. ... 1994I was discovered in the magnitued 8.4 Whirlpool galaxy (aka M51 , NGC 5194 ) in UMa. ... Jerry Armstrong and Tim Puckett discovery image 4/1/94 color . ... Mr. Galaxy discovery image 4/1/94 NEW 9/1/99 . ... Dean Salman image April 1994 NEW 1/26/00 . Associazione Astrofili Spezzini image Undated. Michael Stecker image Undated (color) . ... Leuschner Observatory image Undated . ... Ron Kohl image 4/8/94 NEW 2001/02/14 . ...

Trace: todo . start : saivo : todo . ... SAI VO Projects . CAS . Web Services . TODO . ... Help on Wiki search . ... SIAP Services - create infrastructure for image archives and basic access services via Web-services and browsers. ... SAI CAS Frontend . saivo/todo.txt Last modified: 2007/04/24 21:10 by karpov Back to top . SAI VO | ... SAI MSU | ...

The CHIANTI database consists of 4 primary ASCII files for each ion in the database. contains the energy levels in cm^(-1) It includes both experimental data and theoretical values of the levels energies. ... These energies are from LS coupling and so there is no fine structure splitting. % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration % % Peter Young, Feb 2000 . contains wavelengths, gf and A values for each transition. ...

Next: Interactive Editing of Up: Management of Tables Previous: Displaying Tables . Elements in a table can be inserted, changed , and deleted . These functions are all performed by the WRITE/TABLE or COPY commands (See Table 5.4). The element to be modified must be defined by giving its column and row location. ... Table: Commands to Modify a Table . ... All commands that do not change a table element will only use the subset selected. ... Table: Commands to Transfer Table Data . ...

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 . ...

Name Last modified Size Description . Parent Directory - JOBS_HEALTH 10-Apr-2016 00:00 1.6K JOBS_NAVBAR 10-Apr-2016 00:00 1.2K JOBS_TREND 10-Apr-2016 00:00 4.3K crontab_giraffe 10-Apr-2016 00:00 4.1K .

... 22-May-2007 17:10 . ... 20-Jun-2007 14:23 . ... 23-Apr-2007 13:10 . ...

New precession formula . ... It gives the precession-nutation matrix as the product of four rotational matrices as NP = R 1 (- ) R 3 (- ) R 1 ( ) R 3 ( ) and the precession one similarly as P = R 1 ( - ) R 3 (- ) R 1 ( ) R 3 ( ) . Here and are the angles to specify the location of the ecliptic pole of date in the given inertial frame, and are the true and mean ecliptic angles of precession, respectively, and and are the true and mean obliquities of the ecliptic, respectively. ...

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 ...

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" . ...

... 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 . ...

... The accuracy of calculation of both INTERBALL spacecraft (SC) motion has been estimated at the IKI. ... The 30 days measuring intervals were used during the Tail probe (TP) orbital data treatment, and 15 days intervals - during the Auroral probe (AP) orbit determination. ... http://www.iki.rssi.ru/vprokhor/indap.htm for the Auroral probe; . http://www.iki.rssi.ru/vprokhor/indtp.htm for the Tail probe . ... http://www.iki.rssi.ru/vprokhor/ssc.htm , or http://www.iki.rssi.ru/vprokhor/amisan.htm . ...

... They cover a period of 4 days in which the Supernova continues to rise in brightness (what astronomers call magntiude). ... First Image Taken on March 11 at 8:22 UT. Second Image Taken on March 12 at 8:52 UT. ... The supernova is the same brightness as in the previous image taken 2 hours ago . ... This image, taken 24 hours after the previous image, shows the supernova to be another 0.21mag (or about 25%) brighter. ... Hopefully the images do show that the brightness of the Supernova is changing. ...