... You are here: start ТЛ correlator ТЛ records ТЛ v275b . Trace: т?? v275b . correlator:records:v275b . v275b . ... Observers Wiki . Tid observed with 2 antennas, DSS34 observing RCP and DSS45 observing LCP (going to same recorder, so same data stream contains both polarizations). ... Use AIPS task UVFLG , example inputs to flag all т??badт?? pol channels: . ... Flag file: v275b.uvflg . ... Comments: . ... correlator/records/v275b.txt ТЗ Last modified: 2014/11/11 18:08 (external edit) . ...

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Apr 13 2015 Canis Minor - The Little Dog Observed: No Object IC NGC NGC IC NGC IC 2189 2394 2412 473 2459 2216 Sub Total: 6 Her H44-8 Type Non-Existent Non-Existent Non-Existent Mag Alias/Notes Non-Existent H479-3 Non-Existent Non-Existent (STAR) (STAR) Observed: Yes Object ABELL 20 494 IC IC IC MAC MAC MAC MAC MAC NGC NGC NGC NGC NGC NGC NGC NGC ...

... Data from NOAA SEC and other sources are given. ... Start . NOAA . ... End . ... MFS . ... non symmetrical absorption . ... Trace Flare Catalog and Trace Data Center . RESIK CATALOGUE (20010830-20030429) . ONDREJOV SOLAR RADIO EVENT ARCHIVE ( OSR ) . ... Yohkoh Flare Catalogue(HXT/SXT/SXS/HXS) (1998-2001) . ... Solar Activity Monitoring and Forecasting (Ondrejov) and Central European Solar ARchives (Observatorium Kanzelh he) click number of AR - images chromosphere in H? . ...

These notes summarize an informal HDF-S session at the Joint ESO/Australia workshop ``Looking Deep in the Southern Sky,'' which was held in Sydney, Australia, on 10-12 December 1997. ... AAT: 1 night imaging in broad and narrow (20 Angstrom) bands on HDF-S + environs using the Taurus tunable filter. ... NTT: HDF-S + surrounding region to be imaged under the auspices of the ESO Imaging Survey (EIS). 15 x 15 arcminute field of view imaged in U, g, r, I, J and K. 13 nights allocated for Sept/Oct 1998? ...

... Posts tagged ?Little? ... The notions of missing data are overall different between two communities. ... Astronomers?I?m not sure how they think but my impression so far is that a missing value in one attribute/variable from a object/observation/informant, all other attributes related to that object become useless because that object is not considered in scientific data analysis or model evaluation process. ... To draw a color magnitude diagram, one needs both color and magnitude. ... 2 Comments . ...

... title='Аксессуар Защитная пленка Samsung Galaxy Note 5 Ainy матовая' border='0' align='left' width='120' style='margin-right: 20px;' hspace='7' vspace='5'/> . title='Коробочка удачи' border='0' align='left' width='120' style='margin-right: 20px;' hspace='7' vspace='5'/> .. ...

ESO PR Photo 18b/00 . ... Caption : Images of two of the novae in NGC 1316 that were discovered during the observational programme described in this Press Release. ... In particular, no less than four novae were detected in a single giant galaxy within only 11 days . ... Moreover, the discovery of four novae in one galaxy in the Fornax cluster was possible with only 3 hours of observing time per filter. ... ESO Press Information is available on the WWW at . http://www.eso.org/outreach/press-rel/ . ...

... OOF . ALMA . ... OOF Index . Zernike Polys . GBT example . ... Observed data and analysis . The observed beam maps are shown in the first row of the table below. ... We show the best-fitting aperture and the best-fitting beams as the number of Zernike orders used for the fitting is increased. A sample OOF observed data set (top row) and the results of analysis with increasing number of Zernike polynomials used to parameterise the aperture. ... In-focus beam . ... Observed beams . ...

As it was already mentioned, the idea behind File Juggler is rather simple: using CGI scripts as processing tools and WWW browser as user interface, display the structure and content of typical anonymous FTP server in a convenient, easily navigated form. ... My P5-133 spends about 0.025 ms on one file when doing linear search with simple criterion (690 ms for 27,000 files, search for substring among file names/descriptions with 70 hits). ... Let's now look whether we can handle 1,000,000 files. ...

... In this vibrant, eye-opening tour of milestones in the history of our universe, Chris Impey guides us through space and time, leading us from the familiar sights of the night sky to the dazzlingly strange aftermath of the Big Bang. ... Cambridge 2010, ISBN: 978-0521180665, Paperback $28.99 . ... Finding the Big Bang . ... As a prelude the book traces the evolution of some of the notions of modern cosmology from the late Middle Ages up to the final acceptance of the concept of galaxies in 1925. ...

... The new emission line galaxies are listed in Table 2 containing the following information: . column 1: The object's IAU-type name with the prefix HS. ... This was not corrected in the figure shown in Appendix A. HS1214+3801 : This is seemingly a supergiant H II -region at the very rim of the nearby edge-on disc galaxy (SA(s)cd) NGC 4244 (V hel = 224 kms -1 and B T =10.88). ... To check this option one needs a detailed map of the NGC 4244 velocity field including HS 1214+3801. ...

Astronotes Armagh Planetarium's Stellar Blog! ... Monthly Sky Notes . ... Posted on January 30, 2012 | 1 Comment If you look towards the west just after sunset this February you will see a very bright star in the darkening sky. ... Continue Reading.. ... No Comments It?s BBC Stargazing Live month, so even more of us will be looking skyward this January. ... Posted on December 5, 2011 | 4 Comments Which is the brightest star in the sky (apart from the Sun)? ... Posted on November 17, 2011 | ...

... 237S (SIMBAD/NED BibCode) ================================================================================ Keywords: Sun: UV radiation - atmospheric effects - Sun: atmosphere - lines: identification Description: An ultraviolet atlas of the solar spectrum with a spectral resolution of 15mA in the region 1948-2000A is presented. ... The wavelength atlas with a list of about 550 lines has been synthesized from data at center of the Sun ({mu}=1) and at {mu}=0.89, smoothed out over an area of 30 arcsec. ...

... Science Users Information > Science Activities > Instrument Commissioning > HARPS Laser Frequency Comb . ... HARPS Laser Frequency Comb . ... The first commissioning run of the HARPS Laser Frequency Comb ( LFC ) was held from 8 тАУ 17 April 2015. ... During this commissioning, the emphasis was mainly on calibration but several science spectra were acquired: four asteroids and twenty stars were repeatedly observed to monitor their radial velocity variations and to compare with published data. ...

This 1-minute logo produced by The GIMP . ... Only free software I'm using in my Web-life and only Unix, of course. ... Optimization of animated gifs. ... Look at animated gif published on this page ( Now this gif was changed to much smaller (and optimized) picture ! ... gifsicle -O2 web-secure.gif -o websecure.gif . You can find this nice little utility at Gifsicle home page. ... I did a screenshots of layers dialog in Gimp illustrate how gifsicle did optimization of the original gif. ...

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . Sequence of four video frames captured at 01:05 BST at Armagh Observatory on the night of the 24/25th July 2013, showing the onset, development and demise of the sprite. ... Unlike common lightning discharges, which often jump between clouds or between the clouds and the ground, sprites are associated with similarly powerful electrical fields that occur high above the clouds of the EarthтАЩs atmosphere. ...

... Лекция 2 (40 K) | Лекция 3 (37K) | Лекция 4 (39K) | Лекция 5 (43K) | Лекция 6 (47K) | Лекция 7 (32K) | Лекция 8 (54K) | Лекция 9 (41K) | Лекция 10 (45K) | Лекция 11 (38K) | Лекция 12 (44K) | ... Postscript-файл (36 K) | ... Алгоритмическая сложность и класс P . ... Вероятностное вычисление и класс BPP . ... Идея квантового вычисления. ... Определение и простейшие свойства квантового вычисления. ... Вычисление, устойчивое к ошибкам (классическое и квантовое). ...

... The hotter the gas, the faster they move, and the more energy each of them holds. The free ions and electrons in a plasma behave the same way. Knowing the temperature of the high atmosphere of Earth, or that of the Sun, we can calculate energies expected of ions and electrons found there. However, ions and electrons actually observed in space are often much , much more energetic, and may move at a respectable fraction of the velocity of light (300,000 km/sec or 186,000 miles/sec). ...

ARCSAT ID NUMBER: AS08 DESCRIPTIVE TITLE: Stellar Environments of the Nearest Red Dwarfs PI: Michele Silverstein (GSU) OBSERVER(S): Michele Silverstein (GSU), Todd Henry (GSU) and Tiffany Pewett (GSU) UNCERTIFIED/UNTRAINED OBSERVERS: COLLABORATORS: Wei-Chun Jao (GSU) and Jen Winters (GSU) CONTACT INFORMATION: (PI/OBSERVER email/phone) silverstein@astro.gsu.edu (404-413-6024), thenry@astro.gsu.edu (404-413-6054) TIME REQUESTED: 7 nights 1. MAY 04-10 (note = first week of Q2, if possible) 2. ...