... 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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• lbaops:special-vlba-lba-2012-notes [ATNF VLBI Wiki]
• correlator:records:v255b [ATNF VLBI Wiki]
• VLBI Wiki | Main / LBAObservingNotes

. First page Back Continue Last page Summary Graphics .

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• ABPP GUI notes
• Spectral-Line Observing
• AGES Observing Checklist for CIMA 3.0

Apr 13 2015 Scutum - The Shield Observed: No Object NGC IC 6655 4768 Sub Total : 2 Her Type Non-Existent Non-Existent Mag Alias /Notes Observed: Yes Object IC IC MINK NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC SAND 1287 1295 3-28 6625 6631 6639 6649 6664 6682 6683 6694 6704 6705 6712 2-374 Total : 17 Her Type Nebula R Pl Neb 3b+2 Pl Neb 2+3 Open Cl IV 3 m n ...

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• http://www.wro.org/scodova/RNGC_Objects_by_Constellation-Equ.pdf
• http://www.wro.org/scodova/RNGC_Objects_by_Constellation-Sge.pdf
• http://www.wro.org/scodova/RNGC_Objects_by_Constellation-Lyr.pdf

SAS release notes . ... News Latest News News Archive Newsletter Quarterly Status Report . ... Data Analysis SAS News What is SAS? ... Archive, Pipeline & Catalogues XMM-Newton Science Archive Pipeline Processing System Observation Data Status Time Correlation Fix Serendipitous Source Catalogue OM Serendipitous Source Catalogue Slew Survey Catalogue Latest Slew Results Browsing Interface for RGS Data Live Radiation Monitor Plots Radiation Monitor Files . ... SAS Home . ...

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... 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? . ...

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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? ...

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• HDF-S Followup Notes - Sydney, December 1997
• CALSTIS V2.7 Release Notes
• CALSTIS v2.20 Release Notes

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/ . ...

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• CHIANTI atomic database

We report here on those proposed UIT targets that, in fact, were successfully acquired. Where possible we provide an optical CCD image of the target or the field. Note on Filters: . A1 centered at 2500 angstroms with a width of 1200 angstroms . ... UGC 5675 is another Low Surface Brightness galaxy which is the center of the fourth deep A1 field. ... M32 a very high surface brightness dwarf elliptical companion was observed for 1561 seconds through the B5 filter. ...

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... 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 . ...

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• Overview of CCMTools and some relevant notes Bojan Nikolic web pages (r. 329)
• Notes on the classic CASA build Bojan Nikolic web pages (r. 329)
• Some notes using the Maxima system Bojan Nikolic web pages (r. 329)

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. ...

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• Historical Notes
• Introductory Note about the release 3.3.6
• Image: Gate. Note the small bamboo clamp in the foreground.

... 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. ...

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• ASP: Guest Observer
• ASP: Walter Baade: Master Observer
• ASP: Resource Center

... 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. ...

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• Millimeter continuum of extragal. sources, Steppe et al.
• A VLA Survey of Rich Clusters of Galaxies III
• Notes on specific commands

... 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. ...

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... 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. ...

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• ESO - Gasgano
• GOODS
• ESO - Public Surveys Phase 3 Workshop

... 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. ...

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• Software Store - Programmers Notes
• Taurid swarm years
• Terry Mosely's Bulletins

... 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). ...

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• Probabilistic sense of the notion of improbable (Fall 2008)
• Probabilistic basics of the notion of improbable (Fall 2011)
• Lecture notes

... 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). ...

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• The Polar Aurora
• Ionospheric troughs [Oulu]
• The Polar Aurora -- History

Astronotes Armagh Planetarium's Stellar Blog! ... Monthly Sky Notes . ... Posted on April 6, 2016 | No Comments Spring has truly sprung. ... Continue Reading.. Posted on March 1, 2016 | No Comments See you later February, youтАЩve been a wonderful month, but now it is time to welcome March. ... Posted on February 2, 2016 | ... Posted on January 7, 2016 | ... Posted on December 3, 2015 | ... Posted on November 4, 2015 | ... Posted on October 5, 2015 | ... Posted on September 3, 2015 | ...

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• Monthly Sky Notes | Astronotes - Part 5
• Monthly Sky Notes | Astronotes - Part 3
• Monthly Sky Notes | Astronotes - Part 2

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. ...

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• ARCSAT Observers Nightlog Form
• _notes
• Index of /arc35m/Instruments/_notes

Next: Quantum Efficiency Correction (a.k.a. Up: ROSAT HRI Recipes Previous: Appearance of new HRI . The mean pulse height analyzer channel (PHA) of a spectral distribution will vary depending on its location on the detector. Below is a method to compare observed data with that of preflight calibration measurements. ... For temporal gain variations, see The HRI Calbration Report . ... Retrieve the gain maps (mean PHA) from anonymous ftp at SAO. ... But don't forget temporal gain variations!] ...

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• The AstroStat Slog lecture note
• The AstroStat Slog Blog Archive A short note on Probability for astronomers
• The AstroStat Slog Blog Archive [ArXiv] A Lecture Note, June 17, 2007