... The Galactic low-mass X-ray binary GS 2023+338 was discovered during the burst on May 22, 1989 with the Japanise satellite Ginga (aka Galaxy). The flux reached 17 crabs (this unit of flux measurement is an bright X-ray source, Crab Nebula) at 10-35 keV. ... No other radio telescope worldwide carried out multi-frequency measurements. ... Upon 14 days the radio flux fell below the detection level at the RATAN-600 in relation to the decrease of the X-ray flux. ...

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• Northern Lights and GLORIA
• Discovery of an isolated dwarf spheroidal galaxy neighboring the Local Group
• Sun image

The Chi-Square Goodness of Fit Statistic . This statistic enables us to test whether observed frequencies are close to . those we would expect. ... Expected frequencies . ... For example, if we . have an honest die we would expect 1/6 of all cases to show any of . ... So, for example, if we roll a die 60 times we would expect : . ... If we actually roll a die 60 times we wouldn't expect each of the faces . ... times each face actually comes up is the observed frequency for that face. ...

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• http://zebu.uoregon.edu/2004/es399/chitable.html
• http://zebu.uoregon.edu/~uochep/talks/talks04/tau.pdf
• http://zebu.uoregon.edu/1995/ph161/l15w.html

... Meteors and Meteorites . ... By admin August 2, 2011 Posted in: August . 13 August 2009: A perseid flashes through the sky (Image credit: Andreas M†ґller via wikimedia.org) . ... Not all meteors are sporadic events, the regular meteor showers occur when the Earth bulldozes through a great swarm of meteoroids drifting in orbit round the Sun. ... They are at their best in the pre-dawn hours, as the face of the Earth turning towards the Sun catches more meteors as the Earth moves through space. ...

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• Stargazing in November | Astronotes
• observing | Astronotes - Part 4
• Comet Lovejoy is on the Way | Astronotes

... 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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• Radio survey for new compact HII regions
• Introduction
• The very metal-poor local dwarf galaxies

... Bojan Nikolic web pages (r. 329) . ALMA . ... LibAIR is the atmospheric inference library that is the main core of the algorithms for phase correction of ALMA data using water vapour radiometers that we are developing in Cambridge. ... The library and algorithms are documented in the series of memo?s which are being posted at page on inference of coefficients for use in phase correction. ... ALMA WVR phase correction algorithms and software . ... Introduction to phase correction for ALMA . ...

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• Research
• Astrophysics Group COAST Astronomical Results
• OptInt PmWiki : Conceptual Design Review | History

... The syntax of the output is essentially the same as that expected by dsvalidate and dsverify. The output has the form: dataset dataset items where, dataset items is a list of one or more of name attribute block where block has the form block block items block items is a list of one or more of xmmsas 20050815 1803-6.5.0 XMM-Newton Science Analysis System Page: 2 attribute ...

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• XMM-Newton SAS: Watchout Page
• Description

... Exposure Time Calculator (ETC) . Survey processing . ... VISTA is a 4-m class wide field survey telescope for the southern hemisphere, equipped with a near infrared camera (1.65 degree diameter field of view at VISTA's nominal pixel size) containing 67 million pixels of mean size 0.34 arcsec and available broad band filters at Z,Y,J,H,K s and a narrow band filter at 1.18 micron. A wide field visible camera, if constructed, could also be used on VISTA. ... Tile . ... ESO VISTA Public Surveys . ...

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Last updated 21 August 2003 by JMD . Last link checked 21 August 2003 by JMD . These line plots were made by placing an Ar discharge lamp and power supply about 8 inches away from GRIM's entrance window. ... For most purposes, we advise that observers request a setup similar to the one used here for getting Ar lamp wavecals. ... postscript . jpeg . ... The low resolution of GRIM yields broad lines that make it difficult to distinguish blends, so these are the best guesses. ...

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• Figure 10
• ARCSAT Observers Nightlog Form
• Manastash Ridge Observatory Home Page

MAIN PAGE . ... Nova Cygni August 1975! ... 1975/76: Comet West! ... Dr. Richard West (4th from left) & AAL members visiting SES Betzdorf on occasion of our club's 25th anniversary - October 1996 . Comet West Information . ... It was the brightest comet visible from Earth since Comet West in 1976. ... 1997: Comet Hale-Bopp! ... Thus Comet Hale-Bopp never got closer to Earth than Earth gets to the Sun. ... Comet Hale-Bopp JPL Page . ... 1999: Total solar eclipse over Luxembourg! ...

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Тема : Хвостатые гостьи V (информация для наблюдения комет) .. Показать сообщение отдельно . ... Хвостатые гостьи .. ... после того, как ISON приплыл мимо нас, земля находится на орбитальной траектории, которая пройдет через след частицы кометы (тот, который ISON оставил позади, когда это приближалось к солнцу и это случайно встретит или вокруг 12 января - 15, 2014 . ... лучшее время наблюдения 22:00 LDT (Northern hemisphere 45њ North) .. - радиант расположен вблизи Al'dzhabkhakh (30-Eta Leonis, ? ...

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Variations of total ozone content and lower ozone stratosphere temperature in Antarctic Region during winter-spring period A.V. Grytsai National Taras Shevchenko University of Kyiv Astronomy and Space Physics Department assen@univ.kiev.ua Data, used in the work work Total ozone: Total Ozone Mapping Spectrometer (TOMS) measurements during 1979 - 2005 and Ozone Monitoring Instrument (OMI) ones for 2006, for http://toms.gsfc.nasa.gov/ftpdata.html. ... A long-term TOC decrease is significant. ...

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• MAO NASU :: Topic: Fw: ASTRONET: Task 5.4 - observing schools (1/1)
• MAO NASU :: Topic: August Issue: How We Conquered the Planet (1/1)

... 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. ...

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• The New MAJORDOME: Efficient Scheduling of Autonomous Telescopes
• The ISO Post-Mission Archive
• Kalman Filtering in Chandra Aspect Determination

OBSERVATIONS OF COORBITAL SATELLITES OF SATURN Emel'yanov N., Varfolomeev M. Sternberg State Astronomical Institute, Moscow, e-mail : emelia@sai.msu.ru Institut de MИcanique CИleste et de Calcul des иphИmИrides, Paris, e-mail : emelia@imcce.fr Abstract. To improve the orbital parameters and masses of coorbital satellites of Saturn, Janus and Epimetheus, new observations of these satellites are necessary. ... IN: Saturn. ... New observations of Saturn's coorbital satellites" - Icarus. ...

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• Speckle polarimeter
• IDL programs
• Solar Activity, Weather and Climate

MAJOR MAGNETIC STORMS 1932-1997 ACCORDING TO THE Ap* CRITERIA To view a plot of the number of magnetic storms v.s. sunspots, go to ftp://ftp.ngdc.noaa.gov/STP/GEOMAGNETIC_DATA/APSTAR/magstorm.gif A simpler global index of magnetic activity (other than Kp or Km) is produced in France from the K indices of two nearly antipodal magnetic observatories in England and Australia. ... An AA* index has been derived that is the counterpart of Ap* but is available for the longer span of years. ...

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• http://www.wdcb.ru/stp/data/solar.act/sunspot/sunspot.txt
• http://www.wdcb.ru/stp/data/geomagni.ind/aa/aastar/aastar_readme.htm
• http://www.wdcb.ru/stp/data/solar.act/flux10.7/%20%20penticton.txt

PROJECT ARTIST Title : Astronomy-Related Teacher In-Service Training Type : Award NSF Org : ESI Latest Amendment Date : August 14, 1992 File : a9154832 Award Number: 9154832 Award Instr.: ... It is designed to : (a) provide education in astronomy and basic scientific principles for teachers and (b) provide teachers with the means to communicate these concepts in an inquiry fashion to students. ... The cost sharing of the project will be at least twelve percent of the project. ...

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• Limiting Magnitude Table
• The M111 - "On Line"

... About ATMoB . ... The Observing Committee is starting an Observing Awards Program to promote observing among the membership of the Amateur Telescope Makers of Boston. ... Participant must be a current member of the Amateur Telescope Makers of Boston . ... To qualify for your Observing Award Certificate, turn in your worksheet and drawings to an ATMoB Observing Committee member or observing@atmob.org . ... This Excel sheet has useful macros. ... Copyright (c) Amateur Telescope Makers of Boston, Inc. ...

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• Amateur Telescope Makers of Boston

Next: CONICA: The high resolution Up: VLT Status and Instruments Previous: VLT First Light . ... Infrared instruments for the VLT . Instrument Summary . ... The already approved infrared instruments for the VLT are: . ... CONICA: Coude Near Infrared Camera (P.I. R. Lenzen, MPIA, Heidelberg) - an historical name as this instrument will be used for diffraction limited 1-5 m imaging, polarimetry and spectroscopy with the NAOS, Nasmyth Adaptive Optics System on UT1 (P.I. G. Rousset, ONERA ). ...

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• Future Technology
• NICMOS Observes the Galactic Center
• Design and Status of the NICMOS Cryocooler

Crater Gassendi . ... I made this drawing was made on the 26th of november 2001. If you compare this one with the previous drawing of Gassendi (below) the differences are clear. ... This drawing was made on the 28th of september 2001. After nearly a full month without observations I had a one hour gap between the thicker clouds. ... This drawing was made on the 29th of august 2001. ... This drawing was made on the 27th of august 2001. ... This drawing was made on the 25th of august 2001. ...

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... 13, Moscow 119992, Russia, 2 University of Milano-Bicocca, Piazza della Scienza 3, Milano 20126, Italy, 3 University dell'Insubria, via Vallegio 11, Como 22100, Italy, 4 University of Padova, via Marzolo 8, Padova 35131, Italy We present Log N { Log S distribution for close-by young isolated neutron stars. ... 1 Introduction Neutron stars (NSs) and black holes (BHs) are among the most interesting astrophysical sources. ... 2 Isolated neutron stars In this section we discuss isolated NSs. ...

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• PSR B0042-73 in the Small Magellanic Cloud
• Discussion and conclusions
• Conclusions

Report of the RadioAstron International Science Council meeting of June 18-20, 2012 The RISC congratulated Nicolai Kardashev and the entire Astro Space Center team for their leadership and determination over more than 30 years resulting in the successful launch of RadioAstron and the magnificent early interferometer results in all four frequency bands. ... Recommendations The RISC advised the ASC to develop an Open Skies phase of RadioAstron research beginning mid 2013. ...

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• http://www.asc.rssi.ru/RadioAstron/meetings/telecon/nov16_2011.pdf
• http://www.asc.rssi.ru/RadioAstron/meetings/RA&RISC/2014/summary.pdf
• http://www.asc.rssi.ru/RadioAstron/news/newsl/en/newsl_17_en.pdf