... REGISTER/ROMAFOT int_tab reg_tab [wnd_opt] [obj_opt] . ... However, all the photometric information obtained from the frame as the absolute quantities (magnitudes, colour equations etc.) still have to be derived. ... Table: Romafot Registration Table . ... In case of program stars (search made with SEARCH/ROMAFOT ), these columns are filled with zeros. The instrumental magnitude MAG_CNV is calculated as , where VOL is the integral over the elementary surface to fit the star, calculated from to . ...

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... The absolute flux calibration of NICMOS will be calculated from observations of standard stars with known flux distributions F( ). ... In order to expand the set of IR standard stars in the appropriate flux range for NICMOS, M. Rieke, R. Thompson, and collaborators at the University of Arizona are making photometric observations of solar-analog stars, which will be used to normalize the solar spectrum to the observed IR magnitudes. ... Relative flux references accurate to 1.5% for standard...

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Arecibo Observatory . July 10 17, 2013 . Registration extended to 1 May 2013 . Registration for the school has now closed. ... If accepted for the school, the meeting fee will be $250 . If you have been accepted for the school, please go to the fee payment form to pay your fee and (if staying on-site) your room costs. Home Register Program Travel Form Fee Payment Form Flyer Accommodation NRAO Green Bank Arecibo Observatory . Last updated: Friday, 07-Jun-2013 11:10:53 AST . ...

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• SDSS5 Registration
• Fifth NAIC/NRAO Single Dish Summer School

... Registration will not guarantee that you will be able to attend until you receive an e-mail notification after registration closes. All accepted participants to the Conference will be listed on the web page under Participants. ... The fee will be included in your room bill which can be payed from Monday June 8 to Wednesday June 10 at Spineto reception desk (from 10:30 am to 2:30 pm). Room check-in and conference registration will take place in the afternoon/evening of Sunday June 7. ...

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... User Guide ] Task: uvamp Purpose: Annular averages a uv dataset in bins. ... Categories: uv analysis UVAMP reads a uv dataset, bins the data in annuli according to uv distance and prints/plots vector averaged amplitude versus uvdist. ... No default. ... Key: bin Number of bins, width of bins, and units of bin width. ... Key: type Calculate the amplitude and standard deviation for each bin based on the real and imaginary components (total) or just based on the real component (real). ... Default:...

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• sms2014: Registration Form
• CSIRO Astronomy and Space Science Radio Astronomy School 2012
• Synthesis_Imaging_School

Peremennye Zvezdy", . ... R_data_1.txt NSVS 547680 . ... Combined brightness of two stars: GSC 4347-01515 (= var) and GSC 4347-01707 (constant), was measured in the NSVS survey, thus the amplitude is considerably underestimated. ... The comparison star was GSC 4347-01707 and the check star, USNO-B1.0 1598-0075392. ... The comparison star was USNO-B1.0 1597-0078695 and the check star, USNO-B1.0 1598-0075495. ... The comparison star was GSC 3230-00588 and the check star, USNO-B1.0 1282-0605581. ...

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Each file type known to SAOtng can have user-defined analysis commands associated with it. ... A help line describing the file types . ... For example, the default analysis file currently contains the following: # # Analysis command descriptions: # help # file templates # file types # analysis command line counts -- number of events in region (no background) *.qp *.imh QPOE IMH uiraf '${xraybin}'/x_xspatial.e imcnts source='${filename}' region=$sregion bkgd=0 table=NONE | ...

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• *imexamine* - General analysis of image containing many sources
• Marker Analysis Routines in SAOtng
• Jonathan's ASC documents

... Telescopes . ... The time requests are accepted in an electronic version with on-line form in Russian or English. ... Unregistered request will be disregarded by the Large Telescopes Programm Committee. In exclusive cases the secreatry of the Committee is entitled to accept an observational time request given permission of the Chairman of the Committee or the director of the SAO RAS. The Program Committee considers generally one time request submitted by the principal applicant. ...

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• Multi-Spin Galaxies Conference 2016
• Solar system sector, archive 2002

20-23 September 2016, St.Petersburg, Russia . ... Abstracts . Registration . ... Participants who wish to present a contribution to the conference are invited to submit title, abstract, and type of presentation (poster or 15 min talk including questions) along with the registration form. The deadline for the Abstracts and Early Registration is 30th June 2016 . ... Name and affiliation . Title: . ... Presentation . ... Yes No . ... Oral Poster . Presentation Title: . ... Poster Title: . ...

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• AY2007 (preface)
• AKO-2005
• AY2008 (preface)

... Meta Index / Home Page / Description / Specifying source region shapes . When radiusstyle =`contour', the task calculates the source region shape as an elliptical locus which approximates the contour of the PSF at a given flux value. ... Clearly, in order to calculate the shape of such a flux contour, it is necessary firstly to normalize the PSF to the source brightness and secondly to determine the flux level (in `brightness' units per pixel) at which to find the contour. ...

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• Parallel detection over bands (with no assumptions made about source spectrum)

... SEARCH ASP SITE: Match ALL words Match ANY word . Annual Meeting . ... Registration . ... Online pre-registration for Astronomical Society of the Pacific Annual Meeting is closed. Those wishing to attend the conference proper on Sep. 13-16 can register on-site at the Westin SFO, the conference hotel, at the ASP conference registration table. ... Registration for the meeting includes automatic general membership (at the $55 rate) with the ASP and the new ASP Conference Series publication. ...

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• ASP: A Taste of Real Astronomy ? The ESA/ESO Astronomy Exercises
• ASP's 2011 Annual Meeting
• ASP's 2010 Annual Meeting

Online Registration for Hidden Hollow . May 2 - 4, 2008 . Richfield Astronomical Society/Hidden Hollow Rules : . ... Registration is open until April 18th . ... No cars permitted into the star party area after dark; park in the drive after dark. ... Each adult participant will receive one door prize ticket when checking in; additional tickets may be . ... Number of Adult registrants at $40 each: . Number of Immediate-family-member registrants at $30 each: . ... B. Hubal, 27-Jan-2008 ...

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• Hidden Hollow 2008

... 1 erg = 0.1 microjoules . 1 Jansky = 10**-26 watts per metre square per hertz . 1 Angstrom = 0.1 nanometres . ... 1 Astronomical unit = 1.4960 times 10**11 m . ... Mass of Sun = 1.989 times 10**30 kg . ... Mass of the Earth = 5.976 times 10**24 kg . Mass of Jupiter = 318 times mass of Earth . Solar constant = 1.37 kW per metre . c= 3 times 10**8 metres per second . ... Mass of Proton = 1836.1 times mass of electron . ... Stefan Boltzmann constant = 5.67 times 10**-8 W m**-2 K**-4 . ...

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• The sculpture is accepted
• ANU - RSAA - 5th Stromlo Symposium Registration
• Cepheid Variables

... You will need a formal letter of invitation to get Russian visa and we will provide it to you. ... First, we will need a copy of first two pages of your passport. The best way to do it is to find a scaner, open the passport, put it on the scaner, scan it with 300 dpi resolution in grayscale mode, save as JPEG file and then send the file to ysc@bmstu.ru and please send a copy to coordinator Irina Yurovskikh yurovskikh.i@mail.ru . ...

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• SpaceDTP-2015 - Registration Form (rus)

Next: Status of the BIMA Image Pipeline . ... We describe all the steps of the standard reduction including per pixel error propagation: Bias correction, treatment of bad pixels, flatfielding, and filtering of cosmic ray events. ... We build difference images via image convolution with a technique called OIS (optimal image subtraction, Alard & Lupton 1998), proceed with PSF-fitting, relative photometry on all pixels and finally apply an automatic detection of variable sources. ...

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• Calculating the Position and Velocity Components of HST
• Multiwave Continuum Data Reduction at RATAN-600
• The ISO Post-Mission Archive

... Amorphous carbonaceous materials can show a great diversity of optical properties due to the variability in their microstructure. ... The differently pyrolized celluloses are representative for a suit of carbonaceous material ranging from strongly disordered (insulating) to graphitized (conducting) material. Figure: Complex refractive index of hydrogenated amorphous carbon prepared by pyrolysis (annealing) of cellulose at different temperatures. ...

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• Database of Optical Constants -- Level: welcome
• A Nature of Polar-Ring Candidate Galaxy ZGC 2315+03
• References

Minutes of the galaxies meeting . Discussion Part I: Commissioning, data analysis storage . Discussion Part II: Project plan, use cases, calibration etc. MKSP overview (R. Beck) . LOFAR status and rollout update (M. Brentjens) . Polarization calibration strategies (G. de Bruyn) . ... MKSP relevant LOFAR hardware capabilities (J. Anderson) . ... MKSP Project Plan, Use Cases and Commisioning Plan (J. Anderson) . ... Radio galaxies working group (G. de Bruyn for T. Arshakian) . ...

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• Preliminary results of OOF holography at the GBT
• The use of Positive Matrix Factorization in the analysis of molecular line
• OptInt PmWiki : Tech Meet 9 | History

... To derive the motion of a penny dropped inside an airliner moving at 600 miles/hr (about 1000 km/hr)--should we calculate it with respect to the interior of the airliner, or with respect to the ground? ... And if a similar penny is let go inside an orbiting spaceship--should its motion be calculated relative to the interior of the spaceship, or relative to the Earth outside? ... Each such choice is known as a frame of reference . Some possible frames are -- the interior of the airliner, . ...

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• Space Research Institute (IKI). Experiment Neutral-E.
• News (english)
• Incoherent scatter [Oulu]

Weekly Bulletin on Solar and Geomagnetic Activity Highlights on 14 - 20.03.2016, Forecast on 21 - 28.03.2016, Carrington Rotations 2174, 2175 (18,17.02; 16,50.03.2016) SUNSPOT-FORMING ACTIVITY OF THE SUN WAS ON THE AVERAGE, AND THE LAST THREE DAYS - ON THE LOW LEVEL. ... FLARE ACTIVITY WAS AT THE LOW LEVEL 15, 16 AND 20.03, AND AT THE VERY LOW -ON OTHER DAYS. ... ACCORDING TO THE CENTER IN BOULDER 14-15.03 WAS REGISTERED. ... ACCORDING TO THE CENTER IN BOULDER AND 6-h. SUBSTORM (G0) TO IZMIRAN DATA. ...

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• http://www.izmiran.rssi.ru/services/saf/archive/en/2012/obzor20121015.en.txt
• http://www.izmiran.rssi.ru/services/saf/archive/en/2012/obzor20120220.en.txt
• http://www.izmiran.rssi.ru/services/saf/archive/en/2013/obzor20130812.en.txt

REGISTRATION FORM Astronomical Data Analysis Software and Systems Conference ( ADASS ) 1997 14 - 17 September 1997 Allgau Stern Hotel, Sonthofen, Germany LAST NAME : FIRST NAME : TITLE: INITIALS: AFFILIATION (for name badge): INSTITUTE: DEPARTMENT: STREET: CITY: POSTAL CODE: COUNTRY: TELEPHONE: TELEFAX: E-MAIL: I also plan to attend the Converging Computing Methodologies in Astronomy Conference: YES ( ) NO ( ) Early Registration ...

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• NICMOS Data Calibration and Analysis
• ADASS '97 Program Information
• ADASS 97 Final Program