... 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 . ...

... 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...

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 . ...

... 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. ...

... 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:...

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. ...

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 | ...

... 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. ...

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: . ...

... 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. ...

... 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. ...

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 ...