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901. http://star.arm.ac.uk/~meb/weather/ms_oct15
OCTOBER 2015 TOTAL RAINFALL 42.4 mm ( 1.67 ins) TOTAL SUNSHINE 92.9 hours MAXIMUM TEMPERATURE 20.4 C on day 6 MINIMUM TEMPERATURE 0.8 C on day 15 LOWEST MAXIMUM TEMPERATURE 10.9 C on day 24 HIGHEST MINIMUM TEMPERATURE 11.5 C on day 27 MEAN MAXIMUM TEMPERATURE 14.7 C MEAN MINIMUM TEMPERATURE 6.5 C MEAN TEMPERATURE FOR MONTH 10.6 C ...
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Ссылки http://star.arm.ac.uk/~meb/weather/ms_oct15 -- 1.7 Кб -- 16.11.2015
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902. http://star.arm.ac.uk/~meb/weather/md_oct15
Wind Dir Wind Speed Total Vis Present State Of Rainfall Sunshine 30cm 100cm Maximum Minimum Grass Cloud Weather Ground Min 1 10 2015 1036.3 6.8 6.7 360 5 9 1 45 1 0.00 5.5 13.7 14.0 17.8 3.8 0.9 2 10 2015 1029.9 6.5 6.3 160 2 9 1 45 1 0.00 1.5 13.5 13.9 13.1 3.7 -1.4 3 10 2015 1020.1 9.5 8.0 0 0 7 6 2 1 0.00 0.2 13.4 13.8 12.9 6.5 3.9 4 10 2015 1014.1 10.0 7.7 270 5 0 6 2 1 1.70 8.4 13.4 13.8 15.9 4.6 -2.5 5 10 ...
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Ссылки http://star.arm.ac.uk/~meb/weather/md_oct15 -- 6.3 Кб -- 16.11.2015
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903. http://star.arm.ac.uk/~csl/
. This is a holding page for Cesare Scalia. Further information will follow soon.
904. Armagh Observatory
... Armagh Observatory, 10th November 2015: The results of a new study of the planet Mercury have been announced this week at the Annual Meeting of the Division of Planetary Sciences of the American Astronomical Society at National Harbor, Maryland, USA, by astronomers Apostolos Christou (Armagh Observatory), Rosemary Killen (NASA s Goddard Space Flight Center in Greenbelt, Maryland, USA) and Matthew Burger (Morgan State University in Baltimore, USA). ...
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Ссылки http://star.arm.ac.uk/press/2015/mercury_meteoriod_shower.html -- 13.6 Кб -- 10.11.2015
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905. Armagh Observatory
. Sitemap . Contact . Search . Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . There are no vacancies at present . Last Revised: 2015 October 3rd .
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Ссылки http://star.arm.ac.uk/jobs/2015/index.html -- 4.2 Кб -- 03.11.2015
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906. Armagh Observatory
... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . aroundNorth Installation . The aroundNorth installation was permanently installed in the grounds of Armagh Observatory at the beginning of 2015. It was open to the public the following March. A portable version of the installation was then taken to a number of evocative locations around Northern Ireland during the ten days surrounding the official launch of the new installation in the Observatory Grounds. ...
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Ссылки http://star.arm.ac.uk/press/2015/observatory_releases_aroundnorth_feedback_videos.html -- 8.6 Кб -- 02.11.2015
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907. http://star.arm.ac.uk/~csj/idl/IDLINES/idlines.pro
PRO idlines, specfile, linelist , xlo, xhi, xr, atoms , thresh, rv, $ FIT = kft, EW = kew, NF = knf, ALL = kall, STIS = kst, PRINT = kpr, $ XTEND = kxt, XPAND = kxp, MULT = kmlt, DUPLEX = kdup, QUAD = kfour ;-------------------------------------------------------------------------- ; ; idlines ; ; IDL procedure to display ; a) a region of spectrum , together with a fit, if supplied, ; b) positions and relative strengths (gf or W_lambda) of lines in ; common atomic spectra may ...
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Ссылки http://star.arm.ac.uk/~csj/idl/IDLINES/idlines.pro -- 11.4 Кб -- 02.11.2015
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908. Armagh Observatory
... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... Based on early Kepler data, stensen et al. (2010) found that KIC 9202990 showed a 4 hr and a two-week photometric period. They suggested the 4 hr period was a signature of an orbital period; the longer period was possibly due to precession of an accretion disk and KIC 9202990 was a cataclysmic variable with an accretion disk which is always in a bright state (a nova-like system). ...
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Ссылки http://star.arm.ac.uk/highlights/2015/682.html -- 6.0 Кб -- 02.11.2015
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909. http://star.arm.ac.uk/preprints/2015/682.pdf
MNRAS 000 , 000 ґ 000 (0000) Preprint 26 October 2015 A Compiled using MNRAS L TEX style file v3.0 Continuous `stunted' outbursts detected from the Cataclysmic Variable KIC 9202990 using Kepler data Gavin Ramsay1, Pasi Hakala2, Matt A. Wood3 , Steve B. Howell4 Alan Smale5, Martin Still4,6, Thomas Barclay4,6 1 2 3 4 5 6 Armagh ... We also note the presence of two clear `dips' in the light curve. ... The SC light curve of KIC 9202990, derived from Q5 data, shows one long cycle (top panel). ...
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Ссылки http://star.arm.ac.uk/preprints/2015/682.pdf -- 1652.3 Кб -- 02.11.2015
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910. http://star.arm.ac.uk/~jsv/pub15.pdf
... Light-travel-time diagnostics in early Supernova spectra: substantial mass loss of the IIb progenitor of SN 2013cu through a superwind Gr? afener, G., & Vink, J.S. 2015, A&A accepted 2. ... The VLT-FLAMES Tarantula Survey. ... Mass-loss predictions for evolved very metal-poor massive stars Muijres, L., Vink, J.S., de Koter, A., Hirschi, R., Langer, N., Yoon, S.-C. 2012, A&A 546, 42 37. ... Mass-loss Rates for Very Massive Stars Up to 300 Solar Masses Vink, J.S. 2011, ASPC 440, 83 129. ...
911. The Real Workers
Gerry Doyle's homepage . The real workers are: Aaron Reid ... 2nd year PhD, solar Mihalis Mathioudakis (Queens University Belfast)
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Ссылки http://star.arm.ac.uk/~jgd/slaves.html -- 6.8 Кб -- 29.10.2015
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912. http://star.arm.ac.uk/~csj/idl/FAST/xcorr_fits.pro
PRO xcorr_fits, dfl , mode , gplot , xsave ;; calculates centroids of cross-correlation functions ;; from 2d array ;; dfl is size of window to fit peak (in pixels / 2) ;; mode = 0, fit Gaussian, ;; = 1, fit parabola ;; = 2, compute moments ;; gplot = 0, no plots, ;; = 1, plot ccfs and fits ;; xsave = 0, no save ;; = 1, save last ccf and fit COMMON fitsblock COMMON xcorblock, ccfx, ccfy, ccf2y, ccf2n, nccf, ...
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Ссылки http://star.arm.ac.uk/~csj/idl/FAST/xcorr_fits.pro -- 4.5 Кб -- 20.10.2015
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913. http://star.arm.ac.uk/~csj/idl/FAST/xcorrelate.pro
... Apply filter function ; fft_filter, template , dw, g_cen, g_sig, tempfilt COMMON fitsblock COMMON procblock COMMON xcorblock, ccfx, ccfy , ccf2y, ccf2n, nccf , afits, efits, template COMMON colorblock ;; Announce programme and options print, 'XCORRELATE, star , gplot' print print, 'Cross-correlate a series of spectra with a template ' print IF ( star eq 0) THEN $ print, ' star =', star , '; template = mean spectrum' IF ( ...
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Ссылки http://star.arm.ac.uk/~csj/idl/FAST/xcorrelate.pro -- 5.7 Кб -- 20.10.2015
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914. http://star.arm.ac.uk/~csj/idl/DIPSO/sp2rd.pro
PRO sp2rd, file, x, y, header ; Read a 1d function from a spectrum format 1 file openr,lun,file,/get_lun header = 'a' header2 = 'b' ndat = 1L ReadF, lun, format='(A)', header ReadF, lun, format='(A)', header2 ReadF, lun, ndat x=DblArr(ndat) y=DblArr(ndat) z=DblArr(2L*ndat) i=0L valid = 0 ReadF, lun, z FOR i = 0L,ndat-1 DO BEGIN x(i)= z(2L*i) y(i)= z(2L*i+1) ENDFOR close,lun free_lun, lun END
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Ссылки http://star.arm.ac.uk/~csj/idl/DIPSO/sp2rd.pro -- 1.4 Кб -- 20.10.2015
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915. http://star.arm.ac.uk/~csj/idl/DIPSO/resample.pro
... This is a double precision version and seems to work better. x=x*1.d0 y=y*1.d0 nx = n_elements(x) ; define new grid nxx = (x2-x1)/dx + 1L if (floor( nxx ) mod 2 eq 1) then nxx = nxx + 1.0 xx = Dindgen( nxx )*dx + x1 yy = DblArr( nxx ) c1 = 0L dx2 = dx/2.0D0 FOR ix = 0L, nxx -2 DO BEGIN ; loop over new grid b1 = xx(ix)- dx2 b2 = xx(ix)+ dx2 c2 = 0L IF xx(ix) GT x(0) AND xx(ix) LT x(nx-1) THEN ...
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Ссылки http://star.arm.ac.uk/~csj/idl/DIPSO/resample.pro -- 3.0 Кб -- 20.10.2015
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916. http://star.arm.ac.uk/~jgd/frames_index.html
TOP . The Real Workers . The Observatory's Preprint Page . What does the Sun look like today? . A PR page about the Sun . Solar Educational Links .
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Ссылки http://star.arm.ac.uk/~jgd/frames_index.html -- 2.0 Кб -- 20.10.2015
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917. http://star.arm.ac.uk/~csj/idl/FAST/xvclean.pro
PRO xvclean , tvec, dvec , evec, gplot , flat , tclean , dclean ;; Announce programme and options IF ( gplot ne 2) THEN BEGIN print , 'XVCLEAN, tvec, dvec , gplot , flat , tclean , dclean ' print print , 'clean variable star data by removing outliers and background trends' print , 'Input:' print , 'tvec, dvec : arrays of time and data values ' print , ' ...
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Ссылки http://star.arm.ac.uk/~csj/idl/FAST/xvclean.pro -- 4.6 Кб -- 20.10.2015
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918. http://star.arm.ac.uk/~ron/index.html
. This is a holding page for Rok Nezic. Further information will follow soon.
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Ссылки http://star.arm.ac.uk/~ron/index.html -- 1.1 Кб -- 16.10.2015
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919. Armagh Observatory
... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... Armagh Observatory reports that, if skies are clear on the night of 27/28 September, skywatchers will witness a rare total eclipse of the Moon during the early hours of Monday 28th. ... As the eclipse progresses from penumbral to partial phase, and then towards totality, it is interesting to observe how the dark shadow of the Earth slowly encroaches on the Full Moon until the Moon is nearly completely obscured. ...
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Ссылки http://star.arm.ac.uk/press/2015/sept_total_lunar_eclipse_pr.html -- 8.5 Кб -- 15.10.2015
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920. Armagh Observatory
... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... First three columns show base-difference images of the evolution of the wave in 3 EUV channels (211 , 193 , 171 ) of AIA in which the wave is clearly visible. ... From our study we have quantitatively confirmed previous results that during wave passage the plasma visible in the Atmospheric Imaging Assembly (AIA) 171 channel is getting heated to higher temperatures corresponding to AIA 193 and 211 channels. ...
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Ссылки http://star.arm.ac.uk/highlights/2015/681.html -- 6.7 Кб -- 14.10.2015
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