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http://xmm.vilspa.esa.es/sas/8.0.0/doc/ommag/node9.html.
http://xmm.vilspa.esa.es/sas/8.0.0/doc/ommag/node9.html.
1. http://xmm.vilspa.esa.es/sas/8.0.0/doc/ommag.ps.gz
XMM-Newton Science Analysis System Page: 1 ommag July 2, 2008 Abstract Converts from count rates to magnitudes in the instrumental system. ... Please note that no magnitude is computed for corrected count-rates greater than 1000- for such bright sources the count rate is wrong because it is out of coincidence-loss correction. ... MAG The instrumental magnitude computed using the corrected count rate and using the appropriate calibration constants for the lter. ... Convert this to a limiting magnitude. ...
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Ссылки http://xmm.vilspa.esa.es/sas/8.0.0/doc/ommag.ps.gz -- 48.5 Кб -- 02.07.2008
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2. atfix
... User Guide ] Task: atfix Purpose: Apply various miscellaneous corrections to ATCA visibility data Categories: uv analysis ATFIX performs various miscellaneous offline corrections appropriate for ATCA 3mm data. ... Correct antenna table (when some antennas were off-line) NOTE: This task will usually be used very early in the data reduction process. ... Key: vis The names of the input uv data sets. ... Leave the Tsys calibration as is. constant Apply a constant Tsys between successive Tsys...
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Ссылки http://www.atnf.csiro.au/computing/software/miriad/doc/atfix.html -- 7.3 Кб -- 10.04.2016
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3. Wavelength Calibration at Moderately High Resolution
... The calibration of astrophysical spectra in wavelength based on calibration lamp data suffers from different kinds of uncertainties. Besides inaccuracies in the observational phase, common data reduction practice adds ``pixelation'' errors, due to the fact that the centering method does not use the correct PSF. These model mismatch errors depend, for a given feature, on the sub-pixel location of the line center (David & Verschueren, private communication). ...
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Ссылки http://www.adass.org/adass/proceedings/adass94/decuyperjp.html -- 12.1 Кб -- 03.11.2000
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4. Inference of Coefficients for Use in Phase Correction Bojan Nikolic web pages
... Bojan Nikolic web pages (r. 329) . ... We present a Bayesian approach to calculating the coefficients that convert the outputs of ALMA 183 GHz water-vapour radiometers into estimates of path fluctuations that can be used to correct the observed interferometric visibilities. ... Inference of Coefficients for Use in Phase Correction . ... Simulating Atmospheric Phase Errors, Phase Correction and the Impact on ALMA Science . ... Copyright 2005 -- 2016, Bojan Nikolic feedback welcome ...
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Ссылки http://www.mrao.cam.ac.uk/~bn204/alma/memo-infer.html -- 14.9 Кб -- 04.04.2016
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5. Radio patrol survey by Gregory and Taylor
... 371Gregory Taylor . ... We persent a catalog of 1274 discrete sources detected during a 5 yr, 6 cm, radio-patrol survey of the galactic plane for variavle sources. ... Seventy-five percent of the sources are weaker than 75 mJy, and as a consequence reliable sources and 27 possible variables were detected, of which 64 % exhibited shirt-term variability. ... A comparison with previous centimeter variability studies suggests the possible existence of two distinnct variability components. ...
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Ссылки http://www.sao.ru/cats/doc/GT_patrol.html -- 7.9 Кб -- 18.03.2015
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6. http://scan.sai.msu.ru/lk/
Please enter the lightcurve file name and period search parameters: . Lightcurve file: . ... Apply the Heliocentric correction and convert all dates to Terrestrial Time (TT)? ... Also, the Heliocentric correction cannot be applied to such lightcurves. ... This period search service is also available at the mirror sites: Mirror 1 , Mirror 2 , Mirror 3 , Mirror 4 . You may download the latest source code distribution and install the period search service at your own web server. ...
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7. SN 1989B Light Curve Analysis.
SN 1989B Light Curve Analysis. ... In the light curve depicting their observations, definite trends are noted, here is a "thumb-nail" analysis of the the magnitude estimations of the bright SN (1989B) in the galaxy NGC 3627 (M66). ... The observations were inserted against the V magnitude templete of BL, CCD photometric data, (Wells et. al, (1994) and a color trend (B-V) histogram of the mean type Ia SN (BL)(nutemp.gif). Key Words: Amateur Observations, Supernova, Magnitude Estimates, 1989B . ...
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Ссылки http://www.sai.msu.su/mirrors/isn/analysis.htm -- 5.1 Кб -- 02.02.2012
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8. FOS Closeout Calibration:
An updated set of AIS sensitivity reference files and tables has been delivered. The new calibration derives from the FOS Closeout Calibration analysis. POST-COSTAR: The new files incorporate the results of standard star observations taken over the entire post-COSTAR period (as opposed to the 1994-95 period covered in the previous calibration set). ... The accompanying table lists the best set of FOS sensitivity files and tables. ... STScI Home Page -|- ... Top FOS Page . ...
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Ссылки http://www.stsci.edu/ftp/instrument_news/FOS/closeout_sens.htm -- 3.5 Кб -- 12.05.2000
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9. ASP: Astronomical Society of the Pacific Presents Pricilla and Bart Bok Awards
... The Astronomical Society of the Pacific (ASP), in partnership with the American Astronomical Society (AAS), presented the annual Priscilla and Bart Bok Awards to two high-school students at the Intel International Science and Engineering Fair held May 8 to 13 in Los Angeles, California. ... The Priscilla and Bart Bok Awards are given jointly by the ASP and the AAS. ... Upon his death in 1983, the ASP established the Bart Bok Memorial Fund to support educational projects. ...
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Ссылки http://www.astrosociety.org/news/2011bok.html -- 8.1 Кб -- 02.10.2012
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10. ESO - How good is HAWKI astrometry and how are PSF variations corrected?
... Science . ... Science Users Information > Data Handling and Products > Data Reduction FAQ > How good is HAWKI astrometry and how are PSF variations corrected? ... Science Users Information . Observing Facilities . ... Paranal Facilities . La Silla Facilities . ... Future Facilities and Development . ... Observing with ESO Telescopes . ... Science Software . ... Science Data Products Forum . ... Science Archive Facility . ... ESO Data . ... ESO Data Access Policy . ... ESO Science Newsletter . ...
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Ссылки http://www.eso.org/sci/data-processing/faq/how-good-is-hawki-astrometry-and-how-are-psf-variations-corrected.html -- 22.5 Кб -- 10.04.2016
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11. COMPLEX DATA ANALYSIS
Proceedings of Turbulent Shear Flows XI , 1997. NASA Technical Paper # 3555 , 1997. Proceedings of European Turbulence Conference VI , 1996. ESPRI Research Report # 104, 117-143 (1996) . ... Proceedings of Turbulent Shear Flows X , 1995. ASME Paper 95-GT-437 , 1995. ... Invited AIAA Paper 94-2281 presented at the 1994 AIAA Fluid Dynamics Conference, Colorado Springs, CO. AIAA Paper 94-2323, presented at the 1994 AIAA Fluid Dynamics Conference, Colorado Springs, CO. ...
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Ссылки http://crydee.sai.msu.ru/~vab/Wavelet.rsc/Tutor.dir/data.html -- 4.8 Кб -- 12.04.1998
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12. http://hea-www.harvard.edu/~pgreen/refresponse.txt
REFEREE REPORT: %% %% %% As made clear by the title of the paper and the observational %% evidence presented, the authors believe that the correct %% identification of HS1216+5032 is as a physical quasar pair, albeit %% with one component showing the rather unusual combination of %% BAL troughs and significant radio luminosity. ... Removed most of the discussion of dark lenses and cosmology, and deleted the section on BALQSOs. ... The paper now totals 5.5 pages, down from 10. ...
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Ссылки http://hea-www.harvard.edu/~pgreen/refresponse.txt -- 7.1 Кб -- 14.12.2003
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13. http://www.naic.edu/~phil/usrproj/a1552/a1552.html
... When the strip that contained the galaxy was bandpass corrected, a negative image of the galaxy was present for the entire strip. ... If a continuum source drifted through the beam during this time, the cal deflection would be contaminated. ... The continuum source peaks at strip sample 67. ... You could take more samples (a longer strip) or remove the continuum sources before computing the bandpass correction. ... Top image. ... The bandpass correction does not contain any of the continuum source. ...
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Ссылки http://www.naic.edu/~phil/usrproj/a1552/a1552.html -- 7.2 Кб -- 22.11.2004
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14. Untitled Document
... Unsafe act - a behavioral departure from an accepted, normal, or correct procedure or practice which, in the past, has produced injury or property damage or which has potential for doing so in the future; an unnecessary exposure to a hazard; conduct reducing the degree or safety normally present in an activity. ... Any hazardous unsafe condition, or act that presents a situation of imminent danger to life and/or property requires urgent action. ...
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Ссылки http://www.apo.nmsu.edu/Site/usersguide/SafetyPlan/06SafeSec3.html -- 4.9 Кб -- 20.05.2009
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15. SN1989B in M66
... In the light curve depicting their observations, definite trends are noted, here is a "thumb-nail" analysis of the the magnitude estimations of the bright SN (1989B) in the galaxy NGC 3627 (M66). ... 10 (IAUC # 4742) 2/25 13.3 16 j 2/27 13.5(*) 18 lc 2/28 13.8 19 p 3/1 13.2 20 w 3/2 13.5 21 a 3/4 13.8 23 p 3/6 13.3 25 c 3/7 13.3 26 c 3/8 14.1 27 m 3/8 13.3 27 r 3/9 13.4 28 c 3/9 14.1 28 m 3/10 13.6 29 j 3/10 14.0 29 a 3/11 13.6 30 c 3/11 13.5 30 r 3/11 13.7 30 s 3/13 [13.69 CCD Mag.] ...
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Ссылки http://www.sai.msu.su/mirrors/isn/snimages/sn1989b.html -- 9.7 Кб -- 22.12.2007
[ Сохраненная копия ] Ссылки http://www.rochesterastronomy.org/SNIMAGES/sn1989b.html -- 9.7 Кб -- 10.04.2016
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16. ONE-DIMENSIONAL RADIO MESSAGE FOR "BLIND" ALIENS
Arecibo Proposal No. ... And I guess the primary one-dimensional message is more understandable by unfamiliar aliens and the music is the most universal expression of intellectual activity by means of one-channel ear-like radio link. ... So, I suggest to implement the 1st Theremin Concert for Aliens from Arecibo or Evpatoria Radar facility. ... There were four Messages from Earth to proposed aliens -- two material (Pioneer Plaque and Voyager Record) and two ethereal (Arecibo-1974 and Evpatoria-1999). ...
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Ссылки http://www.cplire.ru/html/ra&sr/irm/1-D-rm.html -- 12.2 Кб -- 30.11.2002
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17. SWXCS
... Catalog . ... The catalog of clusters of galaxies presented in Tundo et al. 2012 , detected from the GRB follow-up fields of XRT archive, containing 72 galaxy clusters with soft net counts > 100. View the catalog and images . ... The tables presented in Tozzi et al. 2013 in preparation . View the redshift information of catalog I . View the X-ray spectra information of catalog I . ROSAT 400d . ROSAT MACS . ROSAT WARPS . ROSAT REFLEX . ... XMM XCS . XMM LSS . ...
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Ссылки http://www.arcetri.astro.it/SWXCS/Catalog.html -- 5.0 Кб -- 20.05.2014
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18. http://www.gao.spb.ru/english/personal/malkin/publ/zm10c.pdf
Central Astronomical Observatory at Pulkovo of Russian Academy of Sciences PUL Analysis Center Pulkovo IVS Analysis Center (PUL) 2009 Annual Rep ort Zinovy Malkin, Natalia Miller, Elena Popova Abstract This report briefly presents the PUL IVS Analysis Center activities during 2009 and plans for the coming year. The main topics of the investigations of PUL staff in that period were ICRF related studies, computation and analysis of EOP series, and VLBI2010 related issues. ...
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Ссылки http://www.gao.spb.ru/english/personal/malkin/publ/zm10c.pdf -- 66.6 Кб -- 08.11.2010
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19. GRB follow-up team
... Team . ... The main goal of observations of GRB host galaxies is accumulation of statistics of their spectroscopic and photometric properties. ... The Hubble diagram for 22 GRB host galaxies with known magnitudes and redshifts (GRB 970228, GRB 970508, GRB 970828, GRB 971214, GRB 980613, GRB 980703, GRB 990123, GRB 990510, GRB 990712, GRB 9912008, GRB 991216, GRB 000131, GRB 000210, GRB 000301C, GRB 000418, GRB 000911, GRB 000926, GRB 001109, GRB 010222, GRB 010921, GRB 011121 and GRB011211). ... 600...
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Ссылки http://mavr.sao.ru/hq/grb/host-obs.html -- 15.6 Кб -- 09.04.2016
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20. http://www.sai.msu.su/gcvs/gcvs/nl75/readme
THE 75th NAME-LIST OF VARIABLE STARS. ... The 75th Name-List consists of two tables. ... the literature, taken from positional catalogues, including USNO A1.0/A2.0 and GSC, or determined by the authors); the range of variability (sometimes the column Min gives, in parentheses, the amplitude of light variation; the symbol ( means that the star , in minimum light, becomes fainter, than the magnitude indicated); and the system of magnitudes used ( P are photographic ...
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Ссылки http://www.sai.msu.su/gcvs/gcvs/nl75/readme -- 7.8 Кб -- 19.04.2000
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