Next: The main observational parameters Up: Spectral survey of Case Previous: CCD observations and data . ... We divided the presentation of the observed galaxies into the two main groups. In Tables 2 and 3 we give some general parameters, line intensities and equivalent widths for 142 galaxies with the detected emission lines. We summarize data in Table 4 for the rest 44 galaxies where we have not detected emission lines (in the blue part of the spectrum). ... Quasar CG 273 . ...

Еще в разделе: (Показать все результаты (>2423) - www.sao.ru/ )

• Results of follow-up spectroscopy
• Radio survey for new compact HII regions
• Radio patrol survey by Gregory and Taylor

... ATNF Home . About ATNF . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Australia Telescope User Committee . ... Astrophysics graduate student programs . ... Australian Square Kilometre Array Pathfinder . Murchison Radio-astronomy Observatory . ... Parkes radio telescope . Australia Telescope Compact Array . Mopra radio telescope . ... Visiting Parkes radio telescope . Visiting Australia Telescope Compact Array . ... Parkes radio telescope webcam . ...

Еще в разделе: (Показать все результаты (>33799) - www.atnf.csiro.au/ )

• Early Scientific Results
• Results
• Preliminary Survey Results

... To be read in conjunction with Section 4.11 of the WFPC2 Instrument Handbook , -Version 4.0. ... 1 The second study found evidence that CTE loss for faint stars has increased with time (Whitmore, 1998). The primary observational consequence of CTE loss is that a point source at the top of the chip appears to be fainter than if observed at the bottom of the chip, due to the loss of electrons as the star is read out down the chip (see Figure 1 ). ... Last updated: 06/16/98 10:38:00 . ...

Еще в разделе: (Показать все результаты (>21263) - www.stsci.edu/ )

• A New Database of Observed Spectral Energy Distributions of Nearby Starburst
• Future Calibrations, Calibration by Observers, and Calibration Outsourcing
• Results and Discussions

... For each observed position the table contains designation of object as in file of observations, the time of observation, the number and name/ preliminary designation of minor planet supposedly identical with observed object, the values of O – C (observed position minus computed one) in right ascension and declination expressed in arcsec, the difference O – C between observed magnitude and computed one, the code of observatory in the Observatory list (see Observatories section). ...

Еще в разделе: (Показать все результаты (>735) - www.ipa.nw.ru/ )

• LAB Ephem. Astronomy-ERA

SKA-3 instrument consists of two energy-angle ( EA ) electrostatic analyzers and two energy-mass ( EM ) time-of-flight analyzers. ... Here you can find more details about SKA-3 instrumentation set. ... Case 218 . ... satellite's trajectory in geomagnetic frame ( blue coloured), UFSIPS scan location and observation moment ( red coloured), interval of the SKA-3 observations ( green coloured) . ... a view of the Nothern polar region at the moment of UFSIPS observations, the scan location is red coloured. ...

Еще в разделе: (Показать все результаты (>1862) - www.cosmos.ru/ )

• IESP-2M Results Page
• HYPERBOLOID Results Page
• Main results of the experimental and theoretical research completed in 2010

Arecibo Galaxy Environment Survey (AGES) The M74 group is a gas-rich galaxy group located at roughly 10 Mpc and is similar in makeup to the Local Group. M74 dominates the surrounding region and is accompanied by several dwarf galaxies, some of which are star-forming. ... We have decided upon a drift mapping approach to scan the entire region. We have defined 5 constant declination scans 5 in length, separated by approximately one full ALFA footprint. ... START TIME (AST) . END TIME (AST) . ...

Еще в разделе: (Показать все результаты (>6120) - www.naic.edu/ )

• The NGC 2903 ALFA Survey
• Alfa_ang - IDL procedure for calculating the optimum rotation angle for ALFA
• Public data products

... Liyong Liu (NAOC) . Site testing on seeing conditions of the astronomical observatories over China are briefly reviewed, including Xionglong station of NAOC, Gaomeigu station of Yunnan Observatory, Delingha station of Purple Mountain Observatory. ... PDF [3.0€аMB] October 8, 09:55 10:20 . ... In this paper, we will review the site survey activities in the past years, and present the site-testing results on the Oma site, including cloud cover, seeing, water vapor, transparency and sky brightness. ...

Еще в разделе: (Показать все результаты (>31) - site2010.sai.msu.ru/ )

... I had also observed that comet in 1994, as it passed the halfway mark (January 1994): observation of the faintest solar system object ever observed. [at that time]. ... We observed it at the 2.2m at ESO in Mar.2001; here is a nice color image (and is also available in Italian , in Hebrew elsewhere.. ... The IfA Hale-Bopp page contains plenty of info and links about that comet; for nice pictures, check out the Images and Spectra page . ... Olivier R. Hainaut (ohainaut at eso.org) . ...

Еще в разделе: (Показать все результаты (>23551) - www.eso.org/ )

• VLTI Calibrator Selection Help Page
• ESO - Science Announcements
• Homepages of Christian A. Hummel

... A comparison of the computed and experimental relations F max ( H), as well as comparison of drift scans of point sources across different horizontal cross-sections of the BP with the corresponding computed cross-sections were made. ... The drift scans of the point source 3С84 (H=87 o ) at the wavelength 7.6 cm across the horizontal cross-sections of the BP (black lines) and the computed horizontal cross-sections of the BP corresponding to them (red lines). ...

Еще в разделе: (Показать все результаты (>1152) - jet.sao.ru/ )

• GRB follow-up team
• The spectrograph design and the observing procedure
• Principal scientific results

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... Many of the fields are spatially . ... These include a pulsating white dwarf which appears to have a hot companion, a number of stars with A-type spectra that vary on a period in the range 20 35 min. Our primary goal is the discovery of new AM CVn systems: we find 66 sources which appear to show periodic modulation on a time-scales less than 40 min and a colour consistent with the known AM CVn systems. ...

Еще в разделе: (Показать все результаты (>2795) - star.arm.ac.uk/ )

• Abstract
• Results & Discussion
• J.G. Doyle, Research Astronomer

... Actual stars are expected to be more complicated than these simulations. ... The spot may be entirely visible most of the time (one would observe a prolonged flux minimum low), and then part of it may disappear over the horizon briefly and then return (slow rise and then fall back to constant level). ... With the set of observations taken here, I have information available from several comparison stars and color information. ... The period found must be consistent with the data from any given night....

Еще в разделе: (Показать все результаты (>3773) - hea-www.harvard.edu/ )

• *counts_plot* - Inspection of Results
• ChaMPlane Bulge Windows Survey
• ChaMPlane

... Astrophysics Group . ... COAST . COAST Astronomical Results . ... Surface Imaging of Betelgeuse . ... This page highlights some astronomical results obtained with COAST over the years. These are listed in chronological order (most recent first). ... Measurements of cyclic variations in the angular diameter of Chi Cygni . ... The first infrared image from an aperture synthesis array . ... The images of Betelgeuse below were reconstructed from COAST data taken in early 2004. ...

Еще в разделе: (Показать все результаты (>2665) - www.mrao.cam.ac.uk/ )

• VLBI observations of the quasar 3C380
• CO in NGC 1530, aperture synthesis of a barred spiral
• Measurements of anisotropies in the Cosmic Microwave Background Radiation on

K-band Arcetri Obscured Supernova Search . What is the KAOSS Project? W hat is the KAOSS Project? Some recent surveys aimed at detecting Supernovae (SNe) in the optical have found that starburst galaxies do not show evidence for an enhanced SN rate, with respect to quiescent galaxies (Richmond et al. ... A similar result was obtained by Navasardyan et al. (2001) who looked for SNe in interacting galaxies, finding no evidence for correlations between SN rate and galaxy properties. ...

Еще в разделе: (Показать все результаты (>9550) - www.arcetri.astro.it/ )

• K-band Arcetri Obscured Supernova Search - Detected Supernovae
• IBIS - Flat Fielding
• CQTau disks (Abstract)

... SUZAKU RESULTS Furuzawa+09 SUZAKU RESULTS Furuzawa+09 No variation of centroid of Fe line Decreasing FWHM of the line with radius SUZAKU RESULTS Furuzawa+09 Consistent with shell spherical expansion Central high FWHM due to blue and redshifted lines SET OF XMM OBSERVATIONS 3 observations of Tycho SNR: Medium (30/12/07): 17-19-12 ks CALmedium (01/01/08): 46-36-33 ks CALclosed (03/0108): 26-26-22 ks SPECTRAL MODELING M2 PERSEUS M2 CALCLOSED M2 TYCHO NEW NRCO ON PERSEUS ? ...

Еще в разделе: (Показать все результаты (>11899) - xmm.vilspa.esa.es/ )

• XMM-Newton OM Response Files Page
• XMM-Newton Trainee Project 2004
• XMM-Newton Planned and Performed Observations

... Home Education Astro Answers Astro Answers ? The Big Bang, Inflation, and Latest Results from BICEP2 . ... Astro Answers . ... Observing Resources for Amateur Astronomers - Part 1: Beginning Observers . Observing Resources for Amateur Astronomers - Part 2: Intermediate Observers . ... A History of the First Forty Years of the Amateur Astronomers Association . ... Amateur Astronomers Medal . ... 2016 Amateur Astronomers Association of New York Designed by Press Customizr Powered by . ...

Еще в разделе: (Показать все результаты (>620) - www.aaa.org/ )

Next: NICMOS Coronagraphic Surveys-Preliminary Results Up: No Title Previous: STScI NICMOS Software . NICMOS Coronagraphic Surveys-Preliminary Results . ... Observations with NICMOS . ... The Evolution of Stars seen with ISOCAM - the Need for NICMOS and VLT Follow Up. ... Results . ... The Formation and Evolution of LMC Rich Star Clusters: NGC 1818 . ... HST-NICMOS Observations of Galactic Bulges: Red Nuclei in Nearby Galaxies . ... Investigating the Evolution of Quasar Host Galaxies with NICMOS . ...

Еще в разделе: (Показать все результаты (>262) - www.stecf.org/ )

• NICMOS Observes the Galactic Center
• NICMOS/HST H-band (F160W) Images of the 30 Dor Starburst Cluster
• The Structure and Composition of High Redshift Radio Galaxies

... Fitting the observed dependence includes calculations of the polarization cross-sections averaged over particles orientation and size distribution, their normalization and the comparison of obtained dependencies with Serkowski's curve representing observational data for a chosen star. ... Variations of the polarization factors with wavelength are shown in Fig. 16 for homogeneous spheroidal particles with PF orientation. ... The distinction between prolate and oblate spheroids is also clearly seen. ...

Еще в разделе: (Показать все результаты (>346) - www.astro.spbu.ru/ )

• Wavelength dependence
• Query Results from Astronomy Database
• A Nature of Polar-Ring Candidate Galaxy ZGC 2315+03

The 14 th International Astronomy Olympiad has been held successfully in Hangzhou (China) on November 8-16, 2009. ... There were 17 teams participated and 1 team observed in the XIV IAO: . ... Sunday, November 8 - Day of arrival . ... Thursday, November 12 - Day of excursions . ... M. G. Gavrilov (IAO Chairman) - Chairman, . J. Zhu (Beijing, XIV IAO-2009 and X IAO-2005 LOC Chairman), . ... Dr. Michael G. Gavrilov, Founding Chairman and Coordinator of the International Astronomy Olympiad (IAO) . ...

Еще в разделе: (Показать все результаты (>1083) - www.issp.ac.ru/ )

... The results are used in quasireal time by the observing process, but also as input by hardware quality control, by the dynamical scheduler, and by the Science Pipeline. Among processing operations are the calibration of the atmospheric absorption, of phase radiometric correction, of pointing scans, of phase and amplitude reference measurements, .. ... Using the last few measurements, we will determine a provisional amplitude calibration curve (to be also used by the Quick Look pipeline). ...

Еще в разделе: (Показать все результаты (>1837) - www.adass.org/ )

• What Happened to the Results?
• SDImager: An Imaging Tool for Single Dish Observations in AIPS++
• ETCs and Observations Simulation at the VLT

SOME RESULTS FROM INTMINS . The experiment can be performed when the electron beam (instrument ISTOCHNIK ) and plasma blobs (instrument ARIEL ) are injected approximately along or perpendicular to the Earth's magnetic field. ... The pulses of frequency of 1000 Hz will generate EM waves and its harmonics. ... To increase the electron gun pulse duration up to D t = 0.5 f -1 ( D t = 5x10 -4 s) and to stabilise their frequency as good as possible. ... Back to the INTMINS Main Page ...

Еще в разделе: (Показать все результаты (>1124) - www.iki.rssi.ru/ )

• Discovery of the Sunspot Cycle
• Pi 2 [Oulu]
• Field-aligned potential drops [Oulu]