Next: Optimization of spectroscopic observations Up: On the problem of Previous: On the problem of . In comparison with spectroscopy of extended extragalactic objects, the task of observing stars with a high spectral resolution is traditionally given lower priority. ... A ``natural'' response of some researchers of stars and starlike objects is preferential use of low and moderate spectral resolution techniques, where one succeeds in minimizing losses at the spectrograph input. ...

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• Optimization of spectroscopic observations
• On the problem of high spectral resolution observations of faint objects

Space Telescope Science Institute . ACS Instrument Handbook Cycle 19 . ... Advanced Camera for Surveys Instrument Handbook for Cycle 19 . ... 2.1 SM4 Repair of ACS . 2.2 Comparison of ACS/WFC and WFC3/UVIS . 2.3 Comparison of ACS/HRC and WFC3/UVIS . ... 4.4 The SBC MAMA . ... Chapter 5: Imaging . ... 5.2 Important Considerations for ACS Imaging . ... 5.5 Ultraviolet Imaging with the SBC . ... 5.5.3 SBC Imaging Filter Shifts . ... 9.6.1 Example 1: WFC Imaging a Faint Point Source . ...

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• Image and Spectrum Recovery
• ACS Instrument Handbook for Cycle 20
• ACS Instrument Handbook

... Дни открытых дверей к юбилею САО РАН (12-14 апреля 2016 г.) . Международная конференция "Dark Ages and White Nights (Spectroscopy of the CMB)" (20-24 июня 2016 г.) . ... Международная конференция MULTI-SPIN GALAXIES - 2016 (26-30 сентября 2016 г.) . Международная астрономическая конференция "Физика звезд: от коллапса до коллапса" (3-7 октября 2016 г.) Архив . ... Подробнее.. ... 10.02.16 . ... БТА в реальном времени . ... Цейсс-1000 в реальном времени . ... Последнее обновление: 22/03/2016 ...

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• Solar system sector, archive 2011
• Hardware sector, archive 1997

... The most precisely determined characteristic for accreting neutron stars (NS's) is their period. ... Period changes show fluctuations. ... Some applications of stochastic processes in astrophysics especially in accreting systems were discussed in Lipunov (1987),Hoshino Takeshima (1993) and Lipunov (1992).In Hoshino Takeshima (1993) the authors, using simple models of MHD turbulence, try to explain aperiodic changes in X-ray luminosity of X-ray pulsars. ... Here, -constant angular momentum. ...

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• AXAF-Chandra

Next: Reduction of long-slit spectra Up: Long-slit spectroscopy Previous: Long-slit spectroscopy . ... pixel -1 and spectral resolution of about 12 ? ... We used the spectrograph ALFOSC equipped with a Loral (W11-3AC) CCD, with a 13 400 slit, and grisms #6 and #7 (110 ?/mm), which provide a spectral dispersion of 1.5 ? ... The seeing during the spectral observations was 08. Next: Reduction of long-slit spectra Up: Long-slit spectroscopy Previous: Long-slit spectroscopy Labaratory "Structure" . ...

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• Optical spectroscopy
• Calar Alto 2.2m observations
• Westerbork Northern Sky Survey

Next: Pulsar bin-mode observations Up: ATCA Bin Mode Observations Previous: ATCA Correlator Bin Modes . Miriad 's atlod task has an option, options=hires which converts a RPFITS file observed in high time resolution bin-mode into an apparently normal dataset with fine time resolution. ... In high resolution time mode, the time difference between consecutive integrations might be smaller than this tolerance. ... Miriad manager . ...

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• Research - The high-velocity clouds of M31
• Resolution of an interferometer
• immerge

Next: CCD Operation Up: Charge Coupled Devices (CCDs) Previous: Charge Coupled Devices (CCDs) . ... However it is only now that a number of important X-ray astronomical applications of CCDs have reached critical development stages, so that this is an appropriate time to review the application of space-borne CCD instruments to cosmic X-ray astronomy, and highlight the particular concerns which are being addressed for X-ray instruments, as distinct from optical applications. ...

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• Energy resolution
• Description

... Empirical and theoretical modeling of 3-D structures in the solar corona is confronted by the tremendous amount of data needed to represent phenomena with a large dynamic range both in size and magnitude, and with a rapid temporal evolution. Octree representation of the 3-D coronal electron distribution offers the right compromise between resolution and size, allowing computation of synthetic images of the solar corona. ... The time interval between images is one day. ...

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• Towards a General Definition for Spectroscopic Resolution
• ISIS: An Interactive Spectral Interpretation System for High Resolution X-Ray
• ETCs and Observations Simulation at the VLT

... We compare ray-traces of the HRMA response to "on-axis" observations of AR Lac and Capella as they move through their dither patterns to images produced from filtered event lists to characterize the effective intrinsic PSF of the HRC-I. A two-dimensional Gaussian, which is often used to represent the detector response, is NOT a good representation of the intrinsic PSF of the HRC-I; the actual PSF has a sharper peak and additional structure. ... Last modified: Tue May 18 14:35:55 EDT 2010 . ...

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• SAO RSDC Home Page - RRA - HRI
• Spectroscopic Data
• Direct Monitoring of Rotational Modulation

Solar High Resolution Studies . ... Solar Group . ... High quality observations obtained in recent years have highlighted the fact that the solar atmosphere is extremely dynamic, and wholly permeated and shaped by magnetic fields at very small spatial scales. ... The Solar Group in Arcetri is initiating a project to study some of the topics and techniques that will be brought to the forefront of solar physics as this new physical regime is explored. ... Small Scale Activity . ...

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• High-resolution Herschel spectroscopy reveals the proto-planetary disk around
• NICMOS3 Detector for Spectroscopy
• Comet Shoemaker-Levy 9

As in the last years, the Ephemerides of Minor Planets for 2015 are prepared by the IAA RAS only in the electronic form. ... Orbital elements of all numbered planets have been determined in IAA all over again on the ground of available observations in the catalog of the Minor Planet Center. ... More detailed information on orbital elements used in the present volume of EMP and their accuracy is given in section "Information on new orbital elements". ... a) information on new orbital elements; . ...

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• Values of asteroid masses

... ST-ECF, ESO, STScI and the NICMOS IDT organized a workshop on near infrared imaging from space and ground was held in Pula on May 26-27, 1998. ... The meeting was held in May 1998, about one year after science observations started with NICMOS, and about half a year before the Infrared Spectrometer and Array Camera (ISAAC) starts to operate on the VLT. Currently, it is expected that NICMOS will operate until the end of 1998. ...

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• NICMOS Observes the Galactic Center
• CONICA: The high resolution near-infrared camera for the ESO VLT
• Near IR Astronomy with the ESO VLT

Proposal Identification No.: A2004 Date Received: 2004 -Sep-30 12:45:57 Technical Page Proposal Type: General Category: Sub-Category: Observation Category: Total Time Requested: Prop osal Title: ABSTRACT: Commensal Astronomy Spectroscopy Galactic 28 Hours An Initial HI Survey of the Taurus Region We propose to carry out a high spectral resolution survey of a 60 square degree region of the Taurus Molecular Cloud. ... X Part of the observing run. ...

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• http://www.naic.edu/vscience/schedule/tpfiles/BlitztagA1340tp.ps
• http://www.naic.edu/vscience/schedule/tpfiles/MathewstagR1261tp.ps
• http://www.naic.edu/vscience/schedule/tpfiles/HoffmantagA1628tp.ps

... Galaxies 81 High resolution HCN and HNC spectroscopy in dark interstellar clouds A.V. Lapinov Institute of Applied Physics of the Russian Academy of Sciences, Nizhny Novgorod, Russia Introduction Dense cores in dark clouds are associated with regions of low mass star formation. ... The fact that in all observed by us starless dark clouds HCN F=2 1 and F=1 1 lines are self-reversed gives HCN molecule a good probe to search for collapsing cores in dark clouds. ...

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• http://www.gao.spb.ru/english/publ-s/viii-rfs/p011.pdf
• http://www.gao.spb.ru/english/as/j2014/presentations/vavilov.pdf
• VIII Russian-Finnish Symposium on Radioastronomy

Peremennye Zvezdy ( Variable Stars ) 33 , No. ... The new variable star HD 305629, with a Cepheid-like light curve, is demonstrated, from our optical observations and ASAS-3 data, to actually be an ellipsoidal variable star on a highly eccentric orbit. ... During a systematic search of variable stars in the publicly available ASAS-3 database (Pojmanski 2002), apparent variability was found in the star HD 305629 (10 51 34 35, -60 47 57 4, J2000.0; Fig. ... The light curve and color curves of HD 305629. ...

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• At the Limit of Diffraction
• XWare > APOD

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... This is the first in a series of papers in which we describe and report the analysis of a large survey of Herbig Ae/Be stars in circular spectropolarimetry. Using the ESPaDOnS and Narval high-resolution spectropolarimeters at the Canada-France-Hawaii and Bernard Lyot Telescopes, respectively, we have acquired 132 circularly-polarised spectra of 70 Herbig Ae/Be stars and Herbig candidates. ...

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• Introduction
• Refereed Journal Publications 2003
• C.J. Butler, Research Astronomer

Optical observations of comet P/Tempel 1 Heike Rauer, JЖrg Knollenberg, Michael Weiler DLR, Institut fЭr Planetenforschung Berlin-Adlershof Observations of comet P/Tempel 1 at optical wavelengths Before and after impact : monitoring · Gas production rates -,,classical optical long- slit spectroscopy: CN, C3, C2, NH2 - variation along heliocentric distance : difference before ­ after? - compare with measurements of parent species at radio, IR · ...

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• http://www.eso.org/sci/libraries/SPIE2010/7739-171_poster.pdf
• ESO - 8th VLTI Summer School: High angular resolution in astrophysics: optical
• High Resolution HST Images of Pluto and Charon (ESO Press Release 09/94)

... Comet Tutorial . ... On July 1, 1993 an image was taken with the Hubble Space Telescope (HST) that clearly shows at least 15 individual fragments in one image frame of the train. ... This made an accurate orbit (or orbits) difficult to determine; however, after numerous observations of the comet, astronmers determined that the comet had passed within 96,000 kilometers (60,000 miles) of the center of Jupiter or 25,000 kilometers (16,000 miles) from the cloud tops during the July 8, 1992, approach. ...

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• Current Solar Wind Conditions
• Sun-aligned arcs [Oulu]
• Dayside aurora [Oulu]

The close position of main satellite and subsatellite (distance between them about 1000 km) and using the similar sets of Faraday cups (VDP and VDP-S) with high resolution measurements (up to 16 Hz for the main satellite and up to 10 Hz for the subsatellite) allow us to determine the small-scale variations of the magnetopause shape and position and to estimate the velocity of the magnetopause motion. ... Two point observation of the magnetopause motion: the INTERBALL project. ...

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• Main research and development work completed in 2009 and ready for
• High resolution IR-spectrometer
• Instrumentation for Fundamental and Applied Space Projects

... Other Characteristics of the Sun: Variability of Rotation, Magnetism, Chemical Structure, Planetary System. ... Methods of Solar Magnetic Fields Measuring: Visual, Photografic, Photoelectric. ... Empiric Datas of Magnetic Fields in Photosphere, Chromosphere and Corona. ... Characteristics of Magnetic Field in Balanced Force Tubes by Potential and Forceless Field. ... Phenomenons in Active Region (Magnetic Field, Spots, Torches, Solar Prominences, Flares, Discharges. ... Magnetic Fields in Flares. ...

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• Practical Astrophysics
• Optical static Fourier spectrometer