Next: About this document Up: FOC Image Restoration Using Previous: Mathematical Methodology . ... Use of a mask was required to ensure that the saturated data were ignored in the resultant restoration which these authors obtained with an observed PSF. ... Hollis and colleagues obtained two public domain FOC F/96 images of the binary system R Aquarii and an observed PSF both in the light of twice ionized oxygen which emits a spectral line at 5007 ?. ... These images are not identical in details, . ...

... As the SN activity in the first generation stellar population must be small at present, the net SN rate in the vicinity of the Sun is approximately proportional to the local density of stars of second generation (or to the star formation rate, which is the same), especially for SN II and SN Ib. If a -like star formation of the first generation stars took place, a hump on the observed - showing the relative fraction of the first generation stars should be observed. ...

... Up: Science Data Pipelines . ... We designed and developed a package which simulates extragalactic point source data within a given field of view and SIRTF band. ... The simulator is modular and extensible to enable multi-wavelength simulations, has been optimized by utilizing parallel processing capabilities, and will be used to test pipeline software. ... The extragalactic simulator is capable of generating large numbers of galaxies within a given patch of sky for SIRTF pipeline testing. ...

... ATNF Home . About ATNF . ... About ATNF overview . News | ... Governance overview . Australia Telescope Steering Committee . ... Australia Telescope User Committee . ... Our people overview . ... Publications overview . ... Parkes radio telescope . ... Australia Telescope 20GHz Survey . ... Visiting Parkes radio telescope . ... Parkes radio telescope webcam . ... This is a first announcement of the workshop entitled "RFI and its impact on the new generation of HI spectral-line surveys". ...

Astronomy Discussion Forums . Forums: . ... Dr. Dick Is Annoying....and Every Generation Is Annoyed In Turn . ... Post Message | ... answers to the post at http://www.astronomy.net/forums/exploration/messages/168.shtml . ... Sorry, I don't intend to be annoying! - doctordick - November 27, 2002 - 19:51 UTC . ... www.astronomy.net . About Astronomy Net | ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

... 10:00-11:00 б  . ... Mikhail Gelfand, Institute for information transmission problems б  RAS, Moscow . 11:00-11:30 discussion+break . ... slides) . ... Global Sequencing: new high-throughput sequencing technologies, hudge bioinformatic challenges . ... Next-generation sequencing technology: new sequencing platforms, new frontiers, new algorithms . ... 13:45-14:00 discussion . ... Center for theoretical problems of physico-chemical pharmacology RAS, Lomonosov Moscow State University, Physics Dept., ...

... In Figures 2 and 3 we show the 6m telescope spectra of blue compact galaxies HS 1013+3809 and HS 1442+4250, in which typical high excitation HII-region narrow emission lines are seen. ... for red part of HS 1442+4250. ... This correction = 354 km s -1 was calculated for HS 1013+3809 and = 202 km s -1 for HS 1442+4250. ... While HS 1013+3809 looks very symmetric and very compact, with intense star formation burst taking place in its very center, HS 1442+4250 is well elongated, resembling edge-on disk...

... Get energy ranges for matrix from the CAL . Write these data out to matrix table in output file . ... Obtain response data from CAL using the corresponding row value for elow and ehigh as arguments . Perform instrumental corrections. ... If necessary, pad out or truncate response row according to the values of TLMIN and TLMAX of the CHANNEL column. If necessary, resample response row according using attributes SPECPIX , SPECVAL and SPECDELT of the spectral file. ...

... Astrophysics Group . ... Meetings . Past meetings . THE@INT Science Discussion Meeting: 6th October 2014, RAS, London . ... We will be holding an afternoon (2pm start) meeting on 6th€аOctober 2014€аto present and discuss the prospects of a new high resolution spectrograph installed on the Isaac Newton Telescope.€а This meeting is in light of the recent call for new instrument ideas ( http://www.ing.iac.es/about-ING/int2014.html ) put forward by the ING group in La Palma. ...

... gradients dependencies on solar wind parameters and IMF; . ... fate of thermal plasma at the dayside magnetopause. velocity-dispersed injections of the thermal and superthermal ions from LLBL at cusp and cleft (lowest energy VDIS-2 events); . ... outer cusp processes, role of outer cusp indentation, plasma entry (laminar reconnection, turbulent diffusion, others), role of turbulent boundary layer; . how is the magnetosheath plasma heated near magnetopause and cusp? . ... cusp/cleft wave emissions. ...

... See also the NAIC spectrum management page. Note that the full ALFA band covers 1225 to 1525 MHz. ... An example was shown of the OH spectrum of an OH/IR star obtained with 3-level sampling usin