... TPSTA is an array of up to 30 station names. One can be 'DEFAULT' which means that the corresponding parameters will be used for stations not explicitly in the list. A station VLBA will match any VLBA stations that are not specified explicitly. Actually it matches any stations with the first four characters ``VLBA''. A station VLA matches any station with the first 3 characters ``VLA'' that is not otherwise specified explicitly. ... Options: Any station name. ...

Next: Calling Parameters Up: CALgetPSFmap Previous: CALgetPSFmap Contents . ... Accuracy Level . ... the PSF is constructed using a single bi-dimensional Gaussian fit involving energy dependent parameters which are tabulated in the CCF. This mode is a fastest way to compute the PSF but with a very limited accuracy. ... The analytical expression use to describe the PSF in the low accuracy mode is as follows. where y and z are expressed in pixels units. is the pixel size expressed in mm. ...

... Observational Zoo of Binaries with Compact Stars . Evolutionary Scenarios of Binary Systems . ... Evolution of Magnetic Rotators . ... Mixing types of E-P-A binary systems with non-zero orbital . ... Binary Pulsar Diversity and High Neutron Star Birth Velocity . ... Ejectors in Massive Binary Systems . ... Other Candidates for Ejecting Stars in Binary Systems . ... Cosmic Rays and Evolution of Binary . ... Sky in Gravitational Waves . ... Gravitational Waves from Coalescing Compact Binary Stars . ...

... SGML . The text/html content type . In this section, we begin the specification of HTML 4.0, starting with the contract between authors, documents, users, and user agents. ... These recommendations are not normative and conformance with this specification does not depend on their realization. ... An HTML document is an SGML document that meets the constraints of this specification. ... A user is a person who interacts with a user agent to view, hear, or otherwise use a rendered HTML document. ...

Next: Running CONSTRICTOR Up: How to use CONSTRICTOR Previous: Parameters Contents . ... OutputBeam.BiasMod(07:12) = 1, 7, 10, 8, 3, 5 OutputBeam.StationID(01:04) = 1, 3, 4, 6 OutputBeam.StationID(05:08) = 1, 2, 4, 5 OutputBeam.Wavelength (01:04) = 849.4e-9, 820.9e-9, 793.9e-9, 768.3e-9 OutputBeam.Wavelength (05:08) = 744.2e-9, 722.9e-9, 701.5e-9, 683.1e-9 OutputBeam.Wavelength (09:12) = 664.6e-9, 648.9e-9, 617.7e-9, 603.5e-9 OutputBeam.Wavelength (13:16) = 590.7e-9, 577.9e-9, 566.5e-9, 556.6e-9 ...

... 2.1 What is Dithering? ... 2.4.1 No Dithering . ... 2.4.4 Dithering for Parallel Images . 2.5 More Detailed Considerations . 2.5.1 Data Quality Issues involved in Dithering . ... 2.5.4 How many Images to Obtain at each Dither Location . ... 3.2.3 Drizzle . ... 3.4 Image Fidelity After Drizzling . ... 4.2.1 Introduction . ... 5.3.2 Parameters . 5.3.3 Basic Examples . ... 5.4.8.1 General Explanation . 5.4.8.2 Parameter Details . ... 5.5 Optimizing the Drizzle Parameters for Your Data . ...

... В четверг, 14 апреля 2016 г., состоится семинар кафедры астрофизики. Повестка дня . ... Начало в 11 час.15 мин. Ауд. ... В четверг, 31 марта 2016 г., состоится семинар кафедры астрофизики . ... В четверг, 24 марта 2016 г. , состоится семинар кафедры. ... В четверг, 17 марта 2016 г. , состоится заседание кафедры. ... ОСП НИИ ПММ Национального исследовательского Томского государственного университета) . ... Copyright 2016 Астрономия в Санкт-Петербургском университете . ...

... The various Inst :Focus scripts allow you to take a series of exposures over a range of secondary mirror focus values, report the resulting FWHMs and optionally adjust the focus to the estimated best value. ... Slitviewer scripts assume the focus star is on the boresight. ... Focus scripts runs in three phases: . ... The script moves the boresight so the focus star is visible next to the slit, sets the focus to Center Focus, takes an exposure and tries to measure the star's FWHM. ...