... Torgashina, Gert de Lange, Leo de Jongb, Pavel A Yagoubovb a The Kotel'nikov Institute of Radio Engineering and Electronics, Moscow, Russia b SRON Netherlands Institute for Space Research, Groningen, the Netherlands Abstract--A Superconducting Integrated Receiver (SIR) developed for balloon borne instrument TELIS covers frequency range 450-650 GHz. The DSB noise temperature was measured as low as 120 K. The SIR application for high resolution spectroscopy of breathed out air has been proven. ...

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• http://www.cplire.ru/html/lab234/pubs/2009-12a.pdf
• http://www.cplire.ru/html/lab234/pubs/2008_16.pdf
• http://www.cplire.ru/html/lab234/pubs/2013_18.pdf

... It was then mounted on the telescope and the cal values were measured using absorber and sky (see measuring the cals on the telescope using absorber and sky for a description). ... Blue: the cal value computed using the absorber and sky (y factor). ... Blue: a 3rd order polynomial fit to the absorber (red) and ratio (blue) cal values versus frequency (the green sky only cal values were not used). ... The 3rd order polynomial fit versus frequency only used the absorber and absorber/sky ratio values. ...

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• Arecibo Observatory 610/700-MHz Band Receiver
• Arecibo Observatory 430-MHz Gregorian Receiver
• ALFA Receiver Temperature Polynomial Fit

The Parkes 21cm Multibeam Receiver is a new facility available on the Parkes Telescope which is operated by the Australia Telescope National Facility (ATNF), CSIRO. The facility consists of a 13-beam cooled 21cm receiver system, located at the prime focus of the 64m dish. ... Completed 21cm Multibeam Receiver being hoisted up to the Parkes focus cabin. ... It is now available, in 64 MHz mode and in pulsar mode, for normal National Facility use. ... Beam 1 . Beams 2-7 . ... Frequency Range . ...

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• Australia Telescope National Facility
• ASKAP Receivers
• mmATCA Receiver Package

In the PROJECT we are using the following peculiar . features of RATAN-600 . ... Brightness temperature sensitivity being equal to the antenna temperature sensitivity .. ... Receiver system .. ... Using aperture averaging effect. dual- beam and dual (multi-) frequency filtration, we demonstrated full filtration of the atmosphere noise down to the receiver noise at all scales of acoustics peaks ( Fig.1 , Fig 2 ). ... We select this frequency as the central one in our project. ... Antenna surface . ...

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• Feed cabin 2
• di_eks

... Flight 1) 2) 3) Flight 1) 2) 3) model FM1 has the following parts: LNA MY-18, serial number PN 01-0252, factory number FM1; receiver box KRT-18, serial number PN 17660-01, factory number FM-001; DC-DC converters IVEP1 and IVEP2, factory number 05. model FM2 has the following parts: LNA MY-18, serial number PN 01-0252, factory number FM2; Receiver box KRT-18 serial number PN 17660-01, factory number FM-002; DC-DC converters IVEP1 and IVEP2 factory number 06. ... See Appendix 1. ... 2003. ... 2004 . ...

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• http://www.asc.rssi.ru/RadioAstron/archives/RAMN/2005/oct.pdf
• http://www.asc.rssi.ru/RadioAstron/documents/receivers/eng/92cm_eng.pdf
• http://www.asc.rssi.ru/RadioAstron/meetings/telecon/dec13_2011.pdf

... Luminosity (L) Ї Ї Ї Ї A source's luminosity is the power that it emits in radiation. ... NB Astronomers often say `flux' when they mean `flux density' Ї SI units are Wm-2Hz -1 -26 filter Ї Also used are Jy 10 Wm-2Hz -1 E= РРРF d dA dt Specific Intensity, Surface Brightness (I) Ї Specific intensity (or surface brightness) is the power received (or emitted) per unit area per unit frequency per unit solid angle. ч F at surface of a spherical source = I Ї Ї Specific intensity is independent of distance...

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• OptInt PmWiki : MROIFastTipTilt / Tech Meet 12
• A possible turn-over in pulsar spectra at mm-wavelengths?
• Astrophysics Group VSA

Next: Introduction . ... We present the results of spectrophotometry of two Blue Compact Galaxies (BCG) known from earlier studies as very metal-poor objects. ... UM 382, according to our data, is significantly more metal-rich: its 12+log(O/H) = 7.76 0.07 in comparison to the cited earlier value 7.45. ... Thus the latter two galaxies should NOT be considered as extremely metal-poor BCGs. galaxies: abundances - galaxies: photometry - galaxies: individual (UM 133, UM 283, UM 382) . Introduction . ...

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• Up-date RC-sources Spectra
• HyperLEDA documentation: parameter: vdis
• What was the measurement?

... SMIS ] . noise temperature of the low noise amplifier less than 100 K . automatic frequency and polarization adjustment of the received signal . double transform of frequency . power supply: single phase, 220 V, 50 Hz . power consumption: less than 30 Wt . the unit measures: 470 x 300 x 130 mm . weight: less than 10 kg . ... Back to SMIS Home Page . ...

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Peremennye Zvezdy ( Variable Stars ) 35 , No. ... We present the results of our new observations of QS Draconis, a recently discovered double-mode high-amplitude Scuti variable, HADS(B) type. ... Our CCD observations in the Johnson bands were performed at the Tien Shan Astronomical Observatory of the V.G. Fesenkov Astrophysical Institute, at the altitude of 2750 m above the sea level. ... The finding chart (Fig. 1) identifies the variable star, comparison star, and check star. ... Fig. ...

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... The following discussion presents Information on how to select and configure the device drivers in a running Unix system. ... Click on a selected type for specific description and configuration documentation, including the clock address, reference ID, driver ID, serial port device name and speed, and features (line disciplines, etc.) ... Type 1 Local Clock Driver ( LOCAL_CLOCK ) . Type 2 Trak 8820 GPS Receiver ( TRAK ) . ... Type 5 TrueTime GPS/GOES/OMEGA Receivers ( TRUETIME ) . ...

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• Heath WWV/WWVH Receiver
• Hewlett Packard 58503A GPS Receiver
• PSTI/Traconex 1020 WWV/WWVH Receiver

Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... Chirp ionosonde main technical characteristics . ... Linear frequency modulated continuous signals sounding method is relatively simple and has wide application in various special-purpose systems. ... Chirp signals which are applying for ionosphere channel diagnostics usually have10KHz/s -- 1MHz/s. We must point out that under modulation speed increasing there is an increase in noise suppression and resolution power. ...

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• East Siberian Center for the Earth's Ionosphere Research. Incoherent Scatter
• East Siberian Center of Earth Ionosphere Research. IS radar Receivers Hall.
• East Siberian Center for the Earth's Ionosphere Research. Specific character

... In the following table we list only the best results for each GPU: GPU b oard ATI 7950 3GB ATI 6950 1GB ATI 7770 1GB CPU Intel Core i5-2400 AMD Athlon II X4 630 Intel CoreDuo Quad CPU Q6600 Driver version 12.6 11.6 12.6 B uffe r numbe 32K 32K 32K 32K 32K 32K lenght and r of buffers B в 512 B в 512 B в 256 B в 512 B в 128 B в 512 M a x S p eed MSample/s 225MS/s Double 370MS/s Single 200MS/s Double 310MS/s Single 60MS/s Double 160MS/s Single Figure 1: SpectralGpu Logo Version 1.0, November 2012. ...

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• Radioastronomy laboratory
• Arcetri designs innovative superconductor microwave filters for the Sardinia
• Fasti Web Site

... Robert L. Stewart (Brigadier General, USA, Ret.) ... SPECIAL HONORS: Awarded Army Distinguished Service Medal , Defense Superior Service Medal , 2 Legion of Merit, 4 Distinguished Flying Crossed, a Bronze Star, a Meritorious Service Medal , 33 Air Medals, the Army Commendation Medal with Oak Leaf Cluster and V Device, 2 Purple Hearts, the National Defense Service Medal , the Armed Forces Expeditionary Recipient of NASA Space Flight Medal (1984 & 1985). ...

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• Astronaut Bio: John E. Blaha (05/2008)
• Astronaut Bio: Steven L. Smith (12/2013)
• Astronaut Bio: Frank Borman

Due to technical issues, on September 11, 1998 the radiolink was switched to 465 MHz channel. Data acquisition is presently performed only by SRC "PLANETA", Data Receiving Center in Obninsk and Western Siberia Data Receiving Center in Nobosibirsk . For conditions of obtaining data from RESURS-01 N3 please contact SRC "PLANETA". ... Registration of full data stream (61.44 Mbit/s) is performed only by Data Receiving Center, SRC "PLANETA", Obninsk. ...

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Stellarium 0.12.3 . ... Classes . ... Class List . ... TuiNodeColor Class Reference . ... void  . ... TuiNodeColor (const QString &text, QObject *receiver, const char *method, Vec3f defValue, TuiNode *parent=NULL, TuiNode *prev=NULL) . ... virtual TuiNodeResponse   . ... TuiNodeEditable (const QString &text, TuiNode *parent=NULL, TuiNode *prev=NULL) . ... TuiNode (const QString &text, TuiNode *parent=NULL, TuiNode *prev=NULL) . ... virtual TuiNode *  . ... virtual void  . ... parent = NULL , . ...

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National Space Agency of Ukraine and . ... The Second International Meeting on WARNING Mission . ... Space Research Institute of Ukrainian National Academy of Sciences - National Space Agency, . ... The Head of Scientific committee of the Project ?Warning? is DR V.G.Bar`yahtar, Academitian of Ukrainian National Academy of Sciences. ... Lviv Center Space Research Institute of Ukrainian National Academy of Sciences, . ... National Space Agency of Ukraine, Bozhenka St. 11, 252022 Kyiv-22, Ukraine. ...

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• TOPSIDE AUTOMATED SOUNDER TOPAS/W
• INFRARED FOURIER-SPECTROMETER SICH-F

STScI . ... Data . ... Calibration . ... The drizzle software requires only the distortion correction files indicated in your image headers (keywords IDCTAB and OFFTAB), which can also be downloaded individually from the STScI uref directory. ... Output files : set build=no to generate separate files for science image (drz_sci.fits) and exposure weight map (drz_weight.fits). ... Intermediate files : set clean=no to keep the intermediate files that are helpful while verifying your output and iterating. ...

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• STScI Preprint #1280
• Baltimore-Washington Starburst Series
• WFC3 Data Handbook

... A. M. Neminsky, P. N. Nikolaev, and D. V. Shovkun . ... The temperature dependence of the magnetic field penetration depth lambda ( T ) is determined down to 0.2 T c by the ac-susceptibility measurements on the Rb 3 C 60 fine powder with small, about 1 K, variation in the grains' superconducting transition temperatures. The lambda ( T ) temperature dependence is exponential at low temperatures, which allows us to determine the energy gap Delta 0 =1.7 k B T c . ...

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• X International Astronomy Olympiad
• International Astronomy Olympiad: Personal data questionnaire
• IX International Astronomy Olympiad: Personal data questionnaire

... We present the algorithm and implementation details for the robust, realtime bandpass removal and calibration routine developed for the HI Parkes All Sky Survey project. ... Traditionally, the bandpass that is present in single-dish 21 cm spectra is removed by observing in a ``signal-reference'' mode. ... The robust bandpass removal algorithm implemented for the HIPASS Project successfully produces calibrated HI emission line spectra for most of the survey data. ...

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• Interactive Fitting of EUVE Emission Line Spectra
• Modelling Spectro-photometric Characteristics of Eclipsing Binaries
• ADASS 2003 Conference Proceedings

Since the light from galaxies represents the integrated contribution of its consitutient stars, then we can learn about stellar populations in galaxies by modelling their light by summing up individual stellar spectra for different kinds of stars. ... The data cover the wavelength range 3500 - 9000 angstroms. ... Retrieve Digital Stellar Spectra Click on the appropriate spectral type. ... Note that the designation V means main sequence, IV means subgiants, III means giants, I means supergiant. ...

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