The netgear prosafe gs110tp is a network switch with: . ... Luis measured the emissions of the netgear prosafe gs110tp switch in the screen room on 06sep12. ... 100 MHz span, 12.5 Khz/rbw. covering 0 to 3000 MHz in 30 spectra . ... The strongest birdie is around 800 MHz at -78dbm . ... The emissions from the switch are much stronger that the power supply . ... 20.836 MHz . ... MHz . ... 14.285 and 100 MHz combs overlap here. strongest birdie 0 to 3000 MHz . ... 100 MHz birdie strongest values in lbw . ...

... Here some data observed on the 6m telescope with IFP installed in the OLD focal reducer are presented. ... Mkn 3: velocity field . ... NGC 5252: [OIII] image . ... NGC 5252 was observed 23 Feb. 1998 in the [OIII]5007 emission line with CCD TK1024 as detector. ... We observed the ionized gas velocity fields of the spiral galaxies with two purpose. ... Restored velocity field of NGC 157 in the reference frame rotating with the pattern speed overlaid on the Ha image of the galaxy . ... NGC 4100 . ...

... VLBI Schedule . ... Two different antenna are used for observing at ASKAP - AK07 has an L-band feed permanently installed while AK32 has an X-band feed installed. ... There are 3 main processes run for ASKAP observing. askap_drv is the main telescope control. It itself consists of a terminal based control process and a GUI. askap_drv must be running. VLBI scheduling is run from a process called "vlbi_drv", while the actual recording is via a command line process called px14_record. ...

README for XFree86 on OS/2 : Checking Compatibility of Video Hardware . ... Edit your CONFIG.SYS file to contain the following line somewhere: DEVICE=Y:\XFree86\lib\xf86sup.sys Of course replace ``Y:'' with the correct drive letter. ... Refer to section Adding Variables to CONFIG.SYS below. ... Start a full screen OS/2 CMD session and enter the following command: [C:\] Y:\XFree86\bin\SuperProbe . ... SuperProbe can identify many more video cards than are supported by XFree86. ...

... Donate to Support Science Literacy . ... 2016 Annual Awards . The ASP is accepting nominations for the organizationтАЩs national annual awards which recognize special achievements in astronomy research, technology, education, and public outreach. ... Shop the AstroShop . ... The Astronomical Society of the Pacific (ASP) is accepting nominations for the organizationтАЩs national annual awards which recognize special achievements in astronomy research, technology, education, and public outreach.. ...

... Does your system have Motif? ... Download and untar XmTel. ... Compile XmTel and copy the binary to /usr/local/bin . ... Check that the XEphem app-defaults file points to the place where the essential fifo and catalog files are located. ... Create the fifos in the xephem/fifos/ directory referred to by the app-defaults file. ... Copy xmtel to a directory in your search path such as /usr/local/bin cp xmtel /usr/local/bin If you use system directories this step must be done as root or superuser. ...

... Resembling a gigantic hubcap in space, a 3,700 light-year-diameter dust disk encircles a 300 million solar-mass black hole in the center of the elliptical galaxy NGC 7052. ... Because the front end of the disk eclipses more stars than the back, it appears darker. ... Despite its size, the disk is 100 times less massive than the black hole. ... The bright spot in the center of the disk is the combined light of stars that have crowded around the black hole due to its strong gravitational pull. ...

... Angular size depends on distance, the farther away an object is, the smaller an angle it covers. ... SDSSJ1430: A Galaxy Einstein Ring . ... IC 4406: A Seemingly Square Nebula . ... These detailed Hubble Space Telescope close-ups feature Jupiter's ancient swirling storm system known as the Great Red Spot. They also follow the progress of two newer storm systems that have grown to take on a similar reddish hue: the smaller "Red Spot Jr." (bottom), and smaller still, a "baby red spot". ...

... QC1 database . ... The quality information is derived in form of QC1 parameters. ... The Health Check monitor collects QC1 parameters and their scores. ... The results are presented in two views: the graphical HEALTH CHECK monitor with the full trending reports, and the QUICK-LOOK monitor with scores. ... The Health Check Monitor is a joint effort of the Quality Control Group in Garching and of Paranal Science Operations. ... You can download the QC1 parameters, and also connect to the QC1 database....

... Bad Astronomy . ... Every few months, one of a series of questions comes up on the USENET group sci.astro involving tides, or the rotation of the Moon, or the recession of the Moon from the Earth. ... Why the Moon's rotation period is the same as the length of time it takes to orbit the Earth (same as number 1, but phrased differently). ... But when this happens, the time it takes for the Earth to rotate once will be slowed to exactly the same time it takes for the Moon to go around the Earth once! ...

... Jump to: Downloads Comments . ... The original version only supported "quotas" for network drives where each home directory was it's own volume. In other words, it just checked the disk/volume size of the home folder and used that as the "quota". While this works in many settings, it doesn't work with actual OS X disk quotas, and it doesn't work with NFS quotas based on rquotad. ... It works with separate hard and soft quotas, and it also works if only hard quotas are implemented. ...

... You can boot Linux either from a floppy or from the hard disk. ... When booting Linux from a floppy disk, the boot sector contains code that just reads the first few hundred blocks (depending on the actual kernel size, of course) to a predetermined place in memory. On a Linux boot floppy, there is no filesystem, the kernel is just stored in consecutive sectors, since this simplifies the boot process. ... For example, when I boot, I it looks like this: љ љ љ љ LILO boot: Loading linux. ...

The study of energetic particles acceleration and transport within the magnetosphere and on its boundaries is the main goal of DOK-2 experiment on Auroral Probe in a frame of INTERBALL project. ... DOK-2 uses two pairs of energetic particle telescopes . ... This information is available only during the most informative Real Time mode of DOK-2. ... Full 56-57 channel spectra accumulated during time intervals from 10 s to 1464 s depending on a particle intensity. ... For this time interval: . ...

... Setting Orientation of and Placing Objects on the DIS Slit . ... Installing Gratings . ... In the control window set the slit, gratings, gratings wavecenters, windowning, and binning, click apply. (advice: if both sets of gratings are to be used during the night, calibrate the 2nd program gratings first then the 1st programs last). ... Does this need dis gratings change#? ... At this point you will need to firmly press the grating in until you feel it 'pop' into place. ... Install gratings in DIS . ...

... Flux density at 1 GHz (/Jy): 1040 . ... Notes: This is the remnant of the SN of AD 1054. ... Optical: Strongly polarised filaments, diffuse synchrotron emission, with `jet' faintly visible. ... VLA at 1.4 GHz, radio detection of `jet'. ... Velusamy 1985, MNRAS, 212, 359. ... Aller & Reynolds 1985, ApJ, 293, L73. ... Comparison of VLA observations at 74 MHz, 327 MHz, 1.5 GHz and 5 GHz for spectral index studies. ... VLA at 5 GHz (1".4) and HST multi-epoch observation for proper motion studies. ...

... At high latitudes, the E-region auroral electrojets and field-aligned currents produce 'radar aurora' that are somewhat more complicated than the equatorial radar echoes. ... Type 4 echoes are a special type of two-stream events associated with anomalous electron heating by the auroral electrojet waves. ... Res. ... Hedberg, and J. A. Nordling, Observations of auroral E-region plasma waves and electron heating with EISCAT and a VHF radar interferometer, J. atmos. terr. ... Observations, J. Geophys. ...

Brown J.C., Telfer D., Li Q., Hanuschik R., Cassinelli J. P., Kholtygin A. The effect of rotational gravity darkening on magnetically torqued Be star discs . ... 1 is not the optimum for creation of hot star discs which, in terms of emission measure for example, is found to occur in a broad peak around So~ 0.5-0.6 depending slightly on the wind velocity law. The relationship of this analytic quasi-steady parametric MTD model to other work on magnetically guided winds is discussed. ...

... We have measured this "redshift" for the pink black holes, and allowed for it in our calculations. ... We see this effect in the emission from gas around these pink black holes, but it is far too small an effect to account for the pinkness. Thus the swirling motions of gas around or into the black holes cannot produc the colour. ... At first we thought that these things were normal blue black holes hidden behind clouds of interstellar dust, that absorbed the blue light and made them appear pink. ...

Launch Vehicle Energia . ... The two-stage LV Energia of a package design using a parallel arrangement of stages and a backside accommodation of payload, has four strap-on boosters of stage I (boosters A) arranged around stage II (core stage TS). LV is installed on a pre-launch integration adapter (YA) serving to mate mechanical, pneudraulic, and electric connections between LV and the launch pad and the ground support equipment for pre-launch processing. ... Launch mass, t . ... SEA LAUNCH . ...

... There are preliminary series of photometric and radio spectral observations of the above-mentioned stars, archival data on the light curves of the stars, results of the search for OH and H 2 O maser emission in IRAS point sources that possess the IR parameters similar to Miras. ... The aim is a detailed study of the maser emission variability. ... In 1996-1997, astronomical observations of Mira Ceti-type stars (miras) were carried out in three spectral ranges: optical, infrared, and radio. ...