... 216, Astronomical Data Analysis Software and Systems IX, eds. N. Manset, C. Veillet, D. Crabtree (San Francisco: ASP), 385 . ... A software system for active control of the KPNO 4-meter primary mirror is presented. The system consists of an embedded PC running RT-Linux, controlling a set of A/D and D/A modules. ... The primary mirror is supported by 33 pressurized units. ... The communication with the Telescope Control System is implemented using a KPNO standard ``software router'' package. ...

xntpd implements a general purpose address-and-mask based restriction list. ... The restriction facility was implemented in conformance with the access policies for the original NSFnet backbone time servers. ... Ignore all packets from hosts which match this entry. ... Default restriction list entries, with the flags ignore, ntpport , for each of the local host's interface addresses are inserted into the table at startup to prevent the server from attempting to synchronize to its own time. ...

vertex control of carriage house file hagen\wpfiles\vertexdoc\ chcontrol To: file From: Jon Hagen Date: Aug. ... The motor currents, measured within the amplifiers, are sent to the PLC as anlog input words IW168 ( Motor 1) and IW170 ( Motor 2) Digital from PLC to DCS Move up from digital output 18.6 Move down from digital output 18.7 Load tach Carriage House 1 from digital output 2.6 Load tach Carriage House 2 from digital output 2.7 Load setpoint Carriage ...

NGC OPTICAL SOFTWARE Claudio Cumani NGC Presentation - 2008, July 16 Differences btw IR and OPT detector controllers: intrinsic 2 "Exposure" handling Optical Rigid scheme for exposures (wipe - integrate - ["move charges on detector while integrating"] - read ). Active intervention of the control-server during the exposure is ti ti th th required (application of new voltages in each state). ... Starting an exposure = starting transfer and storage of data. ...

... 739C As one part of a program to detect complete samples of active extragalactic objects, the 3.36x10^-3 sr field centered on alpha=12h04min, delta=+11deg30' (1950.0) was mapped with the Very Large Array at 1411MHz. Sixty-seven maps cover this field so that no point is more than 15arcmin from the nearest map center. ... The rms map noise is 0.030 + 0.001 mJy, and the resulting source list is complete to a map peak flux density S_p = 0.2 mJy within 25 arcmin of the field center. ...

We present observational radial velocity curves for 12 chromospherically active binary systems and individual measurements for a further 5 systems. ... Six of our target binaries do not agree with published ephemerides or orbital parameters. We also present a rigourous derivation of the resolution limit for binary star cross-correlation radial velocities. ... Key Words: stars:binaries:close-stars:binaries:spectroscopic-techniques: radical velocities. ...

... Projects . Data transfer . ... PPTA projects and allocations . ... Time active (d) . ... Not active . ... PPTA data release 2 . ... unallocated Study timing noise in PPTA pulsars . ... unallocated Reprocess P140 data with PPTA pipeline . ... unallocated Consider the optimal observing strategy for PPTA pulsars . ... unallocated Application of cyclic spectroscopy to PPTA pulsars . ... Profile Domain Pulsar Timing: Developing and applying techniques to PPTA data. ... Tue, 24 Nov 15 03:36:53 +0000 . ...

... Credit: Courtesy CFA , TRACE Team , NASA Explanation: This dramatic high resolution picture looking across the edge of the Sun was taken April 24th by a telescope on board the newly launched Transition Region and Coronal Explorer (TRACE) satellite. It shows graceful arcs of intensely hot gas suspended in powerful looping magnetic fields which soar above a solar active region. ... Publications with keywords: TRACE - prominence . ... Eruptive Prominence . ... A Twisted Solar Eruptive Prominence . ...

... The active time at each angular bin is the sum over frames of the active time contributions from all CCD pixels, within the node-specific telemetry window, which overlap the surface of the bin. ... The active time, per frame, of a normal pixel is the full frame integration time multiplied by the node-specific fractional exposure; bad pixels contribute no active time. ... If an event is rejected for this reason only, then its pixels remain normal in the exposure map. ...

... Location: STScI Cafeteria Conference Room . The STScI Active Galaxies Lunch series provides a forum for interaction between researchers at STScI, JHU and the surrounding area who are interested in astrophysical processes related to active galaxies and black holes. ... Massive Elliptical Galaxies and the Most Massive Black Holes" . ... Lensed, IR-Luminous Galaxies at 1 < z < 3: AGN and Star-Forming Galaxies at the Spitzer Confusion Limit" . ... Feb 9: . Marco Chiaberge (STScI) . ...

... Image Quality of the VLT . Total Optical Control . First light for the ESO VLT unit telescope 1 occurred during the workshop. ... The image shown (Figure 1 ) here was obtained with the VLT on May 16, 1998, in red light (R band), i.e. while the mirror was still uncoated. ... In this diagram (FIgure 2), the measured image quality of the VLT UT1 astronomical images is plotted versus the ``seeing", as measured by the Seeing Monitor, a small telescope also located on top of the Paranal Mountain. ...

. To display the state of any background jobs that you are currently running use the job command. For example: jobs [1] + Running xterm -g 90x55 [2] - Running xterm -g 90x55 . This displays the job number, its state and the command associated with this job. To display the process number use the -l option. For example: jobs -l [1] + 3584 Running xterm -g 90x55 [2] - 3587 Running xterm -g 90x55 .

... May 15, 1998 . TRACE and the Active Sun . Credit: Courtesy CFA , TRACE Team , NASA . ... It shows graceful arcs of intensely hot gas suspended in powerful looping magnetic fields which soar above a solar active region. ... By operating the TRACE instruments during the Sun's increasingly active phase, scientists hope to explore the connections between complex solar magnetic fields and potentially hazardous solar eruptions. ... About APOD > . ... NASA Technical Rep.: ...

. Assumed Source Spectra (2-10 keV): . Normal AGN: a x = 0.5, N H = 3 10 20 cm -2 . Absorbed AGN: a x = 0.5, N H = 3 10 23 cm -2 . An explanation of and further information on these predictions can be found here . Sky Area vs. flux limit (0.5 - 3.5 keV) . Sky Area vs. flux limit (2 - 10 keV) . Home | Science Goals | Survey Strategy | Publications | Images & Data | Education/Outreach | Internal Page (password access only) . Date Last Modified: 22 April 2002 . Contact: Webmaster .

... Notre Dame de Paris Cathedral. ... Notre Dame and Cite Island from la Seine river. ... Luxembourg palace. ... Observatory avenue. ... Marshal Ney monument. ... Trip by Seine river. ... Paris view from Montmartre. ... King Louis XIII monument at Vosges. ... King Louis XIV monument. ... Old view to Seine and Conciergerie. ... Old view to Seine. ... Paris Observatory building. ... Khaltygin, Strelnitsky, Barsukova and Miroshnichenko. ... Louvre view from Seine river bus. ... King Louis XIV. ... Palace....

... Папка-регистратор . ... Браслеты . ... Корпус и браслет выполнены из нержавеющей стали с полным покрытием. ...

... ORAL SESSION . ... Registration /Coffee . ... Sergey Bogachev : Space solar investigations in the Lebedev Institute: from Sputnik-2 to future missions . ... Splinter session. S1 : SOLARIS mission proposal (chair - S.Kuzin) . ... Morning Coffee . ... The Sun from radio to gamma rays: new results from space and ground-based observatories (part 1) . ... Szymon Gburek : SphinX and XRT observations of active regions . ... Artem Ulyanov : Nanoflares in the quiet solar corona: a view from SDO/AIA . ...

Specification: Status Data Byte(s) Description D7----D0 D7----D0 ------------------------------------------------------------------------- Channel Voice Messages ------------------------------------------------------------------------- 1000cccc 0nnnnnnn Note Off event. 0vvvvvvv This message is sent when a note is released (ended). (nnnnnnn) is the note number . (vvvvvvv) is the velocity. 1001cccc 0nnnnnnn Note On event. 0vvvvvvv This ... The numbers are: Local Control. ...

Examples of some of the newly discovered double active nuclei. On the left are traditional astronomical "seeing limited" images from the Sloan Digital Sky Survey; the central box is shown expanded on the right, as observed with the Keck telescope and Adaptive Optics. In one image, there is a further zoom-in on the central portion shown in the upper right.) ...

... Research . Projects . ... The name of the project APEX is a reduction from words " Active Plasma Experiments " . The core of the project are active experiments with injection of electron and (or) plasma beams from a board of the satellite with simultaneous registration of the phenomena, produced by interaction of injected beam with background plasma. ... Active experiments utilise modulated electron beam accelerator and source of modulated xenon plasma beam on the main spacecraft APEX. ...