LONG­TERM RADIO TIME SCALES OF ACTIVE GALACTIC NUCLEI T. Hovatta 1 , M. Tornikoski 1 , M. Lainela 2 , E. Valtaoja 2 , I. Torniainen 1 , M.F. Aller 3 , H.D. Aller 3 1 Mets˜ahovi radio Observatory Mets˜ahovintie 114 02540 Kylm˜al˜a, Finland 2 Tuorla Observatory, University of Turku, Finland 3 Department of Astronomy, University of Michigan tho@kurp.hut.fi We have studied long­term variability time scales of a large sample of Active Galactic Nuclei at several frequencies between 4.8 and 230 GHz. ...

... Data is taken from Hilton (2011): Active M3-M5, 332 hours on 4 stars observing 157 flares; Active M6-M8, 59 hours on 4 stars observing 39 flares; Less Active M3òÀÓM5, 147 hrs on 8 stars observing 28 flares; Inactive M0-M2, 256 hours on 16 stars observing 9 flares; Inactive M3-M5, 153 hours on 6 stars observing 3 flares; Active M0-M1, data from Moffett (1974), Doyle Mathiouidakis (1990) and Dal Evren (2011), 156 hours on 2 stars observing 63 flares. ...

... Classes . ... Classes and global functions for general use. ... Binary search a sorted, linear, data structure. ... casa::Copy_global_functions_throw . ... Internal Utilities_module classes and functions. ... This module is a bag of unrelated mini-modules, classes and global functions. ... A signature for comparison functions is defined (required for comparison functions used in the Sort class), and one such function is provided. objcopy/objmove/objset copies objects from one place to another. ...

Easy DMT: Using the chInterface Class to Create/Upgrade DMT Monitors Rauha Rahkola, Univ. of Oregon LSC Meeting, August 19-22, 2002 LIGO Hanford Observatory Richland, WA LIGO-G020349-00-Z Easy DMT Introduction to the chInterface utility class ! ... Run through the data 1. for each channel, either: ! ... Final report LSC Meeting, August 19-22, 2002 Hanford 3 LIGO-G020349-00-Z Easy DMT The chInterface Model ! ... No Yes Yes Defaults to RMS of data addChannel addFilter New channel? ...

... Science . ... Science Activities > PhD Thesis Topics offered by ESO Faculty Members > Thesis Topic: Properties of kinematically decoupled structures in Early-Type Galaxies . ... Science Users Information . ... ESO-MIDAS . ... ESO Science Newsletter . ... The project consists in measuring the stellar kinematics, stellar populations, dynamics, and morphological properties of the kinematically decoupled structures observed in the inner regions of Early-Type Galaxies. ... Return to list of thesis topics...

... Current APO Weather . ... Search Site . ... Information for New Users . ... Technical Staff pages . Night Logs and Mailing Lists (maintained by APO) . ... Technical Documents and Database Search . ... Observer's Documentation and Procedures . ... Problem Reporting and APO Technical Documents Database Search . ... APO Drawing/Document Management Procedures . ... APO Technical Documents Database Search . Home Astrophysical Research Consortium . ... Mail Lists (maintained by APO) . ...

... Up: Data Analysis Applications . ... Our main goals are: 1) to take advantage of the full capabilities of the AXAF, we intend to provide a more sophisticated modeling capability (i.e., models that are f ( x , y , E , t ), models to simulate the response of AXAF instruments, and models that enable ``joint-mode'' fitting, i.e., combined spatial-spectral or spectral-temporal fitting); and 2) to provide users with a wide variety of models, optimization methods, and fit statistics. ... Multiple data sets...

... Four X-class Flares . Image Credit: NASA , Solar Dynamics Observatory, GSFC . Explanation: Swinging around the Sun's eastern limb on Monday, a group of sunspots labeled active region AR1748 has produced the first four X-class solar flares of 2013 in less than 48 hours. ... Ranked according to their peak brightness in X-rays , X-class flares are the most powerful class and are frequently accompanied by coronal mass ejections (CMEs), massive clouds of high energy plasma launched into space. ...

Stellarium 0.12.3 . ... Classes . ... ClassšMembers . ... StelMainScriptAPIProxy Class Reference . Because the core API runs in a different thread to the main program, direct function calls to some classes can cause problems - especially when images must be loaded, or other non-atomic operations are involved. ... Connect signals from the StelMainScriptAPI to the instance of this class running in the main thread and let the slots do the work which is not possible within StelMainScriptAPI itself. ...

. " The Arecibo Observatory is sponsored by the National Science Foundation. Any opinions, findings and conclusions or recommendations . expressed in this publication are those of the author(s) and do not necessarily reflect the views of the National Science Foundation."

. Pulkovo Observatory of Russian Academy of Sciences is situated . near Saint-Petersburg. It was founded in 1839. 196140, Saint-Petersburg, Pulkovskoye chaussee 65/1 . English version . Russian version . This page has been accessed times since May 1, 1999.

... Delivery Procedures . ... File Structure . Reference Files . ... The procedure compares two FITS reference files tables. ... The compared elements are limited to those specified in the COLUMNS parameter (which is necessary for this program to run). ... The parameter COLUMNS is an n-element array of strings with the names of the columns to compare within the table. ... When a combination is missing (in the new_file ;or in the old_file) the procedure will flag it in the standard output. ...

... A homogeneous chemical analysis of the inner Galactic disk from the first data release of Gaia-ESO . ... Gaia-ESO is a public spectroscopic survey designed with this goal in mind. ... These first results highlight the potential of the Gaia-ESO survey to explore areas of the Milky Way still poorly studied, such as the inner disk, and to give new constraints on Galactic chemical evolution models. ... Map of observed targets of the first data release of the Gaia-ESO Survey. ...

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