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	active galactic nucleus (AGN)
		AGN are found at the heart of active galaxies, including quasars, Seyfert galaxies, blazars, and radio galaxies.
		Since a fl hole, by definition, emits nothing, the radiation from an AGN is believed to come from material heated to several million degrees in an accretion disk before tumbling into the fl hole or, in some cases, being shot away in twin jets along the central engine’s spin axis.
		Within each is a broad range of luminosity, from AGN so weak that they are barely detectable against the light from the central stars of their host galaxy to quasars that are more than 100 times brighter than all the stars in their hosts put together.
	www.daviddarling.info /encyclopedia/A/AGN.html (738 words)

	AGN Projects at SSUO
		In this model, the different forms of AGNs we observe are merely different views of this process from different orientations with respect to the axis of the jet and the accretion disk.
		AGN variability consists of slow irregular fluctuations upon which are superimposed occasional outbursts and declines.
		A more extended description of AGN Variability is available which includes illustrations of various types of lightcurves plus recommendations for the type of photometric data that can be most helpful in improving our understanding of the AGN phenomenon.
	www.phys-astro.sonoma.edu /observatory/research/agn/agnp.html (932 words)

	Active Galactic Nuclei (Site not responding. Last check: 2007-10-18)
		AGN which have about the same luminosity than the host galaxy are called Seyfert galaxies.
		AGN have the peculiarity to emit electro-magnetic radiation over a very broad spectral domain from the infrared to the X-rays.
		To explain the different spectral components of an AGN, it is necessary to refer to many different physical emission processes (synchrotron emission in the radio, inverse comptonization in the X-rays, thermal dust emission in the infrared).
	obswww.unige.ch /~turler/hea/agn.html (511 words)

	tee times @ last minute - AGN FAQ (Site not responding. Last check: 2007-10-18)
		AGN was established in 2002 and has to date more than 30,000 members in Malaysia, Indonesia and Singapore, forming the largest golfing network in Asia.
		AGN is constantly expanding its network by increasing the number of golf courses to include courses in Singapore, The Philippines, China, etc and other countries in Asia.
		AGN is currently the biggest golfing network in Asia and is constantly increasing the list of golf courses that members can enjoy.
	www.teetimeslastminute.org /agn_faq (928 words)

	Beginner's Guide to AGN
		So, at the most basic level, AGNs are simply the cores of galaxies that are not quiescent like normal galaxy cores: for instance, some of them emit an amount of energy comparable to the output of an entire galaxy from their cores, which are regions measuring only parsecs in size.
		Certainly the occurance of AGNs depends on pulling gas from the outer, kpc-scale regions of the disk to the inner regions, but it's not at all clear how this is done (see astro-ph/0407068 and astro-ph/0408282 for very nice overviews).
		Below are the various classes of AGNs that are often seen in the literature with a brief explanation of where they fit in.
	www.cita.utoronto.ca /~everett/agnOverview/agnOverview.html (3773 words)

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	MAST AGN Catalog
		The Active Galactic Nuclei (AGN) catalog is heavily based on A Catalogue of Quasars and Active Nuclei (7th Edition), ESO Scientific Report No. 17, by Véron-Cetty & Véron (1996) [VV96].
		Therefore, for objects without (B-V) colors, V magnitudes have been derived from the given values by subtracting (B-V) values typical of the class to which an object belongs to, unless the reference was to a paper which gave V magnitudes directly.
		One should remember that most AGN are variable so the reported V magnitudes should be taken only as indicative.
	stdatu.stsci.edu /search/agn_catalog.html (688 words)

	AGN Report
		It was stressed that the AGN is responsible to and is a structural component of the SCN.
		The AGN members found that while there was often considerable coordination and cooperation, it was on an ad hoc basis, and worked best in acute emergency situations.
		The AGN were cautioned not to take too superficial a view of country-level coordination since bilaterals and NGOs, important actors in some countries, do not fall within the UN Resident Coordinator system.
	www.unsystem.org /scn/publications/AnnualMeeting/SCN25/agnreport.html (721 words)

	:: Welcome to www.agnmak.com ::
		AGN International Middle and Near East Conference opened in Dubai on 10th December 2002 and ran for two days.
		The conference emphasized on the large opportunities that are opening up for accounting firms especially after the recent scandals in the U.S. and great potentials in the areas like providing quality audits to clients and looking at non-audit services.
		He said that AGN has now presence in 76 countries and a billing of Euro 1.1 billion in 2002.
	www.agnmak.com /conference.htm (163 words)

	AGN Page
		The AGN was involved in the development of many of the SCN symposia and almost all of the special workshops which led to a substantial proportion of the publications that have brought much credit to the SCN albeit sometimes with discomfort to individual UN agencies.
		As chair of the AGN for the past two years, I do not see "holding the AGN in abeyance" as a sign of failure but rather agree with the need to re-examine its role.
		The main strength of the AGN concept past, present, and future, is that it brings independent periodic review of the work of the UN system in food and nutrition.
	www.unsystem.org /scn/archives/scnnews18/ch02.htm (1543 words)

	AGN & the Amateur
		While AGN remain exotic objects and the majority are only detectable with the largest telescopes and most sophisticated equipment, a few of the brighter ones are accessible to the amateur observer, and the contribution of the dedicated amateur can be of a significant benefit to the professional astronomer.
		In favour of a visual approach is the ability to observe several objects in the session; the results are rapidly obtained and the equipment is relatively inexpensive, although realistically a larger aperture is needed for such faint objects.
		While the numbers of AGN available are limited, there are still over a dozen to be observed by the owners of a 40cm or larger telescope.
	members.aol.com /PoynerGary/agn.html (3902 words)

	IntegrationTimes (Site not responding. Last check: 2007-10-18)
		Single SED composites of local "warm" Type 1 and "cooler" Type 2 AGN from the far to near-IR are assumed for the unobscured and obscured objects respectively, independent of luminosity.
		The counts of ULIRGs appear to be less than those of AGN at 24µm due to the large difference in their SED shapes at short wavelengths.
		The flatter redshift distrbution observed for AGN reflects the presence of numerous low-luminosity sources which are only detectable at the lowest redshifts.
	spider.ipac.caltech.edu /staff/fmasci/home/AGN_SIRTF.html (1314 words)

	Terms and Conditions
		AGN does not give any warranties in respect of the Content (including, without limitation, any as to quality, accuracy, completeness or fitness for any particular purpose of such Content), software or services available through the site.
		AGN will require all such service providers to use the information solely to provide the specified services and to otherwise conform with the requirements of this privacy policy.
		AGN uses this information to find out which features of the site are most popular so that the site can be developed in the light of the analysis of your usage.
	www.agn-na.org /terms.htm (1163 words)

	AGN Physics with the SDSS; Princeton, July 2003
		The AGN community is in the midst of a flood of high-quality data spanning the entire electromagnetic spectrum, from the FIRST survey in the radio, Chandra and XMM-Newton in X-rays, 2dF in the optical, 2MASS and SIRTF in the infra-red, and no lack of data from 8m class telescopes.
		Although we are calling this "AGN Physics with the SDSS", by no means is it required that the talks/posters be based upon SDSS data or even mention the SDSS in any way.
		Participation is limited to those that are active in AGN research and will primarily be by invitation, but we have reserved some slots for at-large applications.
	www.astro.princeton.edu /~gtr/sdssagn2003 (751 words)

	tee times @ last minute - AGN Application (Site not responding. Last check: 2007-10-18)
		AGN reserves the right to revoke your membership or refuse membership extension if any form of abuse or inappropriate behaviour is reported.
		The AGN Member's Golfing Guide and Club Listing allows you to enjoy the benefits of participating clubs that are under the contract of J.V. Members are advised to pay special attention to the conditions stipulated.
		J.V. CITRA BUMI (M) SDN BHD as the owner of AGN and its agent(s) shall not be responsible or liable for any participating clubs not honoring the program; however AGN will make every effort to offer an alternative golfing option, as so desired.
	www.teetimeslastminute.org /agn_application (353 words)

	Active Galactic Nuclei
		Quasars are very distant AGN - the most distant quasars mark an epoch when the universe was less than a billion years old and a sixth of its current size.
		In some cases, the size of the AGN is smaller than the size of our solar system.
		Based on X-ray (and other) observations, a good guess is that the power source in AGN is a supermassive fl hole.
	heasarc.gsfc.nasa.gov /docs/objects/agn/agntext.html (225 words)

	X-ray AGN Intro (Site not responding. Last check: 2007-10-18)
		Perhaps the most popularly known instance of AGN are "quasars" which are AGN that are very distant, up to 60 billion light years away.
		Based on X-ray, radio, and other observations, a good guess is that the power source in AGN is a supermassive flhole.
		Many AGN also show evidence for a huge torus of gas around the flhole.
	aether.lbl.gov /www/projects/neutrino/AGN/AGN.html (286 words)

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	AGN
		Active galactic nuclei (AGN) are galaxies that have very energetic central regions, due to either the presence of a fl hole or star formation activity at the core of the galaxy.
		Three main types of AGN are quasars, ("quasi-stellar objects" or QSOs), which are very compact objects that resemble stars in optical images; Seyfert galaxies, characterized by fluctuations in brightness at their cores; and radio galaxies, which emit massive jets of gas powered by fl holes at their cores.
		Other images of AGN can be found in the VLBA 2cm Survey of Compact Radio Sources and the Jodrell Bank Atlas of DRAGNs.
	www.nrao.edu /imagegallery/php/level2.php?class=AGN (289 words)

	Active Galaxies
		In ~10% of the AGN, the MBH + accretion disk somehow produce narrow beams of energetic particles and magnetic fields, and eject them outward in opposite directions away from the disk.
		Radio galaxies, quasars, and blazars are AGN with strong jets, which can travel outward into large regions of intergalactic space.
		Active Galactic Nuclei observed at high (>100 MeV) energies form a subclass known as blazars; a blazar is believed to be an AGN which has one of its relativistic jets pointed toward the Earth so that the emission we observe is dominated by phenomena occurring in the jet region.
	imagine.gsfc.nasa.gov /docs/science/know_l2/active_galaxies.html (1043 words)

	Acute Glomerulonephritis (AGN) - nephrologychannel (Site not responding. Last check: 2007-10-18)
		Acute glomerulonephritis (AGN) is active inflammation in the glomeruli.
		A kidney biopsy is essential to establish a diagnosis of AGN, determine the cause, and create an effective treatment plan.
		The goal of treatment is to stop the ongoing inflammation and lessen the degree of scarring that ensues.
	www.nephrologychannel.com /agn (392 words)

	AGN Watch Papers
		The category ``other AGN Watch papers'' describe observational programs that were built around the primary UV/optical monitoring programs and carried out by smaller groups of AGN Watch members.
		AGN Watch papers that have been accepted for publication but not yet published are either available in preprint form as tarred, gzipped PostScript files [instructions] or as links to astro-ph.
		This is the title of the principal AGN Watch data papers.
	www.astronomy.ohio-state.edu /~agnwatch/papers.html (1497 words)

	High Energy Astrophysics at Penn State : Active Galactic Nucleii ( AGN )
		Members of the Penn State X-ray Astronomy group are involved in both X-ray and optical studies of the supermassive fl holes that reside in the nuclei of active galaxies.
		These AGN may be a small but distinct subclass which show broad optical line emission from an accretion disk.
		This originates when a jet from an AGN is fired nearly along our line of sight.
	www.astro.psu.edu /xray/agn (474 words)

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	AGN Surveys 2003
		The huge amount of data obtained by surveys in all wavebands, from radio to X-rays, has allowed a major progress in the understanding of Active Galactic Nuclei and of their cosmic evolution.
		This conference is intended to give a broad overview of the recent results obtained by AGN surveys over the whole electromagnetic spectrum.
		Topics which will be discussed during the conference are: AGN evolution, contribution to the cosmic background, AGN luminosity functions in different wavebands, multiwavelength properties of AGN, unified model and unconventional AGN, connection with the host galaxies, co-evolution of AGN and galaxies, implications for the local density of supermassive fl holes.
	www.inaoep.mx /~agn2003 (125 words)

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	AGn Listings - (Site not responding. Last check: 2007-10-18)
		All content, ideas and images are copyright to AGn Solutions unless otherwise stated.
		It was a lot earlier than predicted but AGn Listings is now open for business.
		After over a year of downtime, AGn Listings is coming back bigger and better than ever.
	list.acidgloss.net (326 words)

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