... Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer. 2016 January 14 . Infrared Portrait of the Large Magellanic Cloud . ... Explanation: Cosmic dust clouds ripple across this infrared portrait of our Milky Way's satellite galaxy , the Large Magellanic Cloud. ... Dominated by dust emission, the Large Magellanic Cloud's infrared appearance is different from views in optical images . ...

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• APOD: 2012 January 15 - Infrared Portrait of the Large Magellanic Cloud
• APOD: 2009 October 17 - Bright Nebulae in M33
• APOD: 2002 March 7 - Comet Ikeya-Zhang Brightens

... August 6, 1998 . Infrared Horsehead . ... Explanation: This famous cosmic dust cloud was imaged in infrared light by the European Space Agency's Infrared Space Observatory (ISO) satellite. The false-color picture shows the bright infrared emission from dust and molecular gas in part of the Orion star forming region surrounding the Horsehead Nebula . In visible light, the horsehead-shaped dust cloud looks dark against a background of bright glowing gas. ... About APOD > . ...

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• APOD: August 7, 1998 - M65 Without Moth
• APOD: 2000 June 13 - The Keyhole Nebula in Infrared
• APOD: September 5, 1998 - The Pulsar Powered Crab

... Infrared Portrait of the Large Magellanic Cloud . ... Credit Copyright: ESA / NASA / JPL-Caltech / STScI Explanation: Cosmic dust clouds ripple across this infrared portrait of our Milky Way's satellite galaxy , the Large Magellanic Cloud. ... The dust temperatures tend to trace star forming activity. ... Dominated by dust emission, the Large Magellanic Cloud's infrared appearance is different from views in optical images . ... Close Comet and Large Magellanic Cloud . ... The Large Cloud of Magellan...

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• Bright Nebulae in M33
• Астронет > Infrared Portrait of the Large Magellanic Cloud
• Journal "Peremennye Zvezdy"

Brain Research Group >> Research >> Change-point analysis ... << previous next >> . ... When detection of the change-points in alpha band power was performed as in the previous subsection, more than one change-point per second was obtained in average. ... The hypothesis of the hierarchy of EEG segmental descriptions (Kaplan 1998) (see subsection 7.3.2) is a theoretical reason for introducing the adjustment of the change-point detection probability. ...

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• Change-points in EEG components with different pattern
• Other prospects of the change-point based analysis
• Change-points in multi-channel EEG

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