Coldspotz June Visit to Pasadena - Revision history

Chary at 18:23, 8 August 2012

2012-08-08T18:23:41Z

2012-08-08T18:23:26Z

2012-08-08T18:20:47Z

2012-08-08T18:19:46Z

2012-06-19T19:28:08Z

2012-06-19T19:25:25Z

2012-06-19T19:23:25Z

2012-06-18T18:00:02Z

2012-06-17T23:29:10Z

2012-06-17T23:28:18Z

@@ Line 17: / Line 17: @@
 [[File:8.jpg|600px|Welcome to Planck-land]]
-[[File:9.jpg|200px|Tough work!]]
+[[File:9.jpg|400px|Tough work!]]
 '''Concepts Learnt:'''

← Older revision		Revision as of 18:23, 8 August 2012
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	[[File:8.jpg\|600px\|Welcome to Planck-land]]		[[File:8.jpg\|600px\|Welcome to Planck-land]]
		+
		+	[[File:9.jpg\|200px\|Tough work!]]

	'''Concepts Learnt:'''		'''Concepts Learnt:'''

← Older revision		Revision as of 18:20, 8 August 2012
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	[[File:6.jpg\|600px\|Gang@JPL courtesy of Chelen]]		[[File:6.jpg\|600px\|Gang@JPL courtesy of Chelen]]
		+
		+	[[File:7.jpg\|600px\|Presenting results]]

	[[File:8.jpg\|600px\|Welcome to Planck-land]]		[[File:8.jpg\|600px\|Welcome to Planck-land]]

← Older revision		Revision as of 18:19, 8 August 2012
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	[[File:6.jpg\|600px\|Gang@JPL courtesy of Chelen]]		[[File:6.jpg\|600px\|Gang@JPL courtesy of Chelen]]
		+
		+	[[File:8.jpg\|600px\|Welcome to Planck-land]]

	'''Concepts Learnt:'''		'''Concepts Learnt:'''

@@ Line 17: / Line 17: @@
 . Planck vision is not as sharp as WISE. Need WISE to get better position for source. W4 or W3 is the band of choice since
 they both sample dust emission. Sometimes multiple W4 or W3 sources might be within the Planck beam. If one of the sources is
-exceptionally bright, that is most likely our counterpart. Otherwise, there could be multiple contributors to Planck flux densities.
+exceptionally bright, that is most likely our counterpart. Otherwise, there could be multiple sources contributing to the Planck flux density.
-. Fitting a model to data and testing the accuracy of the model using additional data e.g. IRAS, 2MASS
+. Fitting a model to data and testing the accuracy of the model using additional data e.g. other Planck bands, IRAS, 2MASS
-. Deriving a new model which fits all the data and using that to conclude nature of the source.
+. Deriving a new model which fits all the data and using that to conclude nature of the source. Normalization of the model to the measured flux densities is important to get the true best fit.
 . Generating spectral energy distribution of a source (Brightness vs Wavelength). Different classes of objects show different spectral energy
@@ Line 28: / Line 28: @@
 . Using morphology of sources using SDSS or 2MASS to get independent confirmation of nature of source. Always remember to use the
 most accurate coordinates for the source - this is NOT the Planck coordinates.

@@ Line 1: / Line 1: @@
-'''Plan for the Visit:'''  [[Media:schedule.pdf]]
+'''Schedule during the Visit:'''  [[Media:schedule.pdf]]
 [[File:1.jpg|600px|SSC/Caltech Rooftop]]
@@ Line 12: / Line 12: @@
 [[File:6.jpg|600px|Gang@JPL courtesy of Chelen]]

← Older revision		Revision as of 18:00, 18 June 2012
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	[[File:5.jpg\|600px\|That iphone looks so delicious, I could eat it]]		[[File:5.jpg\|600px\|That iphone looks so delicious, I could eat it]]
		+
		+	[[File:6.jpg\|600px\|Gang@JPL courtesy of Chelen]]

← Older revision		Revision as of 23:29, 17 June 2012
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−	'''Plan for the Visit''' [[Media:schedule.pdf]]	+	'''Plan for the Visit:''' [[Media:schedule.pdf]]

	[[File:1.jpg\|600px\|SSC/Caltech Rooftop]]		[[File:1.jpg\|600px\|SSC/Caltech Rooftop]]

← Older revision		Revision as of 23:28, 17 June 2012
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−	'''Plan for the Visit'''[[Media:schedule.pdf]]	+	'''Plan for the Visit''' [[Media:schedule.pdf]]

	[[File:1.jpg\|600px\|SSC/Caltech Rooftop]]		[[File:1.jpg\|600px\|SSC/Caltech Rooftop]]