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Profile Kevin
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Message 329 - Posted: 17 Aug 2012, 5:11:05 UTC

Rob has been busy - check out the new images we are generating on the fly as results come in.

mu = fraction of the total V-band optical depth of the dust seen by young stars contributed by dust in the ambient interstellar medium
ldust = luminosity absorbed and reradiated by dust
m = effective stellar mass
sfr = star formation rate
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Message 330 - Posted: 17 Aug 2012, 8:56:23 UTC
Last modified: 17 Aug 2012, 8:57:38 UTC

Impressive.

Is there a there a colour gradient available to indicate levels of activity?
I assume its blue > purple > red > orange > yellow >white.

Congrats ... never seen a project give participants feed back and results like this in such a short time frame since inception.
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Message 339 - Posted: 17 Aug 2012, 19:05:46 UTC - in response to Message 329.

Great stuff! I seem to working only in the 'suburbs' so far though ;)

Cheers,

Al.

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Profile Kevin
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Message 345 - Posted: 18 Aug 2012, 12:48:16 UTC - in response to Message 330.

You are correct. We won't publish the real numbers until we publush to journals.
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