Interferometric spectrum of Orion from ATF, reduced in CASA.
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The atmospheric transmission during best octile (stringency = 8) conditions at Chajnantor over the ALMA Band 10 window (787-950 GHz) is shown. Some important lines mentioned in the ASAC Enhancement report (Sept 2001) on Band 10 are flagged. Additionally, the ASAC mentioned the scientific utility of this window for Redshifted [C II] emission and also for dust emission . Redshifted [C II] can, of course, cover this band for z=1 - 1.4, a critical period in the evolution of galaxies toward their present form. The band is clearest in its center, of course, which makes that the best frequency locale for dust measurements. Please see Attachment at bottom of agenda
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Emerson VxRSI antenna contractor handover testing begins 4 Feb |
The uv error amplitudes after CLEANing a simulated noiseless 4h observation of an HII region with out26 and its reoptimized version.
. The set is being extended with tapered beams.
| I | Attachment | Action | Size | Date | Who | Comment |
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Band10.pdf | manage | 393 K | 2008-05-28 - 11:11 | AlWootten | Good copy |
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Configurations_update.pdf | manage | 592 K | 2008-05-28 - 11:10 | AlWootten | Good copy |
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