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| − | Noise
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| − | * Basic, Gaussian Noise (TOI) (Desert/Moneti)
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| − | * Glitching (Patanchon/Renault)
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| − | ** Elephants (Giraud-Heraud/Puget)
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| − | * Thermal Fluctuations
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| − | ** 1.6K & 4K (Catalano/Desert)
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| − | * Popcorn Noise (Sanselme)
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| − | ** Baseline Jumps (Sanselme/Kharab)
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| − | ** Split Level Noise (Sanselme/Kharab)
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| − | * 4K Lines (Macias)
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| − | ** Vibration
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| − | * From 4K Cooler (Pajot)
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| − | * <b>From pointing changes</b> (Ganga/Colley): As minutes of data are flagged after pointing changes, we see no evidence for microphonic contamination from pointing changes. More information can be found [[DepointingVibrations | here]].
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| − | * Noise Correlations (Jean-Marc Delouis)
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| − | * Time Sampling (Vibert/Montier)
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| − | ** CMB + Galaxy Calibration (Perdereau/Lagache)
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| − | ** Planets Fluxes (Gudmundsson/Lagache)
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| − | ** Point Source Fluxes (Reijo/Loic/Rosset)
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| − | ** VI Curves (Holmes/Desert)
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| − | * Known gain variation with bolometer plate temperature (Catalano/Desert)
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| − | * Saturation (Lamarre/Catalano/Coulais)
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| − | * ADC Correction (Couchot/Patanchon)
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| − | * Compression (Couchot/Plasczyniski)
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| − | * Band Pass (Spencer/Macias/Pajot)
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| − | * Cross Talk (Montier)
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| − | * Beam
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| − | ** Main (Jones/Roudier)
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| − | ** Dimpling (Oxborrow)
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| − | ** Ruze (Gudmundsson)
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| − | ** FSL (Murphy/Ganga)
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| − | * Time Response (Crill/Haissinski/Lamarre)
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| − | * Focal Plane (Jaffe)
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| − | * Pointing (Benabed/Jaffe)
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| − | * Cross-Scan Sampling (Hanson)
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