Changelog

• 2013-03-25, Mendes: Added change log page.
• 2013-03-26, Moneti: Cosmological Parameters: added caveat no. 2, improved look of tables, and other small changes to improve overall look.
• 2013-03-26, Lewis: Cosmological Parameters: write equations in math mode.
• 2013-03-26, Mendes: Added entry on Q&A page explaining broken links in fits file headers.
• 2013-03-27, Moneti/Cardoso: CMB and astrophysical component maps: update to correct product description, add figures, remove commented text, other cleanup.
• 2013-04-03, Mendes: Sky temperature maps: fixed incorrect links (Ticket ID DTX-918825).
• 2013-04-03, Mendes: CMB and astrophysical component maps: Fixed incorrect links to the new nilc and smica CMB maps.
• 2013-04-12, Zacchei: Sky temperature maps : Added LFI 70 GHz 2048 product and caveats on the use of effective beam with those maps.
• 2013-04-12, Zacchei: Map-making : Added LFI 70 GHz 2048 product.
• 2013-04-13, Rusholme: DatesObs: Added note on incompatibility with Healpix IDL read_fits_map.
• 2013-04-16: Mendes: SREM: Fixed link to the SREM files metadata.
• 2013-04-18: Gregorio: Map-making: Fixed Link to the Noise Monte Carlo Simulations page, end of 2.2.1, typo in the title of 3.2.3 and title of 5. "References" (previously "The Bibliograpy") for consistency with the rest of the ES.
• 2013-04-30: Mendes: References2: Added three missing references.
• 2013-04-30: Moneti: DatesObs: Minor formatting.
• 2013-05-07: Mendes: Catalogues: Fixed typo (second Y_MIN should be Y_MAX) in table.
• 2013-05-07: Moneti: CMB spectrum and Likelihood: added structure of file with masks used in Likelihood paper; fixes references, and other minor improvements.
• 2013-05-07: Moneti: CMB and astroph. comp. maps added structure of file with uinon mask.
• 2013-05-08: Mendes: References2: New references added for use in Beams.
• 2013-05-21: Moneti/Ashdown: CMB and astroph. comp. maps added union mask description and fixed last details. Pending CCB approval.
• 2013-05-21: Jaffe: HFI Detector Pointing: Changes from Reijo Keskitalo and others. Pending CCB approval.
• 2013-06-03: Benabed: CMB spectrum and Likelihood: Add remark that the low-l likelihood code does not currently tests for unphysical cases, and will return a null log likelihood in those cases.
• 2013-06-06: Moneti: Beams: Updates/fixes from Hivon (misc. pbs reported by LM) and Oxborrow on dimpling (NB. keep refs to TICRA reports?). Pending CCB approval.
• 2013-06-10: Mendes: References: Fixed minor problems on a few references.
• 2013-06-11: Oxborrow: Beams: Fixed layout problems with section 2, dimpling effects
• 2013-06-11: Mendes: Updated Operational files template
• 2013-06-18: Vibert: Fixed typos and improved layout in HFI cold optics, HFI performance summary, HFI detector feedhorn model parameters, HFI CO response, HFI time response model, The HFI DPC, Pre-processing, TOI processing, Spectral response, HFI-Validation, Summary of HFI data characteristics, Compact Source catalogues, The RIMO, Effective Beams, Frequency maps angular power spectra.
• 2013-06-20: Mendes: Updated Template:PLASingleFile to take into account changes to the PLAIO affecting links to the RIMO.
• 2013-07-03: Moneti: added table with lensing curl-mode PS to Lensing map.Has this been approved?.
• 2013-07-05: Moneti: fix typos, grammar, english, etc. in CMB spectrum and Likelihood page. Pending: fix links to PLAIO; add scientific description of likelihood masks.
• 2013-07-17: Mendes: References: Fixed a few issues with formating; Added new references.
• 2013-07-18: Mendes: Added a new template containing the base url to simplify changes when the use of the PLAIO at pladev is required. Updated all the PLAIO templates in order to include the new template.
• 2013-07-31: Moneti: added SZ catal validation info to Catalogues and other minor fixes.
• 2013-08-07: Mendes: Sky temperature maps: Added links to LFI point source masks.
• 2013-08-19: Mendes: Sky temperature maps: Corrected wrong description of point source masks for the LFI frequencies. There are no point source masks for the LFI at the 5 and 10 [math]\sigma[/math] levels as was originally stated. For the LFI the point sources are masked at the 4 [math]\sigma[/math] level.