Haslam408 v2ivo://CDS/P/Haslam408/v2CDSFernique P.2014-11-25T15:40:00Z2019-05-05T06:35:00ZCDS Helpdeskcds-question@unistra.frSky surveyRadio astronomyRemazeilles et al. 2014 have re-evaluated and re-processed the rawest Haslam 408 MHz data, available from the Max Planck Institute for Radioastronomy Survey Sampler website, to produce an improved source-subtracted and destriped 408 MHz all-sky map. Large-scale striations associated with correlated low-frequency noise in the scan direction are reduced using a Fourier-based filtering technique. The most important improvement results from the removal of extra-galactic sources. An iterative combination of two techniques - two-dimensional Gaussian fitting and minimum curvature spline surface inpainting - are used to remove the brightest sources (with flux density larger than 2 Jy).Desources destrier map.Original acknowledgement for data: see Remazeilles et al. (2014)2015MNRAS.451.4311Rhttps://alasky.cds.unistra.fr/Haslam408_2014SurveyResearchIsDerivedFromLAMBDA/NASAThis HiPS is distributed under ODbL license by Unistra/CNRShttps://alasky.cds.unistra.fr/Haslam408_2014https://alaskybis.cds.unistra.fr/Haslam408_201439065 441172.6918409984375e-25 2.715032243962499e-25https://alasky.cds.unistra.fr/Haslam408_2014/Moc.fitsRadio