Difference between revisions of "External maps"
| (3 intermediate revisions by the same user not shown) | |||
| Line 42: | Line 42: | ||
Source http://faun.rc.fas.harvard.edu/ameisner/wssa/index.html. | Source http://faun.rc.fas.harvard.edu/ameisner/wssa/index.html. | ||
| − | + | = IRAM = | |
| − | = IRAM | ||
2013 maps of the Crab nebula at 89.189 GHz (HCO+(1-0) transition) in both temperature and polarization, prodouced from observations performed at the IRAM 30m telescope from January 9th to January 12th 2009, are delivered as a tarball of 416 KB in the file | 2013 maps of the Crab nebula at 89.189 GHz (HCO+(1-0) transition) in both temperature and polarization, prodouced from observations performed at the IRAM 30m telescope from January 9th to January 12th 2009, are delivered as a tarball of 416 KB in the file | ||
| Line 49: | Line 48: | ||
: [[File:Crab_IRAM_2010.zip]] | : [[File:Crab_IRAM_2010.zip]] | ||
| − | See README in the tarball for full details. These data were used in {{BibCite|aumont2010}}. | + | See README in the tarball for full details. These data were used in Aumont et al. 2010 {{BibCite|aumont2010}}. |
| + | |||
| + | = QUIJOTE / RADIOFOREGROUNDS = | ||
| + | |||
| + | QUIJOTE 2023 maps at 11, 13, 17 and 19 GHz from the QUIJOTE Wide Field Survey: | ||
| + | |||
| + | * [http://pla.esac.esa.int/pla/aio/product-action?MAP.MAP_ID=quijote_mfi_skymap_11ghz_512_dr1.fits quijote_mfi_skymap_11ghz_512_dr1.fits ] | ||
| + | * [http://pla.esac.esa.int/pla/aio/product-action?MAP.MAP_ID=quijote_mfi_skymap_13ghz_512_dr1.fits quijote_mfi_skymap_13ghz_512_dr1.fits ] | ||
| + | * [http://pla.esac.esa.int/pla/aio/product-action?MAP.MAP_ID=quijote_mfi_skymap_17ghz_512_dr1.fits quijote_mfi_skymap_17ghz_512_dr1.fits ] | ||
| + | * [http://pla.esac.esa.int/pla/aio/product-action?MAP.MAP_ID=quijote_mfi_skymap_19ghz_512_dr1.fits quijote_mfi_skymap_19ghz_512_dr1.fits ] | ||
| + | * [http://pla.esac.esa.int/pla/aio/product-action?MAP.MAP_ID=quijote_mfi_smth_skymap_11ghz_512_dr1.fits quijote_mfi_smth_skymap_11ghz_512_dr1.fits] | ||
| + | * [http://pla.esac.esa.int/pla/aio/product-action?MAP.MAP_ID=quijote_mfi_smth_skymap_13ghz_512_dr1.fits quijote_mfi_smth_skymap_13ghz_512_dr1.fits] | ||
| + | * [http://pla.esac.esa.int/pla/aio/product-action?MAP.MAP_ID=quijote_mfi_smth_skymap_17ghz_512_dr1.fits quijote_mfi_smth_skymap_17ghz_512_dr1.fits] | ||
| + | * [http://pla.esac.esa.int/pla/aio/product-action?MAP.MAP_ID=quijote_mfi_smth_skymap_19ghz_512_dr1.fits quijote_mfi_smth_skymap_19ghz_512_dr1.fits] | ||
| + | |||
| + | Source https://www.iac.es/es/proyectos/quijote and https://research.iac.es/proyecto/quijote/pages/en/data.php | ||
= References = | = References = | ||
<References /> | <References /> | ||
Latest revision as of 15:50, 19 January 2023
In the External Maps section of the Planck Legacy Archive we have included a small set of maps that users frequently use in combination of Planck data.
These is the list of external maps currently available in the PLA:
WMAP[edit]
WMAP K, Ka, Q, V and W bands (23, 33, 41, 61 and 94 GHz) full resolution coadded nine year sky maps in intensity and polarization.
- wmap_band_iqumap_r9_9yr_K_v5.fits
- wmap_band_iqumap_r9_9yr_Ka_v5.fits
- wmap_band_iqumap_r9_9yr_Q_v5.fits
- wmap_band_iqumap_r9_9yr_V_v5.fits
- wmap_band_iqumap_r9_9yr_W_v5.fits
Source http://lambda.gsfc.nasa.gov/product/map
Haslam[edit]
Improved Haslam et al. 408 MHz radio continuum all-sky map desourced and destriped.
Source http://www.jb.man.ac.uk/research/cosmos/haslam_map/
IRIS[edit]
IRIS 12, 25, 60 and 100 microns full resolution infrared maps (IRIS: Improved Reprocessing of the IRAS Survey)
Source http://www.cita.utoronto.ca/~mamd/IRIS/
WISE[edit]
WISE 12 micron low-resolution (NSIDE 2048) full-sky dust map.
Source http://faun.rc.fas.harvard.edu/ameisner/wssa/index.html.
IRAM[edit]
2013 maps of the Crab nebula at 89.189 GHz (HCO+(1-0) transition) in both temperature and polarization, prodouced from observations performed at the IRAM 30m telescope from January 9th to January 12th 2009, are delivered as a tarball of 416 KB in the file
See README in the tarball for full details. These data were used in Aumont et al. 2010 [1].
QUIJOTE / RADIOFOREGROUNDS[edit]
QUIJOTE 2023 maps at 11, 13, 17 and 19 GHz from the QUIJOTE Wide Field Survey:
- quijote_mfi_skymap_11ghz_512_dr1.fits
- quijote_mfi_skymap_13ghz_512_dr1.fits
- quijote_mfi_skymap_17ghz_512_dr1.fits
- quijote_mfi_skymap_19ghz_512_dr1.fits
- quijote_mfi_smth_skymap_11ghz_512_dr1.fits
- quijote_mfi_smth_skymap_13ghz_512_dr1.fits
- quijote_mfi_smth_skymap_17ghz_512_dr1.fits
- quijote_mfi_smth_skymap_19ghz_512_dr1.fits
Source https://www.iac.es/es/proyectos/quijote and https://research.iac.es/proyecto/quijote/pages/en/data.php
References[edit]
- ↑ Measurement of the Crab nebula polarization at 90 GHz as a calibrator for CMB experiments, J. Aumont, L. Conversi, C. Thum, H. Wiesemeyer, E. Falgarone, J. F. Macías-Pérez, F. Piacentini, E. Pointecouteau, N. Ponthieu, J. L. Puget, C. Rosset, J. A. Tauber, M. Tristram, A&A, 514, A70+, (2010).
Planck Legacy Archive
