Difference between revisions of "External maps"

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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.
  
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== 2013 IRAM Maps of the Crab nebula ==
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These is the list of external maps currently available in the PLA:
  
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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
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= WMAP =
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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.
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* [http://pla.esac.esa.int/pla/aio/product-action?MAP.MAP_ID=wmap_band_iqumap_r9_9yr_K_v5.fits wmap_band_iqumap_r9_9yr_K_v5.fits]
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* [http://pla.esac.esa.int/pla/aio/product-action?MAP.MAP_ID=wmap_band_iqumap_r9_9yr_Ka_v5.fits wmap_band_iqumap_r9_9yr_Ka_v5.fits]
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* [http://pla.esac.esa.int/pla/aio/product-action?MAP.MAP_ID=wmap_band_iqumap_r9_9yr_Q_v5.fits wmap_band_iqumap_r9_9yr_Q_v5.fits]
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* [http://pla.esac.esa.int/pla/aio/product-action?MAP.MAP_ID=wmap_band_iqumap_r9_9yr_V_v5.fits wmap_band_iqumap_r9_9yr_V_v5.fits]
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* [http://pla.esac.esa.int/pla/aio/product-action?MAP.MAP_ID=wmap_band_iqumap_r9_9yr_W_v5.fits wmap_band_iqumap_r9_9yr_W_v5.fits]
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Source http://lambda.gsfc.nasa.gov/product/map
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= Haslam =
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Improved Haslam et al. 408 MHz radio continuum all-sky map desourced and destriped.
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* [http://pla.esac.esa.int/pla/aio/product-action?MAP.MAP_ID=haslam408_dsds_Remazeilles2014.fits haslam408_dsds_Remazeilles2014.fits]
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Source http://www.jb.man.ac.uk/research/cosmos/haslam_map/
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= IRIS =
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IRIS 12, 25, 60 and 100 microns full resolution infrared maps (IRIS: Improved Reprocessing of the IRAS Survey)
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* [http://pla.esac.esa.int/pla/aio/product-action?MAP.MAP_ID=IRIS_nohole_1_2048.fits IRIS_nohole_1_2048.fits]
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* [http://pla.esac.esa.int/pla/aio/product-action?MAP.MAP_ID=IRIS_nohole_2_2048.fits IRIS_nohole_2_2048.fits]
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* [http://pla.esac.esa.int/pla/aio/product-action?MAP.MAP_ID=IRIS_nohole_3_2048.fits IRIS_nohole_3_2048.fits]
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* [http://pla.esac.esa.int/pla/aio/product-action?MAP.MAP_ID=IRIS_nohole_4_2048.fits IRIS_nohole_4_2048.fits]
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Source http://www.cita.utoronto.ca/~mamd/IRIS/
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= WISE =
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WISE 12 micron low-resolution (NSIDE 2048) full-sky dust map.
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* [http://pla.esac.esa.int/pla/aio/product-action?MAP.MAP_ID=wssa_sample_2048.fits wssa_sample_2048.fits]
 +
 
 +
Source http://faun.rc.fas.harvard.edu/ameisner/wssa/index.html.
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 +
= 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
  
 
: [[File:Crab_IRAM_2010.zip]]
 
: [[File:Crab_IRAM_2010.zip]]
  
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See README in the tarball for full details. These data were used in {{BibCite|aumont2010}}.
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See README in the tarball for full details. These data were used in Aumont et al. 2010 {{BibCite|aumont2010}}.
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= QUIJOTE / RADIOFOREGROUNDS =
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QUIJOTE 2023 maps at 11, 13, 17 and 19 GHz from the QUIJOTE Wide Field Survey:
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* [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 ]
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* [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 ]
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* [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 ]
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* [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 ]
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* [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]
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* [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]
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* [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]
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* [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]
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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.

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

File:Crab IRAM 2010.zip

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:

Source https://www.iac.es/es/proyectos/quijote and https://research.iac.es/proyecto/quijote/pages/en/data.php

References[edit]

  1. ↑ 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

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