WISE AllWISE Atlas (L3a) Images
Quick Links
Associated Data Products
- Intensity FITS images
- Uncertainty FITS images
- Coverage FITS images
- Positions of spurious sources from diffraction spikes
- Positions of spurious sources from optical ghosts
- Positions of spurious sources from latents
- Positions of spurious sources from halos
Overview
This catalog contains metadata for WISE AllWISE Atlas images. Each row in the catalog consists of metadata for a single coadd, and is uniquely identified by the coadd_id and band columns. A complete listing of available columns can be accessed by clicking the link above.
Metadata queries can be issued at the following URL:
For example, <root>/search/wise/allwise/p3am_cdd?POS=39.00,65.57 returns metadata for coadds containing (RA, Dec) = (39.00, 65.57) deg. Query parameters are documented here.
Generating URLs for data products
Note: MD5 checksums for all data products are stored. Checksum URLs are obtained by simply appending ".md5" to the data product URL.
- Intensity FITS images
-
These are located at:
<server><root>/data/wise/allwise/p3am_cdd/{coaddgrp:s}/{coadd_ra:s}/{coadd_id:s}/{coadd_id:s}-w{band:1d}-int-3.fitsExamples:
- <root>/data/wise/allwise/p3am_cdd/03/0390/0390p605_ac51/0390p605_ac51-w2-int-3.fits
- <root>/data/wise/allwise/p3am_cdd/03/0390/0390p605_ac51/0390p605_ac51-w1-int-3.fits
By appending center and size parameters (e.g <root>/data/wise/allwise/p3am_cdd/03/0390/0390p605_ac51/0390p605_ac51-w1-int-3.fits?center=39.000655,60.577778&size=200pix), one can also download cutouts (see the documentation).
Python code to build a URL:
params = { 'coadd_id': '0293p696_ac51', 'band': 1, } params['coaddgrp'] = params['coadd_id'][:2] params['coadd_ra'] = params['coadd_id'][:4] path = str.format( '{coaddgrp:s}/{coadd_ra:s}/{coadd_id:s}/{coadd_id:s}-w{band:1d}-int-3.fits', **params) url = 'serverroot/data/wise/allwise/p3am_cdd/' + path
C code to build a URL:
char url[256]; char coaddgrp[3]; char coadd_ra[5]; const char *coadd_id = "0293p696_ac51"; const char *server = "serverroot"; int band = 1; memcpy(coaddgrp, coadd_id, 2); coaddgrp[2] = '\0'; memcpy(coadd_ra, coadd_id, 4); coaddgrp[4] = '\0'; snprintf(url, sizeof(url), "%s/data/wise/allwise/p3am_cdd/%s/%s/%s/%s-w%1d-int-3.fits", server, coaddgrp, coadd_ra, coadd_id, coadd_id, band);
Java code to build a URL:
String coadd_id = "0293p696_ac51"; String server = "serverroot"; int band = 1; String url = String.format( "%1$s/data/wise/allwise/p3am_cdd/%2$s/%3$s/%4$s/%4$s-w%5$1d-int-3.fits", server, coadd_id.substring(0,2), coadd_id.substring(0,4), coadd_id, band);
- Uncertainty FITS images
-
These are located at:
<server><root>/data/wise/allwise/p3am_cdd/{coaddgrp:s}/{coadd_ra:s}/{coadd_id:s}/{coadd_id:s}-w{band:1d}-unc-3.fits.gzExamples:
- <root>/data/wise/allwise/p3am_cdd/03/0390/0390p605_ac51/0390p605_ac51-w2-unc-3.fits.gz
- <root>/data/wise/allwise/p3am_cdd/03/0390/0390p605_ac51/0390p605_ac51-w1-unc-3.fits.gz
Append center and size parameters to these URLs to download a cutout instead of a full image (see the cutouts documentation).
A trivial change to the format string in the sample code snippets above suffices to generate these URLs.
- Positions of spurious sources from diffraction spikes
-
These are stored in IPAC ASCII table files containing 2 columns: ra and dec, the J2000 right ascensions and declinations of WISE AllWISE Atlas (L3a) sources believed to be spurious detections from diffraction spikes. If there are no such sources for a frame, then no position table is stored and visiting the URL generated according to the recipe below will return a 404 Not Found HTTP response. The tables are located at:
<server><root>/data/wise/allwise/p3am_cdd/{scangrp:s}/{scan_id:s}/{frame_num:03d}/{scan_id:s}{frame_num:03d}-art-w{band:1d}-D.tblExample:
A trivial change to the format string in the sample code snippets above suffices to generate these URLs.
- Positions of spurious sources from optical ghosts
-
These are stored in IPAC ASCII table files containing 2 columns: ra and dec, the J2000 right ascensions and declinations of WISE AllWISE Atlas (L3a) sources believed to be spurious detections from optical ghosts. If there are no such sources for a frame, then no position table is stored and visiting the URL generated according to the recipe below will return a 404 Not Found HTTP response. The tables are located at:
<server><root>/data/wise/allwise/p3am_cdd/{scangrp:s}/{scan_id:s}/{frame_num:03d}/{scan_id:s}{frame_num:03d}-art-w{band:1d}-O.tblExample:
A trivial change to the format string in the sample code snippets above suffices to generate these URLs.
- Positions of spurious sources from latents
-
These are stored in IPAC ASCII table files containing 2 columns: ra and dec, the J2000 right ascensions and declinations of WISE AllWISE Atlas (L3a) sources believed to be spurious detections from latents. If there are no such sources for a frame, then no position table is stored and visiting the URL generated according to the recipe below will return a 404 Not Found HTTP response. The tables are located at:
<server><root>/data/wise/allwise/p3am_cdd/{scangrp:s}/{scan_id:s}/{frame_num:03d}/{scan_id:s}{frame_num:03d}-art-w{band:1d}-P.tblExample:
A trivial change to the format string in the sample code snippets above suffices to generate these URLs.
- Positions of spurious sources from halos
-
These are stored in IPAC ASCII table files containing 2 columns: ra and dec, the J2000 right ascensions and declinations of WISE AllWISE Atlas (L3a) sources believed to be spurious detections from halos. If there are no such sources for a frame, then no position table is stored and visiting the URL generated according to the recipe below will return a 404 Not Found HTTP response. The tables are located at:
<server><root>/data/wise/allwise/p3am_cdd/{scangrp:s}/{scan_id:s}/{frame_num:03d}/{scan_id:s}{frame_num:03d}-art-w{band:1d}-H.tblExample:
A trivial change to the format string in the sample code snippets above suffices to generate these URLs.