Difference between revisions of "CephC-LABS Data list"

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*[http://irsa.ipac.caltech.edu/applications/wise/ WISE archive]
 
*[http://irsa.ipac.caltech.edu/applications/wise/ WISE archive]
*[http://irsa.ipac.caltech.edu/data/Herschel/HHLI/index.html HHLI page] gives you large files, that are multi-planar. Initially, I just cropped them down and pulled them into separate planes for the versions on the Box drive, but left them in their original tiles (herschel/pacscropped and herschel/spirecropped). I am in the process (5/2017) of combining the individual tiles together. Those are in herschel/bigmosaics. There are giant files as well as cropped down files. There are two different ways to combine the PACS data; I'm not sure which is better (yet).  
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*[http://irsa.ipac.caltech.edu/data/Herschel/HHLI/index.html HHLI page] gives you large files, that are multi-planar. Initially, I just cropped them down and pulled them into separate planes for the versions on the Box drive, but left them in their original tiles (herschel/pacscropped and herschel/spirecropped). I am in the process (5/2017) of combining the individual tiles together. Those are in herschel/bigmosaics. There are giant files as well as cropped down files. There are two different ways to combine the PACS data; I'm not sure which is better (yet). Remember that Herschel/PACS uses "b" for blue and "r" for red wavelength images; SPIRE uses "s" (short), "m" (medium), and "l" (long) to denote their bands. (HEAVY SIGH)
 
| herschel/pacscropped and herschel/spirecropped; herschel/bigmosaics/pacs/ and herschel/bigmosaics/spire
 
| herschel/pacscropped and herschel/spirecropped; herschel/bigmosaics/pacs/ and herschel/bigmosaics/spire
 
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Revision as of 15:54, 18 May 2017

telescope or survey or program wavelengths where to get data where to find it in Box drive
Chandra/ACIS X-ray (~0.001 um) Direct link to Chandra archive (not in there right now)
SDSS optical -- ugriz (0.29-0.9 um) sdss-skyview (so that we remember it's SDSS, from Skyview)
PanSTARRS optical -- grizy (0.48-0.91 um) main page for PanSTARRS panstarrs (tile retrieved does not cover whole area, but there are data over the whole area I believe)
IPHAS optical -- riHa (0.6-0.8 um) data page for IPHAS need to look at Mikami and Ogura (2001; not IPHAS) and Witham et al. (2008; this is IPHAS) to find specific objects with clear Ha excess. iphas (tile retrieved does not cover whole area, but there are data over the whole area I believe)
2MASS NIR -- JHKs (1.2-2.2 um) 2mass-skyview (so that we remember it's 2MASS, from Skyview. Seams between tiles obvious.) 2MASS data also buried in "FinderChartFiles" subdirectory, but those are the tiny tiles retrieved via FinderChart.
Spitzer - cryo era MIR -- i1i2i3i4m1 (3.6-24 um) Spitzer Heritage Archive gives you all data ever taken by Spitzer. BUT this row in the table is meant to be only those data taken when we had cryogen on board, e.g., the first ~5 yrs of the mission. There are three different summations of these same data.
  • (1) done by the SSC as part of the SEIP process.
  • (2) done by Rob Gutermuth for his project and for YSOVAR.
  • (3) summed up myself because I didn't like something about the SEIP mosaics.
(1): spitzer/seip - big tiles, all channels. (2) we do not have those mosaics, only the photometry. (3) spitzer/mycryo - i1, i2, and m1 only THIS IS THE M1 DATA YOU SHOULD PROBABLY USE.
Spitzer - postcryo era, GLIMPSE data MIR -- i1i2 (3.6-4.5 um) Spitzer Heritage Archive gives you all data ever taken by Spitzer. BUT this is from a galactic plane survey called GLIMPSE. Not very deep. Taken at a different time than the YSOVAR data. spitzer/glimpse
Spitzer - postcryo era, YSOVAR data MIR -- i1i2 (3.6-4.5 um) Spitzer Heritage Archive gives you all data ever taken by Spitzer. BUT this is from the YSOVAR campaign, so many, many, many visits. I summed up all of them into one very, very deep mosaic per channel. spitzer/my_YSOVAR
WISE MIR -- w1w2w3w4 (3.5-22 um) FinderChartFiles/*w?.fits
Herschel FIR -- PACS (70,160 um) and SPIRE (250, 350, 500 um)
  • WISE archive
  • HHLI page gives you large files, that are multi-planar. Initially, I just cropped them down and pulled them into separate planes for the versions on the Box drive, but left them in their original tiles (herschel/pacscropped and herschel/spirecropped). I am in the process (5/2017) of combining the individual tiles together. Those are in herschel/bigmosaics. There are giant files as well as cropped down files. There are two different ways to combine the PACS data; I'm not sure which is better (yet). Remember that Herschel/PACS uses "b" for blue and "r" for red wavelength images; SPIRE uses "s" (short), "m" (medium), and "l" (long) to denote their bands. (HEAVY SIGH)
herschel/pacscropped and herschel/spirecropped; herschel/bigmosaics/pacs/ and herschel/bigmosaics/spire
SCUBA Sub-mm -- 450 and 850 um
  • main archive page
  • Need to look at DiFrancesco et al. to find data table with specific sources and fluxes
scuba (Note that data range here is much different than for the other images here)

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