Difference between revisions of "CephC-LABS Data list"
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*[http://skyview.gsfc.nasa.gov/current/cgi/query.pl Skyview gives you larger tiles] | *[http://skyview.gsfc.nasa.gov/current/cgi/query.pl Skyview gives you larger tiles] | ||
| sdss-skyview (so that we remember it's SDSS, from Skyview) | | sdss-skyview (so that we remember it's SDSS, from Skyview) | ||
+ | '''[https://caltech.box.com/s/ncqy372znmox06pqsolwgntp7zoghwla get the images here]''' | ||
|- | |- | ||
| PanSTARRS | | PanSTARRS | ||
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| [https://panstarrs.stsci.edu/ main page for PanSTARRS] | | [https://panstarrs.stsci.edu/ main page for PanSTARRS] | ||
| panstarrs (tile retrieved does not cover whole area, but there are data over the whole area I believe) | | panstarrs (tile retrieved does not cover whole area, but there are data over the whole area I believe) | ||
+ | '''[https://caltech.box.com/s/4alfal5fcd2s2ny4tqqk5g2vhi7uy6qw get the images here]''' | ||
|- | |- | ||
| IPHAS | | IPHAS | ||
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| [http://www.iphas.org/data.shtml 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. | | [http://www.iphas.org/data.shtml 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) | | iphas (tile retrieved does not cover whole area, but there are data over the whole area I believe) | ||
+ | '''[https://caltech.box.com/s/eperz5shclr9t4cmv2sdizb54m4jdrkw get the images here]''' | ||
|- | |- | ||
| 2MASS | | 2MASS | ||
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*(3) summed up myself because I didn't like something about the SEIP mosaics. | *(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. | | (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. | ||
+ | '''[https://caltech.box.com/s/utivn7usw940ck5cx6o678ztv2lfxuew get the IRAC-1 mosaic here]''' | ||
+ | '''[https://caltech.box.com/s/81vgn7ok6d5k1r53zasv06qjo40ttu69 get the IRAC-2 mosaic here]''' | ||
+ | '''[https://caltech.box.com/s/658g03561rq9jzgax1xlp0igbup1s8ao get the IRAC-3 mosaic here]''' | ||
+ | '''[https://caltech.box.com/s/rhj7u5yogyf94upcbe4fyj7er5wxnvtn get the IRAC-4 mosaic here]''' | ||
+ | '''[https://caltech.box.com/s/wj5ntke0kkwhtq9s0f276wzxrtlg34eq get the MIPS-1 mosaic here]''' | ||
|- | |- | ||
| Spitzer - postcryo era, GLIMPSE data | | Spitzer - postcryo era, GLIMPSE data | ||
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*[http://irsa.ipac.caltech.edu/applications/FinderChart/ FinderChart] gives you large tiles | *[http://irsa.ipac.caltech.edu/applications/FinderChart/ FinderChart] gives you large tiles | ||
| FinderChartFiles/*w?.fits | | FinderChartFiles/*w?.fits | ||
+ | '''[https://caltech.box.com/s/yll27xa6zv38zbs28sk74p5p2bvx4dzf get the WISE-1 mosaic here]''' | ||
+ | '''[https://caltech.box.com/s/zihshysrgw3221o2sykt8hptkqjqbdb3 get the WISE-2 mosaic here]''' | ||
+ | '''[https://caltech.box.com/s/6ivjtk2v67yt45n6pkscixhli0gdojg8 get the WISE-3 mosaic here]''' | ||
+ | '''[https://caltech.box.com/s/gp7cd7t8imvx2l8min99wudew5x1lj4g get the WISE-4 mosaic here]''' | ||
|- | |- | ||
| Herschel | | Herschel | ||
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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 combined (5/2017) of the individual tiles together. Those are in herschel/bigmosaics. There are giant files as well as cropped down files, just so you can see them (you may not be able to download or display the big images, depending on your network and RAM; they're really big). There are two different ways to combine the PACS data; <strike>I'm not sure which is better (yet), so they're both in there.</strike> The *js* ones are better for our purposes, and you want the ones cropped from the big mosaics (herschel/bigmosaics/pacs/*js*cropped* and herschel/bigmosaics/spire/*cropped*. Remember that Herschel/PACS uses "b" for blue and "r" for red wavelength images; Herschel/SPIRE uses "s" (short), "m" (medium), and "l" (long) to denote their bands. (HEAVY SIGH) | *[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 combined (5/2017) of the individual tiles together. Those are in herschel/bigmosaics. There are giant files as well as cropped down files, just so you can see them (you may not be able to download or display the big images, depending on your network and RAM; they're really big). There are two different ways to combine the PACS data; <strike>I'm not sure which is better (yet), so they're both in there.</strike> The *js* ones are better for our purposes, and you want the ones cropped from the big mosaics (herschel/bigmosaics/pacs/*js*cropped* and herschel/bigmosaics/spire/*cropped*. Remember that Herschel/PACS uses "b" for blue and "r" for red wavelength images; Herschel/SPIRE uses "s" (short), "m" (medium), and "l" (long) to denote their bands. (HEAVY SIGH) | ||
| <strike>herschel/pacscropped and herschel/spirecropped;</strike> herschel/bigmosaics/pacs/*js*cropped* and herschel/bigmosaics/spire/*cropped* | | <strike>herschel/pacscropped and herschel/spirecropped;</strike> herschel/bigmosaics/pacs/*js*cropped* and herschel/bigmosaics/spire/*cropped* | ||
+ | '''[https://caltech.box.com/s/8lggqf47fpzi0on8eutmqel6d9kvm7xc get the PACS-70 mosaic here]''' | ||
+ | '''[https://caltech.box.com/s/9hujvag6xnk6er4dadi94x4l9v3xedv9 get the PACS-160 mosaic here]''' | ||
+ | '''[https://caltech.box.com/s/529jv11s83le0zvu8ewln8re5ihaimoo get the SPIRE-250 mosaic here]''' | ||
+ | '''[https://caltech.box.com/s/oxbpmujufyud3zym6qo5n3qmz2efrhnw get the SPIRE-350 mosaic here]''' | ||
+ | '''[https://caltech.box.com/s/g6uro4j5dtee2wrmyqj2aodcwox82qgn get the SPIRE-500 mosaic here]''' | ||
|- | |- | ||
| SCUBA | | SCUBA | ||
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*Need to look at DiFrancesco et al. to find data table with specific sources and fluxes | *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) | | scuba (Note that data range here is much different than for the other images here) | ||
+ | '''[https://caltech.box.com/s/oe5m0s2asulpjgsr899hetjeiaq0i34b get the SCUBA-450 mosaic here]''' | ||
+ | '''[https://caltech.box.com/s/486wmx78op183icjnemzloo35uwe06ba get the SCUBA-850 mosaic here]''' | ||
- | - | ||
|} | |} |
Latest revision as of 23:04, 23 July 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): 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.
get the IRAC-1 mosaic here get the IRAC-2 mosaic here get the IRAC-3 mosaic here get the IRAC-4 mosaic here get the MIPS-1 mosaic here |
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
get the WISE-1 mosaic here get the WISE-2 mosaic here get the WISE-3 mosaic here get the WISE-4 mosaic here |
Herschel | FIR -- PACS (70,160 um) and SPIRE (250, 350, 500 um) |
|
get the PACS-70 mosaic here get the PACS-160 mosaic here get the SPIRE-250 mosaic here get the SPIRE-350 mosaic here get the SPIRE-500 mosaic here |
SCUBA | Sub-mm -- 450 and 850 um |
|
scuba (Note that data range here is much different than for the other images here)
get the SCUBA-450 mosaic here get the SCUBA-850 mosaic here - |