CephC-LABS Data list

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)	data access main page at SDSS FinderChart gives you small tiles Skyview gives you larger tiles	sdss-skyview (so that we remember it's SDSS, from Skyview) get the images here
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) get the images here
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) get the images here
2MASS	NIR -- JHKs (1.2-2.2 um)	main page for 2MASS FinderChart gives you small tiles Skyview gives you larger tiles	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. get the images here
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. 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 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)	WISE archive FinderChart gives you large tiles	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)	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 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; I'm not sure which is better (yet), so they're both in there. 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)	herschel/pacscropped and herschel/spirecropped; herschel/bigmosaics/pacs/*js*cropped* and herschel/bigmosaics/spire/*cropped*
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) -