CephC-LABS Data list - Revision history

Rebull at 23:04, 23 July 2017

2017-07-23T23:04:16Z

Rebull at 23:00, 23 July 2017

2017-07-23T23:00:55Z

Rebull at 22:55, 23 July 2017

2017-07-23T22:55:51Z

Rebull at 22:54, 23 July 2017

2017-07-23T22:54:07Z

Rebull at 19:14, 16 July 2017

2017-07-16T19:14:32Z

Rebull at 19:13, 16 July 2017

2017-07-16T19:13:52Z

Rebull at 19:11, 16 July 2017

2017-07-16T19:11:07Z

Rebull at 15:55, 18 May 2017

2017-05-18T15:55:11Z

Rebull at 15:54, 18 May 2017

2017-05-18T15:54:06Z

Rebull at 15:53, 18 May 2017

2017-05-18T15:53:10Z

@@ Line 52: / Line 52: @@
 '''[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 mosaic here]'''
+'''[https://caltech.box.com/s/wj5ntke0kkwhtq9s0f276wzxrtlg34eq get the MIPS-1 mosaic here]'''
 |-
 | Spitzer - postcryo era, GLIMPSE data
@@ Line 81: / Line 81: @@
 *[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*
 |-
 | SCUBA
@@ Line 88: / Line 93: @@
 *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)
+-
 |}

@@ Line 48: / Line 48: @@
 *(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
@@ Line 65: / Line 70: @@
 *[http://irsa.ipac.caltech.edu/applications/FinderChart/ FinderChart] gives you large tiles
 | FinderChartFiles/*w?.fits
 |-
 | Herschel

@@ Line 18: / Line 18: @@
 *[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)
 |-
 | PanSTARRS
@@ Line 23: / Line 24: @@
 | [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)
 |-
 | IPHAS
@@ Line 28: / Line 30: @@
 | [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)
 |-
 | 2MASS

@@ Line 36: / Line 36: @@
 *[http://skyview.gsfc.nasa.gov/current/cgi/query.pl 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.
 |-
 | Spitzer - cryo era

@@ Line 66: / Line 66: @@
+|
 *[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 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/*js*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/*cropped* and herschel/bigmosaics/spire/*cropped*
+| <strike>herschel/pacscropped and herschel/spirecropped;</strike> herschel/bigmosaics/pacs/*js*cropped* and herschel/bigmosaics/spire/*cropped*
 |-
 | SCUBA

@@ Line 66: / Line 66: @@
+|
 *[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). 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)
+*[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; I'm not sure which is better (yet), so they're both in there. 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/ and herschel/bigmosaics/spire
 |-