SDSS Search for PNe in Milky Way Halo!



Useful Links:

PT: http://sdsshost2.apo.nmsu.edu/~snedden/PN/index.html
SDSS: http://cas.sdss.org/dr6/en/
SDSS image download: http://das.sdss.org/DR6-cgi-bin/DAS
DSS: http://archive.stsci.edu/cgi-bin/dss_form
SIMBAD: http://simbad.u-strasbg.fr/simbad/sim-fcoo
Acker Atlas: http://vizier.cfa.harvard.edu/viz-bin/VizieR-2?-kw.cat=V/84 (top button)
Kohoutek Atlas: http://vizier.cfa.harvard.edu/viz-bin/VizieR-2?-kw.cat=IV/24 (top button)
NED: http://nedwww.ipac.caltech.edu/forms/nearposn.html

12 Known SDSS PNe: http://www.astro.washington.edu/cmacleod/PNMW/knownPN/


Candidates:

objIDrunreruncamcolfieldra (h:m:s)dec (d:m:s)ugrizFrom which query?
Click to view587726033317200021146240528711:13:1203:01:1319.8618.8019.4119.9319.99#2
Click to view587725470664753338133140510807:59:0642:52:2319.9818.3718.9624.3622.83#3
Click to view58772599411055005214534045716:38:3546:30:4421.2318.2720.0524.3622.80#3
Click to view587729409158152432224840523617:18:0330:55:3319.4118.3418.8719.8220.02#3
Click to view587730773875556365256640310721:56:1011:56:5219.317.1117.6424.3618.52#4
Click to view58772975167104617123284037216:42:4837:38:1218.8316.6618.419.8822.83#4
Click to view58773543069260190836504058813:33:2449:06:1320.0118.9919.6124.3622.83#4
Click to view587742550677585983530840313314:08:1617:53:5120.5118.4319.1519.8820.19#4
Click to view58774257751654403253144056312:24:2520:35:2721.8418.2719.3824.3622.83#4
Click to view588018056184922161391841410713:56:1550:15:4119.718.1620.9924.3622.82#4
Click to view588007003632762912134541124910:00:2659:22:5516.5615.5016.4217.6718.09#5,7
Click to view588007004198142039134541268416:55:0436:55:1716.7614.5415.7217.1918.79#5,7
Click to view587738947200024705446940313308:41:4725:50:4615.3314.0314.1114.2014.25#6
Click to view587739809959313530467040225115:41:4717:47:3415.2614.0614.1314.2414.32#6
Click to view587742060000509977519440148312:32:2921:23:0118.6517.4517.6017.7217.93#6
Click to view587742576459317342531440331515:02:0915:05:1816.7115.4815.5915.7015.77#6,7
Click to view587742611342884932532240411615:08:2413:25:2518.0216.8016.9817.2217.10#6,7
Click to view58772298173428539875240115511:07:22-1:07:4414.3813.2913.3513.4713.54#6
Click to view587735665312727104370540220315:32:0445:46:0814.7113.0513.6313.7613.89#6,7
Click to view587736541483368542390940216214:38:587:31:3615.3414.0914.0914.1414.20#6
Click to view58772975167196391523284038616:49:1535:51:5415.2613.9614.0814.1814.29#6,7
Click to view587725550659371154135040212108:11:1746:59:5614.5512.8413.2813.3113.38#6,7
Click to view587726015607668755145840439712:16:492:47:2518.5516.9024.8024.3622.83#6,7
Click to view58773697741842030540104069915:14:1130:08:3817.8116.6617.3416.7915.26#7
Click to view587736477059907622389440217815:21:238:13:0614.9813.8914.1714.3314.44#7
Click to view587735043620143162356040426309:49:2638:33:1116.8814.9615.2415.1115.06#7
Click to view587742904474075214539040611112:41:0818:35:5714.9414.0114.2914.4714.40#7
Click to view58774487371651496258494021108:51:5212:04:4714.9112.9713.2813.1813.12#7
Click to view58773077440947843725664046221:29:0311:20:4718.71-999916.2915.9615.76#7
Click to view587730817901658298257640514822:55:07-8:53:0520.7215.0619.1018.8618.73#7
Click HERE for Resulting targets from Query #8 (updated 1/2/08)


Past Queries: (most recent on top)

#8 (Alexei's (M31) cuts, but g doesn't have to be saturated) ----------(The following gave 10673 objects)----------
Select objID, run, rerun, camcol, field, ra, dec, u, g, r, i, z into mydb.pn13

From photoprimary

Where g-r <= -0.1
and u-g >= 0.4
and g < 17

and petroRad_r < 5.0
and sqrt((rowV*rowV)+(colV*colV)) < 1.0
and (psfMag_r - modelMag_r ) < 1.0 and

(flags_u&dbo.fphotoflags('SATURATED'))=0 and
(flags_r&dbo.fphotoflags('SATURATED'))=0 and
(flags_i&dbo.fphotoflags('SATURATED'))=0 and
(flags_z&dbo.fphotoflags('SATURATED'))=0

#7 (Alexei's (M31) cuts) --------------(The following gave 119 objects)--------------------------
Select objID, run, rerun, camcol, field, ra, dec, u, g, r, i, z into mydb.pn13

From photoprimary

Where g-r <= -0.1
and u-g >= 0.4
and g < 17

and petroRad_r < 5.0
and sqrt((rowV*rowV)+(colV*colV)) < 1.0
and (psfMag_r - modelMag_r ) < 1.0 and

(flags_g&dbo.fPhotoFlags('SATURATED'))>0 and
(flags_u&dbo.fphotoflags('SATURATED'))=0 and
(flags_r&dbo.fphotoflags('SATURATED'))=0 and
(flags_i&dbo.fphotoflags('SATURATED'))=0 and
(flags_z&dbo.fphotoflags('SATURATED'))=0

#6 (looser constraints) --------------(The following gave 273 objects)--------------------------
Select objID, run, rerun, camcol, field, ra, dec, u, g, r, i, z into mydb.pn11

From photoprimary

Where g-r < -0.0
and u-g > 1.0
and g < 21.
and petroRad_r < 5.0
and sqrt((rowV*rowV)+(colV*colV)) < 1.0
and (psfMag_r - modelMag_r ) < 1.0 and

(flags_g&dbo.fPhotoFlags('SATURATED'))>0 and
(flags_u&dbo.fphotoflags('SATURATED'))=0 and
(flags_r&dbo.fphotoflags('SATURATED'))=0 and
(flags_i&dbo.fphotoflags('SATURATED'))=0 and
(flags_z&dbo.fphotoflags('SATURATED'))=0

#5 (now want g saturated) --------------(The following gave 12 objects)--------------------------
Select objID, run, rerun, camcol, field, ra, dec, u, g, r, i, z into mydb.pn85

From photoprimary

Where g-r < -0.5
and u-g > 1.0
and r-i < -0.5
and r-z < -0.5
and petroRad_r < 5.0
and sqrt((rowV*rowV)+(colV*colV)) < 1.0
and (psfMag_r - modelMag_r ) < 1.0 and

(flags_g&dbo.fPhotoFlags('SATURATED'))>0 and
(flags_u&dbo.fphotoflags('SATURATED'))=0 and
(flags_r&dbo.fphotoflags('SATURATED'))=0 and
(flags_i&dbo.fphotoflags('SATURATED'))=0 and
(flags_z&dbo.fphotoflags('SATURATED'))=0

#4 -------------------------------(The following gave 263 objects)--------------------------------
Select objID, run, rerun, camcol, field, ra, dec, u, g, r, i, z into mydb.pn6

From photoprimary

Where g-r < -0.5
and u-g > 1.0
and g < 19.0
and r-i < -0.5
and r-z < -0.5
and petroRad_r < 5.0
and sqrt((rowV*rowV)+(colV*colV)) < 1.0
--get rid of objects moving more than 1 degree a day
and (psfMag_r - modelMag_r ) < 0.5
--resolved in r
and

(flags_g&dbo.fPhotoFlags('SATURATED'))=0 and
(flags_u&dbo.fphotoflags('SATURATED'))=0 and
(flags_r&dbo.fphotoflags('SATURATED'))=0 and
(flags_i&dbo.fphotoflags('SATURATED'))=0 and
(flags_z&dbo.fphotoflags('SATURATED'))=0

#3 -------------------------------(The following gave 1,568 objects)--------------------------------
Select objID, run, rerun, camcol, field, ra, dec, u, g, r, i, z into mydb.pn5

From photoprimary

Where g-r < -0.5
and u-g > 1.0
and g < 19.0
and r-i < -0.5
and r-z < -0.5
and petroRad_r < 5.0
and sqrt((rowV*rowV)+(colV*colV)) < 4.0 --get rid of moving objects
and

(flags_g&dbo.fPhotoFlags('SATURATED'))=0 and
(flags_u&dbo.fphotoflags('SATURATED'))=0 and
(flags_r&dbo.fphotoflags('SATURATED'))=0 and
(flags_i&dbo.fphotoflags('SATURATED'))=0 and
(flags_z&dbo.fphotoflags('SATURATED'))=0

#2 -------------------------------(The following gave 1,666 objects)--------------------------------
Select objID, run, rerun, camcol, field, ra, dec, u, g, r, i, z into mydb.pn3

From photoprimary

Where g-r < -0.5
and u-g > 1.0
and g < 19.0
and r-i < -0.5
and r-z < -0.5
and petroRad_r < 5.0
and

(flags_g&dbo.fPhotoFlags('SATURATED'))=0 and
(flags_u&dbo.fphotoflags('SATURATED'))=0 and
(flags_r&dbo.fphotoflags('SATURATED'))=0 and
(flags_i&dbo.fphotoflags('SATURATED'))=0 and
(flags_z&dbo.fphotoflags('SATURATED'))=0

#1 -------------------------------(The following gave 20,366 objects)--------------------------------
Select objID, run, rerun, camcol, field, ra, dec, u, g, r, i, z into mydb.pn2

From photoprimary

Where g-r < -0.5
and u-g > 1.0
and g < 19.0
and

(flags_g&dbo.fPhotoFlags('SATURATED'))=0 and
(flags_u&dbo.fphotoflags('SATURATED'))=0 and
(flags_r&dbo.fphotoflags('SATURATED'))=0 and
(flags_i&dbo.fphotoflags('SATURATED'))=0 and
(flags_z&dbo.fphotoflags('SATURATED'))=0

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White Dwarfs:

Here's a sample of 50 spectroscopically confirmed WDs from Eisenstein et al. (2006): WD list
and here's a list of just the coordinates so you can copy them into the image list tool on SDSS, since we want to know what
these look like so we can filter them out: WD coords
and finally, here are some quick plots showing magnitudes for a sample of 15 WDs: plots


Background image from Harvard-Smithsonian CFA