Source List

Observation details report
Detailed source parameters (including errors) in a comma-separated values file

Click on source number for detailed analysis, including spectral fits if applicable

data idnum idradec telescope instrument x y cnts cntserr rate rateerr SNR poisprob sigmaj sigmin incang offax cnts_soft cnts_hard hr hr_err ext var N_H flux vign flags
Report srcpi bgdpi arf 1 X082804.78+371902.4 chandra ccd7 1107.99 957.789 27.6382 5.2572 0.00453496 0.000862617 24.0965 1 0.604849 0.604849 0 2.21815 F F 3.8e+20 3.47143e-14 1 dsx
Report srcpi bgdpi arf 2 X082817.26+371853.8 chandra ccd7 805.363 940.121 12.2903 3.50575 0.00201663 0.000575236 10.7154 1 0.33748 0.33748 0 0.307438 F F 3.68e+20 1.48934e-14 1 dsx
Report srcpi bgdpi arf 8 X082826.69+371845.8 chandra ccd7 576.911 924.041 12.8851 3.58958 0.00211423 0.00058899 11.2339 1 0.650432 0.650432 0 2.15701 F F 3.66e+20 1.57333e-14 1 dsx
Report srcpi bgdpi arf 4 X082810.92+371910.8 chandra ccd7 959.215 974.709 10.5376 3.99161 0.00172904 0.000654955 9.18726 1 0.25509 0.25509 0 1.009 F F 3.78e+20 1.29383e-14 1 dsx
Report srcpi bgdpi arf 6 X082831.98+371325.9 chandra ccd7 447.591 273.227 9.3259 3.31666 0.00153021 0.000544203 8.13084 1 1.18516 0.751441 50.6399 6.4667 A F 3.65e+20 1.23686e-14 1 dx
Report srcpi bgdpi arf 1 X082748.38+372554.7 chandra ccd6 1006.14 874.591 8.99739 3.31666 0.00147631 0.000544204 11.8866 1 3.30019 1.04123 150.062 8.77421 A F 3.84e+20 1.83499e-14 1 dx
Report srcpi bgdpi arf 2 X082805.50+372431.7 chandra ccd6 591.75 705.583 10.9855 3.46412 0.00180252 0.000568399 14.5131 1 1.4367 1.07188 101.11 5.85339 F F 3.8e+20 2.34019e-14 1 dx
Report srcpi bgdpi arf 3 X082814.12+372234.3 chandra ccd6 383 466.75 7.85003 2.82843 0.00128805 0.000464094 10.3708 1 0.534679 0.492 131.437 3.53421 F F 3.77e+20 1.39217e-14 1 dx
Report srcpi bgdpi arf 3 X082816.58+371848.1 chandra ccd7 821.5 928 3.82034 2.00001 0.000626849 0.000328165 3.33079 0.997635 0.492 0.492 180 0.284204 F F 3.68e+20 4.63262e-15 1 dx
Report 4 X082806.39+372010.3 chandra ccd6 570.5 174.167 2.96878 1.73205 0.000487123 0.000284198 3.9221 0.997148 0.492 0.492 28.155 2.20233 F F 3.79e+20 0 1 d
Report srcpi bgdpi arf 5 X082809.46+372103.2 chandra ccd6 496 281.75 3.92462 2 0.000643959 0.000328164 5.18488 0.99968 0.492 0.492 137.382 2.37748 F F 3.78e+20 6.818e-15 1 dx
Report srcpi bgdpi arf 6 X082802.08+372322.1 chandra ccd6 674.667 564 5.49669 2.4495 0.000901907 0.000401919 7.26177 0.999998 1.38551 0.492 120.714 5.11662 A F 3.8e+20 1.03595e-14 1 dx
Report srcpi bgdpi arf 7 X082755.40+372133.7 chandra ccd6 836.667 343.833 5.89582 2.44949 0.000967397 0.000401917 7.78906 0.999998 0.492 0.492 149.679 4.78985 F T 3.82e+20 1.12105e-14 1 dx
Report srcpi bgdpi arf 5 X082808.22+371946.8 chandra ccd7 1024.17 1047.5 2.88603 1.73206 0.000473546 0.000284199 2.5162 0.988824 0.492 0.492 180 1.69769 F F 3.79e+20 3.57528e-15 1 dx

counts and rate are bgd.-subtracted, based on simple spatial fitting (if done) or extracted counts from aperture otherwise (N.B., in either case aperture counts are given csv file).
cntserr, rateerr = Error on (source) counts and count rate, based on error in total counts
SNR = signal-to-noise ratio, computed using Nsrc/sqrt(Nbgd)
poisprob = Poisson probability of observing total counts given bgd. counts
sigmaj, sigmin = source extent (from detection output or spatial fitting) in units of arcsecs.
incang = position angle of source (inclination from x-axis)
cnts_soft = bgd.-subtracted counts in soft band (0.50 - 2.00 KeV, always taken directly from source aperture rather than model fitting)
cnts_hard = bgd.-subtracted counts in hard band (2.00 - 7.99 KeV, always taken directly from source aperture rather than model fitting)
hr, hr_err = hardness ratio ([cnts_hard-cnts_soft]/[cnts_hard+cnts_soft]) and error
ext = source extension flag: F = false (not extended), T = true (extended), A = asymetric (ratio of sigmaj/sigmin > 1 + x, where x = 0.5 by default)
var = variability flag: U = unknown, F = false (is not variable), T = true
N_H = Galactic column density as determined from LHEASOFT nh program
flux = flux determined from count rate using pimms (in the 0.30-8.00 keV bandpass for a power-law model with ph. index = 1.8)
vign = vignetting correction
Flags: d = detection parameters, s = simple spatial fitting parameters, b = simple spatial fitting failed, p = poor simple spatial fit, x = extracted events parameters, t = temporal anaylsis parameters, i = psf spatial fitting parameters, f = spectral fitting parameters, c = source is confused, u = user-defined source, v = detected source coincident with user-defined source, r = source is in region-of-interest