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 6 X081756.44-072217.2 chandra ccd3 763.841 59.6432 12.0747 3.47487 0.00237463 0.000683374 18.0997 1 0.448431 0.24654 157.934 0.775908 F F 7.35e+20 2.64027e-14 1 dsx
Report srcpi bgdpi arf 2 X081802.95-071912.2 chandra ccd3 566.7 435.2 9.86391 3.16228 0.00193985 0.000621898 14.7858 1 0.606495 0.492 24.1949 3.42714 F F 7.32e+20 2.29599e-14 1 dx
Report 7 X081812.27-072353.5 chandra ccd2 992.75 613.375 7.89951 2.82843 0.00155448 0.000556582 11.7759 1 0.689249 0.492 69.7909 3.4677 F F 7.24e+20 0 1 d
Report srcpi bgdpi arf 6 X081830.48-072501.2 chandra ccd2 442.25 475.625 7.39515 2.82844 0.00145523 0.000556585 11.0241 1 1.66232 0.639391 60.5307 8.0948 A F 7.07e+20 2.11945e-14 1 dx
Report srcpi bgdpi arf 5 X081831.71-072601.8 chandra ccd2 405.25 352.5 6.67582 2.82846 0.00131368 0.000556587 9.95177 1 2.4012 1.78279 69.4336 8.73868 F F 7.05e+20 1.84249e-14 1 dx
Report srcpi bgdpi arf 1 X081804.84-072032.7 chandra ccd3 509.333 271.5 5.9171 2.44949 0.00116367 0.00048172 8.86961 1 0.492 0.492 2.55731e-08 2.38544 F F 7.31e+20 1.35074e-14 1 dx
Report srcpi bgdpi arf 1 X081740.45-072122.3 chandra ccd1 487 916.667 5.81965 2.44949 0.0011445 0.000481721 7.25282 0.999995 0.598498 0.492 140.04 4.84413 F F 7.42e+20 1.33987e-14 1 dx
Report srcpi bgdpi arf 1 X081829.58-072114.5 chandra ccd2 469.333 936.5 5.74802 2.4495 0.0011311 0.000482015 8.56868 0.999999 0.628998 0.492 42.6182 7.58363 F F 7.11e+20 1.60539e-14 1 dx
Report srcpi bgdpi arf 4 X081821.29-072812.8 chandra ccd2 720.333 86.3333 5.60273 2.4495 0.00110251 0.000482016 8.35209 0.999999 1.16399 0.851688 10.1974 7.86107 F F 7.12e+20 1.46839e-14 1 dx
Report srcpi bgdpi arf 5 X081749.82-071430.2 chandra ccd3 963.786 1008.21 5.53147 2.64579 0.00108783 0.000520324 8.29157 0.999993 1.87598 1.19919 6.79547 8.3604 A F 7.36e+20 1.56839e-14 1 dx
Report 3 X081747.44-072004.8 chandra ccd3 1035.75 328.25 3.90964 2 0.000768875 0.000393323 5.86047 0.999899 0.546002 0.492 1.78817 3.84566 F F 7.38e+20 0 1 d
Report srcpi bgdpi arf 1 X081758.64-072509.5 chandra ccd0 679.875 1184.88 3.87804 2.82851 0.00076266 0.000556259 5.12635 0.999681 4.35396 1.30429 92.4968 2.64867 A F 7.31e+20 8.68946e-15 1 dx
Report srcpi bgdpi arf 3 X081831.29-072216.9 chandra ccd2 417.75 809.5 3.60036 2.00001 0.000708484 0.000393565 5.36712 0.999894 1.20395 0.492 61.7933 7.90211 A F 7.09e+20 1.01649e-14 1 dx
Report 2 X081822.96-072104.5 chandra ccd2 669.5 956.833 2.81446 1.73206 0.000553833 0.000340837 4.19556 0.998805 0.627179 0.492 146.31 6.00982 F F 7.17e+20 0 1 d
Report 4 X081812.16-071711.0 chandra ccd3 288 681.5 1.86316 1.41422 0.000366411 0.000278122 2.79283 0.989438 0.9225 0.492 53.1301 6.19833 A F 7.28e+20 0 1 d

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