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 2 X112150.89+042035.8 chandra ccd2 705.7 244.059 90.2865 9.50192 0.0137174 0.00144364 96.3178 1 1.35679 0.804315 102.187 4.22165 F F 3.94e+20 2.55767e-13 1 dsx
Report srcpi bgdpi arf 1 X112223.27+041948.7 chandra ccd0 687.318 543.434 14.7319 3.83822 0.00223825 0.000583149 15.6829 1 0.915762 0.915762 0 4.48569 F F 3.92e+20 2.63181e-14 1 dsx
Report srcpi bgdpi arf 2 X112212.43+041412.2 chandra ccd1 820.889 329.375 15.1305 3.88979 0.00229881 0.000590985 15.7449 1 1.11307 1.11307 0 4.72655 F F 3.92e+20 2.71895e-14 1 dsx
Report srcpi bgdpi arf 2 X112224.44+041749.8 chandra ccd0 651.389 301.278 8.77326 3 0.00133293 0.000455794 9.33958 1 0.539458 0.492 36.9546 4.69197 F F 3.93e+20 1.57076e-14 1 dx
Report srcpi bgdpi arf 3 X112225.09+041815.1 chandra ccd0 631.5 352.667 5.81977 2.44949 0.000884204 0.000372154 6.19544 0.999962 0.492 0.492 31.088 4.80042 F F 3.92e+20 1.04463e-14 1 dx
Report srcpi bgdpi arf 1 X112208.46+041639.4 chandra ccd1 941 628.167 5.73765 2.4495 0.000871728 0.000372155 5.97063 0.999949 0.761607 0.492 58.0909 2.08363 A F 3.94e+20 9.84673e-15 1 dx
Report srcpi bgdpi arf 1 X112155.93+041543.7 chandra ccd3 365.9 133.9 4.81896 2.23607 0.00073215 0.000339729 5.01676 0.999609 0.594995 0.492 45 3.82725 F F 3.94e+20 8.47617e-15 1 dx
Report 1 X112207.20+042217.5 chandra ccd2 209.25 450.25 3.90425 2 0.000593177 0.000303863 4.16507 0.997884 0.505274 0.492 161.565 3.66557 F F 3.92e+20 0 1 d
Report srcpi bgdpi arf 2 X112142.29+041841.9 chandra ccd3 780.75 496.25 3.81707 2.00001 0.000579931 0.000303863 3.97374 0.997394 0.568667 0.492 45 5.88585 F F 3.95e+20 7.36671e-15 1 dx
Report srcpi bgdpi arf 5 X112227.97+041242.4 chandra ccd1 347.75 146.5 3.70725 2.00001 0.000563247 0.000303863 3.85779 0.997384 0.492 0.492 180 8.09282 F F 3.9e+20 7.25166e-15 1 dx
Report srcpi bgdpi arf 3 X112209.60+041647.9 chandra ccd1 906.5 645.5 2.89657 1.73205 0.000440079 0.000263153 3.01418 0.985349 0.492 0.492 90 2.05911 F F 3.94e+20 4.95585e-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