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 1 X123049.14+122329.1 chandra ccd7 353.884 692.245 938.913 43.707 0.19352 0.00900849 36.7848 1 1.48 1.48 0 0.744599 T F 1.94e+20 0 1 dsc
Report 3 X123048.61+122332.4 chandra ccd7 369.64 699.039 1283.01 45.4162 0.264443 0.0093608 50.2658 1 0.69442 0.44838 341.299 0.683941 T F 1.93e+20 0 1 ds
Report 4 X123048.23+122335.1 chandra ccd7 381.023 704.344 117.98 28.4543 0.024317 0.00586475 4.62223 0.999997 0.824558 0.824558 0 0.635132 T F 1.93e+20 0 1 ds
Report 5 X123047.12+122416.1 chandra ccd7 414.068 787.738 58.5177 12.9257 0.0120611 0.00266414 2.29261 0.988824 0.338555 0.338555 0 0.263853 F F 1.93e+20 0 1 ds
Report 13 X123048.27+122350.5 chandra ccd7 379.79 735.649 52.1705 21.7883 0.0107529 0.00449081 2.04394 0.978178 1.5 1.5 0 0.389694 T F 1.93e+20 0 1 ds
Report 15 X123049.38+122328.3 chandra ccd7 346.821 690.587 6009.89 83.3372 1.2387 0.0171767 235.456 1 0.754977 0.412067 337.654 0.799582 A F 1.94e+20 0 1 dsc

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