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 X043918.73+222238.2 chandra ccd7 127.184 429.73 36.2894 6.07075 0.00369801 0.000618629 11.9429 1 0.429142 0.429142 0 1.81513 F F 1.87e+21 0 1 ds
Report srcpi bgdpi arf 2 X043916.98+222515.7 chandra ccd7 176.31 749.888 97.7665 9.88769 0.00996272 0.00100759 32.175 1 1.22364 0.718696 347.391 4.45373 A F 1.86e+21 8.33165e-14 1 dsx
Report srcpi bgdpi arf 3 X043914.19+222643.1 chandra ccd7 254.611 927.056 7.47822 3.00003 0.000762052 0.000305711 2.46109 0.986107 1.34674 0.492 50.2218 5.97999 A F 1.86e+21 6.58635e-15 1 dx
Report srcpi bgdpi arf rmf 4 X043917.79+222103.3 chandra ccd7 153.422 236.947 578.554 24.6107 0.0589565 0.00250791 190.403 1 0.400199 0.400199 0 0.284841 F F 1.87e+21 3.15575e-13 1 dsxf
Report srcpi bgdpi arf 5 X043921.26+222019.0 chandra ccd7 55.1667 146.333 5.78498 2.4495 0.000589506 0.00024961 1.90384 0.973075 0.492 0.492 69.1832 0.814273 F F 1.88e+21 4.79237e-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