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 4 X003413.05-010027.2 chandra ccd7 851.33 1048.89 36.5235 6.20005 0.0181193 0.00307585 26.3779 1 0.421626 0.421626 0 1.02727 F F 2.43e+20 1.31369e-13 1 dsx
Report srcpi bgdpi arf 1 X003443.80-005416.2 chandra ccd2 692.409 431.47 29.8765 5.7446 0.0148215 0.00284986 89.5306 1 3.11081 2.0458 28.1691 10.3638 A F 2.39e+20 2.04013e-13 1 dx
Report 1 X003405.60-005957.3 chandra ccd6 604.314 181.716 18.4425 4.29447 0.00914934 0.00213049 55.5042 1 0.544145 0.544145 0 2.56908 F F 2.43e+20 0 1 ds
Report srcpi bgdpi arf 3 X003431.19-010556.8 chandra ccd7 297.833 378.389 8.35612 3.00001 0.00414542 0.00148829 6.03494 0.999994 2.15236 0.858164 42.649 6.2273 A F 2.43e+20 3.2422e-14 1 dx
Report 1 X003408.34-010045.3 chandra ccd7 994.5 1011.5 2.97502 1.73205 0.00147589 0.00085926 2.14861 0.95451 0.492 0.492 90 1.56404 F F 2.43e+20 0 1 d
Report 2 X003410.81-010030.6 chandra ccd7 919.167 1041.5 2.96995 1.73205 0.00147337 0.00085926 2.14495 0.95451 0.492 0.492 90 1.22718 F F 2.43e+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