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 rmf | 1 | X014622.19+614504.2 | xmm | pn | 316.716 | 311.507 | 161843 | 421.343 | 26.9708 | 0.070216 | 2340.08 | 1 | 6.94166 | 6.94166 | 0 | 1.6145 | F | F | 0.43066 | 7.20505e-11 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf rmf | 2 | X014629.57+614229.6 | xmm | pn | 304.686 | 275.962 | 139.017 | 41.7271 | 0.0231669 | 0.00695374 | 2.01004 | 0.977549 | 6.81296 | 6.81296 | 0 | 1.61816 | F | F | 0.469683 | 7.18749e-14 | 1 | dscx | ||||
| Report | srcpi bgdpi arf | 3 | X014626.90+614318.4 | xmm | pn | 309.036 | 288.051 | 206.815 | 25.4449 | 0.0512472 | 0.00630506 | 2.99033 | 0.998545 | 10.875 | 10.875 | 0 | 1.07585 | T | F | 0.457312 | 1.26277e-13 | 1 | dbcx | ||||
| Report | srcpi bgdpi arf rmf | 4 | X014628.13+614254.1 | xmm | pn | 307.027 | 281.577 | 164.369 | 35.461 | 0.0273917 | 0.00590948 | 2.3766 | 0.990943 | 8.22103 | 8.22103 | 0 | 1.34148 | F | F | 0.463033 | 7.35365e-14 | 1 | dscx | ||||
| Report | srcpi bgdpi arf rmf | 5 | X014630.93+614156.6 | xmm | pn | 302.464 | 268.363 | 198.967 | 30.8235 | 0.0331574 | 0.00513667 | 2.87685 | 0.997902 | 8.04491 | 8.04491 | 0 | 2.08554 | F | F | 0.475786 | 1.00808e-13 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X014728.61+614827.4 | xmm | mos2 | 208.471 | 358.361 | 13.6584 | 8.03905 | 0.00231995 | 0.00136548 | 2.11424 | 0.979915 | 6.40369 | 2.58407 | 110.72 | 7.81541 | F | F | 0.347565 | 6.58714e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X014453.88+614041.3 | xmm | mos1 | 461.219 | 251.696 | 25.9238 | 6.79878 | 0.00440201 | 0.00115447 | 0 | 10.875 | 10.875 | 0 | 12.2786 | F | F | 0.538326 | 8.57529e-14 | 1 | dx | |||||
| Report | srcpi bgdpi arf | 1 | X014454.47+614043.7 | xmm | mos2 | 460.26 | 252.124 | 15.4497 | 6.9246 | 0.00262421 | 0.00117618 | 2.39152 | 0.990132 | 4.05755 | 4.05755 | 0 | 12.2151 | F | F | 0.537689 | 7.88434e-14 | 1 | dsx |
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 - 10.00 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), A = 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