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 | X104924.65-041645.2 | xmm | pn | 111.867 | 245.134 | 93.7977 | 17.487 | 0.0240747 | 0.00448832 | 0 | 10.875 | 10.875 | 0 | 14.0675 | U | U | 3.5e+20 | d | ||||||||
| Report | 2 | X104924.27-041725.0 | xmm | pn | 113.152 | 237.087 | 77.1087 | 15.8796 | 0.0197912 | 0.00407575 | 0 | 10.875 | 10.875 | 0 | 14.1503 | U | U | 3.5e+20 | d | ||||||||
| Report | 3 | X104922.94-041606.2 | xmm | pn | 117.74 | 252.597 | 71.8802 | 15.4454 | 0.0184492 | 0.00396431 | 0 | 10.875 | 10.875 | 0 | 13.5155 | U | U | 3.51e+20 | d | ||||||||
| Report | 4 | X104923.13-041637.7 | xmm | pn | 117.077 | 245.883 | 73.3603 | 16.1548 | 0.0188291 | 0.00414639 | 0 | 10.875 | 10.875 | 0 | 13.6895 | U | U | 3.5e+20 | d | ||||||||
| Report | 5 | X104829.79-041750.7 | xmm | pn | 300.485 | 230.158 | 70.6593 | 15.608 | 0.0181358 | 0.00400605 | 0 | 10.875 | 10.875 | 0 | 4.95246 | U | U | 3.65e+20 | d | ||||||||
| Report | 6 | X104914.28-041543.1 | xmm | pn | 147.512 | 260.143 | 95.4236 | 17.6849 | 0.024492 | 0.00453911 | 0 | 10.875 | 10.875 | 0 | 11.2888 | U | U | 3.53e+20 | 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 - 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