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 | X043455.49+242852.4 | xmm | pn | 318.829 | 310.569 | 1013.43 | 39.1683 | 0.0910052 | 0.00351728 | 55.5457 | 1 | 5.18204 | 5.18204 | 0 | 1.73727 | 622.717 | 644.89 | 0.0174918 | 0.0302054 | F | T | 1.57e+21 | 3.13517e-13 | 1 | dsx |
Report | srcpi bgdpi arf rmf | 1 | X043455.47+242851.6 | xmm | mos1 | 318.908 | 310.4 | 604.317 | 30.0262 | 0.0393418 | 0.00195475 | 47.894 | 1 | 5.26977 | 4.55543 | 81.7146 | 1.72352 | 273.684 | 348.474 | 0.12021 | 0.0427015 | F | T | 1.57e+21 | 6.00604e-13 | 1 | dsx |
Report | srcpi bgdpi arf rmf | 1 | X043455.50+242851.9 | xmm | mos2 | 318.802 | 310.466 | 547.43 | 29.5227 | 0.0356334 | 0.00192169 | 30.4053 | 1 | 5.44273 | 4.1427 | 36.0583 | 1.7213 | 231.911 | 332.851 | 0.178731 | 0.0451922 | F | T | 1.57e+21 | 5.4656e-13 | 1 | dsx |
Report | srcpi bgdpi arf | 2 | X043504.37+242239.4 | xmm | pn | 290.973 | 224.823 | 65.4663 | 17.1932 | 0.00587879 | 0.00154393 | 3.58818 | 0.999764 | 4.77134 | 4.77134 | 0 | 5.35966 | 36.2207 | 25.5242 | -0.173237 | 0.171502 | F | F | 1.58e+21 | 3.60848e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 3 | X043512.57+243019.9 | xmm | pn | 265.236 | 330.706 | 64.7649 | 17.6785 | 0.00581581 | 0.00158751 | 3.54974 | 0.999714 | 7.33462 | 3.79976 | 89.2 | 3.35643 | 16.3475 | 48.779 | 0.497978 | 0.188686 | F | F | 1.59e+21 | 3.75535e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 4 | X043502.43+242919.7 | xmm | pn | 297.059 | 316.203 | 65.9782 | 15.1686 | 0.00592476 | 0.00136213 | 5.69918 | 1 | 10.875 | 10.875 | 0 | 1.2919 | 31.5729 | 31.6957 | 0.00194111 | 0.232522 | T | F | 1.58e+21 | 2.75716e-14 | 1 | dbpx |
Report | srcpi bgdpi arf | 3 | X043504.47+242240.1 | xmm | mos1 | 290.64 | 224.989 | 36.4429 | 11.4776 | 0.00237248 | 0.000747209 | 2.88821 | 0.997355 | 3.64427 | 3.64427 | 0 | 5.35728 | 22.3844 | 14.0931 | -0.2273 | 0.218788 | F | F | 1.58e+21 | 6.24009e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 5 | X043433.62+242738.8 | xmm | pn | 387.483 | 294.214 | 37.5297 | 13.4399 | 0.00337013 | 0.00120688 | 3.47751 | 0.999623 | 10.875 | 10.875 | 0 | 6.46312 | 19.1247 | 18.0387 | -0.0292229 | 0.351075 | F | F | 1.55e+21 | 1.75942e-14 | 1 | dpx |
Report | srcpi bgdpi arf | 2 | X043512.56+243019.1 | xmm | mos1 | 265.28 | 330.517 | 37.5454 | 11.0735 | 0.00244425 | 0.000720897 | 2.97559 | 0.9979 | 5.18707 | 5.18707 | 0 | 3.32196 | 5.50316 | 33.4388 | 0.717366 | 0.259499 | F | F | 1.59e+21 | 4.54695e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 6 | X043537.70+242238.9 | xmm | pn | 186.267 | 224.939 | 25.763 | 12.694 | 0.00231349 | 0.00113991 | 2.45377 | 0.992369 | 10.875 | 10.875 | 0 | 9.72258 | 27.5249 | -2.34179 | -1 | 0.630397 | F | F | 1.61e+21 | 2.01211e-14 | 1 | dx |
Report | srcpi bgdpi arf | 2 | X043512.74+243020.6 | xmm | mos2 | 264.714 | 330.876 | 45.988 | 10.9875 | 0.00299346 | 0.000715199 | 6.31623 | 1 | 10.875 | 10.875 | 0 | 3.39243 | 4.20035 | 40.8534 | 0.813541 | 0.308963 | F | F | 1.59e+21 | 4.55442e-14 | 1 | dbx |
Report | srcpi bgdpi arf | 4 | X043420.18+241814.2 | xmm | mos1 | 429.829 | 163.83 | 25.6874 | 9.76071 | 0.00167228 | 0.000635434 | 3.62145 | 0.999717 | 10.875 | 10.875 | 0 | 13.6375 | 17.0128 | 10.3391 | -0.243994 | 0.36571 | F | F | 1.53e+21 | 4.48419e-14 | 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 - 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