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 | 2 | X104331.13+245520.7 | chandra | ccd7 | 567.813 | 587.515 | 13.3193 | 3.64956 | 0.00767893 | 0.00210407 | 24.0562 | 1 | 0.889732 | 0.889732 | 0 | 2.22393 | T | F | 2.46e+20 | 5.6143e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X104345.48+245714.9 | chandra | ccd7 | 170.7 | 819.3 | 9.81783 | 3.16228 | 0.00566015 | 0.00182311 | 17.7321 | 1 | 0.881044 | 0.492 | 159.672 | 3.34674 | A | F | 2.49e+20 | 4.43022e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X104420.67+245807.0 | chandra | ccd3 | 547.1 | 984.1 | 9.18117 | 3.31666 | 0.0052931 | 0.00191211 | 27.212 | 1 | 0.492 | 0.492 | 127.628 | 11.3208 | F | F | 2.53e+20 | 7.18452e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X104316.72+250520.7 | chandra | ccd6 | 857.333 | 733.667 | 5.52055 | 2.4495 | 0.00318269 | 0.00141218 | 16.5793 | 1 | 2.38665 | 1.4811 | 83.192 | 8.40558 | A | F | 2.46e+20 | 3.70363e-14 | 1 | dx | ||||
| Report | 3 | X104322.22+245737.0 | chandra | ccd7 | 813.7 | 864.1 | 4.9522 | 2.23607 | 0.00285503 | 0.00128913 | 8.94424 | 0.999999 | 0.492 | 0.492 | 47.3818 | 1.94159 | F | F | 2.46e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 6 | X104329.42+245522.3 | chandra | ccd7 | 614.5 | 590.3 | 4.93668 | 2.23607 | 0.00284608 | 0.00128913 | 8.91621 | 0.999999 | 0.492 | 0.492 | 129.345 | 2.21657 | F | F | 2.46e+20 | 2.07578e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X104330.75+245443.1 | chandra | ccd7 | 577.9 | 510.5 | 4.91085 | 2.23607 | 0.00283119 | 0.00128913 | 8.86955 | 0.999999 | 0.614809 | 0.492 | 161.216 | 2.84951 | F | F | 2.46e+20 | 2.08391e-14 | 1 | dx | ||||
| Report | 6 | X104314.13+250020.6 | chandra | ccd6 | 929 | 123.75 | 3.99 | 2 | 0.0023003 | 0.00115303 | 11.9828 | 1 | 0.492 | 0.492 | 60.1282 | 4.68443 | F | F | 2.45e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 4 | X104320.83+250134.1 | chandra | ccd6 | 744 | 273 | 3.98883 | 2 | 0.00229963 | 0.00115303 | 11.9792 | 1 | 0.492 | 0.492 | 90 | 4.59324 | F | F | 2.46e+20 | 2.45222e-14 | 1 | dx | ||||
| Report | 4 | X104328.28+245546.8 | chandra | ccd7 | 646 | 640 | 3.94721 | 2 | 0.00227564 | 0.00115303 | 7.12912 | 0.999983 | 0.493767 | 0.492 | 35.7825 | 1.875 | F | F | 2.46e+20 | 0 | 1 | d | |||||
| Report | 3 | X104319.05+250125.3 | chandra | ccd6 | 793.167 | 255.167 | 2.99959 | 1.73205 | 0.00172931 | 0.000998557 | 9.00834 | 0.999994 | 0.492 | 0.492 | 45 | 4.68291 | F | F | 2.46e+20 | 0 | 1 | d | |||||
| Report | 2 | X104328.35+250118.6 | chandra | ccd6 | 536.167 | 241.5 | 2.98132 | 1.73205 | 0.00171878 | 0.000998557 | 8.95348 | 0.999994 | 0.492 | 0.492 | 2.58572e-08 | 3.7836 | F | F | 2.47e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 5 | X104330.20+250422.9 | chandra | ccd6 | 485 | 616 | 1.85596 | 1.41422 | 0.00106999 | 0.000815322 | 5.5738 | 0.994289 | 0.940769 | 0.492 | 101.31 | 6.81546 | A | F | 2.48e+20 | 1.22323e-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 - 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