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 | X000953.38+255525.6 | chandra | ccd7 | 519.028 | 316.913 | 407.444 | 23.7569 | 0.0209521 | 0.00122166 | 91.862 | 1 | 1.67386 | 1.67386 | 0 | 0.280369 | T | F | 3.42e+20 | 8.00182e-14 | 1 | dsxf | ||||
Report | srcpi bgdpi arf | 2 | X000954.28+255403.5 | chandra | ccd7 | 494.233 | 149.955 | 17.1095 | 4.46086 | 0.000879829 | 0.000229393 | 3.8575 | 0.999687 | 0.599725 | 0.599725 | 0 | 1.10641 | F | F | 3.41e+20 | 6.59781e-15 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 3 | X000952.65+255403.2 | chandra | ccd7 | 538.5 | 148.944 | 8.10548 | 3.00002 | 0.00041681 | 0.000154271 | 1.82746 | 0.955367 | 0.492 | 0.492 | 77.3269 | 1.12215 | F | F | 3.41e+20 | 3.12898e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 4 | X000946.82+255412.2 | chandra | ccd7 | 698.899 | 167.766 | 23.8056 | 5.03644 | 0.00122416 | 0.000258991 | 5.36719 | 0.999998 | 0.435035 | 0.435035 | 0 | 1.80627 | F | F | 3.41e+20 | 9.21293e-15 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 5 | X000958.31+255417.6 | chandra | ccd7 | 383.937 | 178.644 | 14.3725 | 4.12314 | 0.000739079 | 0.000212025 | 3.24041 | 0.998861 | 0.549661 | 0.549661 | 0 | 1.35353 | F | F | 3.42e+20 | 5.53495e-15 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 7 | X000953.02+255538.8 | chandra | ccd7 | 528.789 | 343.714 | 9.56646 | 5.02009 | 0.000491939 | 0.000258149 | 2.15685 | 0.981986 | 0.31282 | 0.31282 | 0 | 0.513349 | F | F | 3.42e+20 | 3.79718e-15 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 8 | X000952.96+255548.0 | chandra | ccd7 | 529.955 | 361.864 | 9.33447 | 3.31665 | 0.000480009 | 0.000170553 | 2.10454 | 0.981986 | 0.573956 | 0.492 | 94.7312 | 0.665099 | F | F | 3.42e+20 | 3.71549e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 9 | X000958.79+255659.8 | chandra | ccd7 | 370.742 | 508.276 | 35.9772 | 6.40408 | 0.00185007 | 0.000329319 | 8.11139 | 1 | 0.609133 | 0.379559 | 115.284 | 2.17091 | A | F | 3.42e+20 | 1.38329e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 10 | X000948.38+255712.3 | chandra | ccd7 | 655.6 | 533.3 | 8.95034 | 3.1623 | 0.000460256 | 0.000162616 | 2.01794 | 0.971227 | 0.492 | 0.492 | 69.1832 | 2.37034 | F | T | 3.42e+20 | 3.42629e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 11 | X001002.78+255746.8 | chandra | ccd7 | 261.337 | 603.903 | 55.3964 | 7.87474 | 0.00284867 | 0.000404945 | 12.4896 | 1 | 0.868802 | 0.40763 | 115.205 | 3.33534 | F | F | 3.43e+20 | 2.1677e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 12 | X001002.63+255819.7 | chandra | ccd7 | 265.349 | 670.808 | 55.5952 | 7.81534 | 0.00285889 | 0.000401891 | 12.5345 | 1 | 0.808614 | 0.808614 | 0 | 3.76306 | F | F | 3.43e+20 | 2.1836e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 14 | X001008.53+255936.6 | chandra | ccd7 | 103.839 | 827.082 | 20.3542 | 4.51156 | 0.00104668 | 0.000232 | 4.58904 | 0.999982 | 2.08153 | 2.08153 | 0 | 5.56235 | F | F | 3.43e+20 | 8.25104e-15 | 1 | dsx | ||||
Report | srcpi bgdpi arf rmf | 15 | X000957.73+255347.4 | chandra | ccd7 | 399.708 | 117.156 | 182.878 | 13.5245 | 0.00940419 | 0.000695476 | 41.2315 | 1 | 0.569873 | 0.458132 | 62.8176 | 1.64345 | F | F | 3.41e+20 | 7.08228e-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 - 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