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 | X135704.45+191907.5 | chandra | ccd7 | 701.107 | 662.115 | 24841.7 | 161.87 | 0.56544 | 0.00368445 | 2117.79 | 1 | 0.420638 | 0.420638 | 0 | 0.0290354 | F | F | 2.49e+20 | 5.25503e-12 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf rmf | 2 | X135708.60+191828.0 | chandra | ccd7 | 581.823 | 581.851 | 140.289 | 12.5071 | 0.00319323 | 0.000284683 | 11.9598 | 1 | 0.436706 | 0.436706 | 0 | 1.17315 | F | F | 2.49e+20 | 2.29314e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 3 | X135704.81+191840.6 | chandra | ccd7 | 690.786 | 607.594 | 69.968 | 10.2701 | 0.00159259 | 0.000233766 | 5.96486 | 1 | 0.977819 | 0.977819 | 0 | 0.466486 | T | F | 2.49e+20 | 1.13885e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 4 | X135704.78+191851.5 | chandra | ccd7 | 691.625 | 629.704 | 75.7173 | 13.1739 | 0.00172346 | 0.00029986 | 6.455 | 1 | 0.802573 | 0.802573 | 0 | 0.293849 | T | F | 2.49e+20 | 1.23183e-14 | 1 | dscpx | ||||
| Report | srcpi bgdpi arf | 5 | X135704.73+191853.8 | chandra | ccd7 | 693.092 | 634.424 | 63.8904 | 9.19018 | 0.00145426 | 0.000209184 | 5.44674 | 1 | 0.7688 | 0.7688 | 0 | 0.245714 | F | F | 2.49e+20 | 1.03926e-14 | 1 | dscx | ||||
| Report | srcpi bgdpi arf | 6 | X135704.60+191859.0 | chandra | ccd7 | 696.89 | 644.856 | 26.2749 | 12.3592 | 0.000598063 | 0.000281317 | 2.23997 | 0.984535 | 0.401374 | 0.401374 | 0 | 0.153805 | F | F | 2.49e+20 | 4.27308e-15 | 1 | dscx | ||||
| Report | srcpi bgdpi arf | 7 | X135705.49+192007.3 | chandra | ccd7 | 671.239 | 783.685 | 56.9899 | 8.7325 | 0.00129719 | 0.000198767 | 4.85846 | 0.999998 | 0.379266 | 0.379266 | 0 | 1.00329 | F | F | 2.49e+20 | 9.29164e-15 | 1 | dsx | ||||
| Report | srcpi bgdpi arf rmf | 8 | X135708.76+191725.3 | chandra | ccd7 | 577.053 | 454.437 | 122.142 | 11.6655 | 0.00278017 | 0.000265527 | 10.4128 | 1 | 0.583417 | 0.353275 | 353.587 | 1.98983 | F | F | 2.49e+20 | 2.02426e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 9 | X135702.74+191841.2 | chandra | ccd7 | 750.354 | 608.653 | 28.0127 | 6.83337 | 0.000637617 | 0.000155539 | 2.38812 | 0.98979 | 1.5 | 0.391902 | 47.3624 | 0.615672 | A | F | 2.49e+20 | 4.56432e-15 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 10 | X135703.29+191849.4 | chandra | ccd7 | 734.548 | 625.318 | 23.4689 | 8.36604 | 0.000534193 | 0.000190426 | 2.00075 | 0.977075 | 1.5 | 0.319211 | 48.919 | 0.45178 | A | F | 2.49e+20 | 3.81859e-15 | 1 | dsbx | ||||
| Report | srcpi bgdpi arf | 11 | X135704.60+191858.2 | chandra | ccd7 | 696.737 | 643.347 | 70.289 | 14.2382 | 0.0015999 | 0.000324085 | 5.99223 | 1 | 1.0494 | 1.0494 | 0 | 0.203257 | T | F | 2.49e+20 | 1.14307e-14 | 1 | dscbx | ||||
| Report | srcpi bgdpi arf | 21 | X135705.98+191931.0 | chandra | ccd7 | 657.101 | 709.867 | 25.6094 | 7.07515 | 0.000582914 | 0.000161043 | 2.18323 | 0.984535 | 1.5 | 0.598606 | 45.905 | 0.527717 | T | F | 2.49e+20 | 4.16729e-15 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 22 | X135717.41+191601.6 | chandra | ccd7 | 328.205 | 284.432 | 35.0082 | 7.01358 | 0.000796846 | 0.000159641 | 2.98449 | 0.997982 | 0.76201 | 0.76201 | 0 | 4.35082 | F | F | 2.49e+20 | 6.02877e-15 | 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