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 | 1 | X175322.53-290535.5 | chandra | ccd0 | 726.326 | 486.555 | 18.3992 | 4.28943 | 0.00854241 | 0.0019915 | 37.3354 | 1 | 1.78121 | 0.824647 | 158.925 | 5.20478 | F | F | 6.57e+21 | 1.21885e-13 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 2 | X175305.25-291630.3 | chandra | ccd1 | 1032.5 | 183.5 | 7.58722 | 2.82844 | 0.00352258 | 0.00131318 | 14.9603 | 1 | 1.30566 | 0.863804 | 53.2522 | 8.11172 | A | F | 6.47e+21 | 5.18932e-14 | 1 | dx | ||||
Report | 1 | X175334.97-291004.1 | chandra | ccd1 | 241.214 | 967.928 | 6.8609 | 2.64575 | 0.00318536 | 0.00122836 | 13.5282 | 1 | 0.830155 | 0.492 | 179.682 | 7.28226 | A | F | 6.27e+21 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 1 | X175259.39-291210.7 | chandra | ccd3 | 146.333 | 532 | 5.95439 | 2.44949 | 0.00276449 | 0.00113724 | 11.8728 | 1 | 0.492 | 0.492 | 65.8168 | 3.82387 | F | F | 6.68e+21 | 3.72534e-14 | 1 | dx | ||||
Report | 3 | X175246.39-290721.9 | chandra | ccd2 | 654.5 | 108.9 | 4.98152 | 2.23607 | 0.00231614 | 0.00103965 | 9.99761 | 1 | 0.492 | 0.492 | 53.3496 | 3.66688 | F | F | 7.04e+21 | 0 | 1 | d | |||||
Report | 2 | X175259.06-290524.4 | chandra | ccd2 | 317.1 | 347.9 | 4.97121 | 2.23607 | 0.00231135 | 0.00103965 | 9.97692 | 1 | 0.492 | 0.492 | 45 | 3.09993 | F | F | 6.92e+21 | 0 | 1 | d | |||||
Report | 2 | X175317.96-290727.0 | chandra | ccd0 | 847.833 | 259.5 | 2.96358 | 1.73205 | 0.00137592 | 0.000804152 | 6.01365 | 0.999881 | 0.492 | 0.492 | 180 | 3.51442 | F | F | 6.58e+21 | 0 | 1 | d | |||||
Report | 5 | X175312.69-291310.6 | chandra | ccd1 | 834.5 | 589.167 | 2.95477 | 1.73205 | 0.00137183 | 0.000804153 | 5.82613 | 0.999851 | 0.492 | 0.492 | 130.269 | 5.25747 | F | F | 6.47e+21 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 1 | X175306.50-290530.3 | chandra | ccd2 | 118.833 | 335.833 | 2.93984 | 1.73205 | 0.00136687 | 0.000805312 | 5.90007 | 0.99987 | 0.492 | 0.492 | 73.155 | 3.03944 | F | F | 6.81e+21 | 1.88907e-14 | 1 | dx | ||||
Report | 4 | X175309.65-291150.1 | chandra | ccd1 | 915.167 | 752.833 | 2.93778 | 1.73205 | 0.00136395 | 0.000804153 | 5.79264 | 0.999851 | 0.492 | 0.492 | 109.903 | 3.7617 | F | F | 6.55e+21 | 0 | 1 | d | |||||
Report | 3 | X175305.21-291301.2 | chandra | ccd1 | 1033.5 | 608.5 | 0.982726 | 1 | 0.000456257 | 0.000464278 | 1.93771 | 0.972082 | 0.492 | 0.492 | 90 | 4.64252 | F | F | 6.57e+21 | 0 | 1 | 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 - 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