Table 3
Table of RXTE observations of other sources.
Data | State/ | 20% | ||||||||||
Source | ObsID | Date | mode | class | N | dt [s] | m | k | L max |
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N ϵ |
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GRS | 10408-01-08-00 | 21.05.1996 | Std1 | μ | 289 | 5 | 8 | 12 | 438 | 3.16 | – | 15 |
GRS | 10408-01-10-00B | 26.05.1996 | SB, ch0-35 | β | 6585 | 0.5 | 6 | 100 | 1439 | 5.00 | – | 33 |
GRS | 10408-01-10-00C | 26.05.1996 | SB, ch0-35 | β | 6547 | 0.5 | 6 | 100 | 1685 | 2.69 | – | 33 |
GRS | 10408-01-12-00B | 05.06.1996 | Std1 | Φ | 5466 | 0.5 | 8 | 50 | 33 | – | – | – |
GRS | 10408-01-12-00C | 05.06.1996 | Std1 | Φ | 6485 | 0.5 | 8 | 50 | 42 | – | – | – |
GRS | 10408-01-12-00D | 05.06.1996 | Std1 | Φ | 6626 | 0.5 | 8 | 50 | 33 | – | – | – |
GRS | 10408-01-17-00 | 22.06.1996 | Std1 | δ | 6812 | 0.5 | 8 | 60 | 300 | 3.17 | – | 17 |
GRS | 20402-01-03-00B | 19.11.1996 | Std1 | ρ | 6543 | 0.5 | 8 | 18 | 458 | 1.63 | – | 33 |
GRS | 20402-01-03-00C | 19.11.1996 | Std1 | ρ | 3720 | 0.5 | 8 | 18 | 372 | 2.47 | – | 34 |
GRS | 20402-01-03-00E | 19.11.1996 | Std1 | ρ | 3407 | 0.5 | 8 | 18 | 309 | 2.68 | – | 30 |
GRS | 20402-01-33-00A | 18.06.1997 | SB, ch0-35 | κ | 6238 | 0.5 | 6 | 50 | 480 | 1.63 | – | 27 |
GRS | 20402-01-33-00B | 18.06.1997 | SB, ch0-35 | κ | 6690 | 0.5 | 6 | 50 | 554 | 1.60 | – | 27 |
GRS | 20402-01-37-01A | 12.07.1997 | SB, ch0-35 | λ | 6619 | 0.5 | 6 | 250 | 1474 | 2.56 | – | 14 |
GRS | 20402-01-37-01B | 12.07.1997 | SB, ch0-35 | λ | 6615 | 0.5 | 6 | 250 | 900 | 2.80 | – | 15 |
GRS | 20402-01-45-02B | 05.09.1997 | SB, ch0-35 | θ | 6612 | 0.5 | 6 | 100 | 985 | 3.29 | – | 27 |
GRS | 20402-01-45-02C | 05.09.1997 | SB, ch0-35 | θ | 6612 | 0.5 | 6 | 100 | 916 | 5.09 | – | 30 |
GRS | 20402-01-45-02D | 05.09.1997 | SB, ch0-35 | θ | 6466 | 0.5 | 6 | 100 | 795 | 4.10 | – | 23 |
GX | 95409-01-12-00 | 26.03.2010 | GE, ch5-25 | HS | 3170 | 0.5 | 8 | 5 | 89 | 2.19 | 5.38 | 22 |
GX | 95409-01-14-06 | 13.04.2010 | GE, ch5-25 | HIMS | 3155 | 0.5 | 8 | 5 | 26 | 0.52 | 0.75 | 8 |
GX | 95409-01-16-05 | 29.04.2010 | GE, ch5-25 | SIMS | 1625 | 1.5 | 8 | 12 | 66 | 2.90 | 3.00 | 14 |
GX | 95409-01-35-02 | 19.09.2010 | GE, ch5-25 | SS | 2906 | 0.5 | 8 | 5 | 42 | 1.59 | 2.05 | 8 |
XTE 1 | 30188-06-02-00A | 07.09.1998 | Std1 | HS* | 3589 | 0.125 | 7 | 15 | 92 | 1.00 | 3.00 | 8 |
XTE 1 | 30188-06-02-00B | 07.09.1998 | Std1 | HS* | 5019 | 0.125 | 7 | 15 | 107 | 0.30 | 3.00 | 15 |
XTE 1 | 30188-06-03-00A | 08.09.1998 | Std1 | HS* | 7102 | 0.25 | 8 | 7 | 115 | 2.89 | – | 25 |
XTE 1 | 30188-06-03-00C | 08.09.1998 | Std1 | HS* | 13595 | 0.25 | 8 | 7 | 125 | 2.76 | – | 25 |
XTE 1 | 30188-06-01-01 | 09.09.1998 | Std1 | HS* | 10718 | 0.125 | 8 | 4 | 114 | 2.52 | – | 22 |
XTE 1 | 30191-01-14-00 | 28.09.1998 | SB, ch0-17 | VHS | 109388 | 0.032 | 9 | 3 | 151 | 6.14 | 25.17 | 13 |
XTE 2 | 60113-01-13-01 | 19.09.2001 | Std1 | HS | 5463 | 0.125 | 8 | 4 | 38 | 0.14 | 0.29 | 15 |
XTE 2 | 60113-01-13-02 | 19.09.2001 | Std1 | HS | 7127 | 0.125 | 8 | 4 | 42 | 0.17 | 0.33 | 18 |
XTE 2 | 60113-01-18-00 | 24.09.2001 | GE, ch5-24 | H/ST | 17715 | 0.1 | 8 | 4 | 19 | −0.30 | 0.22 | 10 |
XTE 2 | 60113-01-18-01A | 24.09.2001 | GE, ch5-24 | H/ST | 19803 | 0.1 | 8 | 4 | 52 | 0.72 | 1.20 | 10 |
XTE 2 | 60113-01-18-01B | 24.09.2001 | GE, ch5-24 | H/ST | 15591 | 0.1 | 8 | 4 | 59 | 0.34 | 0.74 | 9 |
XTE 2 | 60113-01-18-02 | 24.09.2001 | GE, ch5-24 | H/ST | 8581 | 0.1 | 8 | 4 | 46 | 0.93 | 1.14 | 10 |
XTE 2 | 60113-01-19-00 | 25.09.2001 | GE, ch5-24 | H/ST | 19191 | 0.1 | 8 | 4 | 44 | −0.37 | −0.17 | 10 |
XTE 2 | 60113-19-01 | 26.09.2001 | Std1 | SS | 1713 | 0.25 | 8 | 4 | 31 | 0.13 | 0.39 | 12 |
XTE 2 | 60113-19-04 | 27.09.2001 | Std1 | SS | 1346 | 0.25 | 8 | 4 | 22 | −0.28 | −0.25 | 11 |
XTE 2 | 60113-29-00 | 17.10.2001 | Std1 | SS | 6413 | 0.25 | 8 | 5 | 41 | 0.42 | 0.43 | 14 |
GRO | 10255-01-04-00A | 01.08.1996 | SB, ch0-35 | VHS | 3287 | 0.5 | 7 | 10 | 1602 | 2.21 | – | 24 |
GRO | 10255-01-04-00B | 01.08.1996 | SB, ch0-35 | VHS | 6125 | 0.5 | 7 | 10 | 962 | 4.97 | – | 24 |
GRO | 10255-01-04-00C | 01.08.1996 | SB, ch0-35 | VHS | 6837 | 0.5 | 7 | 10 | 201 | −0.45 | 3.00 | 18 |
GRO | 10255-01-18-00A | 02.11.1996 | SB, ch0-35 | VHS | 642 | 5 | 7 | 5 | 58 | 1.85 | – | 14 |
GRO | 10255-01-18-00B | 02.11.1996 | SB, ch0-35 | VHS | 5663 | 0.5 | 7 | 9 | 65 | 2.05 | – | 11 |
GRO | 20402-02-14-00A | 28.05.1997 | SB, ch0-35 | HSS | 699 | 5 | 7 | 10 | 52 | 1.35 | 3.00 | 12 |
GRO | 20402-02-14-00B | 28.05.1997 | SB, ch0-35 | HSS | 620 | 5 | 7 | 10 | 49 | −0.10 | 3.00 | 11 |
GRO | 90058-16-02-00 | 21.02.2005 | Std1 | HS* | 6502 | 0.5 | 7 | 10 | 17 | 0.18 | 1.98 | 3 |
GRO | 90058-16-03-00A | 23.02.2005 | GE, ch5-24 | HS* | 4534 | 0.5 | 7 | 5 | 32 | 0.22 | 1.74 | 24 |
GRO | 90058-16-03-00B | 23.02.2005 | GE, ch5-24 | HS* | 1973 | 0.5 | 7 | 5 | 27 | 0.46 | 1.57 | 17 |
GRO | 90058-16-07-00A | 26.02.2005 | GE, ch5-24 | HS* | 4111 | 0.5 | 7 | 5 | 36 | 0.17 | −0.18 | 23 |
GRO | 90058-16-07-00B | 26.02.2005 | GE, ch5-24 | HS* | 2388 | 0.5 | 7 | 5 | 38 | 1.86 | – | 21 |
GRO | 90019-02-01-00 | 13.03.2005 | Std1 | SIMS* | 1549 | 0.5 | 6 | 12 | 45 | 2.33 | – | 5 |
Notes. The meaning of the shortcuts is as follows: GRS = GRS 1915+105, GX = GX 339-4, XTE 1 = XTE J1550-564, XTE 2 = XTE J1650-500, GRO = GRO J1655-40, Std1 = Standard 1 data mode, SB, ch0-35 = Single bit data mode containing energy channels 0−35 and GE, ch5-25 = generic event data mode using energy channels 5−25 from PCU2. The classification of the source GX 339-4 is given according to Nandi et al. (2012; HS = hard state, HIMS = hard-intermediate state, SIMS = soft-intermediate state, SS = soft state), the classification of the source GRS 1915+105 is given according to Misra et al. (2004),the classification of GRO J1655-40 is according to Sobczak et al. (1999a; VHS = very high state with flaring, HSS = high/soft state) for the 1996/1997 measurement. During the 2005 outburst we used the overall plot of the hardness ratio given in Miller et al. (2008) for an estimation of the spectral state (HS∗− hard state, SIMS∗− soft-intermediate state). Similarly we used the classification, plots and discussion given by Sobczak et al. (1999b) for XTE J1550-564 and by Homan et al. (2003) for XTE J1650-500 (H/ST − hard to soft state transition). In the 6th and 7th columns the number of points used for the lightcurve N with the time bin dt are summarised. In the next columns, the parameters (m,k) od the recurrence analysis and its results – the length of the longest diagonal line for RR ~ 20%, the averaged significance and the averaged significance with respect to the shuffled surrogates
computed for Nϵ different values of ϵ – are presented.
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