2016A&A...588A.103B


Query : 2016A&A...588A.103B

2016A&A...588A.103B - Astronomy and Astrophysics, volume 588A, 103-103 (2016/4-1)

Second ROSAT all-sky survey (2RXS) source catalogue.

BOLLER T., FREYBERG M.J., TRUMPER J., HABERL F., VOGES W. and NANDRA K.

Abstract (from CDS):

Aims. We present the second ROSAT all-sky survey source catalogue, hereafter referred to as the 2RXS catalogue. This is the second publicly released ROSAT catalogue of point-like sources obtained from the ROSAT all-sky survey (RASS) observations performed with the position-sensitive proportional counter (PSPC) between June 1990 and August 1991, and is an extended and revised version of the bright and faint source catalogues.
Methods. We used the latest version of the RASS processing to produce overlapping X-ray images of 6.4°x6.4° sky regions. To create a source catalogue, a likelihood-based detection algorithm was applied to these, which accounts for the variable point-spread function (PSF) across the PSPC field of view. Improvements in the background determination compared to 1RXS were also implemented. X-ray control images showing the source and background extraction regions were generated, which were visually inspected. Simulations were performed to assess the spurious source content of the 2RXS catalogue. X-ray spectra and light curves were extracted for the 2RXS sources, with spectral and variability parameters derived from these products.
Results. We obtained about 135000 X-ray detections in the 0.1-2.4keV energy band down to a likelihood threshold of 6.5, as adopted in the 1RXS faint source catalogue. Our simulations show that the expected spurious content of the catalogue is a strong function of detection likelihood, and the full catalogue is expected to contain about 30% spurious detections. A more conservative likelihood threshold of 9, on the other hand, yields about 71000 detections with a 5% spurious fraction. We recommend thresholds appropriate to the scientific application. X-ray images and overlaid X-ray contour lines provide an additional user product to evaluate the detections visually, and we performed our own visual inspections to flag uncertain detections. Intra-day variability in the X-ray light curves was quantified based on the normalised excess variance and a maximum amplitude variability analysis. X-ray spectral fits were performed using three basic models, a power law, a thermal plasma emission model, and black-body emission. Thirty-two large extended regions with diffuse emission and embedded point sources were identified and excluded from the present analysis.
Conclusions. The 2RXS catalogue provides the deepest and cleanest X-ray all-sky survey catalogue in advance of eROSITA.

Abstract Copyright: © ESO, 2016

Journal keyword(s): X-rays: general - catalogs - surveys

VizieR on-line data: <Available at CDS (J/A+A/588/A103): cat2rxs.dat cat2rxs.fits>

Nomenclature: 2RXS JHHMMSS.s+DDMMSS N=135118.

Status at CDS : All or part of tables of objects will not be ingested in SIMBAD.

Simbad objects: 95

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Number of rows : 95
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 LP 348-40 PM* 00 11 53.0346750552 +22 59 04.593551280   13.20   12.736   M3.5V 34 0
2 LEDA 87392 Sy1 00 39 15.8339634552 -51 17 01.481641692   15.77 15.28 15.66   ~ 130 0
3 M 31 AGN 00 42 44.330 +41 16 07.50 4.86 4.36 3.44     ~ 12650 1
4 RX J004529.8+421908 X 00 45 29.8 +42 19 08           ~ 8 0
5 1RXS J004744.6+423842 X 00 47 44.6 +42 38 42           ~ 1 0
6 V* BL Hyi CV* 01 41 00.3996430344 -67 53 27.470100660   14.9       Am 210 0
7 LP 469-118 Er* 02 08 12.41 +15 08 44.3           M5Ve+M4Ve 30 0
8 1RXS J021756.0+624359 X 02 17 56.0 +62 43 59           ~ 2 0
9 SNR G132.4+02.2 SNR 02 18 46 +62 38.8           ~ 3 0
10 2A 0251+413 ClG 02 54 32.2 +41 35 10           ~ 315 1
11 ACO 426 ClG 03 19 47.2 +41 30 47           ~ 2258 1
12 ACO S 373 ClG 03 38 29.4 -35 27 08           ~ 1827 0
13 NGC 1404 GiP 03 38 51.917 -35 35 39.81 11.53 10.69 10.00 9.03   ~ 751 1
14 StKM 1-497 TT* 04 37 37.4553491592 -02 29 28.950973764   12.04 10.59   8.59 M1.1V 127 0
15 LEDA 16124 G 04 50 06.685 +45 03 05.74   19       ~ 66 1
16 1FGL J0500.1+5237 BL? 04 58 51.300 +51 50 28.00           ~ 133 1
17 1RXS J050036.1+461859 X 05 00 36.1 +46 18 59           ~ 2 0
18 SNR G160.8+02.6 SNR 05 01 00.000 +46 40 00.00           ~ 212 0
19 Mrk 1095 Sy1 05 16 11.4092471904 -00 08 59.157166920   14.30 13.92     ~ 890 1
20 AJG 116 Q? 05 26 30.000 +42 56 00.00           ~ 182 0
21 X LMC X-4 HXB 05 32 49.5556042296 -66 22 13.202721768   13.9 14.0     O8III 669 0
22 M 1 SNR 05 34 30.9 +22 00 53           ~ 6193 1
23 RX J0535.6-6651 HXB 05 35 40.9970566152 -66 51 53.547559416   13.7 13.8     B0.5IIIe 287 0
24 X LMC X-3 HXB 05 38 56.6323605504 -64 05 03.317937504   17 17.2     B2.5Ve 675 0
25 IC 433 G 05 40 31.3524514488 -11 39 56.022239160   14       ~ 31 0
26 1RXS J054042.8-020533 X 05 40 43.10 -02 05 30.3           ~ 4 0
27 NAME SEP reg 06 00 00.000 -66 33 38.55           ~ 173 0
28 SNR G189.1+02.9 SNR 06 17 01 +22 33.9           ~ 6 0
29 V* YY Gem BY* 07 34 37.4474327544 +31 52 10.179641496 11.60 10.56 9.27 7.69 6.67 M0.5VeFe-2 854 0
30 V* UY Vol LXB 07 48 33.71 -67 45 07.7 16.10 17.00 16.9 16.7 17.05 ~ 618 0
31 V* V572 Pup HXB 08 12 28.3575205680 -31 14 52.138451400 12.14 13.03 12.74 12.44   B0.2IVe 70 0
32 V* VV Pup CV* 08 15 06.8009599464 -19 03 17.765706024     13.90     M7V 398 0
33 NAME Pup A BL? 08 24 07 -42 59.8           ~ 600 1
34 NAME Vela XYZ Rad 08 34.0 -45 50           ~ 1230 2
35 NAME Vela Pulsar Psr 08 35 20.65525 -45 10 35.1545     15.10     ~ 2316 1
36 V* GP Vel HXB 09 02 06.8608812864 -40 33 16.899168060 6.85 7.37 6.87 6.31 6.05 B0.5Ia 1505 0
37 ACO S 636 ClG 10 29 41.0957 -35 19 32.908           ~ 225 0
38 Ass Car OB 1 As* 10 38 -59.0           ~ 162 0
39 V* EK UMa CV* 10 51 35.1578195280 +54 04 36.112715220   18       ~ 85 0
40 Mrk 421 BLL 11 04 27.3140835504 +38 12 31.798495872   13.50 12.90 8.31   ~ 2675 1
41 Ass Car OB 2 As* 11 08 -60.2           ~ 82 0
42 1RXS J112441.5-682621 X 11 24 41.41 -68 26 23.3           ~ 2 0
43 BD+12 2343 SB* 11 32 49.4245288344 +12 10 24.938881464   10.13 9.38     G5 18 0
44 ACO 1367 ClG 11 44 44.6 +19 41 59           ~ 1076 1
45 V* EU UMa CV* 11 49 55.7017863576 +28 45 07.294697604           DB+K 76 0
46 SNR G296.1-00.5 SNR 11 51 10 -62 34.0           ~ 53 0
47 AJG 14 BL? 12 09 40 -52 25.0           ~ 287 1
48 IC 3599 Sy1 12 37 41.1939398400 +26 42 27.484266888   15.7 16.5     ~ 178 0
49 ACO 1644 ClG 12 57 11.6 -17 24 34           ~ 366 1
50 V* EV UMa CV* 13 07 53.8583243765 +53 51 30.498937628           ~ 66 0
51 V* V1043 Cen CV* 13 13 17.1147127536 -32 59 12.443490960           ~ 37 0
52 HD 118100 Er* 13 34 43.2063495866 -08 20 31.338030204 11.578 10.552 9.372 8.602 7.930 K5Ve 346 0
53 Mrk 478 Sy1 14 42 07.4714418744 +35 26 22.938625500   14.91 14.58     ~ 533 0
54 1A 1439-61 BL? 14 43 00 -62 30.0           ~ 368 1
55 PG 1501+664 WD* 15 02 09.6299323152 +66 12 19.148868324   16.07 16.37     DZQ1 158 0
56 HD 135363 ** 15 07 56.2473941616 +76 12 02.719373904       8.1   G5V+M2V-M4V 72 0
57 NGC 5905 H2G 15 15 23.3280793632 +55 31 01.926808032   13.6       ~ 273 1
58 V* KY TrA LXB 15 28 16.97 -61 52 57.8   17.5       ~ 101 0
59 Kes 25 BL? 15 53 00.000 -56 10 00.00           ~ 129 0
60 ACO 2147 ClG 16 02 11.96 +15 55 11.5           ~ 403 0
61 ACO 3627 ClG 16 14 22.5 -60 52 07           ~ 296 2
62 1RXS J161954.9-153542 X 16 19 54.9 -15 35 42           ~ 2 0
63 V* V818 Sco LXB 16 19 55.0692669024 -15 38 25.017666540 11.60 12.40 11.1     Oev 1643 0
64 ACO 2199 ClG 16 28 43.31 +39 34 07.6           ~ 1171 1
65 NGC 6240 Sy2 16 52 58.9 +02 24 03   14.31 13.37     ~ 1637 2
66 7C 165211.80+395026.00 BLL 16 53 52.21668403 +39 45 36.6088754 14.09 14.15 13.29 8.26   ~ 2162 2
67 V* HZ Her LXB 16 57 49.8110126616 +35 20 32.486555472 11.90 14.89 13.63 13.88   B3/6ep 2076 0
68 HD 153919 HXB 17 03 56.7725629224 -37 50 38.913331452 6.06 6.78 6.51 6.08 5.90 O6Iafcp 814 1
69 NAME Oph Cluster ClG 17 12 24.7 -23 21 01           ~ 273 0
70 1FGL J1711.7-3944c BL? 17 12 27 -39 41.2     12.27     ~ 723 1
71 NAME NEP reg 18 00 00.000 +66 33 38.55           ~ 359 0
72 SNR G006.4-00.1 SNR 18 00 31.2011719 -23 25 48.001099           ~ 737 1
73 V* V884 Her CV* 18 02 06.4848200016 +18 04 43.839425568   13.315 13.382 14.753   ~ 55 0
74 NGC 6546 OpC 18 07 22 -23 17.8   8.65 8.0     ~ 42 0
75 1RXS J181545.4-164043 X 18 15 45.4 -16 40 43           ~ 2 0
76 SNR G014.1-00.1 SNR 18 16.7 -16 41           ~ 19 0
77 StKM 1-1676 EB* 19 03 17.2839464 +63 59 34.162250   11.889 10.707 10.061   M3.5Ve 23 0
78 X Aql X-1 LXB 19 11 16.0571313336 +00 35 05.868232692           ~ 1136 1
79 V* V1405 Aql LXB 19 18 47.871 -05 14 17.09 20.90 21.40 21.0     ~ 474 0
80 ACO 2319 ClG 19 20 45.3 +43 57 43           ~ 461 1
81 V* QS Tel CV* 19 38 35.8144163880 -46 12 57.106344420           ~ 115 0
82 SNR G053.6-02.2 SNR 19 38.8 +17 14           ~ 150 0
83 HD 226868 HXB 19 58 21.6757355952 +35 12 05.784512688 9.38 9.72 8.91 8.42   O9.7Iabpvar 4337 0
84 V* QQ Vul CV* 20 05 41.9090048400 +22 39 58.839854760   14.688 14.656 14.584   M2 199 0
85 PM J20301+7950 PM* 20 30 07.1514546360 +79 50 46.649720472   14.4 12.242 11.848   M3.0Ve 18 0
86 HD 197481 BY* 20 45 09.5324974119 -31 20 27.237889841   10.05 8.627 9.078 6.593 M1VeBa1 1153 0
87 V* BO Mic BY* 20 47 45.0056152368 -36 35 40.769832192   10.39 9.337   8.216 K3V(e) 198 0
88 NAME Cyg Loop SNR 20 51.0 +30 40           ~ 913 0
89 1RXS J205118.2+310312 X 20 51 18.2 +31 03 12           ~ 2 0
90 V* SS Cyg CV* 21 42 42.8034497592 +43 35 09.867842484 11.07 12.651 12.032 9.326   K5V 1290 1
91 V* AR Lac RS* 22 08 40.8182089680 +45 44 32.107863120 7.09 6.83 6.11     K0IVe+G5IV 724 0
92 V* EV Lac Er* 22 46 49.7312610268 +44 20 02.374381562   11.85 10.26 9.89   M4.0Ve 902 2
93 CTB 109 BL? 23 01 35 +58 53.0           ~ 344 0
94 V* V358 Aqr CV* 23 16 03.6195381912 -05 27 08.910770724     18.0     ~ 26 0
95 3C 461 BL? 23 23 24.000 +58 48 54.00     14.30     ~ 2792 1

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