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Publ. Astron. Soc. Aust., 1999, 16, 175­205
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A Catalogue of X-ray Sources in the Sky Region b etween = -73 and = +27
M. T. Meliani
Instituto Nacional de Pesquisas Espaciais, INPE, Divis~ de Astrof´ ao isica, CP 515, S. Jos´ dos Campos-SP, 12201­970 Brazil e meliani@das.inpe.br Received 1998 November 23, accepted 1999 April 20

Abstract: This Catalogue lists coordinates, X-ray fluxes in different energy ranges, magnitudes and colour indices, optical counterparts, orbital periods of binaries, pulsar periods and other characteristics of 226 X-ray sources (HMXBs, LMXBs, pulsars and galaxies) between = -73 and = +27 . Keywords: catalogues -- X-ray sources: stars, galaxies -- stars: binaries, pulsars

1 Introduction The Catalogue lists 226 selected X-ray emitting ob jects with declinations between -73 +27 . The information was obtained principally from the technical literature published from 1992 to May 1998. Some recently discovered sources, such as RXTE 1550­56 and RXTE 2123­058, have also been included. The layout of the Catalogue follows the standard format used in Bradt & McClintock (1985) and van Paradijs (1995). However, the coordinates for both B1950 and J2000 have been included, as have the X-ray fluxes in six different energy ranges. This work updates and complements the two catalogues referred to in the declination rang considered. In the Catalogue the sources are ordered according to class (A: LMXBs; B: HMXBs and C: other sources) and right ascension. The numbers in square brackets refer to the publications from which the data were obtained, and additional information is given as key words. The Catalogue classifies 60 high-mass X-ray binaries (HMXBs), 35 of which have a pulsar; 124 low-mass X-ray binaries (LMXBs), 8 of which have a pulsar; 9 binaries, 7 of which have a pulsar; 9 simple pulsars; 7 galaxies; and 1 quasar. There are 16 other sources without classification. Optical counterparts are known for 82 sources and they are also listed. A list of ob jects in lexigraphical order is also given in Table 1. The Catalogue will be used to select X-ray sources to be observed with the MASCO telescope (Villela et al. 1995) that is being constructed to operate in the range 40 to 5000 keV. The MASCO telescope will be launched by balloon at latitude -23 in Brazil. About one third of the sources emit above 30 keV and are concentrated in the Galactic Centre, the main target of the MASCO telescope.
Astronomical Society of Australia 1999

2 The Catalogue The Catalogue contents are explained below. The references cited are listed in numerical and alphabetical order at the end. The Catalogue is available electronically from the electronic version of Publications of the Astronomical Society of Australia at http://www.atnf.csiro.au/pasa/16 2/meliani/. First column: The source name related with its sky location in epoch 1950 (B) and/or 2000 (J). The conventional format is hhmm±ddd, where hh and mm indicate the hour and minute of right ascension and ddd indicates the declination. If there is an alternative name, it is also given. The sources that emit above 30 keV are distinguished. Second column: The first line gives the type of source: LMXB: low-mass X-ray binary HMXB: high-mass X-ray binary Binary: binaries sources without classification Pulsar QSO: quasar AGN: active galactic nuclei. The second line gives: (a) if the source is in a binary system; A: atoll source B: X-ray burst source D: `dipping' LMXBs G: globular cluster X-ray source P: X-ray pulsar T: transient X-ray source U: ultra-soft X-ray spectrum Z: Z-type. (b) if the source is a pulsar; SNR: associated with a supernova remnant. The third line gives the type of observation and source position error:
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Table 1. List of ob jects in lexigraphical order 3C273 AV 111 BR Cir BW Cir UW CrB BP CruWra 977 µ2 CruHD 112091 GR Mus HD 63666SAO 235515 HD 65663SAO 250018 HD 77581GP Vel HD 110432SAO 252002 HD 141926SAO 243098 HD 153919V884 Sco HD 154791 HD 161103 He3-640 Hen715V801Cen HV 2554 HV 5682 Kes 73 Lil 1 LS 992 LS 1698 LS 5039 M15AC211 M28 MCG-5-23-16 MMVel MSH 15-32G320 · 4-1 · 2 N67 NCL 101 NGC 1068 NGC 1851 NGC 4507 NGC 4945 NGC 5128 NGC 6440 NGC 6441 (star U1) NGC 6624 NGC 6652 B1226+023 B0050 · 1-7247 B1516-569 B1354-645 B1603+260 B1223-624 B1255-567 B1254-690 B0739-529 B0749-600 B0900-403 B1249-637 B1555-552 B1700-377 B1704+240 J1744 · 7-2713 B1118-615 B1145-619 J0528-6954 B0513 · 9-695 J1841-045 B1730-335 J0812 · 4-3114 B1036-565 J1826 · 2-1450 B1227+119 B1821-24 B0945-397 B1009-45 B1509-58 B0056 · 8-7164 B1811-171 B0240-001 B0512-401 B1232-396 B1304-497 B1322-427 B1745-203 B1746-370 B1820-303 B1832-330 NGC 6712 NGC 7582 NP 0531 QV Nor S84 SK 160 MM Ser NP Ser SK-Ph Ter 2 Ter 5 Ter 6 KY TrA KZ TrA LU TrA V1333 Aql V1343 AqlSS 433 V1405 Aql V1408 Aql V801 Ara V821 Ara V395 Car V779 Cen V822 Cen V830 Cen V850 Cen V691 CrA V616 Mon V2107 Oph V2116Oph V2134 Oph V2216 Oph V2293 Oph V1055 Ori V4134 Sgr V818 Sco V926 Sco V725 Tau UY Vol QZ Vul Wack 2134TH35-42 B1850­087 B2315-426 B0531+219 B1538-522 B0726-260 B0115-737 B1837+049 B1813-140 B0532-664 B1734-307 B1745-248 B1747-313 B1524-617 B1627-673 B1556-605 B1908+005 B1909+048 B1916-053 B1957+115 B1636-536 B1659-487 B0921-630 B1119-603 B1455-314 B1145 · 1-6141 B1258-613 B1822-371 B0620-003 B1705-250 B1729-247 B1658-298 B1728-169 B1716-249 B0614+091 B1755-338 B1617-155 B1735-444 B0535+262 B0748-676 B2000+251 B1024-5732

o: optical x: X-ray i: infrared r: radio. Third column: The first and second lines give right ascension (RA) and declination (DEC) in epoch 1950. The third line gives the galactic longitude and latitude. Fourth column: The first and second lines give the right ascension (RA) and declination (DEC) in epoch 2000. Fifth column: The optical counterpart, if known, and associations. Sixth column: The magnitude and colour indices of the optical counterpart; first line: V second line: B­V third line: U­B. Seventh column: first line: spectral type of optical counterpart second line: interstellar reddening, E B-V .

Eighth column: Gives the X-ray fluxes F x in units of 10-5 photons cm-2 s-1 keV-1 in the ranges: first line: 2­10 keV (or 0 · 1­2 · 4 keV for those sources indicated by an asterisk). second line: 40­80 keV (or 10­40 keV for those sources indicated by an asterisk). third line: 80­180 keV. Ninth column : Gives the X-ray fluxes F x in units of 10-5 photons cm-2 s-1 keV-1 in the ranges: first line: 200­600 keV second line: 600­1000 keV third line: above 1000 keV. The notation nnEm stands for nn â 10m . Tenth column: first line: orbital period in days (d) or hours (h) second line: pulsar period in seconds (s) or milliseconds (ms) third line: the X-ray catalogues and experiments in which the source was listed and/or detected:


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A: Ariel V sky survey (McHardy et al. 1981; Warwick et al. 1981) H: HEAO A-4 sky survey (Levine et al. 1984) M: MIT OSO-7 sky survey (Markert et al. 1979) U: Uhuru sky survey (Forman et al. 1978) X: Catalogue of X-ray binaries (van Paradijs 1995). As: ASCA B: Beppo Sax Bb: Broad Band X-ray Telescope (BBXRT) C: Compton -ray Observatory (Batse, GRO) Cb: Cos B E: Einstein Eg: Egret Exo: Exosat FII: Figaro II (X- and -ray) G: Ginga Gr: Granat Ha: Hakucho K: Kvant OAO: Orbiting Astronomical Observatory P: Prognoz 9 R: ROSAT Rx: Rossi X-ray Timing Explorer (RXTE) S: SAS 3 S2: SAS2 SL: Space Lab T: Tenma V: Vela-5 and Vela-6 satellites The symbol (:) that follows some values indicates imprecise data.

Acknowledgments This work was supported by the Funda¸ao de Amparo c~ a ` Pesquisa do Estado de S~ Paulo (FAPESP) ao process numbers 95/09831­2 and 98/07641­0. The author acknowledges Dr Walter F. Velloso Jr for his suggestions. References
Bradt, H. V., & McClintock, J. E. 1983, ARA&A, 21, 13 Forman, W., Jones, C., Cominsky, L., Julien, P., Murray, S., Peters, G., Tanabaum, H., & Giacconi, R. 1978, ApJS, 38, 357 (IV Catalog Uhuru) Levine, A. M., Lang, F. L., Lewin, W. H. G., et al. 1984, ApJS, 54, 581 (HEAO1-A4 Catalog) McHardy, I. M., Lawrence, A., Pye, J. P., & Pounds, K. A. 1981, MNRAS, 197, 893 Markert, T. H., Winkler, P. F., Laird, F. N., Clark, G. W., Hearn, D. R., Sprot, G. F., Li, F. K., Bradt, H. V., Lewin, W. H. G., & Schnopper, H. W. 1979, ApJS, 39, 573 van Paradijs, J. 1995, in X-ray Binaries, ed. W. H. J. Lewin, J. van Paradijs & E. P. J. van den Heuvel, p. 536 Villela, T., Braga, J., D' Amico, F., & Jayanthi, U. B. 1995, Adv. Space Res., 15, 98 Warwick, R. S., Marshal, N., Fraser, G. W., Watson, M. G., Lawrence, A., Page, C. G., Pounds, K. A., & Ricketts, M. J. 1981, MNRAS, 197, 865 Zeng, Q., Lou, G. F., & Li, S. Z. 1987, Ap&SS, 132, 263.


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