2006ApJ...652..198A

Query : 2006ApJ...652..198A

2006ApJ...652..198A - Astrophys. J., 652, 198-205 (2006/November-3)

High-energy neutrino astronomy using upward-going muons in super-Kamiokande I.

ABE K., HOSAKA J., IIDA T., ISHIHARA K., KAMEDA J., KOSHIO Y., MINAMINO A., MITSUDA C., MIURA M., MORIYAMA S., NAKAHATA M., OBAYASHI Y., OGAWA H., SHIOZAWA M., SUZUKI Y., TAKEDA A., TAKEUCHI Y., HIGUCHI I., ISHIHARA C., ISHITSUKA M., KAJITA T., KANEYUKI K., MITSUKA G., NAKAYAMA S., NISHINO H., OKADA A., OKUMURA K., SAJI C., TAKENAGA Y., CLARK S., DESAI S., DUFOUR F., KEARNS E., LIKHODED S., LITOS M., RAAF J.L., STONE J.L., SULAK L.R., WANG W., GOLDHABER M., CASPER D., CRAVENS J.P., DUNMORE J., KROPP W.R., LIU D.W., MINE S., REGIS C., SMY M.B., SOBEL H.W., VAGINS M.R., GANEZER K.S., HILL J., KEIG W.E., JANG J.S., KIM J.Y., LIM I.T., SCHOLBERG K., TANIMOTO N., WALTER C.W., WENDELL R., ELLSWORTH R.W., TASAKA S., GUILLIAN G., LEARNED J.G., MATSUNO S., MESSIER M.D., HAYATO Y., ICHIKAWA A.K., ISHIDA T., ISHII T., IWASHITA T., KOBAYASHI T., NAKADAIRA T., NAKAMURA K., NITTA K., OYAMA Y., TOTSUKA Y., SUZUKI A.T., HASEGAWA M., HIRAIDE K., KATO I., MAESAKA H., NAKAYA T., NISHIKAWA K., SASAKI T., SATO H., YAMAMOTO S., YOKOYAMA M., HAINES T.J., DAZELEY S., HATAKEYAMA S., SVOBODA R., SULLIVAN G.W., TURCAN D., SWANSON M., CLOUGH A., HABIG A., FUKUDA Y., SATO T., ITOW Y., KOIKE T., JUNG C.K., KATO T., KOBAYASHI K., MALEK M., McGREW C., SARRAT A., TERRI R., YANAGISAWA C., TAMURA N., SAKUDA M., SUGIHARA M., KUNO Y., YOSHIDA M., KIM S.B., YANG B.S., YOO J., ISHIZUKA T., OKAZAWA H., CHOI Y., SEO H.K., GANDO Y., HASEGAWA T., INOUE K., ISHII H., NISHIJIMA K., ISHINO H., WATANABE Y., KOSHIBA M., KIELCZEWSKA D., ZALIPSKA J., BERNS H., GRAN R., SHIRAISHI K.K., STACHYRA A., THRANE E., WASHBURN K., WILKES R.J. (The Super-Kamiokande Collaboration)

Abstract (from CDS):

We present the results from several studies used to search for astrophysical sources of high-energy neutrinos using the Super-Kamiokande I (1996 April-2001 July) neutrino-induced upward-going muon data. The data set consists of 2359 events with minimum energy 1.6 GeV, of which 1892 are through-going and 467 stop within the detector. The results of several independent analyses are presented, including searches for point sources using directional and temporal information and a search for signatures of cosmic-ray interactions with the interstellar medium in the upward-going muons. No statistically significant evidence for point sources or any diffuse flux from the plane of the Galaxy was found, so specific limits on fluxes from likely point sources are calculated. The 90% confidence level (CL) upper limits on upward-going muon flux from astronomical sources that are located in the southern hemisphere and always under the horizon for Super-Kamiokande are ∼1-4x10–15/cm2/s.

Abstract Copyright: ∼

Journal keyword(s): ISM: Cosmic Rays - Elementary Particles - Neutrinos

Simbad objects: 53

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Number of rows : 53
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 SK 160 HXB 01 17 05.1457288392 -73 26 36.014808156 12.23 13.00 13.15   13.17 O9.7Ia+ 918 0
2 ACO 426 ClG 03 19 47.6 +41 30 54           ~ 2508 1
3 HD 22468 RS* 03 36 47.2904292073 +00 35 15.943692002 7.09 6.79 5.90     K2:Vnk 1206 0
4 V* X Per HXB 03 55 23.0777456088 +31 02 45.039836148 6.090 6.840 6.720     O9.5III 1037 0
5 X LMC X-2 LXB 05 20 29.0 -71 57 33 17.20 18.00 18.0     ~ 189 0
6 PSR B0525-66 Psr 05 26 00.7 -66 04 35           ~ 569 1
7 X LMC X-4 HXB 05 32 49.5556042296 -66 22 13.202721768   13.9 14.0 14.290   O8III 714 0
8 M 1 SNR 05 34 31.8 +22 01 03           ~ 6516 1
9 V* CM Tau Psr 05 34 31.9474694616 +22 00 52.153698024           ~ 5476 0
10 SN 1987A SN* 05 35 27.98840 -69 16 11.1134           SNIIpec 5203 2
11 V* V1055 Ori LXB 06 17 07.3565603963 +09 08 13.515857360   18.80 18.5     ~ 594 1
12 PSR J0633+1746 Psr 06 33 54.153 +17 46 12.91           ~ 1308 0
13 V* GP Vel HXB 09 02 06.8608812864 -40 33 16.899168060 6.85 7.37 6.87 6.31 6.05 B0.5Ia 1588 0
14 V* V712 Car EB* 10 23 58.0126366512 -57 45 48.937268268 15.466 15.473 13.5 12.6   O3If*/WN6+O3If*/WN6 176 0
15 Z 184-50 BLL 11 04 27.3140835504 +38 12 31.798495872   13.50 12.90 8.31   ~ 2841 1
16 V* V779 Cen HXB 11 21 15.0920532528 -60 37 25.630264596   14.4 12.27     O9III/Veq 1159 0
17 V* BP Cru HXB 12 26 37.5605188992 -62 46 13.261044684   12.482 10.803 10.304   B1Ia+ 731 0
18 V* V850 Cen HXB 13 01 17.0968941216 -61 36 06.637549788   15.6 14.40     B2Vne 361 0
19 NAME Lupus SN SNR 15 02 22.1 -42 05 49           ~ 1407 1
20 PSR B1509-58 Psr 15 13 47.6 -59 07 54     13.06     ~ 879 1
21 V* BR Cir HXB 15 20 40.8532547060 -57 10 00.206639033   21.4 21.4     B5-A0I 849 1
22 V* QX Nor LXB 16 12 43.0 -52 25 26           ~ 946 1
23 V* V818 Sco LXB 16 19 55.0692669024 -15 38 25.017666540 11.60 12.40 11.1     Oev 1730 0
24 GRB 980618A gB 16 35 52 -47 35.2           ~ 270 0
25 V* V801 Ara LXB 16 40 55.5976953528 -53 45 04.948107156 17.50 18.20 17.5   17.07 ~ 921 0
26 Z 225-7 BLL 16 53 52.21668403 +39 45 36.6088754 14.09 14.15 13.29 8.26   ~ 2304 2
27 V* HZ Her LXB 16 57 49.8110126616 +35 20 32.486555472 11.90 14.89 13.63 13.88   B3/6ep 2172 0
28 V* V821 Ara LXB 17 02 49.3876391280 -48 47 23.087954544         15.322 ~ 2237 0
29 HD 153919 HXB 17 03 56.7725629224 -37 50 38.913331452 6.06 6.78 6.51 6.08 5.90 O6Iafcp 851 0
30 X Ara X-1 LXB 17 06 15.2 -43 02 11           ~ 296 1
31 PSR B1706-44 Psr 17 09 42.62000 -44 29 12.0000     13.30     ~ 670 1
32 NAME Kepler's SN SNR 17 30 40.51 -21 29 14.4           ~ 851 3
33 V* V2216 Oph LXB 17 31 44.17 -16 57 40.9 16.40 17.10 16.8     ~ 329 1
34 V* V2116 Oph Sy* 17 32 02.1532435416 -24 44 44.129169096   20.78 18.4     M6IIIe 719 1
35 V* V926 Sco LXB 17 38 58.2384053021 -44 27 00.699118812 16.90 17.70 17.5     ~ 480 0
36 LDN 10 DNe 17 57.8 -30 06           ~ 4 0
37 NAME Sgr 1801-23 gam 18 00 58.9 -22 56 48           ~ 40 0
38 PSR J1808-2024 Psr 18 08 39.32 -20 24 40.1           ~ 1316 2
39 X Sgr X-4 LXB 18 23 40.57 -30 21 40.6   19.06 18.81     ~ 1056 1
40 PSR B1823-13 Psr 18 26 13.06 -13 34 48.1           ~ 460 1
41 V* V479 Sct HXB 18 26 15.0561548880 -14 50 54.247274304 12.02 12.23 11.27 11.04   ON6V((f))z 613 2
42 V* MM Ser LXB 18 39 57.8 +05 02 13   19.2 19.2     ~ 378 0
43 4U 1901+03 HXB 19 03 39.3926409480 +03 12 15.758070228           B8-9IV 122 0
44 GBS 1900+14 gB 19 07 13 +09 19.6           ~ 906 0
45 X Aql X-1 LXB 19 11 16.0571313336 +00 35 05.868232692           ~ 1186 1
46 SS 433 HXB 19 11 49.5647697480 +04 58 57.827127648   16.854 14.643     A7Ib 2253 4
47 HD 226868 HXB 19 58 21.6757355952 +35 12 05.784512688 9.38 9.72 8.91 8.42   O9.7Iabpvar 4590 0
48 QSO B1959+650 BLL 19 59 59.8520303688 +65 08 54.652536492     12.8 11.21   ~ 699 2
49 V* V1521 Cyg HXB 20 32 25.78 +40 57 27.9           WN4/5-6/7 2035 2
50 V* V1341 Cyg LXB 21 44 41.1544345272 +38 19 17.066570988 15.00 15.13 14.68 15.00   A9III 1229 1
51 X Aqr X-1 CV? ~ ~           ~ 2 0
52 X Aql X-4 X ~ ~           ~ 1 0
53 X Cen X-5 XB* ~ ~           ~ 2 0

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