2023ApJ...953..160A


Query : 2023ApJ...953..160A

2023ApJ...953..160A - Astrophys. J., 953, 160 (2023/August-3)

Search for sub-TeV Neutrino Emission from Novae with IceCube-DeepCore.

ABBASI R., ACKERMANN M., ADAMS J., AGGARWAL N., AGUILAR J.A., AHLERS M., ALAMEDDINE J.M., ALVES A.A.Jr, AMIN N.M., ANDEEN K., ANDERSON T., ANTON G., ARGUELLES C., ASHIDA Y., ATHANASIADOU S., AXANI S.N., BAI X., BALAGOPAL V.A., BARICEVIC M., BARWICK S.W., BASU V., BAY R., BEATTY J.J., BECKER K.-H., BECKER TJUS J., BEISE J., BELLENGHI C., BENZVI S., BERLEY D., BERNARDINI E., BESSON D.Z., BINDER G., BINDIG D., BLAUFUSS E., BLOT S., BONTEMPO F., BOOK J.Y., BOROWKA J., BOSCOLO MENEGUOLO C., BOSER S., BOTNER O., BOTTCHER J., BOURBEAU E., BRAUN J., BRINSON B., BROSTEAN-KAISER J., BURLEY R.T., BUSSE R.S., CAMPANA M.A., CARNIE-BRONCA E.G., CHEN C., CHEN Z., CHIRKIN D., CHOI S., CLARK B.A., CLASSEN L., COLEMAN A., COLLIN G.H., CONNOLLY A., CONRAD J.M., COPPIN P., CORREA P., COUNTRYMAN S., COWEN D.F., DAPPEN C., DAVE P., DE CLERCQ C., DELAUNAY J.J., DELGADO LOPEZ D., DEMBINSKI H., DEOSKAR K., DESAI A., DESIATI P., DE VRIES K.D., DE WASSEIGE G., DEYOUNG T., DIAZ A., DIAZ-VELEZ J.C., DITTMER M., DUJMOVIC H., DUVERNOIS M.A., EHRHARDT T., ELLER P., ENGEL R., ERPENBECK H., EVANS J., EVENSON P.A., FAN K.L., FAZELY A.R., FEDYNITCH A., FEIGL N., FIEDLSCHUSTER S., FIENBERG A.T., FINLEY C., FISCHER L., FOX D., FRANCKOWIAK A., FRIEDMAN E., FRITZ A., FURST P., GAISSER T.K., GALLAGHER J., GANSTER E., GARCIA A., GARRAPPA S., GERHARDT L., GHADIMI A., GLASER C., GLAUCH T., GLUSENKAMP T., GOEHLKE N., GONZALEZ J.G., GOSWAMI S., GRANT D., GRAY S.J., GREGOIRE T., GRIFFIN S., GRISWOLD S., GUNTHER C., GUTJAHR P., HAACK C., HALLGREN A., HALLIDAY R., HALVE L., HALZEN F., HAMDAOUI H., HA MINH M., HANSON K., HARDIN J., HARNISCH A.A., HATCH P., HAUNGS A., HELBING K., HELLRUNG J., HENNINGSEN F., HEUERMANN L., HICKFORD S., HIDVEGI A., HILL C., HILL G.C., HOFFMAN K.D., HOSHINA K., HOU W., HUBER T., HULTQVIST K., HUNNEFELD M., HUSSAIN R., HYMON K., IN S., IOVINE N., ISHIHARA A., JANSSON M., JAPARIDZE G.S., JEONG M., JIN M., JONES B.J.P., KANG D., KANG W., KANG X., KAPPES A., KAPPESSER D., KARDUM L., KARG T., KARL M., KARLE A., KATZ U., KAUER M., KELLEY J.L., KHEIRANDISH A., KIN K., KIRYLUK J., KLEIN S.R., KOCHOCKI A., KOIRALA R., KOLANOSKI H., KONTRIMAS T., KOPKE L., KOPPER C., KOSKINEN D.J., KOUNDAL P., KOVACEVICH M., KOWALSKI M., KOZYNETS T., KRUISWIJK K., KRUPCZAK E., KUMAR A., KUN E., KURAHASHI N., LAD N., LAGUNAS GUALDA C., LAMOUREUX M., LARSON M.J., LAUBER F., LAZAR J.P., LEE J.W., LEONARD DEHOLTON K., LESZCZYNSKA A., LINCETTO M., LIU Q.R., LIUBARSKA M., LOHFINK E., LOVE C., LOZANO MARISCAL C.J., LU L., LUCARELLI F., LUDWIG A., LUSZCZAK W., LYU Y., MA W.Y., MADSEN J., MAHN K.B.M., MAKINO Y., MANCINA S., MARIE SAINTE W., MARIS I.C., MARKA S., MARKA Z., MARSEE M., MARTINEZ-SOLER I., MARUYAMA R., MAYHEW F., McELROY T., McNALLY F., MEAD J.V., MEAGHER K., MECHBAL S., MEDINA A., MEIER M., MEIGHEN-BERGER S., MERCKX Y., MERTEN L., MICALLEF J., MOCKLER D., MONTARULI T., MOORE R.W., MORII Y., MORSE R., MOULAI M., MUKHERJEE T., NAAB R., NAGAI R., NAUMANN U., NAYERHODA A., NECKER J., NEUMANN M., NIEDERHAUSEN H., NISA M.U., NOELL A., NOWICKI S.C., OBERTACKE POLLMANN A., OEHLER M., OEYEN B., OLIVAS A., ORSOE R., OSBORN J., O'SULLIVAN E., PANDYA H., PANKOVA D.V., PARK N., PARKER G.K., PAUDEL E.N., PAUL L., PEREZ DE LOS HEROS C., PETERSON J., PHILIPPEN S., PIEPER S., PIZZUTO A., PLUM M., POPOVYCH Y., PRADO RODRIGUEZ M., PRIES B., PROCTER-MURPHY R., PRZYBYLSKI G.T., RAAB C., RACK-HELLEIS J., RAWLINS K., RECHAV Z., REHMAN A., REICHHERZER P., RENZI G., RESCONI E., REUSCH S., RHODE W., RICHMAN M., RIEDEL B., ROBERTS E.J., ROBERTSON S., RODAN S., ROELLINGHOFF G., RONGEN M., ROTT C., RUHE T., RUOHAN L., RYCKBOSCH D., RYSEWYK CANTU D., SAFA I., SAFFER J., SALAZAR-GALLEGOS D., SAMPATHKUMAR P., SANCHEZ HERRERA S.E., SANDROCK A., SANTANDER M., SARKAR S., SARKAR S., SAVELBERG J., SAVINA P., SCHAUFEL M., SCHIELER H., SCHINDLER S., SCHLUTER B., SCHMIDT T., SCHNEIDER J., SCHRODER F.G., SCHUMACHER L., SCHWEFER G., SCLAFANI S., SECKEL D., SEUNARINE S., SHARMA A., SHEFALI S., SHIMIZU N., SILVA M., SKRZYPEK B., SMITHERS B., SNIHUR R., SOEDINGREKSO J., SOGAARD A., SOLDIN D., SPANNFELLNER C., SPICZAK G.M., SPIERING C., STAMATIKOS M., STANEV T., STEIN R., STEZELBERGER T., STURWALD T., STUTTARD T., SULLIVAN G.W., TABOADA I., TER-ANTONYAN S., THOMPSON W.G., THWAITES J., TILAV S., TOLLEFSON K., TONNIS C., TOSCANO S., TOSI D., TRETTIN A., TUNG C.F., TURCOTTE R., TWAGIRAYEZU J.P., TY B., UNLAND ELORRIETA M.A., UPSHAW K., VALTONEN-MATTILA N., VANDENBROUCKE J., VAN EIJNDHOVEN N., VANNEROM D., VAN SANTEN J., VARA J., VEITCH-MICHAELIS J., VERPOEST S., VESKE D., WALCK C., WATSON T.B., WEAVER C., WEIGEL P., WEINDL A., WELDERT J., WENDT C., WERTHEBACH J., WEYRAUCH M., WHITEHORN N., WIEBUSCH C.H., WILLEY N., WILLIAMS D.R., WOLF M., WREDE G., WULFF J., XU X.W., YANEZ J.P., YILDIZCI E., YOSHIDA S., YU S., YUAN T., ZHANG Z., ZHELNIN P. (The IceCube Collaboration)

Abstract (from CDS):

The understanding of novae, the thermonuclear eruptions on the surfaces of white dwarf stars in binaries, has recently undergone a major paradigm shift. Though the bolometric luminosity of novae was long thought to arise directly from photons supplied by the thermonuclear runaway, recent gigaelectronvolt (GeV) gamma-ray observations have supported the notion that a significant portion of the luminosity could come from radiative shocks. More recently, observations of novae have lent evidence that these shocks are acceleration sites for hadrons for at least some types of novae. In this scenario, a flux of neutrinos may accompany the observed gamma rays. As the gamma rays from most novae have only been observed up to a few GeV, novae have previously not been considered as targets for neutrino telescopes, which are most sensitive at and above teraelectronvolt (TeV) energies. Here, we present the first search for neutrinos from novae with energies between a few GeV and 10 TeV using IceCube-DeepCore, a densely instrumented region of the IceCube Neutrino Observatory with a reduced energy threshold. We search both for a correlation between gamma-ray and neutrino emission as well as between optical and neutrino emission from novae. We find no evidence for neutrino emission from the novae considered in this analysis and set upper limits for all gamma-ray detected novae.

Abstract Copyright: © 2023. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Novae - High energy astrophysics - Neutrino astronomy - Neutrino telescopes

Simbad objects: 80

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Number of rows : 80
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 V* V392 Per No* 04 43 21.3694280976 +47 21 25.869776436           ~ 45 0
2 V* V2860 Ori No* 06 09 57.4531362408 +12 12 25.158377304           ~ 12 0
3 V* V959 Mon No* 06 39 38.5986803977 +05 53 52.878876073           ~ 159 0
4 V* V435 CMa No* 07 13 45.84 -21 12 31.3           ~ 9 0
5 V* V549 Vel No* 08 50 29.6173052127 -47 45 28.322206658   17.67 16.45 15.90 15.09 ~ 20 0
6 V* V906 Car No* 10 36 15.4286177568 -59 35 53.696262804           ~ 90 1
7 V* V357 Mus No* 11 26 12.20 -65 31 08.6           ~ 24 0
8 V* V1405 Cen No* 13 20 55.35 -63 42 19.1           ~ 10 0
9 V* FM Cir No* 13 53 27.59 -67 25 00.9           ~ 15 0
10 V* V1369 Cen No* 13 54 45.3506993424 -59 09 04.093260192   15.5   15.1   ~ 80 0
11 OGLE 2015-NOVA-3 No* 14 07 31.34 -63 13 11.5           ~ 4 0
12 V* V407 Lup No* 15 29 01.79 -44 49 39.5           ~ 41 0
13 PNV J15384000-4744500 No* 15 38 43.86 -47 44 42.1           ~ 6 0
14 V* V555 Nor No* 15 41 45.24 -53 08 05.9           ~ 7 0
15 V* T CrB Sy* 15 59 30.1622265912 +25 55 12.613382940   11.516 10.247 9.70   M3IIIe_sh 735 0
16 PNV J16143400-5330050 No* 16 14 34.00 -53 30 05.0           ~ 5 0
17 V* V1662 Sco No* 16 48 49.62 -44 57 03.2           ~ 9 0
18 V* V1657 Sco No* 16 52 18.87 -37 54 18.9           ~ 7 0
19 V* V1535 Sco Sy* 17 03 26.1705418392 -35 04 17.816830248           ~ 43 0
20 V* V1663 Sco No* 17 03 47.509 -38 16 57.14           ~ 8 0
21 V* V1706 Sco No* 17 07 34.186 -36 08 21.26           ~ 7 0
22 PNV J17120009-4017560 No* 17 12 00.18 -40 17 56.6           ~ 6 0
23 V* V3665 Oph No* 17 14 02.53 -28 49 23.3           ~ 7 0
24 V* V1534 Sco Sy* 17 15 46.8805288368 -31 28 30.310465692           M6III 33 0
25 V* V1661 Sco No* 17 18 06.37 -32 04 27.7           ~ 5 0
26 PNV J17184490-2454220 No* 17 18 45.04 -24 54 22.1           ~ 6 0
27 V* V1656 Sco No* 17 22 51.46 -31 58 37.1           ~ 12 0
28 [KW2003] 11 Mi* 17 24 39.9557643000 -24 21 47.399493024       16.106   ~ 11 0
29 V* V2944 Oph No* 17 29 13.42 -18 46 13.8           ~ 34 0
30 VVV J173034.12-310607.0 CV* 17 30 34.1334502128 -31 06 07.038593604           ~ 8 0
31 V* V1533 Sco No* 17 33 59.43 -36 06 21.6           ~ 9 0
32 V* V2949 Oph No* 17 34 47.75 -24 09 04.2           ~ 9 0
33 V* V3661 Oph No* 17 35 50.41 -29 34 23.8           ~ 11 0
34 V* V1707 Sco No* 17 37 09.54 -35 10 23.2           ~ 11 0
35 V* V1655 Sco No* 17 38 19.31 -37 25 08.7           ~ 6 0
36 AT 2019qfj No* 17 38 31.820 -29 03 47.12           ~ 5 0
37 V* V3731 Oph No* 17 38 35.10 -25 19 02.9           ~ 7 0
38 V* V3662 Oph No* 17 39 46.10 -24 57 55.8           ~ 17 0
39 V* V2677 Oph No* 17 39 56.0 -24 47 42           ~ 23 0
40 PNV J17422408-2053088 No* 17 42 24.11 -20 53 08.6           ~ 7 0
41 V* V1659 Sco No* 17 42 57.68 -33 25 42.9           ~ 7 0
42 OGLE 2015-NOVA-1 No* 17 48 12.82 -32 35 13.4           ~ 9 0
43 OGLE 2016-NOVA-2 CV* 17 49 57.33 -29 14 37.9           ~ 7 0
44 V* RS Oph Sy* 17 50 13.1591484960 -06 42 28.480729788   11.884 10.776 11.228   K5.5/M0IIIe 1094 0
45 VVV NV003 Sy* 17 50 19.27 -33 39 07.3     19     ~ 7 0
46 V* V1324 Sco No* 17 50 53.9093841216 -32 37 21.090962028           ~ 91 0
47 V* V5591 Sgr No* 17 52 25.7939306544 -21 26 21.682062240           ~ 18 0
48 OGLE 2014-NOVA-1 No* 17 55 20.27 -23 23 54.5           ~ 5 0
49 V* V745 Sco Sy* 17 55 22.2260994408 -33 14 58.551839808     17.987   13.353 M2/M6IIIe 242 1
50 PNV J17561375-2942546 No* 17 56 13.75 -29 42 54.6           ~ 4 0
51 OGLE 2012-NOVA-1 No* 17 56 49.39 -27 13 28.2           ~ 6 0
52 V* V5853 Sgr No* 18 01 07.78 -26 31 43.4           ~ 14 0
53 OGLE 2013-NOVA-4 No* 18 01 22.20 -25 18 39.0           ~ 4 0
54 V* V5669 Sgr No* 18 03 32.7413774913 -28 16 05.517235794           ~ 13 0
55 PNV J18040967-1803581 No* 18 04 09.45 -18 03 55.8           ~ 7 0
56 V* V556 Ser CV* 18 09 03.46 -11 12 34.5           ~ 6 0
57 V* V5855 Sgr No* 18 10 28.29 -27 29 59.3           ~ 28 0
58 TCP J18104219-1534184 No* 18 10 42.29 -15 34 18.0           ~ 9 0
59 V* V5667 Sgr No* 18 14 25.15 -25 54 34.7           ~ 15 0
60 V* V5593 Sgr No* 18 19 36.9494206920 -19 07 40.218638268           ~ 12 0
61 V* V5592 Sgr No* 18 20 27.26 -27 44 26.3           ~ 18 0
62 V* V5856 Sgr No* 18 20 52.25 -28 22 12.1           ~ 43 0
63 V* V5850 Sgr CV* 18 22 59.25 -19 14 14.8           ~ 7 0
64 V* V5666 Sgr No* 18 25 08.76 -22 36 02.6           ~ 12 0
65 V* V611 Sct No* 18 25 29.87 -09 47 32.3           ~ 7 0
66 V* V613 Sct No* 18 29 22.93 -14 30 44.2           ~ 9 0
67 V* V3890 Sgr No* 18 30 43.2877623168 -24 01 08.944843980     15.944 14.798 12.611 M5III 207 0
68 V* V612 Sct No* 18 31 45.86 -14 18 55.5           ~ 30 0
69 V* V5668 Sgr No* 18 36 56.827920 -28 55 39.97524       16.028   ~ 120 0
70 V* V659 Sct No* 18 39 59.70 -10 25 41.9           ~ 13 0
71 V* V1724 Aql CV* 18 52 34.96 -00 18 42.3           ~ 16 0
72 V* V1830 Aql No* 19 02 33.38 +03 15 19.0           ~ 11 0
73 V* V1831 Aql No* 19 21 50.15 +15 09 24.8           ~ 13 0
74 V* V569 Vul No* 19 52 08.25 +27 42 20.9           ~ 9 0
75 V* V2659 Cyg No* 20 21 42.3230575202 +31 03 29.401428736           ~ 24 0
76 V* V339 Del No* 20 23 30.6864752010 +20 46 03.777415270   17.50 16.86     ~ 205 0
77 V* V962 Cep No* 20 54 23.75 +60 17 06.9           ~ 13 0
78 V* V2891 Cyg No* 21 09 25.52 +48 10 51.9           ~ 21 0
79 V* V809 Cep No* 23 08 04.71 +60 46 52.1           ~ 21 0
80 NAME Galactic Bulge reg ~ ~           ~ 4326 0

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