Observations of the unidentified TeV gamma-ray source TeV J2032+4130 with the Whipple Observatory 10 m telescope

Date

2007-04-01

Author

Konopelko, A.
Atkins, R. W.
Blaylock, G.
Buckley, J. H.
Butt, Y.
Carter-Lewis, D. A.
Celik, O.
Cogan, P.
Chow, Y. C. K.
Cui, W.
Dowdall, C.
Ergin, Tülün
Falcone, A. D.
Fegan, D. J.
Fegan, S. J.
Finley, J. P.
Fortin, P.
Gillanders, G. H.
Gutierrez, K. J.
Hall, J.
Hanna, D.
Horan, D.
Hughes, S. B.
Humensky, T. B.
Imran, A.
Jung, I.
Kaaret, P.
Kenny, G. E.
Kertzman, M.
Kieda, D. B.
Kildea, J.
Knapp, J.
Kosack, K.
Krawczynski, H.
Krennrich, F.
Lang, M. J.
LeBohec, S.
Moriarty, P.
Mukherjee, R.
Nagai, T.
Ong, R. A.
Perkins, J. S.
Pohl, M.
Ragan, K.
Reynolds, P. T.
Rose, H. J.
Sembroski, G. H.
Schroedter, M.
Smith, A. W.
Steele, D.
Syson, A.
Swordy, S. P.
Toner, J. A.
Valcarcel, L.
Vassiliev, V. V.
Wagner, R. G.
Wakely, S. P.
Weekes, T. C.
White, R. J.
Williams, D. A.
Zitzer, B.

Metadata

Show full item record

This work is licensed under a Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.

Item Usage Stats

202
views

0
downloads

We report on observations of the sky region around the unidentified TeV gamma-ray source (TeV J2032+ 4130) carried out with the Whipple Observatory 10 m atmospheric Cerenkov telescope for a total of 65.5 hr between 2003 and 2005. The standard two-dimensional analysis developed by the Whipple collaboration for a stand-alone telescope reveals an excess in the field of view at a pretrial significance level of 6.1 sigma. The measured position of this excess is alpha = 20(h)32(m)27(s), delta = 41 degrees 39'17" (J2000.0). The estimated integral flux for this gamma-ray source is about 8% of the Crab Nebula flux. The data are consistent with a pointlike source. Here we present a detailed description of the standard two-dimensional analysis technique used for the analysis of data taken with the Whipple Observatory 10 m telescope and the results for the TeV J2032+ 4130 campaign. We include a short discussion of the physical mechanisms that may be responsible for the observed gamma-ray emission, based on possible association with known astrophysical objects, in particular, Cygnus OB2.

Subject Keywords

Space and Planetary Science, Astronomy and Astrophysics

URI

https://hdl.handle.net/11511/35522

Journal

ASTROPHYSICAL JOURNAL

DOI

https://doi.org/10.1086/511262

Collections

Department of Physics, Article

Suggestions

OpenMETU
Core

OBSERVATIONS OF THE SHELL-TYPE SUPERNOVA REMNANT CASSIOPEIA A AT TeV ENERGIES WITH VERITAS Acciari, V. A.; et. al. (IOP Publishing, 2010-05-01) We report on observations of very high energy gamma rays from the shell-type supernova remnant (SNR) Cassiopeia A with the Very Energetic Radiation Imaging Telescope Array System stereoscopic array of four imaging atmospheric Cherenkov telescopes in Arizona. The total exposure time for these observations is 22 hr, accumulated between September and November of 2007. The gamma-ray source associated with the SNR Cassiopeia A was detected above 200 GeV with a statistical significance of 8.3 sigma. The estimated...
A search for supernova remnants in the nearby spiral galaxy M74 (NGC 628) SONBAŞ, EDA; AKYÜZ, AYSUN; Balman, Şölen; Ozel, M. E. (EDP Sciences, 2010-07-01) An optical search was carried out for supernova remnants (SNRs) in the Sc type nearby spiral galaxy M 74, using ground-based observations at the TUBITAK National Observatory (TUG, Antalya/Turkey) and the Special Astrophysics Observatory (SAO, Russia). Observations were supplemented by the spectral analysis of archived X-ray data from XMM-Newton and Chandra. The survey of M74 covered similar to 9 arcmin(2) with [S II], H alpha, and their continuum filters. Interference filter images of M 74 were obtained the...
Upper limits to the SN1006 multi-TeV gamma-ray flux from HESS observations Aharonian, F; et. al. (EDP Sciences, 2005-07-01) Observations of the shell-type supernova remnant SN1006 have been carried out with the HESS system of Cherenkov telescopes during 2003 (18.2 h with two operating telescopes) and 2004 (6.3 h with all four telescopes). No evidence for TeV gamma-ray emission from any compact or extended region associated with the remnant is seen and resulting upper limits at the 99.9% confidence level are up to a factor 10 lower than previously-published fluxes from CANGAROO. For SN1006 at its current epoch of evolution we def...
The first hours of the optical afterglow from the cosmic gamma-ray burst 030329 Burenin, RA; Sunyaev, RA; Pavlinsky, MN; Denisenko, DV; Terekhov, OV; Tkachenko, AY; Aslan, Z; Khamitov, I; Uluch, K; Alpar, MA; Kiziloglu, U; Baykal, Altan; Bikmaev, IF; Sakhibullin, NR; Suleymanov, VF (Pleiades Publishing Ltd, 2003-09-01) We describe the first results Of Our observations of the exceptionally bright optical afterglow from the cosmic gamma-ray burst (GRB) of March 29, 2003 (030329), with the 1.5-m Russian-Turkish telescope (RTT150) installed at the TUBITAK National Observatory (Turkey) at Mount Bakyrlytepe. RTT150 was one of the first medium-class telescopes pointed at the afterglow. The observations began as early as about six hours after the GRB. During the first five hours of our observations, the BVRI flux fell off exactly...
Discovery of a transient magnetar: XTE J1810-197 Ibrahim, AI; Markwardt, CB; Swank, JH; Ransom, S; Roberts, M; Kaspi, V; Woods, PM; Safi-Harb, S; Balman, Şölen; Parke, WC; Kouveliotou, C; Hurley, K; Cline, T (IOP Publishing, 2004-07-01) We report the discovery of a new X-ray pulsar, XTE J1810 - 197, that was serendipitously discovered on 2003 July 15 by the Rossi X-Ray Timing Explorer (RXTE) while observing the soft gamma repeater SGR 1806 - 20. The pulsar has a 5.54 s spin period, a soft X-ray spectrum ( with a photon index of approximate to 4), and is detectable in earlier RXTE observations back to 2003 January but not before. These show that a transient outburst began between 2002 November 17 and 2003 January 23 and that the source's pe...

Citation Formats

A. Konopelko et al., “Observations of the unidentified TeV gamma-ray source TeV J2032+4130 with the Whipple Observatory 10 m telescope,” ASTROPHYSICAL JOURNAL, pp. 1062–1068, 2007, Accessed: 00, 2020. [Online]. Available: https://hdl.handle.net/11511/35522.