The third interplanetary network

K. Hurley; S. Golenetskii; R. Aptekar; E. Mazets; V. Pal'shin; D. Frederiks; I. G. Mitrofanov; D. Golovin; A. Kozyrev; M. Litvak; A. B. Sanin; W. Boynton; C. Fellows; K. Harshman; R. Starr; A. Von Kienlin; A. Rau; K. Yamaoka; M. Ohno; Y. Fukazawa; T. Takahashi; M. Tashiro; Y. Terada; T. Murakami; K. Makishima; S. Barthelmy; J. Cummings; N. Gehrels; H. Krimm; T. Cline; J. Goldsten; E. Del Monte; M. Feroci; M. Marisaldi; M. Briggs; V. Connaughton; C. Meegan; D. M. Smith; C. Wigger; W. Hajdas

doi:10.1063/1.3621810

T. Takahashi, M. Tashiro, Y. Terada, T. Murakami, K. Makishima, S. Barthelmy, J. Cummings, N. Gehrels, H. Krimm, T. Cline, J. Goldsten, E. Del Monte, M. Feroci, M. Marisaldi, M. Briggs, V. Connaughton, C. Meegan, D. M. Smith, C. Wigger, W. Hajdas

Lunar and Planetary Laboratory

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

5 Scopus citations

Abstract

The 3rd interplanetary network (IPN), which has been in operation since 1990, presently consists of 9 spacecraft: AGILE, Fermi, RHESSI, Suzaku, and Swift, in low Earth orbit; INTEGRAL, in eccentric Earth orbit with apogee 0.5 light-seconds; Wind, up to ∼7 light-seconds from Earth; MESSENGER, en route to Mercury; and Mars Odyssey, in orbit around Mars. The IPN operates as a full-time, all-sky monitor for transients down to a threshold of about 6×10^-7 erg cm^-2 or 1 photon cm^-2 _s^-1. It detects ∼335 cosmic gamma-ray bursts per year. These events are generally not the same ones detected by narrower field of view instruments such as Swift, INTEGRAL IBIS, SuperAGILE, and MAXI; the localization accuracy is in the several arcminute and above range. The data are publicly available and can be utilized for a wide variety of studies.

Original language	English (US)
Title of host publication	Gamma Ray Bursts 2010, GRB 2010
Pages	385-388
Number of pages	4
DOIs	https://doi.org/10.1063/1.3621810
State	Published - 2011
Event	Gamma Ray Bursts 2010, GRB 2010 - Annapolis, MD, United States Duration: Nov 1 2010 → Nov 4 2010

Publication series

Name	AIP Conference Proceedings
Volume	1358
ISSN (Print)	0094-243X
ISSN (Electronic)	1551-7616

Other

Other	Gamma Ray Bursts 2010, GRB 2010
Country/Territory	United States
City	Annapolis, MD
Period	11/1/10 → 11/4/10

Keywords

Bursts
Gamma-rays
Instrumentation

ASJC Scopus subject areas

General Physics and Astronomy

Access to Document

10.1063/1.3621810

Cite this

Hurley, K., Golenetskii, S., Aptekar, R., Mazets, E., Pal'shin, V., Frederiks, D., Mitrofanov, I. G., Golovin, D., Kozyrev, A., Litvak, M., Sanin, A. B., Boynton, W., Fellows, C., Harshman, K., Starr, R., Von Kienlin, A., Rau, A., Yamaoka, K., Ohno, M., ... Hajdas, W. (2011). The third interplanetary network. In Gamma Ray Bursts 2010, GRB 2010 (pp. 385-388). (AIP Conference Proceedings; Vol. 1358). https://doi.org/10.1063/1.3621810

Hurley, K, Golenetskii, S, Aptekar, R, Mazets, E, Pal'shin, V, Frederiks, D, Mitrofanov, IG, Golovin, D, Kozyrev, A, Litvak, M, Sanin, AB, Boynton, W, Fellows, C, Harshman, K, Starr, R, Von Kienlin, A, Rau, A, Yamaoka, K, Ohno, M, Fukazawa, Y, Takahashi, T, Tashiro, M, Terada, Y, Murakami, T, Makishima, K, Barthelmy, S, Cummings, J, Gehrels, N, Krimm, H, Cline, T, Goldsten, J, Del Monte, E, Feroci, M, Marisaldi, M, Briggs, M, Connaughton, V, Meegan, C, Smith, DM, Wigger, C & Hajdas, W 2011, The third interplanetary network. in Gamma Ray Bursts 2010, GRB 2010. AIP Conference Proceedings, vol. 1358, pp. 385-388, Gamma Ray Bursts 2010, GRB 2010, Annapolis, MD, United States, 11/1/10. https://doi.org/10.1063/1.3621810

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title = "The third interplanetary network",

abstract = "The 3rd interplanetary network (IPN), which has been in operation since 1990, presently consists of 9 spacecraft: AGILE, Fermi, RHESSI, Suzaku, and Swift, in low Earth orbit; INTEGRAL, in eccentric Earth orbit with apogee 0.5 light-seconds; Wind, up to ∼7 light-seconds from Earth; MESSENGER, en route to Mercury; and Mars Odyssey, in orbit around Mars. The IPN operates as a full-time, all-sky monitor for transients down to a threshold of about 6×10-7 erg cm-2 or 1 photon cm-2 s-1. It detects ∼335 cosmic gamma-ray bursts per year. These events are generally not the same ones detected by narrower field of view instruments such as Swift, INTEGRAL IBIS, SuperAGILE, and MAXI; the localization accuracy is in the several arcminute and above range. The data are publicly available and can be utilized for a wide variety of studies.",

keywords = "Bursts, Gamma-rays, Instrumentation",

author = "K. Hurley and S. Golenetskii and R. Aptekar and E. Mazets and V. Pal'shin and D. Frederiks and Mitrofanov, \{I. G.\} and D. Golovin and A. Kozyrev and M. Litvak and Sanin, \{A. B.\} and W. Boynton and C. Fellows and K. Harshman and R. Starr and \{Von Kienlin\}, A. and A. Rau and K. Yamaoka and M. Ohno and Y. Fukazawa and T. Takahashi and M. Tashiro and Y. Terada and T. Murakami and K. Makishima and S. Barthelmy and J. Cummings and N. Gehrels and H. Krimm and T. Cline and J. Goldsten and \{Del Monte\}, E. and M. Feroci and M. Marisaldi and M. Briggs and V. Connaughton and C. Meegan and Smith, \{D. M.\} and C. Wigger and W. Hajdas",

year = "2011",

doi = "10.1063/1.3621810",

language = "English (US)",

isbn = "9780735409163",

series = "AIP Conference Proceedings",

pages = "385--388",

booktitle = "Gamma Ray Bursts 2010, GRB 2010",

note = "Gamma Ray Bursts 2010, GRB 2010 ; Conference date: 01-11-2010 Through 04-11-2010",

}

TY - GEN

T1 - The third interplanetary network

AU - Hurley, K.

AU - Golenetskii, S.

AU - Aptekar, R.

AU - Mazets, E.

AU - Pal'shin, V.

AU - Frederiks, D.

AU - Mitrofanov, I. G.

AU - Golovin, D.

AU - Kozyrev, A.

AU - Litvak, M.

AU - Sanin, A. B.

AU - Boynton, W.

AU - Fellows, C.

AU - Harshman, K.

AU - Starr, R.

AU - Von Kienlin, A.

AU - Rau, A.

AU - Yamaoka, K.

AU - Ohno, M.

AU - Fukazawa, Y.

AU - Takahashi, T.

AU - Tashiro, M.

AU - Terada, Y.

AU - Murakami, T.

AU - Makishima, K.

AU - Barthelmy, S.

AU - Cummings, J.

AU - Gehrels, N.

AU - Krimm, H.

AU - Cline, T.

AU - Goldsten, J.

AU - Del Monte, E.

AU - Feroci, M.

AU - Marisaldi, M.

AU - Briggs, M.

AU - Connaughton, V.

AU - Meegan, C.

AU - Smith, D. M.

AU - Wigger, C.

AU - Hajdas, W.

PY - 2011

Y1 - 2011

N2 - The 3rd interplanetary network (IPN), which has been in operation since 1990, presently consists of 9 spacecraft: AGILE, Fermi, RHESSI, Suzaku, and Swift, in low Earth orbit; INTEGRAL, in eccentric Earth orbit with apogee 0.5 light-seconds; Wind, up to ∼7 light-seconds from Earth; MESSENGER, en route to Mercury; and Mars Odyssey, in orbit around Mars. The IPN operates as a full-time, all-sky monitor for transients down to a threshold of about 6×10-7 erg cm-2 or 1 photon cm-2 s-1. It detects ∼335 cosmic gamma-ray bursts per year. These events are generally not the same ones detected by narrower field of view instruments such as Swift, INTEGRAL IBIS, SuperAGILE, and MAXI; the localization accuracy is in the several arcminute and above range. The data are publicly available and can be utilized for a wide variety of studies.

AB - The 3rd interplanetary network (IPN), which has been in operation since 1990, presently consists of 9 spacecraft: AGILE, Fermi, RHESSI, Suzaku, and Swift, in low Earth orbit; INTEGRAL, in eccentric Earth orbit with apogee 0.5 light-seconds; Wind, up to ∼7 light-seconds from Earth; MESSENGER, en route to Mercury; and Mars Odyssey, in orbit around Mars. The IPN operates as a full-time, all-sky monitor for transients down to a threshold of about 6×10-7 erg cm-2 or 1 photon cm-2 s-1. It detects ∼335 cosmic gamma-ray bursts per year. These events are generally not the same ones detected by narrower field of view instruments such as Swift, INTEGRAL IBIS, SuperAGILE, and MAXI; the localization accuracy is in the several arcminute and above range. The data are publicly available and can be utilized for a wide variety of studies.

KW - Bursts

KW - Gamma-rays

KW - Instrumentation

UR - https://www.scopus.com/pages/publications/80052483845

UR - https://www.scopus.com/pages/publications/80052483845#tab=citedBy

U2 - 10.1063/1.3621810

DO - 10.1063/1.3621810

M3 - Conference contribution

AN - SCOPUS:80052483845

SN - 9780735409163

T3 - AIP Conference Proceedings

SP - 385

EP - 388

BT - Gamma Ray Bursts 2010, GRB 2010

T2 - Gamma Ray Bursts 2010, GRB 2010

Y2 - 1 November 2010 through 4 November 2010

ER -