The third interplanetary network

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

doi:10.1063/1.3509301

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

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 photoncm^-2 s^-1. It detects ∼346 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, and SuperAGILE; the localization accuracy is in the several arcminute and above range. The uses of the IPN data are described.

Original language	English (US)
Title of host publication	Deciphering the Ancient Universe with Gamma-Ray Bursts
Pages	330-333
Number of pages	4
DOIs	https://doi.org/10.1063/1.3509301
State	Published - 2010
Event	International Symposium "Deciphering the Ancient Universe with Gamma-Ray Bursts" - Kyoto, Japan Duration: Apr 19 2010 → Apr 23 2010

Publication series

Name	AIP Conference Proceedings
Volume	1279
ISSN (Print)	0094-243X
ISSN (Electronic)	1551-7616

Other

Other	International Symposium "Deciphering the Ancient Universe with Gamma-Ray Bursts"
Country/Territory	Japan
City	Kyoto
Period	4/19/10 → 4/23/10

Keywords

Gamma-rays: Bursts
Instrumentation

ASJC Scopus subject areas

General Physics and Astronomy

Access to Document

10.1063/1.3509301

Cite this

Hurley, K., Golenetskii, S., Aptekar, R., Mazets, E., Pal'shin, V., Frederiks, D., Mitrofanov, I. G., Golovin, D., Litvak, M. L., Sanin, A. B., Boynton, W., Fellows, C., Harshman, K., Starr, R., Smith, D. M., Wigger, C., Hajdas, W., Von Kienlin, A., Rau, A., ... Meegan, C. (2010). The third interplanetary network. In Deciphering the Ancient Universe with Gamma-Ray Bursts (pp. 330-333). (AIP Conference Proceedings; Vol. 1279). https://doi.org/10.1063/1.3509301

Hurley, K, Golenetskii, S, Aptekar, R, Mazets, E, Pal'shin, V, Frederiks, D, Mitrofanov, IG, Golovin, D, Litvak, ML, Sanin, AB, Boynton, W, Fellows, C, Harshman, K, Starr, R, Smith, DM, Wigger, C, Hajdas, W, Von Kienlin, A, Rau, A, Yamaoka, K, Ohno, M, Takahashi, T, Fukazawa, Y, Tashiro, M, Terada, Y, Murakami, T, Makishima, K, Barthelmy, S, Cline, T, Cummings, J, Gehrels, N, Krimm, H, Goldsten, J, Del Monte, E, Feroci, M, Marisaldi, M, Briggs, M, Connaughton, V & Meegan, C 2010, The third interplanetary network. in Deciphering the Ancient Universe with Gamma-Ray Bursts. AIP Conference Proceedings, vol. 1279, pp. 330-333, International Symposium "Deciphering the Ancient Universe with Gamma-Ray Bursts", Kyoto, Japan, 4/19/10. https://doi.org/10.1063/1.3509301

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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 {\texttimes} 10-7 erg cm-2 or 1 photoncm-2 s-1. It detects ∼346 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, and SuperAGILE; the localization accuracy is in the several arcminute and above range. The uses of the IPN data are described.",

keywords = "Gamma-rays: Bursts, 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 Litvak, \{M. L.\} and Sanin, \{A. B.\} and W. Boynton and C. Fellows and K. Harshman and R. Starr and Smith, \{D. M.\} and C. Wigger and W. Hajdas and \{Von Kienlin\}, A. and A. Rau and K. Yamaoka and M. Ohno and T. Takahashi and Y. Fukazawa and M. Tashiro and Y. Terada and T. Murakami and K. Makishima and S. Barthelmy and T. Cline and J. Cummings and N. Gehrels and H. Krimm and J. Goldsten and \{Del Monte\}, E. and M. Feroci and M. Marisaldi and M. Briggs and V. Connaughton and C. Meegan",

year = "2010",

doi = "10.1063/1.3509301",

language = "English (US)",

isbn = "9780735408296",

series = "AIP Conference Proceedings",

pages = "330--333",

booktitle = "Deciphering the Ancient Universe with Gamma-Ray Bursts",

note = "International Symposium {"}Deciphering the Ancient Universe with Gamma-Ray Bursts{"} ; Conference date: 19-04-2010 Through 23-04-2010",

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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 - Litvak, M. L.

AU - Sanin, A. B.

AU - Boynton, W.

AU - Fellows, C.

AU - Harshman, K.

AU - Starr, R.

AU - Smith, D. M.

AU - Wigger, C.

AU - Hajdas, W.

AU - Von Kienlin, A.

AU - Rau, A.

AU - Yamaoka, K.

AU - Ohno, M.

AU - Takahashi, T.

AU - Fukazawa, Y.

AU - Tashiro, M.

AU - Terada, Y.

AU - Murakami, T.

AU - Makishima, K.

AU - Barthelmy, S.

AU - Cline, T.

AU - Cummings, J.

AU - Gehrels, N.

AU - Krimm, H.

AU - Goldsten, J.

AU - Del Monte, E.

AU - Feroci, M.

AU - Marisaldi, M.

AU - Briggs, M.

AU - Connaughton, V.

AU - Meegan, C.

PY - 2010

Y1 - 2010

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 photoncm-2 s-1. It detects ∼346 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, and SuperAGILE; the localization accuracy is in the several arcminute and above range. The uses of the IPN data are described.

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 photoncm-2 s-1. It detects ∼346 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, and SuperAGILE; the localization accuracy is in the several arcminute and above range. The uses of the IPN data are described.

KW - Gamma-rays: Bursts

KW - Instrumentation

UR - https://www.scopus.com/pages/publications/78649890599

UR - https://www.scopus.com/pages/publications/78649890599#tab=citedBy

U2 - 10.1063/1.3509301

DO - 10.1063/1.3509301

M3 - Conference contribution

AN - SCOPUS:78649890599

SN - 9780735408296

T3 - AIP Conference Proceedings

SP - 330

EP - 333

BT - Deciphering the Ancient Universe with Gamma-Ray Bursts

T2 - International Symposium "Deciphering the Ancient Universe with Gamma-Ray Bursts"

Y2 - 19 April 2010 through 23 April 2010

ER -