The LOFT (Large Observatory for X-ray Timing) background simulations

R. Campana; M. Feroci; E. Del Monte; Søren Brandt; Carl Budtz-Jørgensen; Niels Lund; J. Alvarez; M. Hernanz; E. Perinati

doi:10.1117/12.925999

The LOFT (Large Observatory for X-ray Timing) background simulations

R. Campana, M. Feroci, E. Del Monte, Søren Brandt, Carl Budtz-Jørgensen, Niels Lund, J. Alvarez, M. Hernanz, E. Perinati

National Space Institute

Research output: Contribution to journal › Conference article › Research › peer-review

Abstract

The Large Observatory For X-ray Timing (LOFT) is an innovative medium-class mission selected for an assessment phase in the framework of the ESA M3 Cosmic Vision call. LOFT is intended to answer fundamental questions about the behavior of matter in theh very strong gravitational and magnetic fields around compact objects. With an effective area of ~10 m<sup>2</sup> LOFT will be able to measure very fast variability in the X-ray fluxes and spectra. A good knowledge of the in-orbit background environment is essential to assess the scientific performance of the mission and to optimize the instrument design. The two main contributions to the background are cosmic diffuse X-rays and high energy cosmic rays; also, albedo emission from the Earth is significant. These contributions to the background for both the Large Area Detector and the Wide Field Monitor are discussed, on the basis of extrensive Geant-4 simulations of a simplified instrumental mass model.© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE).

Original language	English
Journal	Proceedings of S P I E - International Society for Optical Engineering
Volume	8443
Issue number	PART 3
Pages (from-to)	84435O
Number of pages	9
ISSN	0277-786X
DOIs	https://doi.org/10.1117/12.925999
Publication status	Published - 2012
Event	Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray - Amsterdam RAI Convention Ctr., Amsterdam, Netherlands Duration: 1 Jul 2012 → 6 Jul 2012 Conference number: 8443

Conference

Conference	Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray
Number	8443
Location	Amsterdam RAI Convention Ctr.
Country	Netherlands
City	Amsterdam
Period	01/07/2012 → 06/07/2012

Access to Document

10.1117/12.925999

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1 Active

LOFT: LOFT, the Large Observatory For X-ray Timing
Brandt, S., Budtz-Jørgensen, C., Lund, N., Pedersen, S. M., Kuvvetli, I. & Hansen, F.
15/02/2011 → …
Project: Research

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1 Participating in or organising workshops, courses, seminars etc.
1 Membership of commitees, commissions, boards, councils, associations, organisations, or similar

Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray
Søren Brandt (Participant)
1 Jul 2012 → 6 Jul 2012
Activity: Attending an event › Participating in or organising workshops, courses, seminars etc.
European Space Agency - ESA (External organisation)
Søren Brandt (Participant)
25 May 2011 → 31 Dec 2013
Activity: Membership › Membership of commitees, commissions, boards, councils, associations, organisations, or similar

Cite this

@inproceedings{cc42176d997f4977840f291cebf1176a,

title = "The LOFT (Large Observatory for X-ray Timing) background simulations",

abstract = "The Large Observatory For X-ray Timing (LOFT) is an innovative medium-class mission selected for an assessment phase in the framework of the ESA M3 Cosmic Vision call. LOFT is intended to answer fundamental questions about the behavior of matter in theh very strong gravitational and magnetic fields around compact objects. With an effective area of ~10 m2 LOFT will be able to measure very fast variability in the X-ray fluxes and spectra. A good knowledge of the in-orbit background environment is essential to assess the scientific performance of the mission and to optimize the instrument design. The two main contributions to the background are cosmic diffuse X-rays and high energy cosmic rays; also, albedo emission from the Earth is significant. These contributions to the background for both the Large Area Detector and the Wide Field Monitor are discussed, on the basis of extrensive Geant-4 simulations of a simplified instrumental mass model.{\textcopyright} (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). ",

author = "R. Campana and M. Feroci and {Del Monte}, E. and S{\o}ren Brandt and Carl Budtz-J{\o}rgensen and Niels Lund and J. Alvarez and M. Hernanz and E. Perinati",

year = "2012",

doi = "10.1117/12.925999",

language = "English",

volume = "8443",

pages = "84435O",

journal = "Proceedings of SPIE, the International Society for Optical Engineering",

issn = "0277-786X",

publisher = "International Society for Optical Engineering",

number = "PART 3",

note = "Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray ; Conference date: 01-07-2012 Through 06-07-2012",

}

The LOFT (Large Observatory for X-ray Timing) background simulations. / Campana, R.; Feroci, M.; Del Monte, E.; Brandt, Søren ; Budtz-Jørgensen, Carl ; Lund, Niels; Alvarez, J.; Hernanz, M.; Perinati, E.

In: Proceedings of S P I E - International Society for Optical Engineering, Vol. 8443, No. PART 3, 2012, p. 84435O.

Research output: Contribution to journal › Conference article › Research › peer-review

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AU - Campana, R.

AU - Feroci, M.

AU - Del Monte, E.

AU - Brandt, Søren

AU - Budtz-Jørgensen, Carl

AU - Lund, Niels

AU - Alvarez, J.

AU - Hernanz, M.

AU - Perinati, E.

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AB - The Large Observatory For X-ray Timing (LOFT) is an innovative medium-class mission selected for an assessment phase in the framework of the ESA M3 Cosmic Vision call. LOFT is intended to answer fundamental questions about the behavior of matter in theh very strong gravitational and magnetic fields around compact objects. With an effective area of ~10 m2 LOFT will be able to measure very fast variability in the X-ray fluxes and spectra. A good knowledge of the in-orbit background environment is essential to assess the scientific performance of the mission and to optimize the instrument design. The two main contributions to the background are cosmic diffuse X-rays and high energy cosmic rays; also, albedo emission from the Earth is significant. These contributions to the background for both the Large Area Detector and the Wide Field Monitor are discussed, on the basis of extrensive Geant-4 simulations of a simplified instrumental mass model.© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE).

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T2 - Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray

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The LOFT (Large Observatory for X-ray Timing) background simulations

Abstract

Conference

Access to Document

LOFT: LOFT, the Large Observatory For X-ray Timing

Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray

European Space Agency - ESA (External organisation)

Cite this