The LOFT Ground Segment

E. Bozzo; A. Antonelli; A. Argan; D. Barret; P. Binko; Søren Brandt; E. Cavazzuti; T. Courvoisier; J. W. den Herder; M. Feroci; C. Ferrigno; P. Giommi; D. Götz; L. Guy; M. Hernanz; J. J. M. in't Zand; D. Klochkov; E. Kuulkers; C. Motch; D. Lumb; A. Papitto; C. Pittori; R. Rohlfs; A. Santangelo; C. Schmid; A. D. Schwope; P. J. Smith; N. A. Webb; J. Wilms; S. Zane

doi:10.1117/12.2054728

The LOFT Ground Segment

E. Bozzo, A. Antonelli, A. Argan, D. Barret, P. Binko, Søren Brandt, E. Cavazzuti, T. Courvoisier, J. W. den Herder, M. Feroci, C. Ferrigno, P. Giommi, D. Götz, L. Guy, M. Hernanz, J. J. M. in't Zand, D. Klochkov, E. Kuulkers, C. Motch, D. LumbA. Papitto, C. Pittori, R. Rohlfs, A. Santangelo, C. Schmid, A. D. Schwope, P. J. Smith, N. A. Webb, J. Wilms, S. Zane

National Space Institute

Research output: Chapter in Book/Report/Conference proceeding › Article in proceedings › Research › peer-review

Abstract

LOFT, the Large Observatory For X-ray Timing, was one of the ESA M3 mission candidates that completed their assessment phase at the end of 2013. LOFT is equipped with two instruments, the Large Area Detector (LAD) and the Wide Field Monitor (WFM). The LAD performs pointed observations of several targets per orbit (~90 minutes), providing roughly ~80 GB of proprietary data per day (the proprietary period will be 12 months). The WFM continuously monitors about 1/3 of the sky at a time and provides data for about ~100 sources a day, resulting in a total of ~20 GB of additional telemetry. The LOFT Burst alert System additionally identifies on-board bright impulsive events (e.g., Gamma-ray Bursts, GRBs) and broadcasts the corresponding position and trigger time to the ground using a dedicated system of ~15 VHF receivers. All WFM data are planned to be made public immediately. In this contribution we summarize the planned organization of the LOFT ground segment (GS), as established in the mission Yellow Book 1 . We describe the expected GS contributions from ESA and the LOFT consortium. A review is provided of the planned LOFT data products and the details of the data flow, archiving and distribution. Despite LOFT was not selected for launch within the M3 call, its long assessment phase (> 2 years) led to a very solid mission design and an efficient planning of its ground operations.

Original language	English
Title of host publication	Space Telescopes and Instrumentation 2014 : Ultraviolet to Gamma Ray
Editors	Tadayuki Takahashi, Jan-Willem A. der Herder, Mark Bautz
Number of pages	7
Publisher	SPIE - International Society for Optical Engineering
Publication date	2014
Article number	91446A
DOIs	https://doi.org/10.1117/12.2054728
Publication status	Published - 2014
Event	Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray - Palais des congrès de Montréal, Montréal, Canada Duration: 22 Jun 2014 → 26 Jun 2014 Conference number: 9144

Conference

Conference	Space Telescopes and Instrumentation 2014
Number	9144
Location	Palais des congrès de Montréal
Country	Canada
City	Montréal
Period	22/06/2014 → 26/06/2014

Series	Proceedings of S P I E - International Society for Optical Engineering
Volume	9144
ISSN	0277-786X

Keywords

LOFT
X-rays
Ground segment
Space mission

Access to Document

10.1117/12.2054728

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

File

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

SPIE 2014
Søren Brandt (Participant)
22 Jun 2014 → 27 Jun 2014
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

Bozzo, E., Antonelli, A., Argan, A., Barret, D., Binko, P., Brandt, S., Cavazzuti, E., Courvoisier, T., Herder, J. W. D., Feroci, M., Ferrigno, C., Giommi, P., Götz, D., Guy, L., Hernanz, M., Zand, J. J. M. I., Klochkov, D., Kuulkers, E., Motch, C., ... Zane, S. (2014). The LOFT Ground Segment. In T. Takahashi, J-W. A. D. Herder, & M. Bautz (Eds.), Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray [91446A] SPIE - International Society for Optical Engineering. Proceedings of S P I E - International Society for Optical Engineering Vol. 9144 https://doi.org/10.1117/12.2054728

Bozzo, E. ; Antonelli, A. ; Argan, A. ; Barret, D. ; Binko, P. ; Brandt, Søren ; Cavazzuti, E. ; Courvoisier, T. ; Herder, J. W. den ; Feroci, M. ; Ferrigno, C. ; Giommi, P. ; Götz, D. ; Guy, L. ; Hernanz, M. ; Zand, J. J. M. in't ; Klochkov, D. ; Kuulkers, E. ; Motch, C. ; Lumb, D. ; Papitto, A. ; Pittori, C. ; Rohlfs, R. ; Santangelo, A. ; Schmid, C. ; Schwope, A. D. ; Smith, P. J. ; Webb, N. A. ; Wilms, J. ; Zane, S. / The LOFT Ground Segment. Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray. editor / Tadayuki Takahashi ; Jan-Willem A. der Herder ; Mark Bautz. SPIE - International Society for Optical Engineering, 2014. (Proceedings of S P I E - International Society for Optical Engineering, Vol. 9144).

@inproceedings{9c5c38b5388c46f6b3620d8ec39f5cb4,

title = "The LOFT Ground Segment",

abstract = "LOFT, the Large Observatory For X-ray Timing, was one of the ESA M3 mission candidates that completed their assessment phase at the end of 2013. LOFT is equipped with two instruments, the Large Area Detector (LAD) and the Wide Field Monitor (WFM). The LAD performs pointed observations of several targets per orbit (~90 minutes), providing roughly ~80 GB of proprietary data per day (the proprietary period will be 12 months). The WFM continuously monitors about 1/3 of the sky at a time and provides data for about ~100 sources a day, resulting in a total of ~20 GB of additional telemetry. The LOFT Burst alert System additionally identifies on-board bright impulsive events (e.g., Gamma-ray Bursts, GRBs) and broadcasts the corresponding position and trigger time to the ground using a dedicated system of ~15 VHF receivers. All WFM data are planned to be made public immediately. In this contribution we summarize the planned organization of the LOFT ground segment (GS), as established in the mission Yellow Book 1 . We describe the expected GS contributions from ESA and the LOFT consortium. A review is provided of the planned LOFT data products and the details of the data flow, archiving and distribution. Despite LOFT was not selected for launch within the M3 call, its long assessment phase (> 2 years) led to a very solid mission design and an efficient planning of its ground operations.",

keywords = "LOFT, X-rays, Ground segment, Space mission",

author = "E. Bozzo and A. Antonelli and A. Argan and D. Barret and P. Binko and S{\o}ren Brandt and E. Cavazzuti and T. Courvoisier and Herder, {J. W. den} and M. Feroci and C. Ferrigno and P. Giommi and D. G{\"o}tz and L. Guy and M. Hernanz and Zand, {J. J. M. in't} and D. Klochkov and E. Kuulkers and C. Motch and D. Lumb and A. Papitto and C. Pittori and R. Rohlfs and A. Santangelo and C. Schmid and Schwope, {A. D.} and Smith, {P. J.} and Webb, {N. A.} and J. Wilms and S. Zane",

year = "2014",

doi = "10.1117/12.2054728",

language = "English",

series = "Proceedings of S P I E - International Society for Optical Engineering",

publisher = "SPIE - International Society for Optical Engineering",

editor = "Tadayuki Takahashi and Herder, {Jan-Willem A. der} and Mark Bautz",

booktitle = "Space Telescopes and Instrumentation 2014",

note = "Space Telescopes and Instrumentation 2014 : Ultraviolet to Gamma Ray ; Conference date: 22-06-2014 Through 26-06-2014",

}

Bozzo, E, Antonelli, A, Argan, A, Barret, D, Binko, P, Brandt, S, Cavazzuti, E, Courvoisier, T, Herder, JWD, Feroci, M, Ferrigno, C, Giommi, P, Götz, D, Guy, L, Hernanz, M, Zand, JJMI, Klochkov, D, Kuulkers, E, Motch, C, Lumb, D, Papitto, A, Pittori, C, Rohlfs, R, Santangelo, A, Schmid, C, Schwope, AD, Smith, PJ, Webb, NA, Wilms, J & Zane, S 2014, The LOFT Ground Segment. in T Takahashi, J-WAD Herder & M Bautz (eds), Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray., 91446A, SPIE - International Society for Optical Engineering, Proceedings of S P I E - International Society for Optical Engineering, vol. 9144, Space Telescopes and Instrumentation 2014, Montréal, Canada, 22/06/2014. https://doi.org/10.1117/12.2054728

The LOFT Ground Segment. / Bozzo, E.; Antonelli, A.; Argan, A.; Barret, D.; Binko, P.; Brandt, Søren; Cavazzuti, E.; Courvoisier, T.; Herder, J. W. den; Feroci, M.; Ferrigno, C.; Giommi, P.; Götz, D.; Guy, L.; Hernanz, M.; Zand, J. J. M. in't; Klochkov, D.; Kuulkers, E.; Motch, C.; Lumb, D.; Papitto, A.; Pittori, C.; Rohlfs, R.; Santangelo, A.; Schmid, C.; Schwope, A. D.; Smith, P. J.; Webb, N. A.; Wilms, J.; Zane, S.

Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray. ed. / Tadayuki Takahashi; Jan-Willem A. der Herder; Mark Bautz. SPIE - International Society for Optical Engineering, 2014. 91446A (Proceedings of S P I E - International Society for Optical Engineering, Vol. 9144).

Research output: Chapter in Book/Report/Conference proceeding › Article in proceedings › Research › peer-review

TY - GEN

T1 - The LOFT Ground Segment

AU - Bozzo, E.

AU - Antonelli, A.

AU - Argan, A.

AU - Barret, D.

AU - Binko, P.

AU - Brandt, Søren

AU - Cavazzuti, E.

AU - Courvoisier, T.

AU - Herder, J. W. den

AU - Feroci, M.

AU - Ferrigno, C.

AU - Giommi, P.

AU - Götz, D.

AU - Guy, L.

AU - Hernanz, M.

AU - Zand, J. J. M. in't

AU - Klochkov, D.

AU - Kuulkers, E.

AU - Motch, C.

AU - Lumb, D.

AU - Papitto, A.

AU - Pittori, C.

AU - Rohlfs, R.

AU - Santangelo, A.

AU - Schmid, C.

AU - Schwope, A. D.

AU - Smith, P. J.

AU - Webb, N. A.

AU - Wilms, J.

AU - Zane, S.

N1 - Conference code: 9144

PY - 2014

Y1 - 2014

N2 - LOFT, the Large Observatory For X-ray Timing, was one of the ESA M3 mission candidates that completed their assessment phase at the end of 2013. LOFT is equipped with two instruments, the Large Area Detector (LAD) and the Wide Field Monitor (WFM). The LAD performs pointed observations of several targets per orbit (~90 minutes), providing roughly ~80 GB of proprietary data per day (the proprietary period will be 12 months). The WFM continuously monitors about 1/3 of the sky at a time and provides data for about ~100 sources a day, resulting in a total of ~20 GB of additional telemetry. The LOFT Burst alert System additionally identifies on-board bright impulsive events (e.g., Gamma-ray Bursts, GRBs) and broadcasts the corresponding position and trigger time to the ground using a dedicated system of ~15 VHF receivers. All WFM data are planned to be made public immediately. In this contribution we summarize the planned organization of the LOFT ground segment (GS), as established in the mission Yellow Book 1 . We describe the expected GS contributions from ESA and the LOFT consortium. A review is provided of the planned LOFT data products and the details of the data flow, archiving and distribution. Despite LOFT was not selected for launch within the M3 call, its long assessment phase (> 2 years) led to a very solid mission design and an efficient planning of its ground operations.

AB - LOFT, the Large Observatory For X-ray Timing, was one of the ESA M3 mission candidates that completed their assessment phase at the end of 2013. LOFT is equipped with two instruments, the Large Area Detector (LAD) and the Wide Field Monitor (WFM). The LAD performs pointed observations of several targets per orbit (~90 minutes), providing roughly ~80 GB of proprietary data per day (the proprietary period will be 12 months). The WFM continuously monitors about 1/3 of the sky at a time and provides data for about ~100 sources a day, resulting in a total of ~20 GB of additional telemetry. The LOFT Burst alert System additionally identifies on-board bright impulsive events (e.g., Gamma-ray Bursts, GRBs) and broadcasts the corresponding position and trigger time to the ground using a dedicated system of ~15 VHF receivers. All WFM data are planned to be made public immediately. In this contribution we summarize the planned organization of the LOFT ground segment (GS), as established in the mission Yellow Book 1 . We describe the expected GS contributions from ESA and the LOFT consortium. A review is provided of the planned LOFT data products and the details of the data flow, archiving and distribution. Despite LOFT was not selected for launch within the M3 call, its long assessment phase (> 2 years) led to a very solid mission design and an efficient planning of its ground operations.

KW - LOFT

KW - X-rays

KW - Ground segment

KW - Space mission

U2 - 10.1117/12.2054728

DO - 10.1117/12.2054728

M3 - Article in proceedings

T3 - Proceedings of S P I E - International Society for Optical Engineering

BT - Space Telescopes and Instrumentation 2014

A2 - Takahashi, Tadayuki

A2 - Herder, Jan-Willem A. der

A2 - Bautz, Mark

PB - SPIE - International Society for Optical Engineering

T2 - Space Telescopes and Instrumentation 2014

Y2 - 22 June 2014 through 26 June 2014

ER -

Bozzo E, Antonelli A, Argan A, Barret D, Binko P, Brandt S et al. The LOFT Ground Segment. In Takahashi T, Herder J-WAD, Bautz M, editors, Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray. SPIE - International Society for Optical Engineering. 2014. 91446A. (Proceedings of S P I E - International Society for Optical Engineering, Vol. 9144). https://doi.org/10.1117/12.2054728

The LOFT Ground Segment

Abstract

Conference

Keywords

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Projects

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

Activities

SPIE 2014

European Space Agency - ESA (External organisation)

Cite this