Skip to main content
Log in

The Large Observatory for X-ray Timing (LOFT)

  • Original Article
  • Published:
Experimental Astronomy Aims and scope Submit manuscript

Abstract

High-time-resolution X-ray observations of compact objects provide direct access to strong-field gravity, to the equation of state of ultradense matter and to black hole masses and spins. A 10 m2-class instrument in combination with good spectral resolution is required to exploit the relevant diagnostics and answer two of the fundamental questions of the European Space Agency (ESA) Cosmic Vision Theme “Matter under extreme conditions”, namely: does matter orbiting close to the event horizon follow the predictions of general relativity? What is the equation of state of matter in neutron stars? The Large Observatory For X-ray Timing (LOFT), selected by ESA as one of the four Cosmic Vision M3 candidate missions to undergo an assessment phase, will revolutionise the study of collapsed objects in our galaxy and of the brightest supermassive black holes in active galactic nuclei. Thanks to an innovative design and the development of large-area monolithic silicon drift detectors, the Large Area Detector (LAD) on board LOFT will achieve an effective area of ~12 m2 (more than an order of magnitude larger than any spaceborne predecessor) in the 2–30 keV range (up to 50 keV in expanded mode), yet still fits a conventional platform and small/medium-class launcher. With this large area and a spectral resolution of <260 eV, LOFT will yield unprecedented information on strongly curved spacetimes and matter under extreme conditions of pressure and magnetic field strength.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Subscribe and save

Springer+ Basic
$34.99 /Month
  • Get 10 units per month
  • Download Article/Chapter or eBook
  • 1 Unit = 1 Article or 1 Chapter
  • Cancel anytime
Subscribe now

Buy Now

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Fig. 1
Fig. 2
Fig. 3
Fig. 4
Fig. 5
Fig. 6
Fig. 7
Fig. 8
Fig. 9
Fig. 10

Similar content being viewed by others

References

  1. Abramowicz, M.A., Kluźniak, W.: A precise determination of black hole spin in GRO J1655-40. Astron. Astrophys. 374, L19–L20 (2001)

    Article  Google Scholar 

  2. Bueno, J.I., García, I., Plaza, M.A.: SMOS PLM MIRAS hold-down release and deployment mechanisms. In: Warmbein, B. (ed.) 11th European Space Mechanisms and Tribology Symposium, ESMATS 2005, vol. 591, pp. 235–242. ESA Special Publication (2005)

  3. Campana, R., Zampa, G., Feroci, M., Vacchi, A., Bonvicini, V., Del Monte, E., Evangelista, Y., Fuschino, F., Labanti, C., Marisaldi, M., Muleri, F., Pacciani, L., Rapisarda, M., Rashevsky, A., Rubini, A., Soffitta, P., Zampa, N., Baldazzi, G., Costa, E., Donnarumma, I., Grassi, M., Lazzarotto, F., Malcovati, P., Mastropietro, M., Morelli, E., Picolli, L.: Imaging performance of a large-area Silicon Drift Detector for X-ray astronomy. Nucl. Instrum. Methods A 633, 22–30 (2011)

    Article  ADS  Google Scholar 

  4. Demorest, P.B., Pennucci, T., Ransom, S.M., Roberts, M.S.E., Hessels, J.W.T.: A two-solar-mass neutron star measured using Shapiro delay. Nature 467, 1081–1083 (2010)

    Article  ADS  Google Scholar 

  5. Dovčiak, M., Bianchi, S., Guainazzi, M., Karas, V., Matt, G.: Relativistic spectral features from X-ray-illuminated spots and the measure of the black hole mass in active galactic nuclei. Mon. Not. R. Astron. Soc. 350, 745–755 (2004)

    Article  ADS  Google Scholar 

  6. Ebisawa, K., Bourban, G., Bodaghee, A., Mowlavi, N., Courvoisier, T.: High-energy sources before INTEGRAL. INTEGRAL reference catalog. Astrophys. J. 411, L59–L62 (2003)

    ADS  Google Scholar 

  7. Fabian, A.C., Rees, M.J., Stella, L., White, N.E.: X-ray fluorescence from the inner disc in Cygnus X-1. Mon. Not. R. Astron. Soc. 238, 729–736 (1989)

    ADS  Google Scholar 

  8. Feroci, M., Costa, E., Soffitta, P., Del Monte, E., di Persio, G., Donnarumma, I., Evangelista, Y., Frutti, M., Lapshov, I., Lazzarotto, F., Mastropietro, M., Morelli, E., Pacciani, L., Porrovecchio, G., Rapisarda, M., Rubini, A., Tavani, M., Argan, A.: SuperAGILE: the hard X-ray imager for the AGILE space mission. Nucl. Instrum. Methods Phys. Res. A 581, 728–754 (2007)

    Article  ADS  Google Scholar 

  9. Feroci, M., Costa, E., Del Monte, E., Donnarumma, I., Evangelista, Y., Lapshov, I., Lazzarotto, F., Pacciani, L., Rapisarda, M., Soffitta, P., di Persio, G., Frutti, M., Mastropietro, M., Morelli, E., Porrovecchio, G., Rubini, A., Antonelli, A., Argan, A., Barbiellini, G., Boffelli, F., Bulgarelli, A., Caraveo, P., Cattaneo, P.W., Chen, A.W., Cocco, V., Colafrancesco, S., Cutini, S., D’Ammando, F., de Paris, G., Di Cocco, G., Fanari, G., Ferrari, A., Fiorini, M., Fornari, F., Fuschino, F., Froysland, T., Galli, M., Gasparrini, D., Gianotti, F., Giommi, P., Giuliani, A., Labanti, C., Liello, F., Lipari, P., Longo, F., Mattaini, E., Marisaldi, M., Mauri, A., Mauri, F., Mereghetti, S., Moretti, E., Morselli, A., Pellizzoni, A., Perotti, F., Piano, G., Picozza, P., Pilia, M., Pittori, C., Pontoni, C., Preger, B., Prest, M., Primavera, R., Pucella, G., Rappoldi, A., Rossi, E., Sabatini, S., Santolamazza, P., Tavani, M., Stellato, S., Tamburelli, F., Traci, A., Trifoglio, M., Trois, A., Vallazza, E., Vercellone, S., Verrecchia, F., Vittorini, V., Zambra, A., Zanello, D., Salotti, L.: Monitoring the hard X-ray sky with SuperAGILE. Astron. Astrophys. 510, A9 (2010)

  10. Gatti, E., Rehak, P.: Semiconductor drift chamber—an application of a novel charge transport scheme. Nucl. Instrum. Methods Phys. Res. 225, 608–614 (1984)

    Article  ADS  Google Scholar 

  11. Giacconi, R., Kellogg, E., Gorenstein, P., Gursky, H., Tananbaum, H.: An X-ray scan of the galactic plane from UHURU. Astrophys. J. 165, L27 (1971)

    Article  ADS  Google Scholar 

  12. in’t Zand, J.J.M., Weinberg, N.N.: Evidence of heavy-element ashes in thermonuclear X-ray bursts with photospheric superexpansion. Astron. Astrophys. 520, A81 (2010)

  13. Israel, G.L., Belloni, T., Stella, L., Rephaeli, Y., Gruber, D.E., Casella, P., Dall’Osso, S., Rea, N., Persic, M., Rothschild, R.E.: The discovery of rapid X-ray oscillations in the tail of the SGR 1806-20 hyperflare. Astrophys. J. 628, L53–L56 (2005)

    Article  ADS  Google Scholar 

  14. Jahoda, K., Markwardt, C.B., Radeva, Y., Rots, A.H., Stark, M.J., Swank, J.H., Strohmayer, T.E., Zhang, W.: Calibration of the Rossi X-ray timing explorer proportional counter array. Astrophys. J. Suppl. 163, 401–423 (2006)

    Article  ADS  Google Scholar 

  15. Kushpil, S., Crescio, E., Giubellino, P., Idzik, M., Kolozhvari, A., Kushpil, V., Martinez, M.I., Mazza, G., Mazzoni, A., Meddi, F., Nouais, D., Petráček, V., Piemonte, C., Rashevsky, A., Riccati, L., Rivetti, A., Tosello, F., Vacchi, A., Wheadon, R.: Beam test results of the irradiated silicon drift detector for ALICE. Nucl. Instrum. Methods Phys. Res. A 566, 94–99 (2006)

    Article  ADS  Google Scholar 

  16. Laor, A.: Line profiles from a disk around a rotating black hole. Astrophys. J. 376, 90–94 (1991)

    Article  ADS  Google Scholar 

  17. Lattimer, J.M., Prakash, M.: Neutron star structure and the equation of state. Astrophys. J. 550, 426–442 (2001)

    Article  ADS  Google Scholar 

  18. Lattimer, J.M., Prakash, M.: Neutron star observations: prognosis for equation of state constraints. Phys. Rep. 442, 109–165 (2007)

    Article  ADS  Google Scholar 

  19. Leahy, D.A., Morsink, S.M., Chung, Y., Chou, Y.: Constraints on the properties of the neutron star XTE J1814-338 from pulse-shape models. Astrophys. J. 691, 1235–1242 (2009)

    Article  ADS  Google Scholar 

  20. Nouais, D., Beolè, S., Bondila, M., Bonvicini, V., Cerello, P., Crescio, E., Giubellino, P., Idzik, M., Kolozhvari, A., Kouchpil, S., Torres, E.L., Martinez, M.I., Mazza, G., Piano, S., Piemonte, C., Rashevsky, A., Riccati, L., Rivetti, A., Tosello, F., Trzaska, W.H., Vacchi, A., Wheadon, R., The ALICE Collaboration: The ALICE Silicon Drift Detector system. Nucl. Instrum. Methods Phys. Res. A 501, 119–125 (2003)

    Article  ADS  Google Scholar 

  21. Peacock, A., Andresen, R.D., Manzo, G., Taylor, B.G., Villa, G., Re, S., Ives, J.C., Kellock, S.: The gas scintillation proportional counter on EXOSAT. Space Sci. Rev. 30, 525–534 (1981)

    Article  ADS  Google Scholar 

  22. Plaza, M.A., Martinez, L., Cespedosa, F.: The development of the SMOS-MIRAS deployment system. In: Harris, R.A. (ed.) 10th European Space Mechanisms and Tribology Symposium, vol. 524, pp. 231–238. ESA Special Publication (2003)

  23. Rashevsky, A., Bonvicini, V., Burger, P., Piano, S., Piemonte, C., Vacchi, A.: Large area silicon drift detector for the ALICE experiment. Nucl. Instrum. Methods Phys. Res. A 485, 54–60 (2002)

    Article  ADS  Google Scholar 

  24. Shvartsman, V.F.: Neutron stars in binary systems should not be pulsars. Soviet Astron. 15, 342 (1971)

    ADS  Google Scholar 

  25. Stella, L., Vietri, M., Morsink, S.M.: Correlations in the quasi-periodic oscillation frequencies of low-mass x-ray binaries and the relativistic precession model. Astrophys. J. 524, L63–L66 (1999)

    Article  ADS  Google Scholar 

  26. Strohmayer, T.E., Watts, A.L.: Discovery of fast X-ray oscillations during the 1998 giant flare from SGR 1900+14. Astrophys. J. 632, L111–L114 (2005)

    Article  ADS  Google Scholar 

  27. Swank, J.H.: The Rossi X-ray timing explorer: capabilities, achievements and aims. Adv. Space Res. 38(1), 2959–2963 (2006)

    Article  ADS  Google Scholar 

  28. Taylor, B.G., Andresen, R.D., Peacock, A., Zobl, R.: The EXOSAT mission. Space Sci. Rev. 30, 479–494 (1981). doi:10.1007/BF01246069

    Google Scholar 

  29. Turner, M.J.L., Thomas, H.D., Patchett, B.E., Reading, D.H., Makishima, K., Ohashi, T., Dotani, T., Hayashida, K., Inoue, H., Kondo, H., Koyama, K., Mitsusa, K., Ogawara, Y., Takano, S., Awaki, H., Tawara, Y., Nakamura, N.: The large area counter on GINGA. PASJ 41, 345–372 (1989)

    ADS  Google Scholar 

  30. Vacchi, A., Castoldi, A., Chinnici, S., Gatti, E., Longoni, A., Palma, F., Sampietro, M., Rehak, P., Kemmer, J.: Performance of the UA6 large-area silicon drift chamber prototype . Nucl. Instrum. Methods A 306, 187–193 (1991)

    Article  ADS  Google Scholar 

  31. van der Klis, M.: Millisecond oscillations in X-ray binaries. ARA&A 38, 717–760 (2000)

    Article  ADS  Google Scholar 

  32. Zampa, G., Campana, R., Feroci, M., Vacchi, A., Bonvicini, V., Del Monte, E., Evangelista, Y., Fuschino, F., Labanti, C., Marisaldi, M., Muleri, F., Pacciani, L., Rapisarda, M., Rashevsky, A., Rubini, A., Soffitta, P., Zampa, N., Baldazzi, G., Costa, E., Donnarumma, I., Grassi, M., Lazzarotto, F., Malcovati, P., Mastropietro, M., Morelli, E., Picolli, L.: Room-temperature spectroscopic performance of a very-large area silicon drift detector. Nucl. Instrum. Methods A 633, 15–21 (2011)

    Article  ADS  Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Corresponding author

Correspondence to M. Feroci.

Rights and permissions

Reprints and permissions

About this article

Cite this article

Feroci, M., Stella, L., van der Klis, M. et al. The Large Observatory for X-ray Timing (LOFT). Exp Astron 34, 415–444 (2012). https://doi.org/10.1007/s10686-011-9237-2

Download citation

  • Received:

  • Accepted:

  • Published:

  • Issue Date:

  • DOI: https://doi.org/10.1007/s10686-011-9237-2

Keywords

Navigation