Main bibliographic database about transient\ and IR low background photo detectors

Main bibliographic database about transient
and IR low background photo detectors

A. Coulais

Apr 30, 2002

References

[1]
A. Abergel and A. Coulais, New method to correct ISOCAM-LW transient effects : first results, tech. rep., IAS Lab., Septembre 1998.

[2]
A. Abergel, F.-X. Désert, and H. Aussel, IAS model for ISOCAM LW transient correction, technical report, Décembre 1996.

[3]
A. Abergel et al., ISOCAM mapping of the r-Ophiuchi main cloud., Astron. Astrophys., 315:L329-L332, Novembre 1996.

[4]
A. Abergel, M. A. Miville-Deschêne, F.-X. Désert, M. Pérault, H. Aussel, and M. Sauvage, IAS model for ISOCAM LW transient correction, accepted in Experimental Astronomy, Février 1999.

[5]
A. Abergel and M. Pérault, Flight model LW channel : noise due to transients, tech. rep., IAS lab., Juin 1994.

[6]
J. A. Acosta-Pulido, C. Gabriel, and H. O. Castañeda, Transient effects in ISOPHOT data: status of medelling and correction procedures, tech. rep., ESA, 1998.

[7]
P. Agnèse, J. J. Engelmann, and P. Mottier, Results of radiation tests performed on the ISOCAM infrared detector array, IEEE Trans. on Nuclear Science, 38:953-963, Août 1991.

[8]
P. Agnèse, C. Lucas, P. Maillart, P. L. Mottier, Y. Lepennec, and P. Masse, The ISOCAM camera long-wavelength channel detector, Proceedings of SPIE, 1070:124-128, Juillet 1989.

[9]
F. Balleux, Réalisation d'une chaîne de traitement pour les données ISOPHOT C-100, tech. rep., Stage de Magistère, 2000.

[10]
A. Biviano et al., The ISOCAM dark current calibration report, tech. rep., ISOCAM, Novembre 1998.

[11]
A. Biviano et al., The ISOCAM flat field calibration report, tech. rep., ISOCAM, Novembre 1998.

[12]
I. K. Blokhin, T. A. Gorshkova, and V. A. Kholodnov, Nonlinear distortions of the photocurrent of high-resistance impurity photoresistors, Scripta Technica, pp. 106-113, 1989.

[13]
I. K. Blokhin and V. A. Kholodnov, Characteristics of the signal and noise currents in longitudinal extrinsic photoconductors in the background-limited regime, Sov. Phys. Semicond., 20(10):1208-1210, 1986.

[14]
I. K. Blokhin, V. V. Osipov, and I. I. Taubkin, Coordinate dependence of photosensitivity and other pecularities of extrinsic photoconductor detectors at low backgrounds, Infrared Physics, 33(1):9-26, 1992.

[15]
I. K. Blokhin, A. A. Rakhubovskii, and V. A. Kholodnov, Frequency characteristics of an isotypic contact with a high-resistivity semiconductor, Sov. Phys. Semicond., 23(10):1082-1085, 1989.

[16]
J. Blommaert, ISOCAM photometry report, tech. rep., ESA Vilspa, Spain, Mai 1998.

[17]
S. Bouaissi, étude des différents modèles de phénomènes transitoires sur le satellite ISO, tech. rep., Stage de license, 1999.

[18]
N. Bourot, Imagerie en astronomie : correction des transitoires de la caméra ISOCAM, tech. rep., Stage de magistère, 1998.

[19]
E. Caux, Application of Fouks-Schubert transient correction method to LWS data: status and plans, tech. rep., CESR, CNRS, France, 1999.

[20]
C. J. Cesarsky, ISOCAM, in Infrared Astronomy with ISO. L'astronomie infrarouge et la mission ISO., T. Encrenaz and M. Kessler, eds., Les Houches, France, June 13-27, 1991, Nova Science, Commack, N.Y., 1992, pp. 31-50.

[21]
C. J. Cesarsky et al., Camera of the Infrared Space Observatory, Optical Engineering, 33:751-761, Mars 1994.

[22]
C. J. Cesarsky et al., ISOCAM in flight., Astron. Astrophys., 315:L32-L37, Novembre 1996.

[23]
S. E. Church, M. J. Griffin, P. A. R. Ade, M. C. Price, R. J. Emery, and B. M. Swinyard, Performance testing of doped-germanium photoconductors for the ISO Long-Wavelength Spectrometer, in ESA SP-356 Photon Detectors for Space Instrumentation, Décembre 1992, pp. 255-260.

[24]
S. E. Church, M. J. Griffin, M. C. Price, P. A. Ade, R. J. Emery, and B. M. Swinyard, Performance characteristics of doped-Ge photoconductors for the Infrared Space Observatory Long Wavelength Spectrometer, Proceedings of SPIE, 1946:116-125, Octobre 1993.

[25]
S. E. Church, M. C. Price, M. J. Griffin, P. A. R. Ade, R. J. Emery, and B. M. Swinyard, Non-linear effects in doped-germanium photoconductors for the ISO Long Wavelength Spectrometer, in ESA SP-356 Photon Detectors for Space Instrumentation, Décembre 1992, pp. 261-264.

[26]
S. E. Church, M. C. Price, N. M. Haegel, M. J. Griffin, and P. A. R. Ade, Transient response in doped germanium photoconductors under very low background operation, Applied Optics, 35:1597-1604, 1996.

[27]
P. E. Clegg et al., The ISO Long-Wavelength Spectrometer., Astron. Astrophys. Suppl. Ser., 315:L38-L42, Novembre 1996.

[28]
A. Coulais, Étude des équations de Fouks, tech. rep., IAS lab., Octobre 1998.

[29]
A. Coulais, État de l'étude des transitoires LW-ISOCAM sous fort gradient d'illumination, tech. rep., IAS lab., Mai 1999.

[30]
A. Coulais and A. Abergel, Transient correction of the ISOCAM data with the Fouks-Schubert model: first results, tech. rep., IAS Lab., Septembre 1998.

[31]
A. Coulais and A. Abergel, Transient correction of the LW-ISOCAM data with the Fouks-Schubert model : first results, in ISO Conference, Paris, ESA, ESA, Octobre 1998.

[32]
A. Coulais and A. Abergel, Correction des transitoires de la caméra infrarouge du satellite ISO, vol. T-1, GRETSI'99, Septembre 1999, pp. 147-150.

[33]
A. Coulais and A. Abergel, Transient correction of the LW-ISOCAM data for low contrasted illumination, Astron. Astrophys. Suppl. Ser., 141:533-544, Février 2000.

[34]
A. Coulais, B. I. Fouks, J.-F. Giovannelli, A. Abergel, and J. Sée, Transient response of IR detectors used in space astronomy : what we have learned from ISO satellite, in Infrared Spaceborne Remote Sensing VIII, M. Strojnik and B. Andresen, eds., vol. 4131, San Diego, USA, Août 2000, SPIE, pp. 205-217.

[35]
T. de Graauw, Space Infrared/Submm Telescopes: Past and Future, Advances in Space Research, 25:2145-2157, 2000.

[36]
T. de Graauw et al., Observing with the ISO Short-Wavelength Spectrometer., Astron. Astrophys. Suppl. Ser., 315:L49-L54, Novembre 1996.

[37]
C. J. Delattre, About transients, the fitting method, technical report, Juillet 1996.

[38]
C. Delettrez, M. J. Griffin, C. Le Naour, S. Church, and J. Chabaud, The detector signal processing chain of the ISO Long-Wavelength Spectrometer, Experimental Astronomy, 4:213-235, 1994.

[39]
F.-X. Désert, A modified IAS model for ISOCAM LW transient correction, tech. rep., LAOG, Mars 1999. Version 2.0.

[40]
F.-X. Désert et al., A classical approach to faint extragalactic source extraction from ISOCAM deep surveys. Application to the Hubble Deep Field, Astron. Astrophys. Suppl. Ser., 342:363-377, Février 1999.

[41]
ESA, ISO Handbook Volume III (CAM), Version 1.0, Juillet 1999.

[42]
G. G. Fazio, J. L. Hora, S. P. Willner, J. R. Stauffer, M. L. Ashby, Z. Wang, E. V. Tollestrup, J. L. Pipher, W. J. Forrest, C. R. McCreight, S. H. Moseley, W. F. Hoffmann, P. Eisenhardt, and E. L. Wright, Infrared array camera (IRAC) for the Space Infrared Telescope Facility (SIRTF), Proceedings of SPIE, 3354:1024-1031, Août 1998.

[43]
A. M. Filachev, B. I. Fouks, and D. Greenfeld, Nature of distortions of the surface pattern produced by precise electron-beam processing of insulators, Proceedings of SPIE, 3155:78-88, Septembre 1997.

[44]
B. I. Fouks, Injection properties of contacts to high-resistivity semiconductors. I, Sov. Phys. Semicond., 15(9):974-980, Septembre 1981.

[45]
B. I. Fouks, Injection properties of contacts to high-resistivity semiconductors. I-II, Sov. Phys. Semicond., 15(9):974-980, 980-986, Septembre 1981.

[46]
B. I. Fouks, Injection properties of contacts to high-resistivity semiconductors. II, Sov. Phys. Semicond., 15(9):980-986, Septembre 1981.

[47]
B. I. Fouks, Nonstationary behaviour of low background photon detectors, in ESA SP-356 Photon Detectors for Space Instrumentation, Décembre 1992, pp. 167-174.

[48]
B. I. Fouks, Nonstationary processes in extrinsic photoconductors, Proceedings of SPIE, 1762:519-530, Janvier 1993.

[49]
B. I. Fouks, On improvement of ISOPHOT detector operation, results of the visit at MPIA in 1994, tech. rep., MPIA, Mars 1994.

[50]
B. I. Fouks, On problems of operation of low-background IR detectors, Proceedings of SPIE, 2553:489-500, Septembre 1995.

[51]
B. I. Fouks, Active modes of operation of low-background extrinsic IR detectors, Proceedings of SPIE, 2790:38-46, Avril 1996.

[52]
B. I. Fouks, Phenomena in low-background IR detectors under high-energy particles, Proceedings of SPIE, 2817:160-171, Octobre 1996.

[53]
B. I. Fouks, Theory of photoresponse of low-background IR detectors, Proceedings of SPIE, 3122:441-452, Octobre 1997.

[54]
B. I. Fouks, Transient processes in high-field low-background IR detectors under inhomogeneous irradiation. I General statement of the problem, II Application to the ISOCAM detector array, tech. rep., IAS, Décembre 2001.

[55]
B. I. Fouks, V. F. Kocherov, I. I. Taubkin, L. A. Vinokurov, and N. B. Zaletaev, Photoelectric cross talk between the elements of an extrinsic photoconductor detector array at low backgrounds, Proceedings of SPIE, 2269:727-735, Octobre 1994.

[56]
B. I. Fouks, V. F. Kocherov, I. I. Taubkin, L. A. Vinokurov, and N. B. Zaletaev, Photoresponse of low-background extrinsic infrared detector arrays, Optical Engineering, 33:1485-1491, Mai 1994.

[57]
B. I. Fouks and J. Schubert, Precise theoretical description of photoresponse for detectors of ISOPHOT's Si:Ga array, Proceedings of SPIE, 2475:487-498, Juin 1995.

[58]
M. Fujiwara, N. Hiromoto, and K. Araki, Moderate-fast transient response of the Ge:Ga photoconductors, Proceedings of SPIE, 2552:421-429, Septembre 1995.

[59]
C. Gabriel and J. A. Acosta-Pulido, The ISOPHOT interactive analysis (pia), The Universe as Seen by ISO. Eds. P. Cox & M. F.  Kessler. ESA-SP 427., 427:73-76, Mars 1999.

[60]
K. Ganga, G. Helou, R. Hurt, M.-S. Kong, J. Li, E. Valjavec, and D. Van Buren, ISO/CAM transient removal at IPAC, tech. rep., IPAC Lab., Août 1998.

[61]
K. Ganga, M. Kong, L. Jing, and D. Van Buren, Transient removal with the IPAC method, tech. rep., IPAC Lab., Juillet 1998.

[62]
P. García-Lario, A. Coulais, D. Kester, and E. Caux, Transients Working Group Final Report, ESA, Avril 2001.

[63]
U. Groezinger, S. Kirches, D. Lemke, J. Schubert, B. Schulz, and J. Wolf, Characterization of detectors and calibration of the ISOPHOT experiment, in ESA SP-356 Photon Detectors for Space Instrumentation, Décembre 1992, pp. 329-333.

[64]
N. M. Haegel, J. W. Beeman, P. N. Luke, and N. N. Haller, Transient photoconductivity in Ge:Be due to Be+ formation, Physical Review B, 39(6):3677-3682, Février 1989.

[65]
N. M. Haegel, C. R. Brennan, and A. M. White, Transport in extrinsic photoconductors: a comprehensive model for transient response, Journal of Applied Physics, 80(3):1510-1514, Août 1996.

[66]
N. M. Haegel, C. A. Latasa, and A. M. White, Transient response of infrared photoconductors : the roles of contacts and space charge, Applied Physics, A 56:15-21, 1993.

[67]
N. M. Haegel, C. Newton, J. C. Simoes, and A. M. White, Modeling of transient response in far infrared photoconductors, in Submillimeter and far infrared space instrumentation, 30th ESLAB Symp, ed., no. SP-388, ESTEC, Décembre 1996, ESA, ESA, pp. 15-20.

[68]
N. M. Haegel, J. C. Simoes, A. M. White, and J. W. Beeman, Transient behavior of infrared photoconductors: application of a numerical model, Applied Optics, 38(10):1910-1919, Avril 1999.

[69]
N. M. Haegel and A. M. White, Modeling of near-contact field and carrier distributions in extrinsic germanium photoconductors, Infrared Physics, 29(5):915-923, 1989.

[70]
N. Hiromoto, T. Itabe, H. Shibai, H. Matsuhara, T. Nakagawa, and H. Okuda, Three-element stressed Ge:Ga photoconductor array for the infrared telescope in space, Applied Optics, 31:460-465, Février 1992.

[71]
IPAC group, ISOCAM transient treatment at IPAC, tech. rep., IPAC Lab., 1997.

[72]
M. F. Kessler et al., The Infrared Space Observatory (ISO) mission., Astron. Astrophys., 315:L27-L31, Novembre 1996.

[73]
D. Kester, The impact of memory effects correction on SWS data, tech. rep., SRON, Netherlands, 1999.

[74]
C. Lari, IRA model for ISOCAM LW transient correction, tech. rep., IRA, Juin 1997.

[75]
C. Lari et al., A new method for ISOCAM data reduction - I. Application to the European Large Area ISO Survey Southern Field: method and results, MNRAS, 325:1173-1189, Août 2001.

[76]
R. Laureijs, U. Klass, P. Richards, and B. Schulz, ISOPHOT Data Users Manual, V 4.1, ESA, Octobre 1999.

[77]
S. J. Leeks, B. M. Swinyard, T. Lim, and P. E. Clegg, Aspects of LWS processing, The Universe as Seen by ISO. Eds. P. Cox & M. F. Kessler. ESA-SP 427., 427:81-84, Mars 1999.

[78]
D. Lemke et al., ISOPHOT - capabilities and performance., Astron. Astrophys. Suppl. Ser., 315:L64-L70, Novembre 1996.

[79]
M.-A. Miville-Desch^ enes, F. Boulanger, A. Abergel, and J.-P. Bernard, Optimizing ISOCAM data processing using spatial redundancy, Astron. Astrophys. Suppl. Ser., 146:519-530, Novembre 2000.

[80]
A. Moneti, ed., ISO detector workshop, viewgraphs of the presentations, 14-16 Jan., vol. I-II, Villafranca del Castillo, 1998, ESA.

[81]
P. Mottier, P. Agnese, and P. O. Lagage, Si:Ga focal plane arrays for satellite and ground-based telescopes, Proceedings of SPIE, 1494:419-426, Septembre 1991.

[82]
P. Mottier, C. Lucas, M. Ravetto, and P. Agnese, Recent developments on ISOCAM long wavelength channel detector, Proceedings of SPIE, 1341:368-374, Novembre 1990.

[83]
K. Okumura, ISOCAM PSF report, tech. rep., ESA, Vilspa, Juin 1998.

[84]
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[85]
A. I. Patrashin and G. A. Ivanov, Testing unit for measuring photoelectric characteristics of IR arrays, Proceedings of SPIE, 3379:555-560, Juillet 1998.

[86]
M. A. Patrashin, B. I. Fouks, U. Grozinger, D. Lemke, and J. Wolf, Residual conductivity of stressed Ge:Ga photoconductors after low-dose gamma irradiation, Journal of Applied Physics, 82(3):1450-1453, Août 1997.

[87]
M. A. Patrashin, B. I. Fouks, D. Lemke, and J. Wolf, Radiation-induced effects in extrinsic far-infrared detectors, Proceedings of SPIE, 2475:476-486, Juin 1995.

[88]
M. A. Patrashin, M. Fujiwara, N. Hiromoto, and B. I. Fouks, Far-infrared Ge:Ga detector for low-background space-based astronomical observations, Proceedings of SPIE, 3354:232-239, Août 1998.

[89]
M. Pérault, F.-X. Désert, A. Abergel, F. Boulanger, C. Dupraz, A. Soufflot, C. Cesarsky, and L. Vigroux, Infrared Space Observatory camera calibration facility and preflight characterization, Optical Engineering, 33:762-770, Mars 1994.

[90]
W. Press, S. Teukolsky, W. Vetterling, and B. Flannery, Numerical Recipes in FORTRAN, second edition, Cambridge University Press, 1992.

[91]
J. Schubert, Die Eichung des Infrarot-Gitterspektrometers im Satelliten-Experiment ISOPHOT und die Korrektur der Transienten seiner Detektoren, PhD thesis, Max Planck-Institut für Astronomie, Heidelberg, 1995.

[92]
J. Schubert, B. I. Fouks, D. Lemke, and J. Wolf, Transient response of ISOPHOT Si:Ga infrared photodetectors: experimental results and application of the theory of nonstationary processes, Proceedings of SPIE, 2553:461-469, Septembre 1995.

[93]
J. Schubert, G. Roth, J. Wolf, D. Lemke, and B. I. Fouks, Correction and curing of in-orbit-induced nonideal behavior of ISOPHOTS's photodetectors, Proceedings of SPIE, 2268:283-294, Septembre 1994.

[94]
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[95]
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[97]
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[98]
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[99]
J.-L. Starck et al., Faint source detection in ISOCAM images, Astron. Astrophys. Suppl. Ser., 138:365-379, Août 1999.

[100]
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[105]
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[106]
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