34:(ESO) at La Silla Observatory as a Civil Servant ("VSNA: Volontaire du Service National Actif; former name for CoopĂ©rant") and obtained his "Thorough Studies in Astrophysicsâ diploma (DEA) at Paris VI University (Prof. Jean Heyvaerts). After his military service at this observatory he was hired as a âFellowâ. In 1979 he obtained a university degree for âUpper Studies Thesis in Astronomyâ ("ThĂšse de 3eme. Cycle") at Paris VI University under the directorship of Professor Pierre LĂ©na. He was then appointed as a Staff Astronomer at La Silla Observatory, as head of the Night Assistants group and Operations group. In 1986 he led the infra-red section at La Silla Observatory. Doctor in Science in 1990, (Ph.D.) in âAstrophysics and Spatial Techniquesâ with the thesis "Les 1001 nuits de SN 1987A: contribution aux observations dans lâinfrarouge entre 1 et 20 ”m", at Paris VII University (Thesis director: Prof.
125:
Falomo and collaborators); a monitoring in the near-IR range of a sample of Wolf-Rayet stars which shows that condensation of dust in their wind occurs in a short time scale (âŒ1â2 years), and that the newly formed dust shells are dissipated on time scales of about 4 years (with Prof. K.A. van der Hucht and collaborators); observations of the mutual eclipses and occultations between the
Galilean satellites to derive the corrections of the ephemerides during the events and to get the measurements of the position of hotspots on Ioâs visible surface. Together with his observations, a model including the thermal emission of the volcanoes has permitted a close representation of the IR lightcurve and has provided new physical parameters related to the two volcanoes Loki and Pele (with Dr. J.E. Arlot and collaborators).
72:
optimal use of the new international facilities which are and will be partly at their disposal. He was also member of the
National Chilean Telescope Time Allocation Committee which evaluates observing proposals for CTIO and Las Campanas Observatories, and a frequent reviewer of the governmental FONDECYT (âFONdo de DEsarollo en Ciencia Y Tecnologiaâ) and CONECYT (âCONsejo para la Educacion y Tecnologiaâ) proposals for research funding. He collaborated on a regular basis to the REDLASER organization, which gather teachers from the IV region of Chile for divulging astronomy in colleges, as well as with various amateurs associations in France and Europe.
121:(IRAS), of a sample of 81 nearby main-sequence stars of spectral class A, F, G, and K to determine the incidence of dust disks around such main-sequence stars. They concluded that whether all stars arrive on the main sequence surrounded by a disk cannot be established: they showed, in particular that not only some very young stars do not have a disk, but also not all stars destroy their disk in a similar way: some stars as old as the Sun still have significant disks.
103:
characteristic of FU Orionis star and indicative of a hot luminous disk, and they suggested that BBW 76 is virtually identical to the prototype of its class, FU Orionis itself, in all respects except that BBW 76 has not shown the regular fading that FU Orionis has displayed after its eruption in 1936. This may be due to continued replenishment of the circumstellar accretion disk.
247:
interstellar dust. Another
Patrice Bouchetâs scientific interests is related to the ultimate Iron mass in core-collapse supernovae which he investigate measuring the flux in the 10.52 ”m ground state transitions from radioactive 56Co. In December 2015, the NASA/ADS archive found 267 articles authored by Patrice Bouchet in scientific revues, with 3521 citations from his peers.
38:). In 1991 he was promoted Deputy Head of the Astronomy Department at La Silla and became a Senior Faculty Astronomer at ESO. In collaboration with Astronomer Jean Manfroid, he completed the elaboration of a global photometric reduction package, for visible and Infrared data. In 1997 he was hired as a Senior Support Scientist at the
102:
2. In collaboration with Dr. Bo
Reipurth, he has carried out a long-term photometric and spectroscopic monitoring program of the southern FU Orionis-type object BBW76 spanning the period from 1982 to 1997. Both scientists have discovered a change toward later spectral type with increasing wavelength
66:
During his 30 years in Chile, Patrice
Bouchet has been deeply involved in the Public Relations and outreach activities in Chile for ESO first, and then for CTIO: that included exhibits, and numerous conferences and lectures in Chilean Universities, basic schools and colleges, as well as large public
128:
5. Between 1983 and 1990, he realized 9 stellar occultations by
Neptune in the near-IR, which gave 22 temperature profiles of the planet upper stratosphere. These observations confirmed the general increase of temperature from the tropopause to the lower thermosphere of Neptune. During one of these
876:
Roques, F.; Sicardy, B.; French, R.G.; Hubbard, W.B.; Barucci, A.; Bouchet, P.; Brahic, A.; Gehrels, J.-A.; Gehrels, T.; Grenier, I.; Le Bertre, T.; Lecacheux, J.; Maillard, J.P.; McLaren, R.A.; Perrier, C.; Vilas, F.; Waterworth, M.D. (1994). "Neptune's upper stratosphere, 1983-1990: ground-based
71:
working group (in
Spanish, "Grupo de Astrofisica, Cosmologia y Gravitacion"), the goal of which is to gather competences from Chilean scientists all over the country, be they physicists or astronomers, in order to conduct efficient science, and to teach it to next generation, in order to make an
124:
4. In collaboration with various groups, he has been also involved in many other studies including a monitoring of the bright quasar 3C273 with (Prof. Thierry
Courvoisier from Geneva Observatory and his collaborators); an homogeneous J, H, K, L photometry of 42 BL Lac objects (with Prof. Renato
94:
1. Under his leadership, infrared data have been continuously acquired on supernova SN1987A since its outburst. Observations have been carried out from the visible to 10 and 20 ”m at ESO and CTIO, and at 230 GHz (1.3 mm) with the sub-mm SEST telescope . These data have been used to derive the
54:
survey (1997-1999). He was
Project Scientist and Manager for the Tip-Tilt system at the 4-m Blanco Telescope and received a âSpecial AURA Rewardâ for his achievements in that field. In 2000, he was appointed at the NOAO Gemini Science Center for the mid-IR instrument T-ReCS attached at the
246:
Patrice
Bouchetâs present investigations include the study of supernova SN 1987A which exploded in the LMC, the interactions between the ejecta and the circumstellar environment, in particular through a monitoring of the dust, in order to investigate whether supernovae produce much of the
95:
bolometric flux and led to the discovery of dust condensation in the ejecta of the supernova. Images taken in the HeI line (1.083 ”m) with the CTIO Blanco 4-m tel and the Tip-Tilt system yield him to detect the emergence of bright spots in the inner equatorial ring before HST did (
772:
Proceedings of the 143rd Symposium of the International Astronomical Union held in Sanur, Bali, Indonesia, June 18-22, 1990. Edited by Karel A. van der Hucht and Bambang Hidayat. International Astronomical Union. Symposium no. 143, Kluwer Academic Publishers,
198:; elaboration of the more complete and accurate bolometric light curve of the supernova ever published; discovery of hot spots in the inner equatorial ring; first mid-infrared imaging of the inner equatorial ring; recovery of the dusty ejecta after day 6000.
605:
Habing, H.J.; Bouchet, P.; Dominik, C.; Encrenaz, T.; Heske, A.; Jourdain de Muizon, M.; Kessler, M.F.; Laureijs, R.; Leech, K.; Metcalfe, L. (1996). "First results from a photometric infrared survey for Vega-like disks around nearby main-sequence stars".
633:
Habing, H.J.; Dominik, C.; Dominik, C.; Jourdain de Muizon, M.; Laureijs, R.J.; Kessler, M.F.; Leech, K.; Metcalfe, L.; Salama, A.; Siebenmorgen, R.; Trams, N.; Bouchet, P. (2001). "Incidence and survival of remnant disks around main-sequence stars".
67:
conferences all over the country, as well as interfacing with the press media (TV and Newspapers). He wrote a 380 pages book for students ("El Universo y la Vida", in Spanish). He has been an active founding member of the inter-University
549:
van der Bliek, N.S.; Bouchet, P.; Habing, H.J.; Jourdain de Muizon, L.S.; Blackwell, D.E.; Gustafsson, B.; Hammersley, P.L.; Kessler, M.F.; Lim, T.L.; Manfroid, J. (1992). "Standard stars for the Infrared Space Observatory, ISO".
268:
Press Abstracts from the Sixteenth Lunar and Planetary Science Conference, held March 11â15, 1985, in Houston, TX. LPI Contribution 559, published by the Lunar and Planetary Institute, 3303 Nasa Road 1, Houston, TX 77058, 1985,
76:
243:âą RHG Exceptional Achievement "for Engineering Team to ISIM Cryo Vacuum Test Team for the James Webb Space Telescope Integrated ScienceModule", from the Director C.J. Scolese, Goddard Space Flight Center, NASA (May 2015)
413:
Bouchet, P.; Dwek, E.; Danziger, J.; Arendt, R.G.; De Buizer, I.J.; Park, S.; Suntzeff, N.B.; Kirschner, R.B; Challis, P. (2006). "SN 1987A after 18 Years: Mid-Infrared Gemini and Spitzer Observations of the Remnant".
577:
Hammersley, P.L.; Jourdain de Muizon, M.; Kessler, M.F.; Bouchet, P.; Joseph, R.D.; Habing, H.J.; Salama, A.; Metcalfe,L. (1998). "Infrared standards for ISO. I. A new calibration of mid infrared photometry".
848:
Descamps, P.; Arlot, J.-E.; Thuillot, W.; Colas, F.; Vu, D.T.; Bouchet, P.; Hainaut, O. (1989). "Observations of the volcanoes of Io, Loki and Pele, made in 1991 at the ESO during an occultation by Europa".
47:
688:
TĂŒrler, M.; Paltani, S.; Courvoisier, T. J.-L.; Aller, M.F.; Aller, H.D.; Blecha, A.; Bouchet, P.; Lainela, M.; MCHardy, I.M.; Robson, E.I. (1999). "30 years of multi-wavelength observations of 3C 273".
231:âą Special AURA, Inc. Award for achievement of the Tip-Tilt system at the 4-m Blanco Telescope at Cerro Tololo Interamerican Observatory (National Optical Astronomical Observatories). (April 1999)
794:
Williams, P. M.; van der Hucht, K. A.; van Wyk, F.; Marang, F.; Whitelock, P.; Bouchet, P.; Setia Gunawan, D.Y.A. (2012). "Recurrent dust formation by WR 48a on a 30-year time-scale".
904:
Suntzeff, N. B.; Phillips, M.M.; Elias, J.H.; Cowley, A. P.; Hartwick, F. D. A.; Bouchet, P. (1993). "On the origin of a sample of suspected CH stars in the Large Magellanic Cloud".
661:
Courvoisier, T.J.-L.; Robson, E.I.; Hughes, D.H.; Blecha, A.; Bouchet, P.; Krisciunas, K.; Schwarz, H.E. (1988). "Rapid infrared and optical variability in the bright quasar 3C273".
441:
Bouchet, P.; Lequeux, J.; Maurice, E.; Prévot, L.; Prévot-Burnichon, M.L. (1986). "The visible and infrared extinction law and the gas-to-dust ratio in the Small Magellanic Cloud".
821:
Arlot, J.-E.; Thuillot, W.; Bouchet, P.; Gouiffes, Ch.; Schmider, F.-X. (1989). "Mutual events of the Galilean satellites - an analysis of the observations made in 1985 at ESO".
266:
Hubbard, W.B.; Brahic, A.; Bouchet, P.; Elicer, L.-R.; Haefner, R.; Manfroid, J.; Roques, F.; Sicardy, B.; Vilas, F. (1985). "Occultation Detection of a Neptune Ring Segment".
164:
for this sample is Mbol=-5.3 while the brightest members reach Mbol =-6.2. These stars are also significantly bluer and somewhat brighter in the average than the âtypicalâ
237:âą James Webb Space Telescope Significant Award from NASA, âFor significant contribution to the Mid Infra-Red Instrument (MIRI) on the JWST Observatoryâ. (May 2012)
240:âą James Webb Space Telescope Significant Achievement Award by the NASA JWST Project "In recognition of extraordinary dedication and contributionsâ. (March 2014)
468:
Lawrence, S.S.; Sugerman, B.E.; Bouchet,P; Crotts, A.P.S.; Uglesich, R.; Heathcote, S. (2000). "On the Emergence and Discovery of Hot Spots in SNR 1987A".
75:
From 2006 to present he is a Researcher/Engineer at the Astrophysics Division of the Commission for Atomic Energy and Alternatives Energies (in French,
743:
Falomo, R.; Bersanelli, M.; Bouchet, P.; Tanzi, E.G. (1993). "The optical to near-infrared emission of BL Lac objects - Simultaneous observations".
495:
Sugerman, B.E.; Lawrence, S.S.; Crotts,A.P.S.; Bouchet, P.; Heathcote, S. (2002). "Evolution and Geometry of Hot Spots in Supernova Remnant 1987A".
234:âą James Webb Space Telescope Significant Achievement Award from ESA, âIn recognition of extraordinary contribution to the JWST missionâ. (May 2012)
79:, CEA-Saclay) with a Research Directorship. He is the Project Manager for the Centre of Expertise for the mid-infrared MIRI instrument aboard the
383:
Bouchet, P.; Danziger, L. (1993). "Infrared Photometry and Spectrophotometry of Supernova 1987A - Part Two - 1987NOV to 1991MAR Observations".
39:
23:, his infrared observations of supernova SN 1987A in the Large Magellanic Cloud , and the dust extinction in the Small Magellanic Cloud .
770:
Williams, P. M.; van der Hucht, K. A.; Thé, P.S.; Bouchet, P.; Roberts, G. (1991). "Recurrent Dust Formation by Wolf-Rayet Stars".
323:
Suntzeff, N. B.; Bouchet, P. (1990). "The bolometric light curve of SN 1987A. I - Results from ESO and CTIO U to Q0 photometry".
716:
Bersanelli, M.; Bouchet, P.; Falomo, R.; Tanzi, E.G. (1992). "Homogeneous J, H, K, L photometry of a sample of BL Lac objects".
353:
Bouchet, P.; Danziger, L.; Lucy, L (1991). "Bolometric light curve of SN 1987A - Results from day 616 to 1316 after outburst".
118:
31:
522:
Reipurth, B.; Hartmann, L.; Kenyon, S.J.; Smette, A.; Bouchet, P. (2002). "Evolution of the FU Orionis Object BBW 76".
110:
80:
59:
South telescope. In 2005 he left Chile to come back to his country where he was appointed as invited Scientist at
225:
173:
202:
169:
145:
133:(together with Reinhold Haëfner and Jean Manfroid, in collaboration with André Brahic and his group).
913:
886:
858:
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161:
56:
27:
114:
60:
19:
is a French astrophysicist born 03/26/1953 in Brest (France) reknown for his discovery of the
26:
He obtained a "Special Studies in Astrophysics" diploma at Haute-Provence Observatory (prof.
917:
890:
702:
647:
619:
591:
454:
396:
306:
35:
20:
160:, and therefore are not members of the old stellar population in the LMC. Indeed, the mean
293:
Manfroid, J.; Haefner, R.; Bouchet, P. (1986). "New evidence for a ring around Neptune".
862:
834:
807:
780:
756:
729:
674:
563:
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508:
481:
427:
366:
336:
276:
153:
117:, he used photometric measurements made with ISO, complemented by some data from the
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3. Part of his attention has been also focused on the photometric calibration of the
165:
149:
137:
96:
191:âą Discovery by IR spectroscopy of the presence of water ice in comet P/Halley.
226:
http://link.springer.com/referenceworkentry/10.1007%2F978-3-540-29925-7_4269
30:; âDiplome dâEtudes SpĂ©cialesâ, DES) in 1976. In 1977 he was working at the
194:âą Discovery and modeling of the dust condensation in the ejecta of
157:
141:
113:(ISO) satellite. Together with Professor Harm Habing and his group from
195:
130:
172:
which seems to indicate that they belong to a young population of
51:
152:
are more luminous than the red giant branch tip of the Galactic
48:
The Association of Universities for Research in Astronomy (AURA)
43:
221:
107:
77:
Commissariat Ă l'Ă©nergie atomique et aux Ă©nergies alternatives
877:
stellar occultation observations III. Temperature profiles".
42:(CTIO), by the National Optical Astronomical Observatory,
176:
stars (AGB), possibly with ages near 100 millions years.
136:
6. He performed near-Infrared photometry on a sample of
201:âą Elaboration of the dust extinction law in the
148:(LMC), and showed with Prof. Nick Suntzeff that these
129:
observations, he discovered the arc-like ring around
63:
in charge of the European Large Projects for France.
906:Astronomical Society of the Pacific, Publications
796:Monthly Notices of the Royal Astronomical Society
218:The Minor Planet MP4313 has been given his name
318:
316:
288:
286:
97:http://www.noao.edu/outreach/press/pr0002.html
261:
259:
186:Discovery of the arc-like ring around Neptune
8:
580:Astronomy and Astrophysics Supplement Series
408:
406:
378:
376:
348:
346:
222:https://fr.wikipedia.org/%284313%29_Bouchet
17:Patrice Jean Emmanuel Bouchet de Puyraimond
255:
50:for working as Project Manager for the
40:Cerro Tololo Interamerican Observatory
691:Astronomy and Astrophysics Supplement
7:
14:
119:Infrared Astronomical Satellite
1:
32:European Southern Observatory
938:
879:Astronomy and Astrophysics
636:Astronomy and Astrophysics
608:Astronomy and Astrophysics
443:Astronomy and Astrophysics
385:Astronomy and Astrophysics
295:Astronomy and Astrophysics
111:Infrared Space Observatory
81:James Webb Space Telescope
497:The Astrophysical Journal
470:The Astrophysical Journal
416:The Astrophysical Journal
524:The Astronomical Journal
918:1994A&A...288..985R
891:1994A&A...288..985R
703:1999A&AS..134...89T
648:2001A&A...365..545H
620:1996A&A...315L.233H
592:1998A&AS..128..207H
455:1985A&A...149..330B
397:1993A&A...273..451B
307:1986A&A...157L...3M
174:Asymptotic Giant Branch
203:Small Magellanic Cloud
170:Large Magellanic Cloud
146:Large Magellanic Cloud
823:Astronomical Journal
745:Astronomical Journal
718:Astronomical Journal
355:Astronomical Journal
325:Astronomical Journal
162:bolometric magnitude
863:1992Icar..100..235D
835:1989AJ.....98.1890A
808:2012MNRAS.420.2526W
781:1991IAUS..143..417W
757:1993AJ....106...11F
730:1993AJ....106...11F
675:1988Natur.335..330C
564:1992Msngr..70...28V
536:2002AJ....124.2194R
509:2002ApJ...572..209S
482:2000ApJ...537L.123L
428:2006ApJ...650..212B
367:1991AJ....102.1135B
337:1990AJ.....99..650S
277:1985LPICo.559...35H
180:Major Achievements:
140:suspected of being
57:Gemini Observatory
28:Charles Fehrenbach
115:Leiden University
61:Paris Observatory
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36:Lodewijk Woltjer
21:Rings of Neptune
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166:carbon stars
150:carbon stars
138:carbon stars
135:
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123:
105:
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93:
85:
74:
68:
65:
25:
16:
15:
802:(3): 2526.
476:(2): L123.
361:(1): 1135.
156:giants and
885:(1): 985.
857:(1): 235.
530:(4): 219.
503:(2): 209.
449:(2): 330.
422:(1): 212.
391:(2): 451.
331:(1): 650.
251:References
773:Dordrecht
751:(1): 11.
724:(1): 28.
301:(1): L3.
90:Research:
829:: 1890.
216:âą
158:CH stars
142:CH stars
914:Bibcode
887:Bibcode
859:Bibcode
831:Bibcode
804:Bibcode
777:Bibcode
775:: 417.
753:Bibcode
726:Bibcode
699:Bibcode
671:Bibcode
669:: 330.
644:Bibcode
642:: 545.
616:Bibcode
614:: L23.
588:Bibcode
586:: 207.
560:Bibcode
532:Bibcode
505:Bibcode
478:Bibcode
451:Bibcode
424:Bibcode
393:Bibcode
363:Bibcode
333:Bibcode
303:Bibcode
273:Bibcode
212:Awards:
196:SN1987A
168:in the
144:in the
131:Neptune
851:Icarus
697:: 89.
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