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Journal articles on the topic 'Observatoire astronomique'

Author: Grafiati

Published: 27 July 2024

Last updated: 31 July 2025

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1

Pellegrini, Enola. "Maria Clara Eimmart (1676-1707), a woman astronomer in Nuremberg." Source(s) – Arts, Civilisation et Histoire de l’Europe, no. 20 (June 26, 2023): 11–28. http://dx.doi.org/10.57086/sources.780.

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La mise au point de la lunette astronomique, puis la diffusion du télescope en Europe permettent la naissance de l’astronomie moderne au cours du XVIIe siècle. De nombreuses villes européennes se dotent alors de leur propre observatoire astronomique, comme Paris en 1667, Londres en 1675, et Nuremberg en 1678. Au XVIIe siècle, les femmes sont quasiment absentes de la communauté scientifique européenne, qui ne leur reconnaît alors pas les mérites de leurs travaux, souvent effectués dans l’ombre de leur père ou de leur époux. Le cas de la ville de Nuremberg et des observations astronomiques de Ma

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2

Joannes, Nicolas. "Pratiques photographiques amateures à la Société astronomique de France (1882-1915) : diffusion, apprentissage et professionnalisation." Cahiers François Viète III-18 (2025): 191–231. https://doi.org/10.4000/13dhx.

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L’apparition de la revue L’Astronomie en 1882 et de la Société astronomique de France cinq ans plus tard, offre des espaces de diffusion et de pratique privilégiés pour les astronomes. Cet article propose d’examiner la frontière fluctuante entre différentes catégories d’astronomes à la fin du xixe siècle, des professionnels des observatoires d’État jusqu’aux « purs » amateurs, en passant par des astronomes « privés », en s’appuyant sur la production astrophotographique et le parcours de plusieurs membres de la Société considérés comme amateurs. Nous montrerons que leurs contributions, clichés

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3

Ferrari, Chiara. "Le Square Kilometre Array (SKA) : un radiotélescope géant pour étudier l’aube et l’évolution du cosmos." Reflets de la physique, no. 67 (November 2020): 10–14. http://dx.doi.org/10.1051/refdp/202067010.

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La radioastronomie à basse fréquence vit aujourd’hui sa renaissance à travers la construction du Square Kilometre Array (SKA). Deux réseaux de milliers d’antennes, opérant dans les domaines de longueur d’onde métriques et centimétriques, permettront de cartographier les différentes phases de l’histoire de l’Univers, de l’apparition des premières sources lumineuses jusqu’aux systèmes d’astres évolués que nous observons aujourd’hui. Mais SKA n’est pas seulement un grand observatoire astronomique : il s’agit d’un projet international qui fait face à des défis considérables, en bénéficiant de la p

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Benkaldoun, Zouhair, Jonathan J. Makela, and John W. Meriwether. "Solar initiative at Oukaimeden Observatory." Proceedings of the International Astronomical Union 8, S294 (2012): 479–80. http://dx.doi.org/10.1017/s1743921313002950.

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AbstractThe solar research program at Oukaimeden Observatory started in 1988 with the helioseimological IRIS network. The Moroccan researchers involved in this research have analyzed solar observations in order to detect and characterize the solar sphere modes of oscillations. In the coming year, the researchers at the Oukaimeden Observatory will add new research capabilities by joining the International Space Weather Initiative (ISWI), installing a suite of optical instruments, comprising a Remote Equatorial Nighttime Observatory of Ionospheric Regions (RENOIR). The scope and objectives to be

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5

Rey-Watson, Joyce. "Online Bibliographic Resources in Astronomy and Astrophysics." International Astronomical Union Colloquium 110 (1989): 84–86. http://dx.doi.org/10.1017/s0252921100003006.

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Online searches may be performed in astronomy and astrophysics either by OBJECT or by SUBJECT. Until recently, although object searches could be performed on a variety of databases in the physical sciences, results were poor and incomplete. Only if an object were mentioned by name in the title or abstract could one hope for any hits at all. The greatest blessing to befall the astronomical community was the advent of SIMBAD (Sets of Identifications, Measurements and Bibliography for Astronomical Data), a database in which searches are conducted by OBJECT only. It is produced and accessible from

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Bianchi, Simone, and Daniele Galli. "Les Observatoires astronomiques en Italie." Nuncius 30, no. 1 (2015): 195–227. http://dx.doi.org/10.1163/18253911-03001008.

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In the autumn of 1863 Otto Wilhelm Struve, director of the Pulkovo Astronomical Observatory in Russia, visited most of the observatories in Italy. The report that he wrote on this occasion provides an overview on the conditions of astronomical research in Italy just after the unification of the country. Later Struve sent a French translation of his report to the Italian astronomer Giovan Battista Donati, who used it to promote the construction of the Arcetri Observatory in Florence, which was inaugurated in 1872. We present here a transcription of the French translation of Struve’s report and

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Genova, Françoise, Raymond P. Norris, M. S. Bessel, et al. "COMMISSION 5: Documentation and Astronomical Data." Proceedings of the International Astronomical Union 1, T26A (2005): 327–33. http://dx.doi.org/10.1017/s1743921306004789.

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AbstractThe triennial report of Commission V Documentation and Astronomical Data/Documentation et Données Astronomiques covers 2002–2005 activities, and in particular the activities of the five Working Groups: Working Group Astronomical Data; Working Group Designations; Working Group Libraries; Working Group FITS; Working Group Virtual Observatories; and of Task Force for the Preservation and Digitization of Photographic Plates.

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8

Seidelmann, P. Kenneth, E. Myles Standish, Claude Froeschle, et al. "Division I: Fundamental Astronomy: (Astronomie Fondamentale)." Transactions of the International Astronomical Union 24, no. 1 (2000): 3–6. http://dx.doi.org/10.1017/s0251107x00002522.

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The last three years have been marked by changes, highlights and progress. Organizationally, commission 7 has joined Division I and plans proceed for commissions 8 and 24 to merge in 2000. They have had a common vice president during this triennium. Sadly, the Royal Greenwich Observatory was closed after over 200 years, but Her Majesty’s Nautical Almanac Office has continued at Rutherford Appleton Laboratory. In St Petersburg, Russia, the Institute of Theoretical Astronomy was abolished, with some of the personnel relocated to the Institute of Applied Astronomy and Pulkova Observatory. In Pari

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9

Marsden, B. G. "6. Astronomical Telegrams (Telegrammes Astronomiques) (Committee of the Executive Committee)." Transactions of the International Astronomical Union 21, no. 1 (1991): 13–14. http://dx.doi.org/10.1017/s0251107x00009755.

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The year 1990, within the triennium covered by the present report, marked a number of significant anniversaries for the Central Bureau, including 70 years since its foundation at the Brussels Observatory, 25 years since the transfer of the Bureau’s operations to the Smithsonian Astrophysical Observatory (and 22 years of Dr. Marsden’s service as Director), and the issuance of the 5000th Circular. The amount of work done at the Bureau has increased enormously in this time, but especially within the past decade, as a result of the demands of modern astronomers and astrophysicists who are respondi

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10

Neichel, Benoit, and Gérard Rousset. "La tomographie de l’atmosphère au service de l’astrophysique." Photoniques, no. 95 (January 2019): 29–33. http://dx.doi.org/10.1051/photon/20199529.

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Depuis près de 30 ans, l’optique adaptative (OA) se développe en astronomie pour corriger les effets de la turbulence atmosphérique et recouvrer la limite de diffraction des grands télescopes au sol. Récemment, les OAs grand champ avec étoiles laser s’appuyant sur la tomographie de l’atmosphère ont été démontrées dans plusieurs observatoires pour offrir une correction dans un champ de vue accru et une bonne couverture du ciel. Ces techniques sont aujourd’hui étendues pour satisfaire les besoins des extrêmement grands télescopes qui verront le jour au milieu des années 2020.

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11

Glaus, Beat. "Rudolf Wolf: Lehrer, Forschungsorganisator und Wissenschaftshistoriker. Zu seinem 100.Todesjahr." Gesnerus 50, no. 3-4 (1993): 223–41. http://dx.doi.org/10.1163/22977953-0500304005.

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Rudolf Wolf (1816-1893): Astronomer;, Research Organizer, Historian of Sciences Rudolf Wolf is remembered by the scientific comm unity above all as a pion eer of sun spots research. On the centennial anniversary of his death it is appropriate to review his other achievements, which have been wrongly neglected. Wolf organized various astronomical, geodetic and meteorological projects. For example, it ivas on his initiative that the Federal Observatory in Zurich, designed by the famous architect Gottfried Semper, was built. He taught at academic institutions m Berne and Zurich and developed the

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12

Sadat, R. "Astronomy in Algeria." Highlights of Astronomy 10 (1995): 668–69. http://dx.doi.org/10.1017/s1539299600012508.

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Astronomy in Algeria is linked to the Algiers Observatory which is the only place where there is any astronomical activity. The Observatory was built in 1889 and was an important contributor to the famous Carte du del project. After independence, because there were so few Algerian astronomers and the site had deteriorated, the activity of the Observatory slowed down significantly.In 1980, the year of the violent El-Ansam earthquake, a decision was taken, on the initiative of the present director (M. Benhallou, Professor of Seismology) to create an Algerian earthquake-surveillance network. This

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13

Mrkos, A., E. Roemer, B. G. Marsden, et al. "6. Astronomical Telegrams (Télégrammes Astronomiques) (Committee of the Executive Committee)." Transactions of the International Astronomical Union 20, no. 1 (1988): 13–14. http://dx.doi.org/10.1017/s0251107x00006878.

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The commission has been able to continue its work during the last triennium with a minimum of effort. Thanks for this and for the untiring dedication are due to the Director of the Bureau, B. G. Marsden. We are also grateful to the Smithsonian Astrophysical Observatory for its general support.According to the annoucement published in the IAU Information Bulletin no 58, K. A. Thernöe died on 1987 March 7. He was the director of the Central Telegram Bureau during the years 1960 - 1964 in Copenhagen and for many years he served as principal substitute for Julie Vinter Hansen when she ran the Bure

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14

Birkle, K., H. Belleman, and H. Elsässer. "The Schmidt Telescope at Calar Alto Observatory." Symposium - International Astronomical Union 161 (1994): 46–48. http://dx.doi.org/10.1017/s007418090004701x.

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The Schmidt telescope at Calar Alto Observatory, Spain, was installed there in 1980 by the Max-Planck-Institut für Astronomie, Heidelberg, and has been operated since then by this institute; originally it had been operational at the Hamburg Observatory since 1955. The corrector plate and mirror have 80 cm and 120 cm diameter respectively; focal length is 240 cm. A field 5.5 deg by 5.5 deg is photographed on 24 cm by 24 cm curved plates. Two objective prisms of 1.7 deg and 4.0 deg refractive angle are available (Heckmann 1955; Birkle 1984). Thousands of direct and spectral plates have been take

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15

Agati, Jean-Louis, Sébastien Caille, André Debackère, et al. "Activities and Achievements of the Double Star Committee of the Société Astronomique de France." Proceedings of the International Astronomical Union 2, S240 (2006): 509–26. http://dx.doi.org/10.1017/s174392130700645x.

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In a synthesis article (see ref. below), the double star expert Paul COUTEAU put the work of French pioneers of double stars observation in the perspective of the double star work carried in the world. After Antoine Yvon VILLARCEAU and Camille FLAMMARION, one prominent pioneer of double stars was Robert JONCKHEERE (1888–1974), an amateur before circumstances prompted him to become a professional astronomer, who devoted his life to double stars. Kenneth Glyn Jones wrote a biography and Charles Fehrenbach his obituary. Jean-Claude Thorel studied his life and career in double star observations (s

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16

Chassefière, Eric. "Friedrich Christoph Mayer and his theory of the aurora borealis." Aurorae Borealis Studia Classica 11 (April 8, 2021): 1–5. http://dx.doi.org/10.7557/16.5786.

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The eleventh volume in the series presents two articles on the aurora borealis by Friedrich Christoph Mayer (1697–1729), a mathematician at the Imperial Academy of Sciences in Saint Petersburg. The first paper, titled “De Luce Boreali” (On the Northern Light), was presented during a session at the newly founded Academy in October 1726. It was printed two years later (1728) in the very first volume of its official periodical, the Commentarii Academiae Scientiarum Imperialis Petropolitanae. The second paper, also bearing the title “De Luce Boreali”, constitutes the author’s ‘second thoughts’ on

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17

Larivière, Vincent. "L’astrophysique au Québec depuis 1945 : émergence et consolidation d’une communauté scientifique périphérique." Scientia Canadensis 32, no. 2 (2009): 21–46. http://dx.doi.org/10.7202/038159ar.

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Résumé Cet article étudie l’émergence et la consolidation des activités de recherche en astrophysique dans les universités québécoises. Deux étapes marquent son développement. Premièrement, on constate l’émergence de certaines activités de recherche. À l’Université Laval, ces travaux émanent d’un groupe de physiciens non spécialistes en astronomie qui réussit, grâce à des fonds internes à l’institution, à se faire construire un modeste télescope. À l’Université de Montréal, la situation est autre : les astrophysiciens n’ont pas de télescope avec lequel observer, mais contribuent à l’avancement

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18

Debaz, Josquin. "Stations de biologie marine et observatoires astronomiques à la fin du xixe siècle : deux reflets d’une même politique scientifique ?" Cahiers François Viète, no. II-8/9 (September 1, 2016): 137–58. http://dx.doi.org/10.4000/cahierscfv.2560.

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19

Gros, Monique. "<italic>Observatoires et Patrimoine Astronomique Français</italic>, edited by Guy Boistel, 2005." Journal of Astronomical History and Heritage 10, no. 2 (2007): 159–60. http://dx.doi.org/10.3724/sp.j.1440-2807.2007.02.15.

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20

Marx, S., H. Lehmann, M. Pluto, and R. Ziener. "T A U M O K—Multi-Object Spectroscopy with the Tautenburg Schmidt Telescope." International Astronomical Union Colloquium 148 (1995): 52. http://dx.doi.org/10.1017/s0252921100021680.

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A multi-object camera for the Tautenburg Schmidt Telescope (134/200/400) was developed and constructed in cooperation with the Max-Planck-Institut für Astronomie in Heidelberg and the Thüringer Landesstemwarte Tautenburg. The experience with the “Spaltspinne” for the 3.5 m Telescope of the Calar Alto Observatory (Pitz 1993) was the foundation of TAUMOK. The technical concept was given by Pitz et al. (1993).Thirty six rods controlled by a processor can be moved in an area with a diameter of 16 cm. This area covers a field of 2.3° in the focal plane which is flattened by a plano-convex lens. Eac

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Lehmann, H., R. Ziener, M. Ball, and E. Pitz. "TAUMOK - a Multi-Object Spectrograph for the Tautenburg Schmidt Telescope." International Astronomical Union Colloquium 149 (1995): 219–20. http://dx.doi.org/10.1017/s0252921100022995.

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TAUMOK is a joint project of the Max Planck Institut für Astronomie Heidelberg and the Thüringer Landessternwarte Tautenburg. It is based on the concept of the “Spaltspinne” (Pitz 1993) now in operation at the Calar Alto Observatory. A first describtion of the technical concept was given by Pitz et al. (1993). TAUMOK was built at the MPIA Heidelberg in collaboration with astronomers and technicians from Tautenburg. It is now in the test phase and will have its first operation at the Tautenburg telescope in the middle of this year.The use of a Schmidt telescope gives a very wide field for multi

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22

Buga, M., P. Fernique, C. Bot, M. G. Allen, F. Bonnarel, and M. Brouty. "Bibliography, catalogs, pixel data: Management of heterogeneous Big Data at CDS by the documentalists." EPJ Web of Conferences 186 (2018): 02001. http://dx.doi.org/10.1051/epjconf/201818602001.

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High speed Internet and the evolution of data storage space in terms of cost-effectiveness has changed the way data are managed today. Large amounts of heterogeneous data can now be visualized easily and rapidly using interactive applications such as “Google Maps”. In this respect, the Hierarchical Progressive Survey (HiPS) method has been developed by the Centre de Données astronomiques de Strasbourg (CDS) since 2009. HiPS uses the hierarchical sky tessellation called HEALPix to describe and organize images, data cubes or source catalogs. These HiPS can be accessed and visualized using applic

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23

Jeong, Il-Gyo, and Bon-Chul Koo. "SRAO CO Observation of Supernova Remnants in l = 70° to 190°." Proceedings of the International Astronomical Union 9, S296 (2013): 183–87. http://dx.doi.org/10.1017/s1743921313009447.

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AbstractWe present the results 12CO J = 1–0 line observations of eleven Galactic supernova remnants (SNRs) between l = 70° and 190° obtained using the Seoul Radio Astronomy Observatory (SRAO) 6-m radio telescope. We detected CO emission towards most of the remnants. In seven SNRs, molecular clouds show a good spatial relation with their radio morphology: G73.9+0.9, G84.2−0.8, G85.4+0.7, G85.9−0.6, G93.3+6.9 (DA530), 94.0+1.0 (3C 434.1), and G182.4+4.3. Two SNRs are particularly interesting. In G85.4+0.7, there is a filamentary molecular cloud aligned along the south-east boundary of the remnan

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24

Keller-Schnider, Hans Urs. "Acta Historica Astronomiae. Im Auftrag des Arbeitskreises Astronomiegeschichte in der Astronomischen Gesellschaft hrsg. von Wolfgang R. Dick und Jürgen Hamel. Frankfurt am Main, Verl. Harri Deutsch. ISSN 1422-8521. Vol. 5: Beiträge zur Astronomiegeschichte. Band 2, hrsg. von W. R.Dick und J. Hamel. 1999.225 S.III. DM 32.-. ISBN 3-8171-1590-3. - Vol. 6: Treasure-hunting in astronomical plate archives. Proceedings of the International Workshop held at Sonneberg Observatory, March 4 to 6,1999. Ed. by P. Kroll, C. la Dous,H.-J. Bräuer. 1999.266 S. 111. DM 38.-. ISBN 3-8171 - 1599-7. - Vol. 7: Erhard Weigel - 1625 bis 1699, barocker Erzvater der deutschen Frühaufklärung. Beiträge des Kolloquiums anlässlich seines 300. Todestages am 20. März 1999 in Jena, hrsg. von R. E. Schielicke, K.-D. Herbst und St. Kratochwil. 1999.172 S. III. DM 28.-. ISBN 3-8171-1600-4." Gesnerus 58, no. 1-2 (2001): 148–49. http://dx.doi.org/10.1163/22977953-0580102011.

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25

Morel, P., J. C. Pecker, A. Flammarion, et al. "Camille Flammarion's observatory: towards a revival." Proceedings of the International Astronomical Union 5, S260 (2009). http://dx.doi.org/10.1017/s1743921311003553.

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AbstractCamille Flammarion's observatory, located in Juvisy-sur-Orge in the suburbs of Paris, has been idle since 1962. Property of the Société Astronomique de France (SAF), it was made available to the city of Juvisy-sur-Orge since 1971, and contains a unique collection of objects and books currently being sorted out. The observatory is being restored by the SAF, thanks to the support of the city of Juvisy-sur-Orge, the French Académie des Sciences and the “Amis de Camille Flammarion” association. In 2006, the Maxime Goury Laffont foundation funded the refurbishment of the 240 mm refractor an

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26

"Commission 5: Documentation and Astronomical Data Documentation et Donnees Astronomiques." Transactions of the International Astronomical Union 21, no. 1 (1991): 7–12. http://dx.doi.org/10.1017/s0251107x00009743.

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The aims of this report are, firstly, to review the activities of Commission 5 since the previous report and, secondly, to draw attention to other relevant activities. It is based mainly on contributions (shortened in some cases) from the chairmen of Working Groups and Task Groups, but other items of general interest have been included.The report on the meetings of the Commission at the IAU General Assembly in Baltimore in August 1988 was published in Trans. IAU 20B, 109–118, while the membership is listed on page K10 and the IAU Style Manual is printed as Chapter 8 on pages Siii-Sxii and S1-S

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27

Szücs-Csillik, Iharka, and Zoia Maxim. "Școala clujeană de astronomie culturală / The School of Cultural Astronomy from Cluj-Napoca." Analele Banatului XIX 2021, January 1, 2022. http://dx.doi.org/10.55201/dveo4978.

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In 1952, Professor Gheorghe Chiş from the Astronomical Institute together with the academician Constantin Daicoviciu initiated the idea of the existence of a Dacian calendar by deciphering the sanctuaries in the capital of Dacia at Sarmizegetusa Regia, and thus laying the foundations of Archaeoastronomy in Romania. This interdisciplinary branch has expanded over time due to new excavations, which have created to more detailed research, as it has led some researchers to think about the need to describe numerical calculation methods based on some huge databases. The School of Cultural Astronomy

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