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491:. It consists of two wide-field telescopes, one narrow field telescope, and one ultra-wide field telescope. A prototype system was installed in 1996 and a second in 1997, both in the same enclosure as the 10-inch astrograph. The three larger telescopes were installed in 2000. The ultra-wide device was added in 2002 when the existing telescopes were moved to a new, smaller enclosure. Location:
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1118:
Kollmeier, Juna A.; Zasowski, Gail; Rix, Hans-Walter; Johns, Matt; Anderson, Scott F.; Drory, Niv; Johnson, Jennifer A.; Pogge, Richard W.; Bird, Jonathan C.; Blanc, Guillermo A.; Brownstein, Joel R.; Crane, Jeffrey D.; De Lee, Nathan M.; Klaene, Mark A.; Kreckel, Kathryn; MacDonald, Nick; Merloni,
1119:
Andrea; Ness, Melissa K.; O'Brien, Thomas; Sanchez-Gallego, Jose R.; Sayres, Conor C.; Shen, Yue; Thakar, Ani R.; Tkachenko, Andrew; Aerts, Conny; Blanton, Michael R.; Eisenstein, Daniel J.; Holtzman, Jon A.; Maoz, Dan; et al. (2017). "SDSS-V: pioneering panoptic spectroscopy".
688:
design with seven 8.4 m (28 ft) segments. The telescope will have a light-gathering area of 368 m (3,960 sq ft), which is roughly fifteen times greater than one of the
Magellan telescopes. The mirrors are being fabricated by the
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Herbst, T.; Bilgi, Pavaman (2020). "The SDSS-V local volume mapper telescope system". In
Marshall, Heather K; Spyromilio, Jason; Usuda, Tomonori (eds.).
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321:. Cerro Las Campanas, situated near the southern end of this ridge and standing over 2,500 m (8,200 ft) tall, will be the future site of the
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The 1.0 m (39 in) Swope
Telescope was the first telescope installed at LCO, and began operating in 1971. It is named after CIS astronomer
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Coulter, D. A.; Foley, R. J.; Kilpatrick, C. D.; Drout, M. R.; Piro, A. L.; Shappee, B. J.; Siebert, M. R.; Simon, J. D.; Ulloa, N. (2017-10-16).
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A 0.25 m (10 in) astrograph operated at the site for some time, and was used to discover
Supernova 1987A (
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under construction at LCO, with commissioning expected to begin in 2029. It is 24.5 m (80 ft) effective
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Telescope in 2002. They are managed by LCO for an international consortium of institutions which includes LCO.
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317:. The LCO's telescopes and facilities are positioned near the northern end of a 7 km (4.3 mi)
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The Pi of the Sky project operated two wide-angle cameras that searched for the optical signature of
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480:± 1 meter, altitude of the base of the building 2,275 metres (7,464 ft) over mean sea level.
1336:"Swope Supernova Survey 2017a (SSS17a), the optical counterpart to a gravitational wave source"
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at LCO starting in 2004. The installation was moved to a commercial telescope hosting site in
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was located at LCO from 1995 to 2004. It is now located at the Pampa La Bola site of the
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Established in 1969, LCO is CIS's primary observatory, having taken over this role from
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The
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The 1.3 m (51 in) Warsaw
Telescope is the main instrument of the
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The 2.5 m (98 in) du Pont
Telescope is named after industrialist
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and Oscar
Duhalde became the first official observers of Supernova 1987A (
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consists of four telescopes (siderostats) each with 0.16 m diameter near
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1296:"The Giant Magellan Telescope Organization Breaks Ground in Chile"
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1098:"High-Resolution Optical Spectroscopy - University of Birmingham"
1225:"Complejo Astronómico El Leoncito - Helen Sawyer Hogg Telescope"
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340:, while the main office in Chile is in La Serena, close to the
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1075:. Harvard Smithsonian Center for Astrophysics. Archived from
717:, the optical counterpart to the gravitational wave source
368:
are two identical single-mirror reflecting telescopes. The
1010:"The Henrietta Swope Telescope — Las Campanas Observatory"
546:. It consists of a pair of four 0.18 m (7.1 in)
968:"The Irénée du Pont Telescope — Las Campanas Observatory"
905:"Magellan Telescopes (6.5m) | The Carnegie Observatories"
355:, located 23 kilometres (14 mi) to the southwest.
336:
area. The headquarters of
Carnegie Observatories is in
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Magellan telescopes, Warsaw and Swope telescopes (LTR)
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693:
Mirror
Laboratory, and the first was started in 2005.
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Association of Universities for Research in Astronomy
1298:(Press release). GMTO Corporation. 11 November 2015.
947:"The du Pont Telescope | The Carnegie Observatories"
487:(ASAS) is a project to monitor the southern sky for
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989:"The Swope Telescope | The Carnegie Observatories"
926:"Magellan Telescopes — Las Campanas Observatory"
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774:Clay telescope (one of the Magellan telescopes)
1052:"All Sky Automated Survey - The ASAS-3 System"
383:and has been in operation since 1977. It is a
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8:
640:Telescope (HSHT) was operated at LCO by the
554:on a common mount. It was installed in 2009.
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1781:Buildings and structures in Coquimbo Region
721:, was discovered with the Swope telescope.
372:Telescope saw first light in 2000, and the
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1166:. Vol. 11445. SPIE. p. 114450J.
858:Overbye, D., Zegers, M. (April 18, 2023),
750:Warsaw telescope dome and control building
642:University of Toronto Southern Observatory
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41:
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18:
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1164:Ground-based and Airborne Telescopes VIII
1141:"SDSS-V Pioneering panoptic spectroscopy"
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332:due to increasing light pollution in the
644:from 1971 to 1997. It is now located at
432:Observatory. Installed in 1996, it is a
426:Optical Gravitational Lensing Experiment
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1241:
850:
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884:"History | The Carnegie Observatories"
31:Telescopes at Las Campanas Observatory
1310:"Overview - Giant Magellan Telescope"
618:The 4.0 m (13.1 ft) NANTEN
559:Birmingham Solar Oscillations Network
7:
256:Location of Las Campanas Observatory
1776:Astronomical observatories in Chile
1452:Astronomical observatories in Chile
1248:"SN1987A's Twentieth Anniversary".
561:(BiSON) operates at station at LCO.
1312:. GMTO Corporation. Archived from
1227:. Complejo Astronómico El Leoncito
860:"A Giant Telescope Grows in Chile"
834:List of astronomical observatories
14:
1616:National Astronomical Observatory
391:corrector lens, and was built by
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1204:"The NANTEN2 Telescope | NANTEN"
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57:Carnegie Institution for Science
1273:. Pi of the Sky. Archived from
1054:. Warsaw University Observatory
1033:. Warsaw University Observatory
627:Llano de Chajnantor Observatory
564:The Local Volume Mapper of the
292:Las Campanas Observatory (LCO)
1:
1031:"General Description of OGLE"
702:On February 24, 1987 at LCO,
646:Leoncito Astronomical Complex
636:The 0.61 m (24 in)
364:The 6.5 m (260 in)
351:The observatory is served by
151:2,380 m (7,810 ft)
1771:1971 establishments in Chile
1608:Santiago Metropolitan Region
991:. The Carnegie Observatories
949:. The Carnegie Observatories
907:. The Carnegie Observatories
886:. The Carnegie Observatories
522:ASAS South Telescopes at LCO
713:On August 17, 2017 at LCO,
1797:
1411:The Carnegie Observatories
1206:. University of Birmingham
1100:. University of Birmingham
1012:. Las Campanas Observatory
970:. Las Campanas Observatory
928:. Las Campanas Observatory
404:Ritchey-Chrétien telescope
385:Ritchey-Chrétien telescope
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682:extremely large telescope
278:
265:
234:
24:
1596:Giant Magellan Telescope
839:Mount Wilson Observatory
678:Giant Magellan Telescope
588:29.010833°S 70.7006500°W
485:All Sky Automated Survey
330:Mount Wilson Observatory
323:Giant Magellan Telescope
273:Related media on Commons
213:Giant Magellan Telescope
20:Las Campanas Observatory
1370:10.1126/science.aap9811
593:-29.010833; -70.7006500
511:29.010250°S 70.701417°W
471:Warsaw Telescope at LCO
460:29.009944°S 70.701639°W
395:and L&F Industries.
342:University of La Serena
516:-29.010250; -70.701417
465:-29.009944; -70.701639
37:Alternative names
822:BiSON Solar Telescope
620:millimeter-wavelength
599:LVM telescopes at LCO
132:29.01597°S 70.69208°W
75:Observatory code
1073:"HAT-South homepage"
664:San Pedro de Atacama
629:and is known as the
430:University of Warsaw
408:Boller & Chivens
393:Boller & Chivens
338:Pasadena, California
137:-29.01597; -70.69208
1591:Magellan Telescopes
1488:Llano de Chajnantor
1362:2017Sci...358.1556C
1346:(6370): 1556–1558.
1258:2007eso..pres....8.
1145:Bulletin of the AAS
786:Magellan telescopes
691:Steward Observatory
631:NANTEN2 Observatory
583: /
506: /
455: /
366:Magellan Telescopes
218:Magellan Telescopes
128: /
21:
1460:Antofagasta Region
1172:10.1117/12.2561419
864:The New York Times
440:. Exact location:
305:(CIS). Located in
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1250:ESO Press Release
738:du Pont telescope
671:Future telescopes
638:Helen Sawyer Hogg
613:Former telescopes
419:Tenant telescopes
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1731:Solar System
1586:Las Campanas
1585:
1576:Cerro Tololo
1556:Cerro Pachón
1343:
1339:
1329:
1318:. Retrieved
1314:the original
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1275:the original
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447:29°00′35.8″S
370:Walter Baade
350:
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296:astronomical
291:
290:
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1719:Outer space
1707:Spaceflight
1252:: 8. 2007.
704:Ian Shelton
698:Discoveries
591: /
552:astrographs
550:reflecting
514: /
463: /
374:Landon Clay
334:Los Angeles
299:observatory
161:Established
135: /
110:Coordinates
16:Observatory
1765:Categories
1353:1710.05452
1320:2012-01-24
1281:2012-01-24
1231:2012-01-23
1210:2012-01-24
1151:(7). 2020.
1126:1711.03234
1104:2012-01-24
1083:2012-01-24
1058:2012-01-24
1037:2012-01-24
1016:2012-01-24
995:2012-01-24
974:2012-01-24
953:2012-01-24
932:2012-01-24
911:2012-01-24
890:2012-01-24
845:References
597: (
542:using the
540:exoplanets
538:to detect
531:± 5 meter.
520: (
469: (
402:. It is a
359:Telescopes
348:facility.
197:Telescopes
164:1969
123:70°41′31″W
120:29°00′57″S
1743:Education
1683:Astronomy
1394:206664790
1378:0036-8075
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412:Gascoigne
406:built by
389:Gascoigne
315:La Serena
1644:Category
1581:La Silla
1386:29038368
869:22 April
828:See also
719:GW170817
708:SN 1987A
686:aperture
666:in 2011.
653:SN 1987A
548:Takahasi
148:Altitude
98:Location
1755:Science
1657:Portals
1523:Paranal
1512:NANTEN2
1358:Bibcode
1340:Science
1254:Bibcode
725:Gallery
410:with a
387:with a
176:Website
104:, Chile
1560:Gemini
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680:is an
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1390:S2CID
1348:arXiv
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1121:arXiv
307:Chile
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1570:SOAR
1538:SWGO
1502:ASTE
1497:ALMA
1492:APEX
1382:PMID
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1176:ISBN
871:2023
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557:The
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183:.lco
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