461:'s life. Our current understanding of how the masses of stars are distributed at birth was produced by Gilmore's team. In the early 1990s with a student he obtained the still standard estimate of the mass surface density associated with the discs. This study set the pattern of future work. He pioneered the use of spectral surveys to unravel the Galaxy's history through its chemistry and established that stars in the halo of the Galaxy are chemically distinct from stars in the Galaxy's satellites, even though much of the
44:
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in the southern hemisphere of the sky. He measured the magnitudes of about 130 quasars from a large number of photographic plates. He found the results were best explained by the infall of gas on to supermassive black holes. This research led to the award of a PhD degree in 1979.
518:
Wilkinson, Mark I., Jan T. Kleyna, N. Wyn Evans, Gerard F. Gilmore, Michael J. Irwin, and Eva K. Grebel. "Kinematically cold populations at large radii in the Draco and Ursa minor dwarf spheroidal galaxies." The
Astrophysical Journal Letters 611, no. 1 (2004):
514:
Watkins, L. L., N. W. Evans, Vasily
Belokurov, M. C. Smith, Paul C. Hewett, Daniel M. Bramich, Gerard F. Gilmore et al. "Substructure revealed by RR Lyraes in SDSS Stripe 82." Monthly Notices of the Royal Astronomical Society 398, no. 4 (2009):
522:
Smartt, Stephen J., Justyn R. Maund, Margaret A. Hendry, Christopher A. Tout, Gerard F. Gilmore, Seppo
Mattila, and Chris R. Benn. "Detection of a red supergiant progenitor star of a Type II-plateau supernova." Science 303, no. 5657 (2004):
506:
Mackey⋆, A. D., and G. F. Gilmore. "Surface brightness profiles and structural parameters for 53 rich stellar clusters in the Large
Magellanic Cloud." Monthly Notices of the Royal Astronomical Society 338, no. 1 (2003):
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found stars having radial velocities that were different to those of
Galactic stars. They concluded that these belonged to a dwarf galaxy in the process of merging with our own Galaxy, and which is today called the
510:
Maund, Justyn R., Stephen J. Smartt, Rolf P. Kudritzki, Philipp
Podsiadlowski, and Gerard F. Gilmore. "The massive binary companion star to the progenitor of supernova 1993J." Nature 427, no. 6970 (2004):
1403:
329:
that represented the distribution of stars as two simple components. Gilmore and Reid argued the observed numbers of stars implied the existence of an additional component they called the
321:, between 1979 and 1984. He used the expertise gained during his PhD to measure brightnesses and numbers of stars from photographic sky surveys. Working with Neil Reid with data from the
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to measure the stars' radial velocities, and consequently to determine the surface mass density of the
Galactic disc. They showed that there was little or no
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and
Christopher Tout, Gilmore determined the numbers of low-mass stars in the disc of the Galaxy, improving on previous measurements.
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878:"The Mass Distribution in the Galactic Disc. – I A Technique to Determine the Integral Surface Mass Density of the Disc near the Sun"
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921:"The Mass Distribution in the Galactic Disc. – II Determination of the Surface Mass Density of the Galactic Disc Near the Sun"
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Gilmore remained at the
University of Canterbury as a postgraduate research student. He used the 0.61-metre telescope at
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that extends through the disc. Consequently, dark matter within the Galaxy does not concentrate within the disc.
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spacecraft that is measuring the positions, motions and brightnesses of millions of stars in the Galaxy.
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During a survey of the motions of stars in the central regions of the Galaxy, Rodrigo Ibata, Gilmore and
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835:"New light on faint stars – III. Galactic structure towards the South Pole and the Galactic thick disc"
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Observational extragalactic astronomy : an investigation of southern quasars and related objects
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Professor of
Experimental Philosophy, in the Institute of Astronomy, at the University of Cambridge
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in the University of Cambridge. In 2000 he was promoted to professor of experimental philosophy.
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companions of the Galaxy to determine the relative contribution of dark matter to these systems.
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Observational extragalactic astronomy: an investigation of southern quasars and related objects
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469:. In 1994 with a student he discovered the Galaxy's most important satellite after the
361:. Working with Konrad Kuijken, he used spectra of faint stars in the region around the
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964:"The Mass Distribution in the Galactic Disc. – III The Local Volume Mass Density"
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Gilmore has had an important role in the design and scientific strategy of the
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of stars to study the structure of the Galaxy, particularly by measuring their
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473:. As its leading UK proponent, Gilmore played a big role in selection of
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325:, he found an excess of faint stars compared to standard models of the
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Gerry Gilmore leads efforts to understand the structure and origin of
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Gilmore has collaborated with a large number of scientists, including
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577:(Doctoral thesis). UC Research Repository, University of Canterbury.
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403:. He has used observations of the radial velocities of stars in the
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that exists alongside the main Galactic disc and the stellar halo.
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in 1984 on being awarded an advanced research fellowship by the
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293:), where he was awarded a Bachelor of Science degree in 1973.
457:, and helped to show that the thick disc formed early in the
224:
789:"The distribution of low-mass stars in the Galactic disc"
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to understand its structure and evolutionary history.
373:
within the disc other than that part of the Galactic
269:. His research has centred on studying stars in the
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661:(1994). "A dwarf satellite galaxy in Sagittarius".
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34:
1404:People educated at St Bede's College, Christchurch
615:
489:Gilmore was awarded a Master of Arts degree and a
969:Monthly Notices of the Royal Astronomical Society
926:Monthly Notices of the Royal Astronomical Society
883:Monthly Notices of the Royal Astronomical Society
840:Monthly Notices of the Royal Astronomical Society
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794:Monthly Notices of the Royal Astronomical Society
313:Gerry Gilmore worked as a research fellow at the
48:Gerry Gilmore presenting first results from the
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755:ORCID database record: ID 0000-0003-4632-0213.
453:that first showed that the Galaxy possesses a
1017:
787:Kroupa, P.; Tout, C. A.; Gilmore, G. (1993).
8:
1024:
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300:to monitor changes in the brightnesses of
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31:
1384:Fellows of the Royal Astronomical Society
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962:Kuijken, Konrad; Gilmore, Gerard (1989).
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919:Kuijken, Konrad; Gilmore, Gerard (1989).
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876:Kuijken, Konrad; Gilmore, Gerard (1989).
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439:Fellow of the Royal Society (FRS) in 2013
1414:Academics of the University of Cambridge
1374:New Zealand fellows of the Royal Society
351:Science and Engineering Research Council
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539:
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630: ed.). A & C Black.
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481:. He is the driving force behind the
7:
1389:20th-century New Zealand astronomers
465:must consist of stars stripped from
1379:Fellows of the Institute of Physics
394:Sagittarius Dwarf Spheroidal Galaxy
121:Sagittarius Dwarf Spheroidal Galaxy
52:at 11 November 2016 meeting of the
25:
729:Institutional personal home page.
718:Institute of Astronomy, Cambridge
298:Mount John University Observatory
547:"Professor Gerard F Gilmore FRS"
323:United Kingdom Schmidt Telescope
1409:University of Canterbury alumni
617:"GILMORE, Prof. Gerard Francis"
283:St Bede's College, Christchurch
833:Gilmore, G.; Reid, N. (1983).
410:In 1994 he was appointed to a
1:
179:European Southern Observatory
765:Gerry Gilmore's publications
635:UK public library membership
309:Royal Observatory, Edinburgh
1348:Prince Andrew, Duke of York
1430:
367:Anglo-Australian Telescope
353:. He used observations of
253:(born 7 November 1951) is
54:Royal Astronomical Society
626:. Vol. 2015 (online
215:
159:
41:
1225:Maria Grazia Spillantini
1205:Christopher J. Schofield
862:10.1093/mnras/202.4.1025
771:bibliographic database.
441:. His nomination reads:
287:University of Canterbury
281:Gilmore was educated at
100:University of Canterbury
991:10.1093/mnras/239.2.651
948:10.1093/mnras/239.2.605
905:10.1093/mnras/239.2.571
816:10.1093/mnras/262.3.545
773:(subscription required)
628:Oxford University Press
491:Doctor of Science (ScD)
405:dwarf spheroidal galaxy
347:University of Cambridge
337:University of Cambridge
267:University of Cambridge
259:Experimental Philosophy
174:University of Cambridge
106:University of Cambridge
487:
449:. He led a revival of
437:Gilmore was elected a
343:Institute of Astronomy
263:Institute of Astronomy
242:Gerard Francis Gilmore
65:Gerard Francis Gilmore
1185:William D. Richardson
495:Clare Hall, Cambridge
423:European Space Agency
341:Gilmore moved to the
571:Gilmore, G. (1979).
1297:Margaret Buckingham
1235:Brigitta Stockinger
982:1989MNRAS.239..651K
939:1989MNRAS.239..605K
896:1989MNRAS.239..571K
853:1983MNRAS.202.1025G
807:1993MNRAS.262..545K
677:1994Natur.370..194I
451:star-count analysis
363:South Galactic Pole
1399:People from Timaru
433:Awards and honours
365:obtained with the
50:Gaia space mission
1356:
1355:
1245:Jean-Paul Vincent
1135:Gillian Griffiths
633:(Subscription or
551:The Royal Society
471:Magellanic Clouds
359:radial velocities
315:Royal Observatory
239:
238:
161:Scientific career
119:Discovery of the
18:Gerard F. Gilmore
16:(Redirected from
1421:
1332:Eli Yablonovitch
1155:Gideon Henderson
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847:(4): 1025–1047.
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740:"Gerard Gilmore"
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553:. Archived from
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375:dark matter halo
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207:Doctoral advisor
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1307:John Hutchinson
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1230:Douglas Stephan
1215:Stephen Simpson
1165:Stephen P. Long
1160:Guy Lloyd-Jones
1090:Michael Burrows
1085:Gilles Brassard
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767:indexed by the
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714:"Gerry Gilmore"
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557:on 9 June 2015.
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93:Alma mater
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75:7 November 1951
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653:Ibata, R. A.;
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501:Selected works
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1037:Royal Society
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257:Professor of
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77:(age 72)
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40:
36:Gerry Gilmore
33:
30:
19:
1317:Elliott Lieb
1265:Robert Young
1180:Paul O'Brien
1145:Phil Hawkins
1140:Joanna Haigh
1130:Martin Green
1115:Nigel Glover
973:
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747:. Retrieved
734:
721:. Retrieved
668:
662:
659:Irwin, M. J.
621:
573:
555:the original
493:degree from
488:
479:Gaia mission
455:"thick" disc
444:
436:
420:
416:astrophysics
409:
398:
386:
382:Pavel Kroupa
379:
340:
312:
295:
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241:
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193:
167:Institutions
160:
29:
1394:1951 births
1312:Eric Kandel
1281:Bill Bryson
1255:Terry Wyatt
1220:Terry Speed
1200:John Savill
1150:Edith Heard
1075:Mervyn Bibb
749:19 November
723:19 November
655:Gilmore, G.
371:dark matter
291:New Zealand
86:New Zealand
1363:Categories
1210:Paul Sharp
1195:Kerry Rowe
1175:Anne Mills
1070:Mike Bevan
1065:Keith Ball
801:(3): 545.
637:required.)
591:10092/7584
549:. London:
528:References
515:1757–1770.
467:satellites
447:our Galaxy
412:readership
331:thick disc
71:1951-11-07
1100:Ara Darzi
623:Who's Who
497:in 2002.
289:(both in
277:Education
265:, at the
261:, in the
108:(MA, ScD)
102:(BS, PhD)
1302:Chen Zhu
1274:Honorary
1039:elected
523:499–503.
319:Scotland
285:and the
255:Emeritus
1290:Foreign
1048:Fellows
1041:in 2013
1035:of the
1033:Fellows
978:Bibcode
935:Bibcode
892:Bibcode
849:Bibcode
803:Bibcode
693:4335789
673:Bibcode
507:85–119.
355:spectra
345:of the
302:quasars
220:Website
211:Ken Fea
769:Scopus
691:
664:Nature
459:Galaxy
327:Galaxy
271:Galaxy
251:FInstP
200:(1979)
198:
189:Thesis
151:FInstP
142:(2002)
136:(2015)
127:Awards
82:Timaru
1341:Royal
744:ORCID
689:S2CID
475:ESA's
380:With
233:/~gil
751:2016
725:2016
519:L21.
511:129.
463:halo
427:Gaia
248:FRAS
227:.cam
146:FRAS
61:Born
986:doi
974:239
943:doi
931:239
900:doi
888:239
857:doi
845:202
811:doi
799:262
681:doi
669:370
587:hdl
579:doi
483:ESO
425:'s
414:in
245:FRS
231:.uk
229:.ac
225:ast
140:ScD
134:FRS
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