The AAO/UKST SuperCOSMOS Hα survey
Identifieur interne : 00A217 ( Main/Exploration ); précédent : 00A216; suivant : 00A218The AAO/UKST SuperCOSMOS Hα survey
Auteurs : Quentin A. Parker [Australie] ; S. Phillipps ; M. J. Pierce ; M. Hartley [Australie] ; N. C. Hambly [Royaume-Uni] ; M. A. Read [Royaume-Uni] ; H. T. Macgillivray [Royaume-Uni] ; S. B. Tritton [Royaume-Uni] ; C. P. Cass [Australie] ; R. D. Cannon [Australie] ; M. Cohen [États-Unis] ; J. E. Drew [Royaume-Uni] ; D. J. Frew [Australie] ; E. Hopewell [Royaume-Uni] ; S. Mader [Australie] ; D. F. Malin [Australie] ; M. R. W. Masheder ; D. H. Morgan [Royaume-Uni] ; R. A. H. Morris ; D. Russeil [France] ; K. S. Russell [Australie] ; R. N. F. WalkerSource :
- Monthly Notices of the Royal Astronomical Society [ 0035-8711 ] ; 2005-09.
Descripteurs français
- Pascal (Inist)
- Wicri :
- topic : Atlas.
English descriptors
- KwdEn :
- Aperture photometry, Apjs, Arcmin, Arcmin extracts, Arcmin region, Arcsec, Artefact, Astrometric, Astrometric reduction procedure, Astronomical catalogues, Atlas, Bandpass, Best area, Bottom image, Bright areas, Calibration, Calibration factor, Calibration process, Calibration scheme, Cent contour, Cent level, Central area, Central stars, Central wavelength, Centre, Centred, Characteristic curve, Circular aperture, Clear aperture, Colour, Colour correction, Comparison plot, Comparison plots, Continuum, Continuum emission, Continuum images, Continuum point sources, Continuum subtraction, Contour plot, Correction, Data product, Data products, Diffuse emission, Direct comparison, Downloaded, Edinburgh, Eld, Emission features, Emission line objects, Emission line stars, Emission structure, Emitter, Emulsion, Emulsion sensitivity, Emulsion surface, Entire survey, Equivalent area, Exposure pairs, Faint limit, Fainter magnitudes, First epoch, Frew, Frew parker, Full resolution, Further details, Galactic, Galactic emission, Galactic plane, Galactic planes, Galactic snrs, Gaustad, Geocoronal, Geocoronal contribution, Geocoronal emission, Georgelin, Good data, Hambly, High reddening, High resolution, Histogram equalization, Image ellipticity, Image grade, Image quality, Imaging, Incident angle, Intensity calibration, Intensity space, Intensity values, Iphas survey, Large numbers, Less correction, Limited areas, Line emission, Linear part, Linear portion, Linear relation, Linear response, Lter, Lter artefacts, Lter bandpass, Lter response, Lter transmission, Macgillivray, Magellanic Clouds, Magellanic clouds, Magnitude range, Meaburn, Mechanical deformation, Mnras, Nebula, Normal incidence, Observatory, Online, Original survey, Other surveys, Overlap region, Overlap regions, Pan, Parker russeil, Pasa, Phillipps, Phillipps parker, Photographic data, Photographic material, Photometric, Photometry, Pixel, Pixel data, Pixel value, Planetary nebula, Planetary nebulae, Point sources, Powerful tool, Rayleigh, Rayleigh value, Region centred, Residual, Response curves, Royal observatory edinburgh, Russeil, Same area, Same region, Saturn satellite, Schmidt, Schmidt telescope, Several areas, Shassa, Shassa data, Shassa images, Shassa intensity calibration, Shassa pixels, Shassa values, Show evidence, Similar depth, Spatial resolution, Spurious, Spurious images, Standard ukst survey data, Star formation, Stellar, Stellar evolution, Stellar locus, Stellar photometry, Supercosmos, Supercosmos counts, Supercosmos data, Supercosmos intensity counts, Supercosmos scans, Supernova remnants, Surface brightness, Survey, Survey atlas, Survey data, Survey data products, Survey figure, Survey pairs, Telescope, Telescope beam, Ucac catalogue, Ukst, Ukst beam, Uncancelled stars, Vertical scatter, Wham, Whole survey, Wide range, astronomical data bases: miscellaneous, catalogues, photometry, stars: emission line, surveys.
- Teeft :
- Aperture photometry, Apjs, Arcmin, Arcmin extracts, Arcmin region, Arcsec, Artefact, Astrometric, Astrometric reduction procedure, Bandpass, Best area, Bottom image, Bright areas, Calibration, Calibration factor, Calibration process, Calibration scheme, Cent contour, Cent level, Central area, Central stars, Central wavelength, Centre, Centred, Characteristic curve, Circular aperture, Clear aperture, Colour, Colour correction, Comparison plot, Comparison plots, Continuum emission, Continuum images, Continuum point sources, Continuum subtraction, Contour plot, Correction, Data product, Data products, Diffuse emission, Direct comparison, Downloaded, Edinburgh, Eld, Emission features, Emission line objects, Emission structure, Emitter, Emulsion, Emulsion sensitivity, Emulsion surface, Entire survey, Equivalent area, Exposure pairs, Faint limit, Fainter magnitudes, First epoch, Frew, Frew parker, Full resolution, Further details, Galactic, Galactic emission, Galactic plane, Galactic snrs, Gaustad, Geocoronal, Geocoronal contribution, Geocoronal emission, Georgelin, Good data, Hambly, High reddening, High resolution, Histogram equalization, Image ellipticity, Image grade, Image quality, Imaging, Incident angle, Intensity calibration, Intensity space, Intensity values, Iphas survey, Large numbers, Less correction, Limited areas, Line emission, Linear part, Linear portion, Linear relation, Linear response, Lter, Lter artefacts, Lter bandpass, Lter response, Lter transmission, Macgillivray, Magellanic clouds, Magnitude range, Meaburn, Mechanical deformation, Mnras, Nebula, Normal incidence, Observatory, Online, Original survey, Other surveys, Overlap region, Overlap regions, Parker russeil, Pasa, Phillipps, Phillipps parker, Photographic data, Photographic material, Photometric, Photometry, Pixel, Pixel data, Pixel value, Planetary nebula, Planetary nebulae, Point sources, Powerful tool, Rayleigh, Rayleigh value, Region centred, Residual, Response curves, Royal observatory edinburgh, Russeil, Same area, Same region, Schmidt, Schmidt telescope, Several areas, Shassa, Shassa data, Shassa images, Shassa intensity calibration, Shassa pixels, Shassa values, Show evidence, Similar depth, Spatial resolution, Spurious, Spurious images, Standard ukst survey data, Star formation, Stellar, Stellar evolution, Stellar locus, Stellar photometry, Supercosmos, Supercosmos counts, Supercosmos data, Supercosmos intensity counts, Supercosmos scans, Supernova remnants, Surface brightness, Survey, Survey atlas, Survey data, Survey data products, Survey figure, Survey pairs, Telescope, Telescope beam, Ucac catalogue, Ukst, Ukst beam, Uncancelled stars, Vertical scatter, Wham, Whole survey, Wide range.
Abstract
The UK Schmidt Telescope (UKST) of the Anglo‐Australian Observatory completed a narrow‐band Hα plus [N ii] 6548, 6584‐Å survey of the Southern Galactic Plane and Magellanic Clouds in late 2003. The survey, which was the last UKST wide‐field photographic survey and the only one undertaken in a narrow‐band, is now an online digital data product of the Wide‐Field Astronomy Unit of the Royal Observatory Edinburgh (ROE). The survey utilized a high specification, monolithic Hα interference bandpass filter of exceptional quality. In conjunction with the fine‐grained Tech‐Pan film as a detector it has produced a survey with a powerful combination of area coverage (4000 square degrees), resolution (∼1 arcsec) and sensitivity (≤5 Rayleighs), reaching a depth for continuum point sources of R≃ 20.5. The main survey consists of 233 individual fields on a grid of centres separated by 4° at declinations below +2° and covers a swathe approximately 20° wide about the Southern Galactic Plane. The original survey films were scanned by the SuperCOSMOS measuring machine at the Royal Observatory, Edinburgh, to provide the online digital atlas called the SuperCOSMOS Hα Survey (SHS). We present the background of the survey, the key survey characteristics, details and examples of the data product, calibration process, comparison with other surveys and a brief description of its potential for scientific exploitation.
Url:
- https://api.istex.fr/document/7D1180DFEB06B9964E159DCD6568AAE9B26A5DFE/fulltext/pdf
- https://api.istex.fr/document/D6276BED7D62FB067443F2193817ECCDA3997AC7/fulltext/pdf
DOI: 10.1111/j.1365-2966.2005.09350.x
Affiliations:
- Australie, France, Royaume-Uni, États-Unis
- Angleterre, Californie, Grand Londres, Nouvelle-Galles du Sud, Écosse
- Berkeley (Californie), Londres, Sydney, Édimbourg
Links toward previous steps (curation, corpus...)
- to stream Istex, to step Corpus: 001764
- to stream Istex, to step Curation: 001764
- to stream Istex, to step Checkpoint: 001772
- to stream Istex, to step Corpus: 002797
- to stream Istex, to step Curation: 002797
- to stream Istex, to step Checkpoint: 001730
- to stream Main, to step Merge: 00AD81
- to stream PascalFrancis, to step Corpus: 004788
- to stream PascalFrancis, to step Curation: 001915
- to stream PascalFrancis, to step Checkpoint: 004344
- to stream Main, to step Merge: 00AF94
- to stream Main, to step Curation: 00A217
Le document en format XML
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<profileDesc><textClass><keywords scheme="KwdEn" xml:lang="en"><term>Aperture photometry</term>
<term>Apjs</term>
<term>Arcmin</term>
<term>Arcmin extracts</term>
<term>Arcmin region</term>
<term>Arcsec</term>
<term>Artefact</term>
<term>Astrometric</term>
<term>Astrometric reduction procedure</term>
<term>Astronomical catalogues</term>
<term>Atlas</term>
<term>Bandpass</term>
<term>Best area</term>
<term>Bottom image</term>
<term>Bright areas</term>
<term>Calibration</term>
<term>Calibration factor</term>
<term>Calibration process</term>
<term>Calibration scheme</term>
<term>Cent contour</term>
<term>Cent level</term>
<term>Central area</term>
<term>Central stars</term>
<term>Central wavelength</term>
<term>Centre</term>
<term>Centred</term>
<term>Characteristic curve</term>
<term>Circular aperture</term>
<term>Clear aperture</term>
<term>Colour</term>
<term>Colour correction</term>
<term>Comparison plot</term>
<term>Comparison plots</term>
<term>Continuum</term>
<term>Continuum emission</term>
<term>Continuum images</term>
<term>Continuum point sources</term>
<term>Continuum subtraction</term>
<term>Contour plot</term>
<term>Correction</term>
<term>Data product</term>
<term>Data products</term>
<term>Diffuse emission</term>
<term>Direct comparison</term>
<term>Downloaded</term>
<term>Edinburgh</term>
<term>Eld</term>
<term>Emission features</term>
<term>Emission line objects</term>
<term>Emission line stars</term>
<term>Emission structure</term>
<term>Emitter</term>
<term>Emulsion</term>
<term>Emulsion sensitivity</term>
<term>Emulsion surface</term>
<term>Entire survey</term>
<term>Equivalent area</term>
<term>Exposure pairs</term>
<term>Faint limit</term>
<term>Fainter magnitudes</term>
<term>First epoch</term>
<term>Frew</term>
<term>Frew parker</term>
<term>Full resolution</term>
<term>Further details</term>
<term>Galactic</term>
<term>Galactic emission</term>
<term>Galactic plane</term>
<term>Galactic planes</term>
<term>Galactic snrs</term>
<term>Gaustad</term>
<term>Geocoronal</term>
<term>Geocoronal contribution</term>
<term>Geocoronal emission</term>
<term>Georgelin</term>
<term>Good data</term>
<term>Hambly</term>
<term>High reddening</term>
<term>High resolution</term>
<term>Histogram equalization</term>
<term>Image ellipticity</term>
<term>Image grade</term>
<term>Image quality</term>
<term>Imaging</term>
<term>Incident angle</term>
<term>Intensity calibration</term>
<term>Intensity space</term>
<term>Intensity values</term>
<term>Iphas survey</term>
<term>Large numbers</term>
<term>Less correction</term>
<term>Limited areas</term>
<term>Line emission</term>
<term>Linear part</term>
<term>Linear portion</term>
<term>Linear relation</term>
<term>Linear response</term>
<term>Lter</term>
<term>Lter artefacts</term>
<term>Lter bandpass</term>
<term>Lter response</term>
<term>Lter transmission</term>
<term>Macgillivray</term>
<term>Magellanic Clouds</term>
<term>Magellanic clouds</term>
<term>Magnitude range</term>
<term>Meaburn</term>
<term>Mechanical deformation</term>
<term>Mnras</term>
<term>Nebula</term>
<term>Normal incidence</term>
<term>Observatory</term>
<term>Online</term>
<term>Original survey</term>
<term>Other surveys</term>
<term>Overlap region</term>
<term>Overlap regions</term>
<term>Pan</term>
<term>Parker russeil</term>
<term>Pasa</term>
<term>Phillipps</term>
<term>Phillipps parker</term>
<term>Photographic data</term>
<term>Photographic material</term>
<term>Photometric</term>
<term>Photometry</term>
<term>Pixel</term>
<term>Pixel data</term>
<term>Pixel value</term>
<term>Planetary nebula</term>
<term>Planetary nebulae</term>
<term>Point sources</term>
<term>Powerful tool</term>
<term>Rayleigh</term>
<term>Rayleigh value</term>
<term>Region centred</term>
<term>Residual</term>
<term>Response curves</term>
<term>Royal observatory edinburgh</term>
<term>Russeil</term>
<term>Same area</term>
<term>Same region</term>
<term>Saturn satellite</term>
<term>Schmidt</term>
<term>Schmidt telescope</term>
<term>Several areas</term>
<term>Shassa</term>
<term>Shassa data</term>
<term>Shassa images</term>
<term>Shassa intensity calibration</term>
<term>Shassa pixels</term>
<term>Shassa values</term>
<term>Show evidence</term>
<term>Similar depth</term>
<term>Spatial resolution</term>
<term>Spurious</term>
<term>Spurious images</term>
<term>Standard ukst survey data</term>
<term>Star formation</term>
<term>Stellar</term>
<term>Stellar evolution</term>
<term>Stellar locus</term>
<term>Stellar photometry</term>
<term>Supercosmos</term>
<term>Supercosmos counts</term>
<term>Supercosmos data</term>
<term>Supercosmos intensity counts</term>
<term>Supercosmos scans</term>
<term>Supernova remnants</term>
<term>Surface brightness</term>
<term>Survey</term>
<term>Survey atlas</term>
<term>Survey data</term>
<term>Survey data products</term>
<term>Survey figure</term>
<term>Survey pairs</term>
<term>Telescope</term>
<term>Telescope beam</term>
<term>Ucac catalogue</term>
<term>Ukst</term>
<term>Ukst beam</term>
<term>Uncancelled stars</term>
<term>Vertical scatter</term>
<term>Wham</term>
<term>Whole survey</term>
<term>Wide range</term>
<term>astronomical data bases: miscellaneous</term>
<term>catalogues</term>
<term>photometry</term>
<term>stars: emission line</term>
<term>surveys</term>
</keywords>
<keywords scheme="Pascal" xml:lang="fr"><term>Atlas</term>
<term>Catalogue astronomique</term>
<term>Continuum</term>
<term>Etoile raie émission</term>
<term>Nuages Magellan</term>
<term>Pan</term>
<term>Photométrie</term>
<term>Plan galactique</term>
<term>Satellite Saturne</term>
<term>Source ponctuelle</term>
</keywords>
<keywords scheme="Teeft" xml:lang="en"><term>Aperture photometry</term>
<term>Apjs</term>
<term>Arcmin</term>
<term>Arcmin extracts</term>
<term>Arcmin region</term>
<term>Arcsec</term>
<term>Artefact</term>
<term>Astrometric</term>
<term>Astrometric reduction procedure</term>
<term>Bandpass</term>
<term>Best area</term>
<term>Bottom image</term>
<term>Bright areas</term>
<term>Calibration</term>
<term>Calibration factor</term>
<term>Calibration process</term>
<term>Calibration scheme</term>
<term>Cent contour</term>
<term>Cent level</term>
<term>Central area</term>
<term>Central stars</term>
<term>Central wavelength</term>
<term>Centre</term>
<term>Centred</term>
<term>Characteristic curve</term>
<term>Circular aperture</term>
<term>Clear aperture</term>
<term>Colour</term>
<term>Colour correction</term>
<term>Comparison plot</term>
<term>Comparison plots</term>
<term>Continuum emission</term>
<term>Continuum images</term>
<term>Continuum point sources</term>
<term>Continuum subtraction</term>
<term>Contour plot</term>
<term>Correction</term>
<term>Data product</term>
<term>Data products</term>
<term>Diffuse emission</term>
<term>Direct comparison</term>
<term>Downloaded</term>
<term>Edinburgh</term>
<term>Eld</term>
<term>Emission features</term>
<term>Emission line objects</term>
<term>Emission structure</term>
<term>Emitter</term>
<term>Emulsion</term>
<term>Emulsion sensitivity</term>
<term>Emulsion surface</term>
<term>Entire survey</term>
<term>Equivalent area</term>
<term>Exposure pairs</term>
<term>Faint limit</term>
<term>Fainter magnitudes</term>
<term>First epoch</term>
<term>Frew</term>
<term>Frew parker</term>
<term>Full resolution</term>
<term>Further details</term>
<term>Galactic</term>
<term>Galactic emission</term>
<term>Galactic plane</term>
<term>Galactic snrs</term>
<term>Gaustad</term>
<term>Geocoronal</term>
<term>Geocoronal contribution</term>
<term>Geocoronal emission</term>
<term>Georgelin</term>
<term>Good data</term>
<term>Hambly</term>
<term>High reddening</term>
<term>High resolution</term>
<term>Histogram equalization</term>
<term>Image ellipticity</term>
<term>Image grade</term>
<term>Image quality</term>
<term>Imaging</term>
<term>Incident angle</term>
<term>Intensity calibration</term>
<term>Intensity space</term>
<term>Intensity values</term>
<term>Iphas survey</term>
<term>Large numbers</term>
<term>Less correction</term>
<term>Limited areas</term>
<term>Line emission</term>
<term>Linear part</term>
<term>Linear portion</term>
<term>Linear relation</term>
<term>Linear response</term>
<term>Lter</term>
<term>Lter artefacts</term>
<term>Lter bandpass</term>
<term>Lter response</term>
<term>Lter transmission</term>
<term>Macgillivray</term>
<term>Magellanic clouds</term>
<term>Magnitude range</term>
<term>Meaburn</term>
<term>Mechanical deformation</term>
<term>Mnras</term>
<term>Nebula</term>
<term>Normal incidence</term>
<term>Observatory</term>
<term>Online</term>
<term>Original survey</term>
<term>Other surveys</term>
<term>Overlap region</term>
<term>Overlap regions</term>
<term>Parker russeil</term>
<term>Pasa</term>
<term>Phillipps</term>
<term>Phillipps parker</term>
<term>Photographic data</term>
<term>Photographic material</term>
<term>Photometric</term>
<term>Photometry</term>
<term>Pixel</term>
<term>Pixel data</term>
<term>Pixel value</term>
<term>Planetary nebula</term>
<term>Planetary nebulae</term>
<term>Point sources</term>
<term>Powerful tool</term>
<term>Rayleigh</term>
<term>Rayleigh value</term>
<term>Region centred</term>
<term>Residual</term>
<term>Response curves</term>
<term>Royal observatory edinburgh</term>
<term>Russeil</term>
<term>Same area</term>
<term>Same region</term>
<term>Schmidt</term>
<term>Schmidt telescope</term>
<term>Several areas</term>
<term>Shassa</term>
<term>Shassa data</term>
<term>Shassa images</term>
<term>Shassa intensity calibration</term>
<term>Shassa pixels</term>
<term>Shassa values</term>
<term>Show evidence</term>
<term>Similar depth</term>
<term>Spatial resolution</term>
<term>Spurious</term>
<term>Spurious images</term>
<term>Standard ukst survey data</term>
<term>Star formation</term>
<term>Stellar</term>
<term>Stellar evolution</term>
<term>Stellar locus</term>
<term>Stellar photometry</term>
<term>Supercosmos</term>
<term>Supercosmos counts</term>
<term>Supercosmos data</term>
<term>Supercosmos intensity counts</term>
<term>Supercosmos scans</term>
<term>Supernova remnants</term>
<term>Surface brightness</term>
<term>Survey</term>
<term>Survey atlas</term>
<term>Survey data</term>
<term>Survey data products</term>
<term>Survey figure</term>
<term>Survey pairs</term>
<term>Telescope</term>
<term>Telescope beam</term>
<term>Ucac catalogue</term>
<term>Ukst</term>
<term>Ukst beam</term>
<term>Uncancelled stars</term>
<term>Vertical scatter</term>
<term>Wham</term>
<term>Whole survey</term>
<term>Wide range</term>
</keywords>
<keywords scheme="Wicri" type="topic" xml:lang="fr"><term>Atlas</term>
</keywords>
</textClass>
</profileDesc>
</teiHeader>
<front><div type="abstract" xml:lang="en">The UK Schmidt Telescope (UKST) of the Anglo‐Australian Observatory completed a narrow‐band Hα plus [N ii] 6548, 6584‐Å survey of the Southern Galactic Plane and Magellanic Clouds in late 2003. The survey, which was the last UKST wide‐field photographic survey and the only one undertaken in a narrow‐band, is now an online digital data product of the Wide‐Field Astronomy Unit of the Royal Observatory Edinburgh (ROE). The survey utilized a high specification, monolithic Hα interference bandpass filter of exceptional quality. In conjunction with the fine‐grained Tech‐Pan film as a detector it has produced a survey with a powerful combination of area coverage (4000 square degrees), resolution (∼1 arcsec) and sensitivity (≤5 Rayleighs), reaching a depth for continuum point sources of R≃ 20.5. The main survey consists of 233 individual fields on a grid of centres separated by 4° at declinations below +2° and covers a swathe approximately 20° wide about the Southern Galactic Plane. The original survey films were scanned by the SuperCOSMOS measuring machine at the Royal Observatory, Edinburgh, to provide the online digital atlas called the SuperCOSMOS Hα Survey (SHS). We present the background of the survey, the key survey characteristics, details and examples of the data product, calibration process, comparison with other surveys and a brief description of its potential for scientific exploitation.</div>
</front>
</TEI>
<affiliations><list><country><li>Australie</li>
<li>France</li>
<li>Royaume-Uni</li>
<li>États-Unis</li>
</country>
<region><li>Angleterre</li>
<li>Californie</li>
<li>Grand Londres</li>
<li>Nouvelle-Galles du Sud</li>
<li>Écosse</li>
</region>
<settlement><li>Berkeley (Californie)</li>
<li>Londres</li>
<li>Sydney</li>
<li>Édimbourg</li>
</settlement>
</list>
<tree><noCountry><name sortKey="Masheder, M R W" sort="Masheder, M R W" uniqKey="Masheder M" first="M. R. W." last="Masheder">M. R. W. Masheder</name>
<name sortKey="Morris, R A H" sort="Morris, R A H" uniqKey="Morris R" first="R. A. H." last="Morris">R. A. H. Morris</name>
<name sortKey="Phillipps, S" sort="Phillipps, S" uniqKey="Phillipps S" first="S." last="Phillipps">S. Phillipps</name>
<name sortKey="Pierce, M J" sort="Pierce, M J" uniqKey="Pierce M" first="M. J." last="Pierce">M. J. Pierce</name>
<name sortKey="Walker, R N F" sort="Walker, R N F" uniqKey="Walker R" first="R. N. F." last="Walker">R. N. F. Walker</name>
</noCountry>
<country name="Australie"><region name="Nouvelle-Galles du Sud"><name sortKey="Parker, Quentin A" sort="Parker, Quentin A" uniqKey="Parker Q" first="Quentin A." last="Parker">Quentin A. Parker</name>
</region>
<name sortKey="Cannon, R D" sort="Cannon, R D" uniqKey="Cannon R" first="R. D." last="Cannon">R. D. Cannon</name>
<name sortKey="Cass, C P" sort="Cass, C P" uniqKey="Cass C" first="C. P." last="Cass">C. P. Cass</name>
<name sortKey="Frew, D J" sort="Frew, D J" uniqKey="Frew D" first="D. J." last="Frew">D. J. Frew</name>
<name sortKey="Hartley, M" sort="Hartley, M" uniqKey="Hartley M" first="M." last="Hartley">M. Hartley</name>
<name sortKey="Mader, S" sort="Mader, S" uniqKey="Mader S" first="S." last="Mader">S. Mader</name>
<name sortKey="Malin, D F" sort="Malin, D F" uniqKey="Malin D" first="D. F." last="Malin">D. F. Malin</name>
<name sortKey="Parker, Quentin A" sort="Parker, Quentin A" uniqKey="Parker Q" first="Quentin A." last="Parker">Quentin A. Parker</name>
<name sortKey="Parker, Quentin A" sort="Parker, Quentin A" uniqKey="Parker Q" first="Quentin A." last="Parker">Quentin A. Parker</name>
<name sortKey="Russell, K S" sort="Russell, K S" uniqKey="Russell K" first="K. S." last="Russell">K. S. Russell</name>
</country>
<country name="Royaume-Uni"><region name="Écosse"><name sortKey="Hambly, N C" sort="Hambly, N C" uniqKey="Hambly N" first="N. C." last="Hambly">N. C. Hambly</name>
</region>
<name sortKey="Drew, J E" sort="Drew, J E" uniqKey="Drew J" first="J. E." last="Drew">J. E. Drew</name>
<name sortKey="Hopewell, E" sort="Hopewell, E" uniqKey="Hopewell E" first="E." last="Hopewell">E. Hopewell</name>
<name sortKey="Macgillivray, H T" sort="Macgillivray, H T" uniqKey="Macgillivray H" first="H. T." last="Macgillivray">H. T. Macgillivray</name>
<name sortKey="Morgan, D H" sort="Morgan, D H" uniqKey="Morgan D" first="D. H." last="Morgan">D. H. Morgan</name>
<name sortKey="Read, M A" sort="Read, M A" uniqKey="Read M" first="M. A." last="Read">M. A. Read</name>
<name sortKey="Tritton, S B" sort="Tritton, S B" uniqKey="Tritton S" first="S. B." last="Tritton">S. B. Tritton</name>
</country>
<country name="États-Unis"><region name="Californie"><name sortKey="Cohen, M" sort="Cohen, M" uniqKey="Cohen M" first="M." last="Cohen">M. Cohen</name>
</region>
</country>
<country name="France"><noRegion><name sortKey="Russeil, D" sort="Russeil, D" uniqKey="Russeil D" first="D." last="Russeil">D. Russeil</name>
</noRegion>
</country>
</tree>
</affiliations>
</record>
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