The DOI matches its Crossref record; 24 of the 24 references it cites were found in a registry or an index.
The Detection of a Population of Submillimeter-Bright, Strongly Lensed Galaxies
Open accessAbstract
Through a Lens Brightly: Astronomical sources detected in the submillimeter range are generally thought to be distant, dusty galaxies undergoing a vigorous burst of star formation. They can be detected because the dust absorbs the light from stars and reemits it at longer wavelengths. Their properties are still difficult to ascertain, however, because the combination of interference from dust and the low spatial resolution of submillimeter telescopes prevents further study at other wavelengths. Using data from the Herschel Space Telescope, Negrello et al. (p. 800 ) showed that by searching for the brightest sources in a wide enough area in the sky it was possible to detect gravitationally lensed submillimeter galaxies with nearly full efficiency. Gravitational lensing occurs when the light of an astronomical object is deflected by a foreground mass. This phenomenon increases the apparent brightness and angular size of the lensed objects, making it easier to study sources that would be otherwise too faint to probe.
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Cites
Herschel Space Observatory: An ESA facility for far-infrared and submillimetre astronomy
Pilbratt, G. L., Riedinger, J. R., Passvogel, T., Crone, G., Doyle, D., Gageur, U., Heras, A. M., Jewell, C., Metcalfe, L., Ott, S., et al. (2010) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201014759 · Cited by 3,180
The Photodetector Array Camera and Spectrometer (PACS) on the Herschel Space Observatory
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The Herschel-SPIRE instrument and its in-flight performance
Griffin, M. J., Abergel, A., Abreu, A., Ade, P. A. R., André, P., Augueres, J.-L., Babbedge, T., Bae, Y., Baillie, T., Baluteau, J.-P., et al. (2010) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201014519 · Cited by 2,198
Self-citationVelocity dispersions and mass-to-light ratios for elliptical galaxies
Faber, S. M., & Jackson, R. E. (1976) · The Astrophysical Journal · doi:10.1086/154215 · Cited by 1,497
A simple model to interpret the ultraviolet, optical and infrared emission from galaxies
da Cunha, E., Charlot, S., & Elbaz, D. (2008) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2008.13535.x · Cited by 1,234
Self-citationA Deep Submillimeter Survey of Lensing Clusters: A New Window on Galaxy Formation and Evolution
Smail, I., Ivison, R. J., & Blain, A. W. (1997) · The Astrophysical Journal · doi:10.1086/311017 · Cited by 1,180
Self-citationA Redshift Survey of the Submillimeter Galaxy Population
Chapman, S. C., Blain, A. W., Smail, I., & Ivison, R. J. (2005) · The Astrophysical Journal · doi:10.1086/428082 · Cited by 1,163
Self-citationA Redshift Survey of the Submillimeter Galaxy Population
Chapman, S. C., Blain, A. W., Smail, I., & Ivison, R. J. (2004) · CERN Document Server (European Organization for Nuclear Research) · Cited by 746
Self-citationEales, S., Dunne, L., Clements, D., Cooray, A., De Zotti, G., Dye, S., Ivison, R., Jarvis, M., Lagache, G., Maddox, S., et al. (2010) · Publications of the Astronomical Society of the Pacific · doi:10.1086/653086 · Cited by 589
Self-citationKoopmans, L. V. E., Treu, T., Bolton, A. S., Burles, S., & Moustakas, L. A. (2006) · The Astrophysical Journal · doi:10.1086/505696 · Cited by 558
Cited by
Cool Gas in High-Redshift Galaxies
Carilli, C. L., & Walter, F. (2013) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-082812-140953 · Cited by 1,107
Dusty star-forming galaxies at high redshift
Casey, C. M., Narayanan, D., & Cooray, A. (2014) · Physics Reports · doi:10.1016/j.physrep.2014.02.009 · Cited by 800
Self-citationSpace Warps – I. Crowdsourcing the discovery of gravitational lenses
Marshall, P. J., Verma, A., More, A., Davis, C. P., More, S., Kapadia, A., Parrish, M., Snyder, C., Wilcox, J., Baeten, E., et al. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv2009 · Cited by 117
“…use of relatively clean signals such as the presence of emission or absorption features at two distinct redshifts in the same optical spectrum (e.g. Bolton et al. 2004), or the strong “magnification bias” towards detecting strongly-lensed sources in the sub-mm waveband (e.g. Negrello et al. 2010).”
BackgroundSelf-citationWilde, J., Serjeant, S., Bromley, J. M., Dickinson, H., Koopmans, L. V. E., & Metcalf, R. B. (2022) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stac562 · Cited by 31
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Metadata
- Authors
- Negrello, M., Hopwood, R., De Zotti, G., Cooray, A., Verma, A., Bock, J., Frayer, D. T., Gurwell, M. A., Omont, A., Neri, R., Dannerbauer, H., Leeuw, L. L., Barton, E., Cooke, J., Kim, S., da Cunha, E., Rodighiero, G., Cox, P., Bonfield, D. G., Jarvis, M. J., Serjeant, S., Ivison, R. J., Dye, S., Aretxaga, I., Hughes, D. H., Ibar, E., Bertoldi, F., Valtchanov, I., Eales, S., Dunne, L., Driver, S. P., Auld, R., Buttiglione, S., Cava, A., Grady, C. A., Clements, D. L., Dariush, A., Fritz, J., Hill, D., Hornbeck, J. B., Kelvin, L., Lagache, G., Lopez-Caniego, M., Gonzalez-Nuevo, J., Maddox, S., Pascale, E., Pohlen, M., Rigby, E. E., Robotham, A., Simpson, C., Smith, D. J. B., Temi, P., Thompson, M. A., Woodgate, B. E., York, D. G., Aguirre, J. E., Beelen, A., Blain, A., Baker, A. J., Birkinshaw, M., Blundell, R., Bradford, C. M., Burgarella, D., Danese, L., Dunlop, J. S., Fleuren, S., Glenn, J., Harris, A. I., Kamenetzky, J., Lupu, R. E., Maddalena, R. J., Madore, B. F., Maloney, P. R., Matsuhara, H., Michaowski, M. J., Murphy, E. J., Naylor, B. J., Nguyen, H., Popescu, C., Rawlings, S., Rigopoulou, D., Scott, D., Scott, K. S., Seibert, M., Smail, I., Tuffs, R. J., Vieira, J. D., van der Werf, P. P., & Zmuidzinas, J.
- Venue
- Science
- Published
- 2010-11-05
- Volume
- 330
- Issue
- 6005
- Pages
- 800-804
- ISSN
- 0036-8075 (ISSN-L)
- 1095-9203
- OpenAlex
- W2155870677
- Cited by
- 419
- References
- 24
- FWCI
- 18.24
- Type
- journal article
- Language
- en
- Open access
- green
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- Negrello, M., Hopwood, R., De Zotti, G., Cooray, A., Verma, A., Bock, J., Frayer, D. T., Gurwell, M. A., Omont, A., Neri, R., Dannerbauer, H., Leeuw, L. L., Barton, E., Cooke, J., Kim, S., da Cunha, E., Rodighiero, G., Cox, P., Bonfield, D. G., . . . Zmuidzinas, J. (2010). The Detection of a Population of Submillimeter-Bright, Strongly Lensed Galaxies. Science. https://doi.org/10.1126/science.1193420
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