The DOI matches its Crossref record; 71 of the 71 references it cites were found in a registry or an index.
The VIMOS VLT Deep Survey final data release: a spectroscopic sample of 35 016 galaxies and AGN out to z~ 6.7 selected with 17.5 ≤iAB ≤ 24.75
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Context. Deep representative surveys of galaxies at different epochs are needed to make progress in understanding galaxy evolution.
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Cites
SExtractor: Software for source extraction
Bertin, E., & Arnouts, S. (1996) · Astronomy and Astrophysics Supplement Series · doi:10.1051/aas:1996164 · Cited by 10,866
Self-citationThe Sloan Digital Sky Survey: Technical Summary
York, D. G., Adelman, J., Anderson, Jr., Anderson, S. F., Annis, J., Bahcall, N. A., Bakken, J. A., Barkhouser, R., Bastian, S., Berman, E., et al. (2000) · The Astronomical Journal · doi:10.1086/301513 · Cited by 10,366
THE SEVENTH DATA RELEASE OF THE SLOAN DIGITAL SKY SURVEY
Abazajian, K. N., Adelman-McCarthy, J. K., Agüeros, M. A., Allam, S. S., Prieto, C. A., An, D., Anderson, K. S. J., Anderson, S. F., Annis, J., Bahcall, N. A., et al. (2009) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/182/2/543 · Cited by 5,341
Eisenstein, D. J., Zehavi, I., Hogg, D. W., Scoccimarro, R., Blanton, M. R., Nichol, R. C., Scranton, R., Seo, H., Tegmark, M., Zheng, Z., et al. (2005) · The Astrophysical Journal · doi:10.1086/466512 · Cited by 4,629
Eisenstein, D. J., Zehavi, I., Hogg, D. W., Scoccimarro, R., Blanton, M. R., Nichol, R. C., Scranton, R., Seo, H., Tegmark, M., Zheng, Z., et al. (2005) · Cited by 2,568
The UKIRT Infrared Deep Sky Survey (UKIDSS)
Lawrence, A., Warren, S. J., Almaini, O., Edge, A. C., Hambly, N. C., Jameson, R. F., Lucas, P., Casali, M., Adamson, A., Dye, S., et al. (2007) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2007.12040.x · Cited by 2,441
Self-citationThe 2dF Galaxy Redshift Survey: spectra and redshifts
Colless, M., Dalton, G., Maddox, S., Sutherland, W., Norberg, P., Cole, S., Bland-Hawthorn, J., Bridges, T., Cannon, R., Collins, C., et al. (2001) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2001.04902.x · Cited by 2,367
High-redshift galaxies in the Hubble Deep Field: colour selection and star formation history to z 4
Madau, P., Ferguson, H. C., Dickinson, M. E., Giavalisco, M., Steidel, C. C., & Fruchter, A. (1996) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/283.4.1388 · Cited by 2,055
The Cosmic Evolution Survey (COSMOS): Overview
Scoville, N., Aussel, H., Brusa, M., Capak, P., Carollo, C. M., Elvis, M., Giavalisco, M., Guzzo, L., Hasinger, G., Impey, C., et al. (2007) · The Astrophysical Journal Supplement Series · doi:10.1086/516585 · Cited by 2,007
Self-citationAccurate photometric redshifts for the CFHT legacy survey calibrated using the VIMOS VLT deep survey
Ilbert, O., Arnouts, S., McCracken, H. J., Bolzonella, M., Bertin, E., Le Fèvre, O., Mellier, Y., Zamorani, G., Pellò, R., Iovino, A., et al. (2006) · Astronomy & Astrophysics · doi:10.1051/0004-6361:20065138 · Cited by 1,683
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Dark Energy Survey Year 3 results: Cosmological constraints from galaxy clustering and weak lensing
Abbott, T. M. C., Aguena, M., Alarcon, A., Allam, S., Alves, O., Amon, A., Andrade-Oliveira, F., Annis, J., Avila, S., Bacon, D., et al. (2022) · Physical Review D · doi:10.1103/physrevd.105.023520 · Cited by 1,124
The Hyper Suprime-Cam SSP Survey: Overview and survey design
Aihara, H., Arimoto, N., Armstrong, R., Arnouts, S., Bahcall, N. A., Bickerton, S., Bosch, J., Bundy, K., Capak, P. L., Chan, J. H. H., et al. (2018) · Publications of the Astronomical Society of Japan · doi:10.1093/pasj/psx066 · Cited by 1,087
Self-citationEuclid: I. Overview of the Euclid mission
Euclid Collaboration, Mellier, Y., Abdurro’uf, Acevedo Barroso, J. A., Achúcarro, A., Adamek, J., Adam, R., Addison, G. E., Aghanim, N., Aguena, M., et al. (2025) · Astronomy & Astrophysics · doi:10.1051/0004-6361/202450810 · Cited by 616
Self-citationSecond data release of the Hyper Suprime-Cam Subaru Strategic Program
Aihara, H., AlSayyad, Y., Ando, M., Armstrong, R., Bosch, J., Egami, E., Furusawa, H., Furusawa, J., Goulding, A., Harikane, Y., et al. (2019) · Publications of the Astronomical Society of Japan · doi:10.1093/pasj/psz103 · Cited by 511
Dark Energy Survey Year 3 results: Cosmology from cosmic shear and robustness to data calibration
Amon, A., Gruen, D., Troxel, M. A., MacCrann, N., Dodelson, S., Choi, A., Doux, C., Secco, L. F., Samuroff, S., Krause, E., et al. (2022) · Physical Review D · doi:10.1103/physrevd.105.023514 · Cited by 437
Metadata
- Authors
- Le Fèvre, O., Cassata, P., Cucciati, O., Garilli, B., Ilbert, O., Le Brun, V., Maccagni, D., Moreau, C., Scodeggio, M., Tresse, L., Zamorani, G., Adami, C., Arnouts, S., Bardelli, S., Bolzonella, M., Bondi, M., Bongiorno, A., Bottini, D., Cappi, A., Charlot, S., Ciliegi, P., Contini, T., de la Torre, S., Foucaud, S., Franzetti, P., Gavignaud, I., Guzzo, L., Iovino, A., Lemaux, B., López-Sanjuan, C., McCracken, H. J., Marano, B., Marinoni, C., Mazure†, A., Mellier, Y., Merighi, R., Merluzzi, P., Paltani, S., Pellò, R., Pollo, A., Pozzetti, L., Scaramella, R., Tasca, L., Vergani, D., Vettolani, G., Zanichelli, A., & Zucca, E.
- Venue
- Astronomy & Astrophysics
- Publisher
- EDP Sciences
- Published
- 2013-10-29
- Volume
- 559
- Pages
- A14
- ISSN
- 0004-6361 (ISSN-L)
- 1432-0746
- OpenAlex
- W1993283828
- Cited by
- 408
- References
- 71
- FWCI
- 16.59
- Type
- journal article
- Language
- en
- Open access
- hybrid
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- CoChat. (2026). Citation check: The VIMOS VLT Deep Survey final data release: a spectroscopic sample of 35 016 galaxies and AGN out to z~ 6.7 selected with 17.5 ≤iAB ≤ 24.75. https://app.cochat.ai/papers/10.1051/0004-6361/201322179
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- Le Fèvre, O., Cassata, P., Cucciati, O., Garilli, B., Ilbert, O., Le Brun, V., Maccagni, D., Moreau, C., Scodeggio, M., Tresse, L., Zamorani, G., Adami, C., Arnouts, S., Bardelli, S., Bolzonella, M., Bondi, M., Bongiorno, A., Bottini, D., Cappi, A., . . . Zucca, E. (2013). The VIMOS VLT Deep Survey final data release: a spectroscopic sample of 35 016 galaxies and AGN out to z~ 6.7 selected with 17.5 ≤iAB ≤ 24.75. Astronomy & Astrophysics. https://doi.org/10.1051/0004-6361/201322179
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