A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE)

Boselli, A; Fossati, M.; Ferrarese, L.; Boissier, S; Consolandi, G.; Longobardi, A.; Amram, P.; Balogh, M; Barmby, P.; Boquien, M.; Boulanger, F; Braine, J.; Buat, V.; Burgarella, D.; Combes, F.; Contini, T.; Cortese, L; Côté, P; Côté, S; Cuillandre, J. -C.; Drissen, L.; Epinat, B.; Fumagalli, M; Gallagher, S.; Gavazzi, G; Gomez-Lopez, J.; Gwyn, S.; Harris, W.; Hensler, G.; Koribalski, B.; Marcelin, M.; McConnachie, A.; Miville-Deschênes, M. -A.; Navarro, J.; Patton, D.; Peng, E. W.; Plana, H.; Prantzos, N.; Robert, C.; Roediger, J.; Roehlly, Y.; Russeil, D.; Salome, P.; Sánchez-Janssen, R.; Serra, P; Spekkens, K.; Sun, M; Taylor, J.; Tonnesen, S.; Vollmer, B.; Willis, J.; Wozniak, H.; Burdullis, T.; Devost, D; Mahoney, B; Manset, N.; Petric, A; Prunet, S.; Withington, K.

doi:10.1051/0004-6361/201732407

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A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE) : I. Introduction to the survey★

Author(s): A. Boselli , M. Fossati , L. Ferrarese , S. Boissier , G. Consolandi , A. Longobardi , P. Amram , M. Balogh , P. Barmby , M. Boquien , F. Boulanger , J. Braine , V. Buat , D. Burgarella , F. Combes , T. Contini , L. Cortese , P. Côté , S. Côté , J. C. Cuillandre , L. Drissen , B. Epinat , M. Fumagalli , S. Gallagher , G. Gavazzi , J. Gomez-Lopez , S. Gwyn , W. Harris , G. Hensler , B. Koribalski , M. Marcelin , A. McConnachie , M. A. Miville-Deschenes , J. Navarro , D. Patton , E. W. Peng , H. Plana , N. Prantzos , C. Robert , J. Roediger , Y. Roehlly , D. Russeil , P. Salome , R. Sanchez-Janssen , P. Serra , K. Spekkens , M. Sun , J. Taylor , S. Tonnesen , B. Vollmer , J. Willis , H. Wozniak , T. Burdullis , D. Devost , B. Mahoney , N. Manset , A. Petric , S. Prunet , K. Withington

Publication date (Electronic): June 15 2018

Journal: Astronomy & Astrophysics

Publisher: EDP Sciences

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X-ray emission from clusters of galaxies

Craig L. Sarazin (1986)

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Is Open Access

The Sloan Digital Sky Survey: Technical Summary

D. G. York (2000)

The Sloan Digital Sky Survey (SDSS) will provide the data to support detailed investigations of the distribution of luminous and non- luminous matter in the Universe: a photometrically and astrometrically calibrated digital imaging survey of pi steradians above about Galactic latitude 30 degrees in five broad optical bands to a depth of g' about 23 magnitudes, and a spectroscopic survey of the approximately one million brightest galaxies and 10^5 brightest quasars found in the photometric object catalog produced by the imaging survey. This paper summarizes the observational parameters and data products of the SDSS, and serves as an introduction to extensive technical on-line documentation.