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Cited article:

HIghMass-HIGH H I MASS, H I-RICH GALAXIES ATz∼ 0 SAMPLE DEFINITION, OPTICAL AND Hα IMAGING, AND STAR FORMATION PROPERTIES

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The Astrophysical Journal 793 (1) 40 (2014)
https://doi.org/10.1088/0004-637X/793/1/40

On the origin of the faint-end of the red sequence in high-density environments

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The Astronomy and Astrophysics Review 22 (1) (2014)
https://doi.org/10.1007/s00159-014-0074-y

The applicability of far-infrared fine-structure lines as star formation rate tracers over wide ranges of metallicities and galaxy types

Ilse De Looze, Diane Cormier, Vianney Lebouteiller, et al.
Astronomy & Astrophysics 568 A62 (2014)
https://doi.org/10.1051/0004-6361/201322489

The bivariateK-band-submillimetre luminosity functions of the local HRS galaxy sample

P. Andreani, L. Spinoglio, A. Boselli, et al.
Astronomy & Astrophysics 566 A70 (2014)
https://doi.org/10.1051/0004-6361/201322747

COMPARING Hα AND H I SURVEYS AS MEANS TO A COMPLETE LOCAL GALAXY CATALOG IN THE ADVANCED LIGO/VIRGO ERA

Brian D. Metzger, David L. Kaplan and Edo Berger
The Astrophysical Journal 764 (2) 149 (2013)
https://doi.org/10.1088/0004-637X/764/2/149

The Herschel Virgo Cluster Survey – XIV. Transition-type dwarf galaxies in the Virgo cluster

Ilse De Looze, Maarten Baes, Alessandro Boselli, et al.
Monthly Notices of the Royal Astronomical Society 436 (2) 1057 (2013)
https://doi.org/10.1093/mnras/stt1626

The GALEX Arecibo SDSS Survey – VIII. Final data release. The effect of group environment on the gas content of massive galaxies

Barbara Catinella, David Schiminovich, Luca Cortese, et al.
Monthly Notices of the Royal Astronomical Society 436 (1) 34 (2013)
https://doi.org/10.1093/mnras/stt1417

Towards understanding the relation between the gas and the attenuation in galaxies at kpc scales

M. Boquien, A. Boselli, V. Buat, et al.
Astronomy & Astrophysics 554 A14 (2013)
https://doi.org/10.1051/0004-6361/201220768

Galactic star formation enhanced and quenched by ram pressure in groups and clusters

Kenji Bekki
Monthly Notices of the Royal Astronomical Society 438 (1) 444 (2013)
https://doi.org/10.1093/mnras/stt2216