taxonID	type	format	identifier	references	title	description	created	creator	contributor	publisher	audience	source	license	rightsHolder	datasetID
03DF87FDFFBEB4321F88FC32FA35360D.taxon	http://purl.org/dc/dcmitype/StillImage	image/png	https://zenodo.org/record/7663506/files/figure.png	https://doi.org/10.5281/zenodo.7663506	FIGURE 2. Kalanchoe ×sampsonii. A. At flowering maturity plants of this shrubby nothospecies reach a height of about 0.5 m. B. Through heterosis, inflorescences are more branched and have a wider spread than in either of the parents. C. Peduncles are more intensely reddish-infused than in K. ×hankeyi, but less than in K. sexangularis. D. Flowers (corolla tube and corolla lobes) are more intensely yellow than those of either of the parents. E. Flowers, here in lateral view, of K. ×sampsonii (centre) are often intermediate between those of K. longiflora (left, one of the parents of K. ×hankeyi) and K. sexangularis (right), but the corolla tube is more intensely yellow. F. Corolla lobes of K. ×sampsonii (centre) are more intensely yellow than those of K. longiflora (left, one of the parents of K. ×hankeyi) and K. sexangularis (right, the other parent of K. ×hankeyi). G.A White-bellied sunbird, Cinnyris talatala, feeding on the copiously nectariferous flowers of K. ×sampsonii. H. Jason D.S. Sampson (1979–), after whom K. ×sampsonii is named, next to a very large specimen of K. ×estrelae on the Hatfield campus of the University of Pretoria; photograph taken on 10 June 2022. All photographs taken by Gideon F. Smith.	FIGURE 2. Kalanchoe ×sampsonii. A. At flowering maturity plants of this shrubby nothospecies reach a height of about 0.5 m. B. Through heterosis, inflorescences are more branched and have a wider spread than in either of the parents. C. Peduncles are more intensely reddish-infused than in K. ×hankeyi, but less than in K. sexangularis. D. Flowers (corolla tube and corolla lobes) are more intensely yellow than those of either of the parents. E. Flowers, here in lateral view, of K. ×sampsonii (centre) are often intermediate between those of K. longiflora (left, one of the parents of K. ×hankeyi) and K. sexangularis (right), but the corolla tube is more intensely yellow. F. Corolla lobes of K. ×sampsonii (centre) are more intensely yellow than those of K. longiflora (left, one of the parents of K. ×hankeyi) and K. sexangularis (right, the other parent of K. ×hankeyi). G.A White-bellied sunbird, Cinnyris talatala, feeding on the copiously nectariferous flowers of K. ×sampsonii. H. Jason D.S. Sampson (1979–), after whom K. ×sampsonii is named, next to a very large specimen of K. ×estrelae on the Hatfield campus of the University of Pretoria; photograph taken on 10 June 2022. All photographs taken by Gideon F. Smith.	2023-02-21	Smith, Gideon F.		Zenodo	biologists	Smith, Gideon F.			
