The main goal of SUCANES has been to compile all the data available for identified pre- and proto-BD
candidates. Data gathering has been done using literature, public DBs (VizieR) and catalogues. We
have included all objects already classified as pre- and proto-BDs candidates. In addition, we have
also considered unclassified VeLLOs as suitable pre- or proto-BD candidates. All objects included have been classified as Class 0 or Class I in published works.
SUCANES Data Base contains continuum photometry covering from optical to cm range (Optical, NIR,
Spitzer, Herschel, sub-mm and cm). It also contains derived physical parameters: Internal luminosity (Lint),
bolometric luminosity (Lbol), bolometric temperature (Tbol), dust mass (Mdust) and total mass (Mtotal). Finally, we provide limited information about molecular gas detections and
presence of molecular
outflows (detected/non-detected), and some of the derived properties (e.g. momentum rate or mass-
loss rate).
The team
Ana María Pérez García (CAB/INTA-CSIC): Science & Data processing lead
Almudena García López (ISDEFE): Software engineer
Nuria Huélamo (CAB/INTA-CSIC): Project Scientist
Ricardo Pérez Martínez (ISDEFE): Scientist
Eva Verdugo (ESA/ESAC): ESA Technical Officer
Scientific advisors:
Itziar de Gregorio Monsalvo, Oscar Morata, Aína Palau
Image credits & copyrigth:
Susana Cabañero Rodríguez, Carlos Valcárcel
If you use the SUCANES DB for your work, an acknowledgment as described below would be appreciated:
This work has made use of the SUCANES database, a joint project funded by ESA Faculty under contract No. 4000129603/19/ES/CM, ISDEFE and CSIC.