PESSTO Working AreasWithin the PESSTO community we can roughly differentiate between three key working areas. I. all_@_pesstoThis is the working area for all top level pessto communication e.g. meetings, general telecons, policies etc. The whole of the pessto community can be reached by emailing all_@_pessto.org.II. Operation GroupsWithin the community there are currently 6 operation groups (listed below). For more details please see the operations homepage on this wiki.Operation group title: Group Leader (Affiliation), mailinglist@pessto.org Science Board: Mark Sullivan [Chair] (Southampton), scienceboard_@_pessto.org Observations: Mark Sullivan (Southampton), observers_@_pessto.org Targets and Alerts: Andrea Pastorello (Pastorello), alerts_@_pessto.org Data Reduction & Quality Control: Stefano Valenti (Padova), datareduction_@_pessto.org Archive: Ofer Yaron (Weizmann), archive_@_pessto.org General Operations: Stephen Smartt (QUB) III. ScienceThere are also current 15 key science groups (listed below). For more details please see the individual group pages on this wiki (linked below) or the science groups homepage.Science group title: Lead Scientist (Affiliation)
PESSTO CommunicationsA place for everything and everything in its place:There are currently 4 online resources available to the pessto community for communication and collaboration. Each of the resources serves a specific purpose, so please read the following to ensure that all pessto related information is posted to the correct place. I. Wiki
II. pessto.org
III. Google Drive
IV. Group Mailing ListsThere are various mailing lists for specific groups within the pessto community. These are to be used for quick communication and alerting key people to new info posted to the wiki or google docs.All Members
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Subpages (14):
Blue transients
Extincted/reddened SNe
Faint, (fast) and non‐interacting
Normal SNe Ia
Optical Spectropolarimetry of PESSTO bright targets
Over‐luminous SNe Ic
Remote thermonuclear SNe Ia
Statistical analysis of PESSTO classifications
Sub‐luminous SNe Ia 91bg‐like
Super‐Chandrasekhar SNe Ia
Supernovae with identified progenitors
The extremes of interacting core collapse supernovae
Type Ib/c SNe: normal, broad‐lined and GRB‐related events
Weak IIP
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