May 2005 – My WordPress Site

Absorption lines detected toward NRAO 150. The left panel shows previous detections including the o-H2CO (11,0 − 11,1) line at 4.8 GHz and the o-c-C3H2 (11,0 − 10,1) line at 18 GHz observed at the VLA (Liszt & Lucas 1995; Liszt et al. 2012) , and the CS (2-1) (98 GHz), o-c-C3H2 (21,2 − 10,1)(85.3 GHz), CCH(1, 3/2, 2 − 0, 1/2, 1) (87.3 GHz), and HCO+ (1 − 0) (89.2 GHz) lines (Lucas & Liszt 1994; Liszt & Lucas 1995; Lucas & Liszt 1996b, 2000, 2002) observed with the PdBI. The right panel presents the new observations including the o-H2CO(21,1 − 10,2) , o-H213CO(21,1 − 10,2), and p-H2CO (20,2 − 10,1) lines, the CS(3-2), C34S(3-2) lines, and the c-C3H2 transitions listed in Table 2. All displayed spectra have been normalized by the continuum strength. Vertical offsets have been used for clarity. -- astro-ph.GA

Astrobiology (general), Conferences and Meetings, NASA Astrobiology Program

UCLA Conference Brings Together World-Renowned Scientists to Address ‘Astrobiology: Life Among the Stars’

by Keith CowingMay 11, 2005June 23, 2024

A UCLA symposium on Friday, May 13, will feature internationally renowned scientists addressing “Astrobiology: Life Among the Stars.”

Concentrations are shown in µg/kg. Black circles represent seawater sampling locations; red stars denote the shoreline position of microbialite sampling transects (coordinates listed in Supplementary Table 3). Black lines represent boundaries of provinces in Hamelin Pool as previously defined32. The map is overlaid on Copernicus Sentinel data (2025) accessed via Copernicus Browser (CC BY 4.0). -- Nature Communications

Astrobiology (general), Conferences and Meetings, NASA Astrobiology Program

The 2005 General Meeting of the NASA Astrobiology Institute

by Keith CowingMay 5, 2005June 23, 2024