A Gram-stain-negative, strictly anaerobic, non-motile, rod-shaped bacterium, designated SFB93T, was isolated from the intertidal sediments of South San Francisco Bay, located near Palo Alto, CA, USA. SFB93Twas capable of acetylenotrophic and diazotrophic growth, grew at 22–37 °C, pH 6.3–8.5 and in the presence of 10–45 g l−1NaCl. Phylogenetic analyses based on 16S rRNA gene sequencing showed that SFB93Trepresented a member of the genusSyntrophotaleawith highest 16S rRNA gene sequence similarities toSyntrophotalea acetylenicaDSM 3246T(96.6 %),Syntrophotalea carbinolicaDSM 2380T(96.5 %), andSyntrophotalea venetianaDSM 2394T(96.7 %). Genome sequencing revealed a genome size of 3.22 Mbp and a DNA G+C content of 53.4 %. SFB93Thad low genome-wide average nucleotide identity (81–87.5 %) and <70 % digital DNA–DNA hybridization value with other members of the genusSyntrophotalea. The phylogenetic position of SFB93Twithin the familySyntrophotaleaceaeand as a novel member of the genusSyntrophotaleawas confirmed via phylogenetic reconstruction based on concatenated alignments of 92 bacterial core genes. On the basis of the results of phenotypic, genotypic and phylogenetic analyses, a novel species,Syntrophotalea acetylenivoranssp. nov., is proposed, with SFB93T(=DSM 106009T=JCM 33327T=ATCC TSD-118T) as the type strain. 
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                            Mapping the Milky Way in 5D with 170 Million Stars
                        
                    
    
            Abstract We presentAugustus, a catalog of distance, extinction, and stellar parameter estimates for 170 million stars from 14 mag <r< 20 mag and with ∣b∣ > 10° drawing on a combination of optical to near-infrared photometry from Pan-STARRS, 2MASS, UKIDSS, and unWISE along with parallax measurements from Gaia DR2 and 3D dust extinction maps. After applying quality cuts, we find 125 million objects have “high-quality” posteriors with statistical distance uncertainties of ≲10% for objects with well-constrained stellar types. This is a substantial improvement over the distance estimates derived from Gaia parallaxes alone and in line with the recent results from Anders et al. We find the fits are able to reproduce the dereddened Gaia color–magnitude diagram accurately, which serves as a useful consistency check of our results. We show that we are able to detect large, kinematically coherent substructures in our data clearly relative to the input priors, including the Monoceros Ring and the Sagittarius Stream, attesting to the quality of the catalog. Our results are publicly available at doi:10.7910/DVN/WYMSXV. An accompanying interactive visualization can be found athttp://allsky.s3-website.us-east-2.amazonaws.com. 
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                            - Award ID(s):
- 2406729
- PAR ID:
- 10612806
- Author(s) / Creator(s):
- ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; more »
- Publisher / Repository:
- The Astrophysical Journal
- Date Published:
- Journal Name:
- The Astrophysical Journal
- Volume:
- 970
- Issue:
- 2
- ISSN:
- 0004-637X
- Page Range / eLocation ID:
- 121
- Format(s):
- Medium: X
- Sponsoring Org:
- National Science Foundation
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