Align D-galacturonate transporter (MFS superfamily) (characterized)
to candidate PP_3600 PP_3600 glucarate transporter
Query= reanno::WCS417:GFF828 (454 letters) >FitnessBrowser__Putida:PP_3600 Length = 454 Score = 754 bits (1946), Expect = 0.0 Identities = 368/451 (81%), Positives = 407/451 (90%), Gaps = 12/451 (2%) Query: 1 MQATKPTHVRYLILLMLFLVTTINYADRATIAIAGSSLQKDLGIDAVTLGYIFSAFGWAY 60 MQATK THVRYLIL MLFLVTTINYADRATIAIAGSSLQKDLGIDAVTLGYIFSAFGWAY Sbjct: 1 MQATKKTHVRYLILFMLFLVTTINYADRATIAIAGSSLQKDLGIDAVTLGYIFSAFGWAY 60 Query: 61 VAGQIPGGWLLDRFGSKKVYALSIFTWSLFTVLQGYVGEFGVSTAVVALFMLRFMVGLAE 120 VAGQIPGGWLLDRFGSK VYA SIFTWSLFT+LQG+VG V+ AVV LF LRF+VG AE Sbjct: 61 VAGQIPGGWLLDRFGSKNVYAFSIFTWSLFTLLQGFVGGLPVAWAVVTLFTLRFLVGFAE 120 Query: 121 APSFPGNARIVAAWFPTAERGTASAIFNSAQYFATVLFAPLMGWIVYSFGWQHVFIVMGV 180 APSFPGNARIVAAWFPT ERGTASAIFNSAQYFAT LFAP+MGWIV+SFGW+HVF+VMGV Sbjct: 121 APSFPGNARIVAAWFPTQERGTASAIFNSAQYFATALFAPIMGWIVFSFGWEHVFVVMGV 180 Query: 181 IGIIFSLIWLKVIHSPRQHPMINEAEFNHIAANGAMVDMDQDKGKGKKTDGPKWDYIRQL 240 +GIIFS++WLK I++PRQHP I+++E HI NG +VDMDQ +G +DGPKW YI+QL Sbjct: 181 LGIIFSMVWLKTIYNPRQHPRISQSELEHIEQNGGLVDMDQKRG----SDGPKWGYIKQL 236 Query: 241 LTNRMMLGVYLGQYCINGITYFFLTWFPVYLVQDRGMTILKAGFIASLPAICGFIGGVLG 300 LT+RM+LGVYLGQYCIN ITYFFLTWFPVYLVQ+RGMTILKAGFIASLPA+CGFIGGVLG Sbjct: 237 LTSRMLLGVYLGQYCINAITYFFLTWFPVYLVQERGMTILKAGFIASLPAVCGFIGGVLG 296 Query: 301 GVISDYLLRKGHSLTFARKAPIIGGLLISSSIVACNYVDIEWMVVGFMALAFFGKGVGAL 360 GVISD+LLR+G+SLTF+RK PI+ GLL+S+++V CNYVD EWMVVGFM LAFFGKG+GAL Sbjct: 297 GVISDWLLRRGNSLTFSRKLPIVCGLLLSTTMVFCNYVDAEWMVVGFMTLAFFGKGIGAL 356 Query: 361 GWAVVSDTSPKQIAGLSGGLFNTFGNLASITTPIVIGYIISTTGSFKWALVFVGANALVA 420 GWAVV+DTSPKQIAGLSGGLFNTFGN+ASITTPIVIGYIIS TGSFKWALV+VGANALVA Sbjct: 357 GWAVVADTSPKQIAGLSGGLFNTFGNIASITTPIVIGYIISATGSFKWALVYVGANALVA 416 Query: 421 VFSYLVIVGPIKRVVLK--------EPPTQG 443 VFSYLVIVGPIKR+ L+ EP T G Sbjct: 417 VFSYLVIVGPIKRIELRDAAPKPHAEPATDG 447 Lambda K H 0.327 0.142 0.444 Gapped Lambda K H 0.267 0.0410 0.140 Matrix: BLOSUM62 Gap Penalties: Existence: 11, Extension: 1 Number of Sequences: 1 Number of Hits to DB: 915 Number of extensions: 50 Number of successful extensions: 6 Number of sequences better than 1.0e-02: 1 Number of HSP's gapped: 1 Number of HSP's successfully gapped: 1 Length of query: 454 Length of database: 454 Length adjustment: 33 Effective length of query: 421 Effective length of database: 421 Effective search space: 177241 Effective search space used: 177241 Neighboring words threshold: 11 Window for multiple hits: 40 X1: 15 ( 7.1 bits) X2: 38 (14.6 bits) X3: 64 (24.7 bits) S1: 40 (21.7 bits) S2: 51 (24.3 bits)
This GapMind analysis is from Sep 17 2021. The underlying query database was built on Sep 17 2021.
Each pathway is defined by a set of rules based on individual steps or genes. Candidates for each step are identified by using ublast (a fast alternative to protein BLAST) against a database of manually-curated proteins (most of which are experimentally characterized) or by using HMMer with enzyme models (usually from TIGRFam). Ublast hits may be split across two different proteins.
A candidate for a step is "high confidence" if either:
Otherwise, a candidate is "medium confidence" if either:
Other blast hits with at least 50% coverage are "low confidence."
Steps with no high- or medium-confidence candidates may be considered "gaps." For the typical bacterium that can make all 20 amino acids, there are 1-2 gaps in amino acid biosynthesis pathways. For diverse bacteria and archaea that can utilize a carbon source, there is a complete high-confidence catabolic pathway (including a transporter) just 38% of the time, and there is a complete medium-confidence pathway 63% of the time. Gaps may be due to:
GapMind relies on the predicted proteins in the genome and does not search the six-frame translation. In most cases, you can search the six-frame translation by clicking on links to Curated BLAST for each step definition (in the per-step page).
For more information, see the paper from 2019 on GapMind for amino acid biosynthesis, the paper from 2022 on GapMind for carbon sources, or view the source code.
If you notice any errors or omissions in the step descriptions, or any questionable results, please let us know
by Morgan Price, Arkin group, Lawrence Berkeley National Laboratory