GapMind for catabolism of small carbon sources

 

Aligments for a candidate for mglC in Acidovorax sp. GW101-3H11

Align MglC aka B2148, component of Galactose/glucose (methyl galactoside) porter (characterized)
to candidate Ac3H11_2880 Ribose ABC transport system, permease protein RbsC (TC 3.A.1.2.1)

Query= TCDB::P23200
         (336 letters)



>FitnessBrowser__acidovorax_3H11:Ac3H11_2880
          Length = 350

 Score =  134 bits (338), Expect = 3e-36
 Identities = 96/308 (31%), Positives = 161/308 (52%), Gaps = 16/308 (5%)

Query: 20  VVLLVLLAII-IFQDPTFLSLLNLSNILTQSSVRIIIALGVAGLIVTQGTDLSAGRQVGL 78
           V+ LVLL I     +  F +  N+ N+LT+++   IIA+G+  +I++ G DLS G    +
Sbjct: 44  VIGLVLLCIAGTLLNSNFATYDNVMNVLTRTAFIGIIAVGMCFVIISGGIDLSVG---SM 100

Query: 79  AAVVAATLLQSMDNANKVFPEMATMPIALVI--LIVCAIGAVIGLINGLIIAYLNVTPFI 136
           AA++A +++  M   N + P + +   A+V+  L+   +GAV GL++GL+I    + PFI
Sbjct: 101 AALIAGSVILFM---NAMAPVLGSPMAAVVVGMLLAVVLGAVFGLVHGLLITKGRIEPFI 157

Query: 137 TTLGTMIIVYGINSLYYDFVGASPISGFDSGFSTFAQGFVALGSFRLSYITFYALIAVAF 196
            TLGT+    GI   Y  +         ++  S             +    +  L+    
Sbjct: 158 VTLGTL----GIFRAYLTYFSNGGAITLENDLSDIYSPVYYANLLGVPIPVWIFLLVAIV 213

Query: 197 VWVLWNKTRFGKNIFAIGGNPEAAKVSGVNVGLNLLMIYALSGVFYAFGGMLEAGRIGSA 256
             V+ N+T +G+ + AIG N + A+ + V+V    ++ Y L GV      +L   R+GSA
Sbjct: 214 GGVILNRTAYGRYVQAIGSNEQVAQYAAVDVHKIKILTYMLLGVCVGIATLLYVPRLGSA 273

Query: 257 TNNLGFMYELDAIAACVVGGVSFSGGVGTVIGVVTGVIIFTVIN--YGLTYIGVNPYWQY 314
           +   G ++EL+AIAA +VGG    GG G++ G V G I+ +VI+    LT I ++ Y   
Sbjct: 274 SPTTGLLWELEAIAAVIVGGTVLKGGAGSITGTVVGAILLSVISNILNLTSI-ISVYLNA 332

Query: 315 IIKGAIII 322
            ++G +II
Sbjct: 333 AVQGFVII 340


Lambda     K      H
   0.327    0.143    0.415 

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: 306
Number of extensions: 20
Number of successful extensions: 3
Number of sequences better than 1.0e-02: 1
Number of HSP's gapped: 2
Number of HSP's successfully gapped: 1
Length of query: 336
Length of database: 350
Length adjustment: 29
Effective length of query: 307
Effective length of database: 321
Effective search space:    98547
Effective search space used:    98547
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: 49 (23.5 bits)

This GapMind analysis is from Sep 17 2021. The underlying query database was built on Sep 17 2021.

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About GapMind

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:

where "other" refers to the best ublast hit to a sequence that is not annotated as performing this step (and is not "ignored").

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