Align histidine permease (characterized)
to candidate N515DRAFT_2630 N515DRAFT_2630 amino acid/polyamine/organocation transporter, APC superfamily
Query= reanno::pseudo3_N2E3:AO353_12275 (468 letters) >FitnessBrowser__Dyella79:N515DRAFT_2630 Length = 454 Score = 511 bits (1317), Expect = e-149 Identities = 241/443 (54%), Positives = 330/443 (74%), Gaps = 1/443 (0%) Query: 6 NGLKRGLSARHIRFMALGSAIGTGLFYGSASAIQMAGPAVLLAYLIGGAAVFMVMRALGE 65 + L+RGL RHIR MALGSAIG GLF GSA+AI++AGPA+LL+YL+GG A+F++MRALGE Sbjct: 5 DSLQRGLQERHIRLMALGSAIGVGLFLGSANAIRLAGPAILLSYLLGGVAIFIIMRALGE 64 Query: 66 MAVHNPVAGSFGQYASTYLGPMAGFILGWTYAFEMVIVGMADVTAFGIYMGFWFPEVSRW 125 MAV NPVAGSF +YA YLGP+ G++ GW Y F ++ +A++TA G+YMG WFP+V +W Sbjct: 65 MAVQNPVAGSFSRYAQDYLGPLPGYLTGWNYWFMWLMTCIAEITAVGVYMGVWFPDVPQW 124 Query: 126 IWVLGVVSIVGGLNLCNVKVFGEMEFWLSLLKVAAIVAMILGGFGIMLFGISTAPGQVTD 185 IW L + +G +NL VK +GE EFW +++KV IV MI+GG +++FG+ G T Sbjct: 125 IWALAALVTMGAVNLAAVKAYGEFEFWFAMIKVVTIVLMIVGGGAMIVFGLGNQ-GVPTG 183 Query: 186 ISNLWTQGGFMPNGMGGLIASFAVVMFAFGGIEIIGVTAGEAKDPQHVLPRAINAVPLRI 245 ISNLWT GGFMPNG G++ + +VMFA+ G+E+IG+TAGEA +P+ +P AIN+V RI Sbjct: 184 ISNLWTHGGFMPNGAKGMLMALQMVMFAYLGVEMIGLTAGEADNPKKSIPDAINSVFWRI 243 Query: 246 LLFYVLTMLVLMSIFPWQQIGSQGSPFVQIFDKLGISSAATILNIVVITAAISAINSDIF 305 L+FYV + V+MSI+PW ++G+ GSPFV F++LGI SAA I+N VV+TAA+S+ N I+ Sbjct: 244 LIFYVGALFVIMSIYPWNELGTHGSPFVMTFERLGIKSAAGIINFVVLTAALSSCNGGIY 303 Query: 306 GAGRMMFGLAQQGHAPKGFAHLSRNGVPWMTVVVMSVALLLGVLLNYLIPENVFLLIASI 365 GRM+F LAQQG AP+ FA S +G+P V+V VALL GVLLNYL+P VF+ + S Sbjct: 304 STGRMLFNLAQQGQAPRTFAVTSPSGIPNRAVLVSLVALLFGVLLNYLVPAKVFVWVTSA 363 Query: 366 ATFATVWVWLMILFTQVAMRRSMTAEQVAQLKFPVPFWPYAPMAAIAFMLFVFGVLGYFP 425 ATF +W W ++L TQ+ RR ++ Q +QL F +PF+PYA A+AF++ V G++GYFP Sbjct: 364 ATFGAIWTWGIVLITQMKYRRGLSEAQRSQLVFRMPFFPYASYLALAFLVLVVGLMGYFP 423 Query: 426 DTQAALIVGVVWIVLLVLAYLMW 448 DT+ ALIVG +W+VLL + Y ++ Sbjct: 424 DTRVALIVGPLWLVLLTVLYYVF 446 Lambda K H 0.329 0.142 0.441 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: 737 Number of extensions: 38 Number of successful extensions: 2 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: 468 Length of database: 454 Length adjustment: 33 Effective length of query: 435 Effective length of database: 421 Effective search space: 183135 Effective search space used: 183135 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 (21.8 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