GapMind for catabolism of small carbon sources

 

Aligments for a candidate for aatJ in Pseudomonas fluorescens FW300-N2C3

Align ABC transporter for L-Asparagine and possibly other L-amino acids, periplasmic substrate-binding component (characterized)
to candidate AO356_18230 AO356_18230 ABC transporter

Query= reanno::pseudo13_GW456_L13:PfGW456L13_4770
         (304 letters)



>FitnessBrowser__pseudo5_N2C3_1:AO356_18230
          Length = 304

 Score =  579 bits (1493), Expect = e-170
 Identities = 291/304 (95%), Positives = 298/304 (98%)

Query: 1   MRIVPHILGAAIAAALISTPVFAAELTGTLKKIKESGTITLGHRDASIPFSYIADASGKP 60
           MRIVPH+LGAAIAAALISTPVFAAELTGTLKKIKESG ITLGHRDASIPFSYIADASGKP
Sbjct: 1   MRIVPHLLGAAIAAALISTPVFAAELTGTLKKIKESGVITLGHRDASIPFSYIADASGKP 60

Query: 61  VGYSHDIQLKVVEALKKDLDMPNLQVKYNLVTSQTRIPLVQNGTVDLECGSTTNNVERQQ 120
           VGYSHDIQLKVVEA+KKDLD+PNLQVKYNLVTSQTRIPLVQNGTVDLECGSTTNNVERQQ
Sbjct: 61  VGYSHDIQLKVVEAIKKDLDLPNLQVKYNLVTSQTRIPLVQNGTVDLECGSTTNNVERQQ 120

Query: 121 QVDFSVGIFEIGTRLLSKADSKYKDFPDLAGKNVVTTAGTTSERILKAMNADKQMGMNVI 180
           QVDFSVGIFEIGTRLL+K DSKYKDF DL GKNVVTTAGTTSER+LK+MNADKQMGMNVI
Sbjct: 121 QVDFSVGIFEIGTRLLTKKDSKYKDFDDLKGKNVVTTAGTTSERLLKSMNADKQMGMNVI 180

Query: 181 SAKDHGESFQMLETGRAVAFMMDDALLAGEAAKAKKASDWAVTGTPQSYEIYGCMVRKGD 240
           SAKDHGESFQMLE GRAVAFMMDDALLAGEAAKAKKA DWAVTGTPQSYEIYGCM+RKGD
Sbjct: 181 SAKDHGESFQMLEGGRAVAFMMDDALLAGEAAKAKKADDWAVTGTPQSYEIYGCMMRKGD 240

Query: 241 EPFKKAVDDAIKATYASGEINKIYEKWFMQPIPPKGLNLNFPMSDELKALIAKPTDKAAD 300
           EPFKKAVDDAIKATYASGEINKIYEKWFMQPIPPKGLNLNFPMSDELKALIAKPTDKAAD
Sbjct: 241 EPFKKAVDDAIKATYASGEINKIYEKWFMQPIPPKGLNLNFPMSDELKALIAKPTDKAAD 300

Query: 301 DKKS 304
           DKKS
Sbjct: 301 DKKS 304


Lambda     K      H
   0.315    0.131    0.368 

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: 400
Number of extensions: 7
Number of successful extensions: 1
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: 304
Length of database: 304
Length adjustment: 27
Effective length of query: 277
Effective length of database: 277
Effective search space:    76729
Effective search space used:    76729
Neighboring words threshold: 11
Window for multiple hits: 40
X1: 16 ( 7.3 bits)
X2: 38 (14.6 bits)
X3: 64 (24.7 bits)
S1: 41 (21.5 bits)
S2: 48 (23.1 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