Echinodermata consists of five classes: Crinoidea (feather stars and sea lillies), Ophiuroidea (brittle stars and basket stars), Asteroidea (sea stars), Echinoidea (sea urchins, sea biscuits, and sand dollars), and Holothuroidea (sea cucumbers). These animals have a rich fossil record, unique biomechanical properties, experimentally tractable embryos, and as such have been a favorite subject of study for more than 150 years. Along with Hemichordata, Echinodermata form a clade called Ambulacraria that are the sister group of Chordata, which include vertebrates.

Echinoderms are easily recognized due to striking synapomorphies. The most obvious is their pentaradial (five-fold) body symmetry that is characteristic of adults (earlier stages exhibit bilateral symmetry). They have a unique water vascular system, which is characterized by canals connecting small tube feet on the lateral side of the animals. The water vascular system is used for essential functions such as feeding, locomotion, waste disposal, and respiration. The “spiny skin” from which these animals get their name is an endoskeleton made up of calcareous plates called ossicles that is composed of high magnesium calcite formed as solid test, plates or ossicles depending on the class of echinoderms. Lastly, the ossicles are connected by ligaments made of collagen that are normally rigid, but may become flexible upon various neuronal stimuli.

The vast majority of genomic work thus far has focused on the classic developmental model, the sea urchin Stronglycentrotus purpuratus [1]. The genome of this sea urchin has produced many important findings of great interest, including the discovery of a rearrangement event in evolution that led to an unusual Hox cluster organization [2], a well-characterized gene network for the specification of endoderm and mesoderm [3], and insight into the effect of ocean acidification on biomineralization [4]. More recently the genomes of the sea star Patiria miniata, the sea urchin Lytechinus variegatus, the sea cucumber Parastichopus parvimensis, and the brittle star Ophiothrix spiculata have been made available in Echinobase [5].

Here we provide genome sequences from species within three different echinoderm clades: Australostichopus mollis, commonly known as the brown sea cucumber (Fig. 1a), the brittle star Ophionereis fasciata (Fig. 1b), and Patiriella regularis, known as the New Zealand common cushion star (Fig. 1c). These species can be found in the shallow waters surrounding New Zealand.

These data can be used for the gene family phylogenetic analyses, domain/gene losses, and presence of small non-coding RNAs among other applications (e.g., [6]). They will be particularly useful in a comparative framework with existing Echinoderm genomes, for example to identify highly conserved non-coding regions. Finally, these data will be a key resource for labs working on these animals in the lab or in the field (e.g., designing markers, probes, and genome-editing constructs).

Raw sequence data for all three species were produced from a single male, a single female, and the offspring of these two adults (Additional file 1: Table S1). For each individual sequenced, reads were barcoded and raw reads were submitted to the European Nucleotide Archive (ENA) separately (Additional file 2: Table S2). This sequencing strategy was originally used in order to employ a genetic mapping approach to genome assembly [7], and is not ideal for the standard de novo assembly strategy described herein. Nevertheless, when it became apparent that genetic mapping approach would not be feasible due to personnel, we applied a more traditional approach, and generated a useful set of data.

Parental tissue and larvae from each species were stored in ethanol prior to DNA extraction. DNA was extracted using Zymo DNA clean kit and was used to prepare Nextera libraries for 2 × 100 PE (paired end) sequencing on Illumina HiSeq2000 at BGI Shenzhen.

We used Augustus v3.0.3 [14] to generate ab initio gene predictions for the best assemblies of each of the echinoderm species. We created a training set with the Strongylocentrotus purpuratus v3.1 scaffolds and corresponding predicted gene models from Echinobase [5]. We used “generic,” “human,” and the custom model “strongylocentrotus_purpuratus” as values for the -species parameter. To compare the three different sets of gene predictions we BLASTed both human and S. purpuratus protein models against the protein predictions from Augustus using BLASTP v2.2.31+ [15] with an E-value cutoff of 1e-6 and limiting to a single target sequence (blastp -query query.fa -db aug.fa -evalue 1e-6 -outfmt 6 -max_target_seqs 1). For all species BLAST searches against the Augustus protein sequences generated with the custom S. purpuratus model resulted in the most hits (Additional file 3: Table S3). We therefore chose these predictions as our final sets.

We generated 49,301 A. mollis, 102,838 O. fasciata, and 1135 P. regularis gene predictions (Additional file 4: Table S4). In the case of A. mollis and O. casciata these numbers are substantially higher than the 22,709 published S. purpuratus gene models. The high number in A. mollis and O. casciata might be due to multiple fragmented predictions representing single genes. P. regularis has substantially fewer predictions, which might suggest that in most cases, the scaffolds were too short even to predict partial genes.

All data including sequencing reads and assemblies have been submitted to the ENA under the following project accessions: Australostichopus mollis = PRJEB10682; Patiriella regularis = PRJEB10600; Ophionereis fasciata = PRJEB10339. Supporting data is also archived in the GigaScience GigaDB database [16], and additional resources are available from http://ryanlab.whitney.ufl.edu/genomes/.