An Indo-Pacific coral spawning database

The discovery of multi-species synchronous spawning of scleractinian corals on the Great Barrier Reef in the 1980s stimulated an extraordinary effort to document spawning times in other parts of the globe. Unfortunately, most of these data remain unpublished which limits our understanding of regional and global reproductive patterns. The Coral Spawning Database (CSD) collates much of these disparate data into a single place. The CSD includes 6178 observations (3085 of which were unpublished) of the time or day of spawning for over 300 scleractinian species in 61 genera from 101 sites in the Indo-Pacific. The goal of the CSD is to provide open access to coral spawning data to accelerate our understanding of coral reproductive biology and to provide a baseline against which to evaluate any future changes in reproductive phenology. Measurement(s) Point in Time Date and Time Data Type • Spawning Technology Type(s) Observation • digital curation Sample Characteristic - Organism Scleractinia Sample Characteristic - Environment ocean Sample Characteristic - Location Pacific Ocean • Indian Ocean region Measurement(s) Point in Time Date and Time Data Type • Spawning Technology Type(s) Observation • digital curation Sample Characteristic - Organism Scleractinia Sample Characteristic - Environment ocean Sample Characteristic - Location Pacific Ocean • Indian Ocean region Machine-accessible metadata file describing the reported data: https://doi.org/10.6084/m9.figshare.13100552


Background & Summary
Scleractinian corals are the ecosystem engineers of coral reefs, the most species-rich marine ecosystems. Scleractinian corals have a bipartite life history, with a sessile adult stage and a planktonic larval stage that allows dispersal among reefs. Corals produce larvae in one of two ways: gametes are broadcast-spawned for external fertilization or the eggs are retained for internal fertilization, followed by the release of planula larvae from the polyp. The discovery of multi-species synchronous spawning on the Great Barrier Reef 1 stimulated a large effort to document coral spawning times in other regions of the world. Similar multi-species spawning events sensu 2 have now been documented in over 25 locations throughout the Indo-Pacific [3][4][5] . However, much additional data on coral sexual reproductive patterns remain unpublished. Even when spawning data are published, there is often insufficient detail, such as the precise time and duration of spawning, to address many important questions. Consequently, predicting the month of spawning has been the focus of many studies to date 6 .
Coral spawning times can be used to address many significant and fundamental questions in coral reef ecology. Most coral species are notoriously difficult to identify and spawning times have been used to infer pre-zygotic barriers to fertilization and thus assist decisions about species boundaries 7,8 . While proximate cues associated with the month of spawning are reasonably well understood in some taxa 6,9 , the relationship between cues for the date and time of spawning are poorly understood. Similarly, potential phylogenetic patterns and geographical variation in spawning times are only beginning to be explored 10 . Knowing when corals spawn is also important for managing coastal development. For example, in Western Australia, legislation requires dredging operations to cease during mass spawning events 11,12 . Coral spawning is also an economic boon for tourist operators in many parts of the world, such as the Great Barrier Reef. Furthermore, population level records of spawning times provide a baseline against which to evaluate potential changes in spawning synchrony or seasonality associated with anthropogenic disruptions to environmental cues, in particular, sea surface temperature 13 . Knowledge of the timing of spawning is also essential for accurately estimating levels of connectivity among populations, given season differences in current flow 14 . The value of long-term species level data on coral spawning has recently been demonstrated in a test of the influence of temperature and wind on the night of coral spawning 15 .
In this data descriptor, we present the Coral Spawning Database (CSD). The CSD includes spawning observations for reef building coral species from the Indo-Pacific. The CSD includes 6178 observations (3085 of which were unpublished) of the time or day of spawning for 300+ scleractinian species in 61 genera (Online-only Table 1) from 101 sites (Fig. 1) in the Indo-Pacific. The goals of the CSD are: (i) to assemble the scattered and mostly unpublished observations of scleractinian coral spawning times and (ii) to make these data readily available to the research community. Our vision is to help advance many aspects of coral reef science and conservation at a time of unprecedented environmental and societal change. # A list of authors and their affiliations appears at the end of the paper.

DATA DeSCRIPToR oPeN Methods
The CSD includes spawning times for broadcast spawning scleractinian coral species in the Indo-Pacific. There are two sources for these data: the literature and unpublished observations. Published literature was selected based on the authors' knowledge of the subject area and a literature search using the terms "coral AND spawn*". Over 50 researchers known by the authors to have extensive data on coral spawning times were approached to contribute unpublished data. This initial invitation led to a subsequent round of invitations to additional contributors. Of course, we encourage any researchers with data we have missed to contribute their observations in the annual update of the database. The database focusses on spawning times. Many other biological variables related to coral reproduction, such as fecundity, are available in the Coral Traits Database 16 .
The database is available as a Microsoft Access relational database or an Excel spreadsheet. To minimise repetition in data entry, spawning observation information is entered in three primary tables (Fig. 2). The first ("tblSitesForSpawningObservations") is used to enter geographic information on each study site; the second  ("tblSpawningObervations") contains details of the spawning activity recorded at each site; the third ("tblRefer-encesForSpawningObervations") contains either full bibliographic details for published studies or details of the source of unpublished data. To assist with data analysis, three accessory tables are also linked. The first ("tblEcore-gionsVeron2015") allows sites to be grouped into the biogeographical Ecoregions proposed by 17 or by broader region (e.g. Indian Ocean, Western and Central Pacific, Eastern Pacific). The remaining two tables allow the coral species to be grouped systematically for analysis. The first ("tblCoralSpecies") has a list of over 1600 coral species with genus and species names (primarily from 18 or subsequent descriptions of new species) mapped to currently accepted names (primarily from 19 ) where the taxonomy has changed. The second ("tblSystematics") allows species to be grouped into major clades or currently accepted families 19 as revealed by molecular studies 20 The next four fields contain benchmarks for comparing spawning among sites for different species or groups of species 23 . The first is the date of the nearest full moon (DoNFM) to the date of spawning (with 75% of spawning recorded in the week after the full moon). This allows all spawning dates to be calculated in terms of days before or after the full moon (DoSRtNFM). Sunset provides a benchmark for comparing the times of spawning for most spawners (over 90% of spawning started within 4 hours of sunset) and sunrise for a few daytime spawners such as Pocillopora verrucosa. Dates of full moon and times of sunrise and sunset are available for given locations from the web (e.g. www.timeanddate.com) and can be entered manually. However, they can also be calculated automatically in the database based on the date, time zone and, for sunrise and sunset, the latitude and longitude. Excel spreadsheets are also available on request from the corresponding authors to calculate dates of full moon and times of sunrise and sunset in addition to a data entry template.
www.nature.com/scientificdata www.nature.com/scientificdata/  Here enter the time the colony was first observed spawning as the Start_time and the Quality_start as ' Approx' . Leave the End_time blank and set No_end to True. 2. A colony is followed closely until spawning is observed to begin but the precise time when spawning ends is not recorded. However, the colony is observed to be still dribbling spawn 30 minutes after spawning started.
Here enter the Quality_start_ as 'Exact' with the End_time set to 30 minutes after the Start_time and the Quality_end set to ' Approx' . 3. A colony is followed closely from the beginning until the end of spawning.
Here enter the times and note Quality_start and Quality_end as 'Exact' . 4. A colony is placed in a bucket and checked every 30 minutes. At the first observation there is no evidence of spawning, 30 min later the surface of the water is covered in bundles and the colony is no longer spawning. Here enter the time of the first observation as the start time and the time of the second observation as the end time and set Quality_start and Quality_end to ' Approx' . 5. Only the night of spawning is known, for example, gametes are no longer apparent in a tagged and sequentially sampled colony.
Here don't enter either a start time or an end time and leave Quality_start and Quality_end blank. Set No_ start and No_end to True.

Species identifications.
Species were generally identified following 18,24 or by comparing skeletons to the type material or the original descriptions of nominal species. Specimens identified following 18,24 were updated to the currently accepted names at the World Register of Marine Species 19 . The database also allows for uncertainties in species identifications to be indicated with the use of a series of open nomenclature qualifiers 25,26 that allow the assignment of specimens to a nominal species with varying degrees of certainty. Specimens that closely resemble the type of a nominal species are given the qualifier cf. (e.g. Acropora cf. nasuta). Specimens that have morphological affinities to a nominal species but appear distinct are given the qualifier aff. (e.g. Acropora aff. pulchra): these specimens are either geographical variants of species with high morphological plasticity or potentially undescribed species. Species that could not be matched with the type material of any nominal species were labelled as sp. in addition to the location where they were collected (e.g. Acropora sp_1_Fiji). These specimens are most probably undescribed species. For 1% of records spawning colonies were only identified to genus (e.g. Montipora sp.). Contact the sources of these data for further information on the species identity.

Data Records
A snapshot of the data contained in this descriptor can be downloaded from figshare 27 . The data includes 6178 observations, 3085 of which were unpublished with the remainder gleaned from the literature  . These data have been through a rigorous quality control and editorial process. Annual updates of the dataset will be uploaded to figshare as new version and also made available at any time on request from the Editor (JRG

Technical Validation
The database is governed on a voluntary basis, by an Editor (JRG), Assistant Editors (JB & AGB), a Taxonomy Advisor (AHB) and a Database Administrator (AJE). Quality control of data and editorial procedures include: 1. Contributor approval. Database users must request permission to become a database contributor. 2. Editorial approval. Once a contributor sends data to the Editor, the data will be checked and if correctly formatted will be forward to the Database Administrator 3. User feedback. Data issues can be reported for any observation by email to the Editor (2021) 8 www.nature.com/scientificdata www.nature.com/scientificdata/ 125. Wolstenholme, J., Nozawa, Y., Byrne, M. & Burke, W. Timing of mass spawning in corals: potential influence of the coincidence of lunar factors and associated changes in atmospheric pressure from northern and southern hemisphere case studies.