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Relocated event catalog for 2014-2024 seismicity at Campi Flegrei

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Catalogs of Deep Long Period Earthquakes at Klyuchevskoy Volcanic Group (Kamchatka) 2011-2012

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Data products associated with "Probabilistic Forward Modeling of Galaxy Catalogs with Normalizing Flows"

These are the data products associated with "Probabilistic Forward Modeling of Galaxy Catalogs with Normalizing Flows" by J. F. Crenshaw, et. al. This includes the input catalog and the outputs of the workflow described here https://github.com/jfcrenshaw/pzflow-paper, as well as a gzip of the github repo.

Synthetic Emission Line Catalog and High-Resolution SEDs for SPHEREx Galaxy Simulations

Overview: This repository contains the synthetic galaxy models derived from multi-wavelength photometry in the COSMOS field (166k galaxies over 1.27 sq. deg., 18 < i < 25) and from the GAMA survey (44k galaxies over 217 sq. deg., i < 18). These encompass a representative sample of galaxies SPHEREx will observe, and should be applicable for other surveys as well. <ul> <li>Synthetic emission line strengths in the rest-frame optical/near-infrared (H-alpha, H-beta, Paschen-alpha, [OIII], [OII], [NII], [SII])</li> <li>High-resolution SEDs (0.1 - 8 micron), which are produced by 1) fitting a library of 160 galaxy templates to multi-band photometry and 2) inserting emission lines with strengths predicted by an empirical model that depends on galaxy type, redshift and stellar mass.</li> </ul> These products were made using the modeling framework Conditional LIne Painting on Synthetic Spectra (CLIPonSS), the details of which are summarized in Feder+2023b (<a href="https://arxiv.org/abs/2312.04636">arXiv link here</a>). The synthetic emission line catalog is validated against a variety of LF measurements, line ratio trends and direct line comparisons.  Data description: High-resolution SEDs: The SEDs are stored in .FITS files, for which each galaxy SED has its own Header Data Unit (HDU). This format was chosen due to the fact that the wavelength sampling for the 160 galaxy empirical and model-based templates varies, i.e., we do not perform any interpolation onto a homogenized wavelength grid. In cases where emission lines are added but the continuum template resolution is coarse, the resolution is increased in the vicinity of the emission line(s) to adequately sample the line profiles. Each galaxy's HDU is indexed by its Farmer ID (for COSMOS) or alternatively its uberID (GAMA). The COSMOS SEDs are split into three files for relative ease of access, while the GAMA sources are all in one file. Emission line catalogs: The emission line catalogs are stored in .csv format with the following information: Tractor_ID (or uberID) [integer]: Unique identifier for each source RA/DEC [float, in degrees]: Celestial coordinates imag [AB]: i-band magnitude mass_best [float]: log-stellar masses estimated through SED fitting process ebv [float]: Galaxy intrinsic dust extinction (ranging from ebv=0 to 1) redshift [float]: Best-fit redshift from COSMOS2020 (GAMA) catalogs bfit_tid [integer]: Best fit template ID from library of templates dustlaw [integer]: Best fit dust law (1=Prevot, 2=Calzetti, 3=Seaton, 4=Allen, 5=Fitzpatrick) L_{line} [float, erg s-1]: Line luminosities from empirical model F_{line} [float, erg cm-2 s-1]: Line fluxes from empirical model ew_ha [float, Angstrom]: Equivalent width of H-alpha from empirical model Fitting templates: We include the 31 model-based templates and 129 empirical templates from Brown+2014. In the Brown templates we have removed any relevant lines that were directly measured in the initial spectra, however we do not fit for/remove PAH features. These can serve as the basis for other empirically based galaxy simulations with different emission line prescriptions. Any questions regarding the use of these data products or related issues can be directed to Richard Feder (link to <a href="https://richardfeder.github.io/">personal website</a>).

Catalog-level blinding on the bispectrum for DESI-like galaxy surveys

Points used in the Figures in the paper "Catalog-level blinding on the bispectrum for DESI-like galaxy surveys".

Cataloging Distant Galactic Open Clusters: Identification of 739 New Star Clusters Beyond 5 kpc Utilizing GAIA DR3 Data

The figures of the 739 open clusters that report in our paper (Cataloging Distant Galactic Open Clusters: Identification of  739 New Star Clusters Beyond 5 kpc Utilizing GAIA DR3 Data)  complete King's model  profile fitting, sky charts and 5-panels ( spatial distribution, proper-motion distribution, parallax statistics, parallax distribution, and CMD) .

Earthquake catalog at the Blanco Transform Fault Zone between 2012 and 2013

The csv file provides an earthquake catalog derived from data of ocean-bottom seismometers operated between 2012 and 2013 at the Blanco Transform Fault Zone. The data file is in ASCII text format. The first row is a column header that describes the content of the catalog: Earthquake origin date, time, latitude, longitude, depth and local magnitude. Not all earthquakes have a local magnitude estimate due to data selection.

opencc-by-4.0Jul 2018View details →

Wide-field Infrared Survey Explorer (WISE) Catalog of Periodic Variable Stars

Wide-field Infrared Survey Explorer (WISE) Catalog of Periodic Variable Stars  Xiaodian Chen, Shu Wang, Licai Deng, Richard de Grijs and Ming Yang  We have compiled the first all-sky mid-infrared variable-star catalog based on Wide-field  Infrared Survey Explorer (WISE) five-year survey data. Requiring more than 100 detections  for a given object, 50,282 carefully and robustly selected periodic variables are discovered,  of which 34,769 (69%) are new. Most are located in the Galactic plane and near the equatorial  poles. A method to classify variables based on their mid-infrared light curves is established  using known variable types in the General Catalog of Variable Stars. Careful classification of  the new variables results in a tally of 21,427 new EW-type eclipsing binaries, 5654 EA-type   eclipsing binaries, 1312 Cepheids, and 1231 RR Lyraes. By comparison with known variables   available in the literature, we estimate that the misclassi- fication rate is 5% and 10% for  short- and long-period variables, respectively. A detailed comparison of the types, periods,   and amplitudes with variables in the Catalina catalog shows that the independently obtained   classifications parameters are in excellent agreement. This enlarged sample of variable   stars will not only be helpful to study Galactic structure and extinction properties,   they can also be used to constrain stellar evolution theory and as potential candidates for  the James Webb Space Telescope.   These supplementary materials contain ALLWISE and NEOWISE-R single-exposure photometry tables of variables list  in Table 2 and 6 of the paper, and light curve figures for the 50,282 periodic variables in Table 2.  SourceID is identifier join these attachments to Table 2 and 6. Example: For variable star WISEJ094812.4+093448 in Table 2, the SourceID=170 is adopted to search  corresponding single-exposure information in both 'allwise12.txt' and 'neowise12.txt'.   File Description: allwise12.txt                Single exposure photometry data of variables from ALLWISE.    Bytes Format Units   Label   Explanations -----------------------------------------------------------------------------------------     1- 8  I5     ---  SourceID   Internal source identifier             10- 20 F11.7  deg     RAdeg   Right Ascension in decimal degrees (J2000)                    22- 32 F11.7  deg     DEdeg   Declination in decimal degrees (J2000)    34- 47 F14.8  day      MJD    Modified Julian date of the mid-point of the observation        49- 54 F6.3   mag     W1mag   Single exposure WISE W1 (3.35 micron) band magnitude   56- 63 F6.3   mag    eW1mag   W1 band uncertainty   65- 77 F6.3   mag     W2mag   Single exposure WISE W2 (4.6 micron) band magnitude    79- 86 F6.3   mag    eW1mag   W2 band uncertainty -----------------------------------------------------------------------------------------      neowise12.txt                Single exposure photometry data of variables from NEOWISE-R.    Bytes Format Units   Label   Explanations -----------------------------------------------------------------------------------------    1- 8  I5     ---  SourceID   Internal source identifier             10- 21 F11.7  deg     RAdeg   Right Ascension in decimal degrees (J2000)                    23- 34 F11.7  deg     DEdeg   Declination in decimal degrees (J2000)    36- 44 F6.3   mag     W1mag   Single exposure WISE W1 (3.35 micron) band magnitude   46- 54 F6.3   mag    eW1mag   W1 band uncertainty   56- 64 F6.3   mag     W2mag   Single exposure WISE W2 (4.6 micron) band magnitude    66- 74 F6.3   mag    eW1mag   W2 band uncertainty   76- 90 F14.8  day      MJD    Modified Julian date of the mid-point of the observation -----------------------------------------------------------------------------------------   figure0.zip -- figure23.zip  Full figures of 50282 WISE variables. They are divided into 24  packages by the order of Right Ascension.

openother-openNov 2018View details →

gwastro/1-ogc: v1.0 of the 1-OGC Catalog of Compact Binary Merger Candidates

Introduction This repository contains the first Open Gravitational-wave Catalog (1-OGW), which is obtained by using the public data from Advanced LIGO's first observing run to search for compact-object binary mergers. Our analysis is based on new methods that improve the separation between signals and noise in matched-filter searches for gravitational waves from the merger of compact objects. We make available our complete catalog of events, including the sub-threshold population of candidates. The catalog contains approximately 150,000 candidate events. We note that since the vast majority of the events in the catalog are likely to be noise, we have provided information to rank and select candidate events. The three most significant signals in our catalog correspond to the binary black hole mergers <a href="https://journals.aps.org/prl/abstract/10.1103/PhysRevLett.116.061102">GW150914</a>, <a href="https://journals.aps.org/prl/abstract/10.1103/PhysRevLett.116.241103">GW151226</a>, and <a href="https://journals.aps.org/prd/abstract/10.1103/PhysRevD.93.122003">LVT151012</a>, respectively. We observe these signals at a true discovery rate of 99.92%. We find that LVT151012 alone has a 97.6% probability of being astrophysical in origin. No other significant binary black hole candidates are found, nor did we observe any significant binary neutron star or neutron star--black hole candidates. The catalog is stored in the file '1-OGC.hdf'. There are a variety of tools to access <a href="https://www.hdfgroup.org/">hdf files</a> from numerous computing languages. Here we will focus on access through python and <a href="www.h5py.org">h5py</a>. Analysis Details Details of the analysis are available in this <a href="https://arxiv.org/abs/1811.01921">preprint paper</a> and the configuration files needed to create the analysis workflows are provided in the <a href="https://github.com/gwastro/1-ogc/tree/master/workflow/configuration">workflow/configuration</a> directory.

Figure 3 in TaXonomic Catalog of the Brazilian Fauna: Hydraenidae (Insecta: Coleoptera), diversity and distribution

Figure 3. Number of Hydraenidae species recorded from Brazil by year (1923–2022).

Figure 1 in TaXonomic Catalog of the Brazilian Fauna: Hydraenidae (Insecta: Coleoptera), diversity and distribution

Figure 1. Known distribution of Hydraenidae species from Brazil.

opencc-by-4.0Dec 2023View details →

Fig. 1 in Catalog of the genus Plocia Newman, 1842 (Cerambycidae: Lamiinae: Apomecynini) of the Philippines with the description of a new species from Davao De Oro Mindanao Island

Fig. 1. Habitus ofPlocia maglanai sp. nov.: A. Dorsal, B. Ventral, C. Lateral, D. Frons.

Catalogue of Life: Catalog of Life for DH (20 Feb 2019 dump)

https://eol-jira.bibalex.org/browse/TRAM-803 Data sets for the assembly of the EOL dynamic hierarchy.

Catalogue of Life: Catalog of Life Extract for DH (TRAM-797)

CoL with the following branches removed: Viruses (using ICTV), Bacteria, Archaea, Chromista, Protozoa (using NCBI + WoRMS + CoL Protist Extract), Aves (using IOC), Amphibia (using ASW), Odonata (using WOL), Bombycoidea (using Kitching et al. 2018), Anthelidae (now Bombycoidea), Onychophora (using Oliveira et al. 2012), Phthiraptera (duplicates Psocodea Species File data). Data sets for the assembly of the EOL dynamic hierarchy.

Catalogue of Life: Catalog of Life Protists

CoL Ciliophora, Oomycota, Polycystina, Eccrinida, Microsporidia, Mycetozoa, Chaetocerotaceae, Naviculaceae branches. Data sets for the assembly of the EOL dynamic hierarchy.

Catalogue of Life: Catalog of Life Protists (20 Feb 2019 dump)

https://eol-jira.bibalex.org/browse/TRAM-803 Data sets for the assembly of the EOL dynamic hierarchy.

opencc-by-4.0Dec 2023View details →

Figure 1 in The taxonomic catalog of the Brazilian fauna: Dermaptera and Phasmatodea (Insecta), with commentaries on species list, types, authorship and distribution

Figure 1. Number of species by biome: (A) Dermaptera; (B) Phasmatodea.

Catalog of Hymenoptera in America North of Mexico

Catalog of Hymenoptera in America North of Mexico / Prepared cooperatively by specialists on the various groups of Hymenoptera under the direction of Karl V. Krombein and Paul D. Hurd, Jr. Smithsonian Institution and David R. Smith and B. D. Burks Systematic Entomology Laboratory, Insect Identification and Beneficial Insect Introduction Institute Science and Education Administration, United States Department of Agriculture. Smithsonian Institution Press, Washington, DC, 1979.

opencc-by-4.0Apr 2024View details →

FRB Mock Catalog and Reproduction Package for "Birth and Evolution of Fast Radio Bursts: Strong Population-Based Evidence for a Neutron-Star Origin"

<h3>Quickstart: FRB Mock Catalog</h3> A simulated 1-day catalog of one-off FRBs, that allows users to access the FRB population without installing the entire frbpoppy package. Download and unzip 1_Day_FRB_Sky_on_Earth.txt.zip (175 MB). This human and machine readable file contains 3.5E6 FRBs that are brighter than 0.01 Jy ms, the best limit in one-off FRB detection currently. The simulated catalog is produced by the perfect telescope in frbpoppy, free of selection effects, that observed 4pi of sky for 24 hrs, with minimum detectable fluence 0.01 Jy ms, for the best-fit no-delay SFR model. This file can be read using the accompanying jupyter notebook "starting_with_mock_catalog.ipynb". If you use this, please cite Wang & van Leeuwen 2024 (A&A), <a href="https://doi.org/10.1051/0004-6361/202450673">https://doi.org/10.1051/0004-6361/202450673</a> <h3>Reproduction package for the paper "Birth and Evolution of Fast Radio Bursts: Strong Population-Based Evidence for a Neutron-Star Origin"</h3> ReproductionPackage.zip is a basic reproduction package for the paper "Birth and Evolution of Fast Radio Bursts: Strong Population-Based Evidence for a Neutron-Star Origin" by Wang & van Leeuwen (2024).  * arXiv: [<a href="https://arxiv.org/abs/2405.06281">2405.06281</a>]   * DOI: [<a href="https://doi.org/10.1051/0004-6361/202450673">10.1051/0004-6361/202450673</a>]  <h3>Installation</h3> First pull or download and `frbpoppy` from <https://github.com/TRASAL/frbpoppy>. Then download `ReproductionPackage.zip` and extract it starting in the frbpoppy/ base directory. The scripts to produce the Figures are found in folder `frbpoppy/tests/markov_chain_monte_carlo/`. The data used for these Figures resides in folder `frbpoppy/data/populations/mcmc/`. <h3>Software</h3> The methods and software packages used to produce the results are listed in the paper (including links to the relevant publications and/or packages):  FRBPOPPY: <https://github.com/TRASAL/frbpoppy>  TRASAL:   <https://github.com/TRASAL> <h3>Raw Data</h3> The data are publicly available at  https://www.wis-tns.org/