astroquery: An Astronomical Web-Querying Package in Python

Abstract

astroquery is a collection of tools for requesting data from databases hosted on remote servers with interfaces exposed on the internet, including those with web pages but without formal application program interfaces (APIs). These tools are built on the Python requests package, which is used to make HTTP requests, and astropy, which provides most of the data parsing functionality. astroquery modules generally attempt to replicate the web page interface provided by a given service as closely as possible, making the transition from browser-based to command-line interaction easy. astroquery has received significant contributions from throughout the astronomical community, including several significant contributions from telescope archives. astroquery enables the creation of fully reproducible workflows from data acquisition through publication. This paper describes the philosophy, basic structure, and development model of the astroquery package. The complete documentation for astroquery can be found at http://astroquery.readthedocs.io/.

Accepted to AJ. The documentation is at http://astroquery.readthedocs.io/ and the repository is at https://github.com/astropy/astroquery/

References in corpus (2)

• Astropy: A Community Python Package for Astronomy
• Protoplanetary Disks in the Orion OMC1 Region Imaged with ALMA

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• True spin-orbit obliquities distribution: data-driven confirmation of no clustering of misaligned planets
• UNIONS Optical Identifications for VLASS Radio Sources in the Euclid Sky (UNVEIL) I. A Catalog of ~146,000 Radio Galaxies up to z~5
• VLTI/GRAVITY upper limit on near-infrared emission from the nearby 33 Msun black hole Gaia BH3
• Optimal Follow-Up of Gravitational-Wave Events with the UltraViolet EXplorer (UVEX)
• lightcurver: A Python Pipeline for Precise Photometry of Multiple-Epoch Wide-Field Images
• Tackling the Problem of Distributional Shifts: Correcting Misspecified, High-Dimensional Data-Driven Priors for Inverse Problems
• Machine learning-based identification of Gaia astrometric exoplanet orbits
• Past the outer rim, into the unknown: structures beyond the Kuiper Cliff
• Discovery of Five Green Pea Galaxies with Double-peaked Narrow [OIII] Lines
• A LOFAR sample of luminous compact sources coincident with nearby dwarf galaxies
• Prospects for a local detection of dark matter with future missions to Uranus and Neptune
• CoSHA: Code for Stellar properties Heuristic Assignment -- for the MaStar stellar library
• Removing Atmospheric Fringes from Zwicky Transient Facility i-Band Images using Principal Component Analysis
• The H IX galaxy survey III: The gas-phase metallicity in HI eXtreme galaxies
• Testing ultralow amplitude Cepheid candidates in the Galactic disk by TESS and Gaia
• Web of resonances and possible path of evolution of the small Uranian satellites
• Supernova Siblings and Spectroscopic Host-Galaxy Properties
• Precise radial velocities of giant stars -- XVII. Distinguishing planets from intrinsically induced radial velocity signals in evolved stars
• Learning novel representations of variable sources from multi-modal $\text{Gaia}$ data via autoencoders
• Characterization of low-mass companions to $\text{Kepler}$ objects of interest observed with APOGEE-N
• Prospects for localising Planet 9 with a future Uranus mission
• Unsupervised learning for variability detection with Gaia DR3 photometry. The main sequence-white dwarf valley
• A Search for Extra-Tidal RR Lyrae in the Globular Cluster NGC 5024 and NGC 5053
• Multi-epoch spectro-photometric characterization of the minimoon 2024 PT${}_5$ in the visible and near-infrared
• A high stellar multiplicity rate amongst TESS planet candidates in the Neptunian desert using Gaia DR3 astrometry
• A Unified Multi-Wavelength Data Analysis Workflow with gammapy. Constraining the Broadband Emission of FSRQ OP 313
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• Accurate photometric calibration by fitting the system transmission
• A NuSTAR study of quasi-periodic oscillations from the ultraluminous X-ray sources in M82
• Memories of past close encounters in extreme trans-Neptunian space: Finding unseen planets using pure random searches
• Separated twins or just siblings? A multi-planet system around an M dwarf including a cool sub-Neptune
• Probing stellar rotation in the Pleiades with gravity-mode pulsators
• A link between the size and composition of comets
• Detecting Intermediate-Mass Black Holes out to 20 Mpc with ELT/HARMONI: The Case of FCC 119
• Enhancing the detection of low-energy M dwarf flares: Wavelet-based denoising of CHEOPS data
• Polarimetric differential imaging with VLT/NACO. A comprehensive PDI pipeline for NACO data (PIPPIN)
• NGC 3521 as the Milky Way near twin: spectral energy distribution from UV to radio decameter ranges
• Cataclysmic Variable Candidates Identified in eROSITA-DE DR1,XMM-Newton, Swift, and ROSAT Catalogs
• Technosignature Searches with Real-time Alert Brokers
• A Machine Learning made Catalog of FR-II Radio Galaxies from the FIRST Survey
• Radio properties of high-redshift galaxies at $z\ge 1$
• Keck Near-Infrared Detections of Mab and Perdita
• A WISPR of the Venus Surface: Analysis of the Venus Nightside Thermal Emission at Optical Wavelengths
• Hertzsprung gap stars in nearby galaxies and the Quest for Luminous Red Novae Progenitors
• ALMACAL X: Constraints on molecular gas in the low-redshift circumgalactic medium
• Physical properties of the slow-rotating near-Earth asteroid (2059) Baboquivari from one apparition
• Recent arrivals to the main asteroid belt
• Modeling the Photometric Variability of Alpha${}^2$ CVn with a Dynamical Magnetosphere
• Companions to Kepler giant stars: A long-period eccentric substellar companion to KIC 3526061 and a stellar companion to HD 187878
• A rotation-based census of blue lurker candidates in open clusters
• The Astronomical Telescope of the University of Stuttgart (ATUS): Development, Optimization, and Lessons Learned
• The systemic recoil velocity distribution and the scale height of field millisecond pulsar systems: Implications on neutron star retention fractions in star clusters
• A broad-line quasar with unexplained extreme velocity offsets: post-shock outflow?
• The Atacama Cosmology Telescope: Systematic Transient Search of Single Observation Maps
• Ejected from home: C/1980 E1 (Bowell) and C/2024 L5 (ATLAS)
• MUPHOTEN : a MUlti-band PHOtometry Tool for TElescope Network
• Dynamical simulation of the Interstellar Comet 3I/ATLAS
• Effect of different Non-Gravitational accelerations on the trajectory of Interstellar Comet 3I/ATLAS
• The highest mass Kepler red giants -- II. Spectroscopic parameters, the amplitude-activity relation, and unexpected halo orbits
• A High-Precision, Differentiable Code for Solar System Ephemerides
• Validating Gaia DR3 Pulsating Variable Classifications with TESS: Building Reliable $\delta$ Scuti and $\gamma$ Doradus Stars Catalogs (In Progress)
• The Stripped-Star Ultraviolet Magellanic Cloud Survey (SUMS): The UV Photometric Catalog and Stripped Star Candidate Selection
• FindPOTATOs: Minor Planet Observation Linking Software
• Insights on the Rotational State and Shape of Asteroid (203) Pompeja from TESS Photometry
• Automated Identification of the Tip of the Red Giant Branch in Globular Clusters with Gaia Data
• A study on late time UV-emission in core collapse supernovae and the implications for the peculiar transient AT2018cow
• Covertly Active Comet (139359) 2001 ME1
• Photometric Identification of Unresolved Binary Stars in Nearby Open Star Clusters
• gallifrey: JAX-based Gaussian process structure learning for astronomical time series
• Direct Imaging Discovery of Giant Exoplanet $\beta$ Pictoris d: A Decade-Long Game of Hide-and-Seek
• Optical Counterparts to X-ray sources in LSST DP1
• Precise Parameters from Bayesian SED Fitting Indicate Thermally-Driven Mass Loss Likely Driver of Radius Valley
• Identification of Anomalous E+A Galaxies in GAMA Using an Isolation Forest
• Time delay measurements with Broken Power Law model
• 200,000+ Deep Learning-inferred Periods of Stellar Variability from the All-Sky Automated Survey for Supernovae
• Chemodynamics of BoötesI with $S^5$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints
• An investigation of the magnetic activity of HD 134319 based on TESS photometry and ground-based spectroscopy
• Characterizing the host galaxies and delay times of Ca-rich gap transients vs 91bg-like SNe and normal Type Ia SNe
• Starkiller: subtracting stars and other sources from IFU spectroscopic data through forward modeling
• Enhanced Astrometry of the Rapid ASKAP Continuum Survey for Precise Localisation of Fast Radio Bursts
• Direct Images of CO2 Absorption in the Atmosphere of a Super-Jupiter: Enhanced Metallicity Suggestive of Formation in a Disk
• The asymmetric structure of the inner disc around HD 142527 A with VLTI/MATISSE
• Dippers from TESS Full-frame Images. II. Spectroscopic Characterization of Four Young Dippers
• Twisted extreme trans-Neptunian orbital parameter space: statistically significant asymmetries confirmed
• Dynamical masses of young stellar objects with the VLBA: DYNAMO-VLBA: Radio binary stars in Orion
• Catalog of Integrated-Light Star Cluster Light Curves in TESS
• Centaur 2013 VZ70: Debris from Saturn's irregular moon population?
• Halo Photometry and Asteroseismology for 98 of the Brightest Stars Observed by TESS
• FluxCT V2.0: Updates to a Web Tool Identifying Contaminating Flux in Space Telescope Data
• A ready-to-deploy MLOps software platform for satellite and NEO detection at meter-class ground-based observatories
• Dynamic Photometric Variability in Three Young Brown Dwarfs in Taurus: Detection of Optical Flares with TESS data
• Exploring Young Stellar Variability with Gaia DR3 light curves
• Semi-Supervised Learning for Lensed Quasar Detection
• Hiding behind a curtain of dust: Gas and dust properties of an ultra-luminous strongly-lensed z = 3.75 galaxy behind the Milky Way disk
• Bar Evolution in Edge-on Galaxies: A Demographic Study of Boxy/Peanut Bulges
• Twinkle Twinkle Little Star, Roman Sees Where You Are: Predicting Exoplanet Transit Yields in the Rosette Nebula with the Nancy Grace Roman Space Telescope
• The Progenitor of the S147 Supernova Remnant
• Signatures of Galactic Expansion in Gaia DR3: Implications for the JWST Early-Galaxy Puzzle
• $\mathtt{KOBEsim}$: a Bayesian observing strategy algorithm for planet detection in radial velocity blind-search surveys
• Pulsars identified in the LOFAR Two-metre Sky Survey at 144 MHz
• Surface Properties of Near-Sun Asteroids
• Rate of Repeating Tidal Disruption Events with 5--19 years interval
• Fast, dust-poor outflows in the local candidate dual AGN MCG-03-34-64 observed with VLT/ERIS
• Low-frequency-selected Fast Radio Burst Host Galaxy Candidates
• The Properties of Fast Yellow Pulsating Supergiants: FYPS Point the Way to Missing Red Supergiants
• Coronal and chromospheric emission in A-type stars
• The Directly-Imaged Exoplanet Host Star 51 Eridani is a Gamma Doradus Pulsator
• Scientific Validation of the SPARC4 Pipeline: Multi-band Imaging, Polarimetry, and Photometric Time Series for Improved Characterization of Transiting Exoplanets
• Evidence for Environmental Stripping in the Coma Cluster
• JWST-TST High Contrast: First Direct Spectroscopy of GJ 504 b reveals Clouds and Possible Metal Enrichment
• TOI-3757 b: A low density gas giant orbiting a solar-metallicity M dwarf
• GJ 3929 b as the First Complete Rocky Worlds DDT Data Set
• The forced orbital planes of the Plutinos and other resonant KBOs
• The Inbound Gas and Dust Evolution of Interstellar Comet 3I/ATLAS from Optical Spectroscopy and Multi-band Photometry
• Alfred: A Flexible, User-Friendly Python Package for Exoplanet Confirmation
• Spin Parameters and Shape Models of Near-Earth Asteroids (4660) Nereus, (21088) Chelyabinsk, (66146) 1998 TU3, and (297418) 2000 SP43
• Rotation of young solar-type stars as seen by Gaia and K2
• Shepherding Miorita and its flock: A group of near-Earth asteroids driven by apsidal and von Zeipel-Lidov-Kozai secular resonances. A source of low-perihelion asteroids
• Encapsulating Textual Contents into a MOC data Structure for Advanced Applications
• Reprocessing the NEAT Dataset: Preliminary Results
• Dust and Volatiles in the Disintegrating Comet C/2019 Y4 (ATLAS)
• Which molecule traces what: chemical diagnostics of protostellar sources
• Tilsotua: Reproducing Slitmask Sky Positions for use with the LRIS Multislit Archive
• Testing OH Megamaser Identification Methods in HI Surveys: Updated Source-Flagging Algorithms and New Detections in ALFALFA
• Development of Radar and Optical Tracking of Near-Earth Asteroids at the University of Tasmania
• Evidence for Ultra-Diffuse Galaxy Formation Through Tidal Heating of Normal Dwarfs
• Overcoming Separation Between Counterparts Due to Unknown Proper Motions in Catalogue Cross-Matching
• Search for L5 Earth Trojans with DECam
• The Calar Alto CAFOS Direct Imaging First Data Release
• Full-frame data reduction method: a data mining tool to detect the potential variations in optical photometry
• CHILES VII: Deep Imaging for the CHILES project, a SKA prototype
• The Perkins INfrared Exosatellite Survey (PINES) I. Survey Overview, Reduction Pipeline, and Early Results
• Revisiting BD-06 1339b: A Likely False Positive Caused by Stellar Activity
• The TESS-Keck Survey. XI. Mass Measurements for Four Transiting sub-Neptunes orbiting K dwarf TOI-1246
• Nebular abundance gradient in the Cartwheel galaxy using MUSE data
• Simulating Photometric Images of Moving Targets with Photon-mapping
• XClass: An Automated Multiwavelength Machine-Learning Pipeline for Classification of Extragalactic X-ray Sources. I. Pipeline Description
• The Atacama Cosmology Telescope: Extragalactic Point Sources in the Southern Surveys at 150, 220 and 280 GHz observed between 2008-2010
• When the horseshoe fits: Characterizing 2023 FY3 with the 10.4 m Gran Telescopio Canarias and the Two-meter Twin Telescope
• A large sub-Neptune transiting the thick-disk M4V TOI-2406