cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.18727/archive/30
title: Deep U Band and R Imaging of GOODS-South

description: As part of the Great Observatories Origins Deep Survey (GOODS), deep imaging in the Chandra Deep Field South (CDF-S) has been carried out, using the VIMOS instrument mounted at the Melipal Unit Telescope of the VLT at ESO's Cerro Paranal Observatory, Chile. This data release contains the coadded images in U band from the ESO large programme 168.A-0485 (P.I. C. Cesarsky) which have been obtained in service mode observations between August 2004 and fall 2006.The 1-sigma depth for VIMOS U band in the area covered by the GOODS-ACS observations is ~30 AB (within an aperture of 1" radius, ranging from 29.5 and 30.2 AB). The PSF of the VIMOS U band mosaic is ~0.8" FWHM, but varies over the field. Also included in this data release is a coadded image in R band obtained from data retrieved from the ESO archive. Due to the different observing strategies adopted in the programmes the resulting coverage of the GOODS-ACS area is more complex than for the U band. The depth of the VIMOS R band mosaic over the ACS area ranges from ~28 AB to 29 AB (1-sigma, 1" aperture radius). The PSF of the VIMOS R band mosaic is ~0".7 FWHM and varies over the field.
description: This is a dynamic dataset; it is growing as new data is added. The DOI refers to the newest available dataset.
DOI: 10.5281/zenodo.5171880
title: metapsyData: R Package to Access the Metapsy Databases

description: The <code>metapsyData</code> package allows to access the Metapsy meta-analytic psychotherapy databases direct in your <code>R</code> environment. Once installed, simply run the <code>data</code> function (e.g. <code>data(DepPsychDB)</code>) to save the data locally. The documentation of the package is also hosted by rdrr.io. The interactive Metapsy web application (metapsy.org) uses <code>metapsyData</code> in the background. You can open the Metapsy website in <code>R</code> by running <code>open_app()</code>. The raw data files can be accessed in the associated GitHub repository under <code>data</code>. To search for available databases in <code>metapsyData</code>, type in <code>metapsyData::</code> in your RStudio console.
description: {"references": ["Harrer, M., Ebert, D. D., Karyotaki, E., Cuijpers, P. (2020). MetaPsyR: Access the Meta-Analytic Psychotherapy Database. R package version 0.1.0. DOI: 10.5281/zenodo.5171880."]}
DOI: 10.5281/zenodo.5171859
title: metapsyData: R Package to Access the Metapsy Databases

description: The <code>metapsyData</code> package allows to access the Metapsy meta-analytic psychotherapy databases direct in your <code>R</code> environment. Once installed, simply run the <code>data</code> function (e.g. <code>data(DepPsychDB)</code>) to save the data locally. The documentation of the package is also hosted by rdrr.io. The interactive Metapsy web application (metapsy.org) uses <code>metapsyData</code> in the background. You can open the Metapsy website in <code>R</code> by running <code>open_app()</code>. The raw data files can be accessed in the associated GitHub repository under <code>data</code>. To search for available databases in <code>metapsyData</code>, type in <code>metapsyData::</code> in your RStudio console.
description: {"references": ["Harrer, M., Ebert, D. D., Karyotaki, E., Cuijpers, P. (2020). MetaPsyR: Access the Meta-Analytic Psychotherapy Database. R package version 0.1.0. DOI: 10.5281/zenodo.5171880."]}
DOI: 10.18727/archive/31
title: The Great Observatories Origins Deep Survey - VLT/VIMOS spectroscopy

description: Multi-object spectroscopy of faint galaxies in the Chandra Deep Field South (CDFS) has been carried out, as part of the Great Observatories Origins Deep Survey (GOODS), using the VIsible Multi-Object Spectrograph (VIMOS) instrument mounted at the Melipal Unit Telescope of the VLT at ESO's Cerro Paranal Observatory, Chile. This data release contains the redshift catalog resulting from the full data set of the GOODS/VIMOS spectroscopic campaign of the ESO/GOODS large programme 171.A-3045 (P.I. C. Cesarsky) which have been obtained in service mode observations between September 2004 and January 2007.
description: This is a dynamic dataset; it is growing as new data is added. The DOI refers to the newest available dataset.
DOI: 10.18727/archive/32
title: Reduced data from programme 60.A-9392(B) - GW follow-up

description: NaCo imaging observations were carried out under ESO program 60.A-9392(A), PI A. Kaufer, to constrain the spectral energy distribution at 3.80 micron of the source identified by the LIGO-VIRGO GW 170817 and the gamma-ray burst GRB 170817A alerts. The data were acquired in eleven different nights, from late-Aug –to early-Sep 2017, mostly under good conditions. The NaCo imaging was carried out with the L’ filter and the L27 camera, with a pixel scale of 0.027 arcsec/pixel . The FWHM of the photometric standard star observed together with the science data indicates a seeing of about 0.11 arcsec. The images from individual nights were co-added us- ing the offset parameters from the headers. The extended nearby galaxy NGC 4993 falls inside the NaCo field of view, and it was detected on some of the the combined frames, but no unresolved sources were detected in the field. This release includes only processed images form the nights when NGC 4993 was detected, because a standard was observed only on one night, and the galaxy was used to perform a consistent photometric calibration across the data from different nights. Detection limits were derived for single night observations, and for image products obtained from multiple nights combined together
description: This is a dynamic dataset; it is growing as new data is added. The DOI refers to the newest available dataset.
DOI: 10.18727/archive/33
title: HARPS reduced data obtained by standard ESO pipeline processing

description: This is the release of reduced 1-D spectra from the HARPS (High Accuracy Radial velocity Planet Searcher) at the ESO La Silla 3.6m telescope. The release covers practically all HARPS science data in High RV Accuracy Mode (HAM) and High Efficiency Mode (EGGS). All data were reduced automatically using the Data Reduction Software (DRS) pipeline developed by the HARPS Consortium. Data obtained before 29 May 2015 were processed with version 3.5 of the pipeline. Data obtained after that date with version 3.8 of the pipeline, configured in a way that the results are compatible with the results from version 3.5. The products come in the standard ESO 1-D FITS binary table format along with a TAR file containing all output files generated by the pipeline.
description: This is a dynamic dataset; it is growing as new data is added. The DOI refers to the newest available dataset.
DOI: 10.18727/archive/34
title: HAWK-I reduced data obtained by standard ESO pipeline processing

description: This data collection provides pipeline-reduced images obtained with HAWK-I, a near-infrared (0.85 − 2.5 μm) wide-field imager. In 2016, the full HAWK-I archived dataset, comprising the observations from the beginning of regular operations (April 2008) until September 2015, was reduced by the Cambridge Astronomy Survey Unit (CASU) using newly developed calibration and science recipes. As of 2017, the ESO Quality Control (QC) Group took over to continue the pro- cessing of HAWK-I science data, starting with data taken in October 2015 and with further data being added at regular intervals.
description: This is a dynamic dataset; it is growing as new data is added. The DOI refers to the newest available dataset.
DOI: 10.18727/archive/35
title: HUGS - Hawk-I UDS and GOODS Survey

description: HUGS (an acronym for Hawk-I UDS and GOODS Survey) is a ultra–deep IR imaging survey executed with the Hawk-I imager at the VLT, that observed in the K and Y bands the UKIDSS Ultra Deep Survey (UDS) and the Great Observatories Origins Deep Survey (GOODS)-South fields covered by the CANDELS survey. The HUGS survey was designed to cover the two CANDELS fields accessible from Paranal that do not have suitably-deep K-band images: a sub-area of UDS and GOODS-S. The depth of the images was chosen to be 0.5mag shallower than obtained with the Wide Field Camera 3 (WFC3/IR) at the Hubble Space Telescope (HST) in H160, as appropriate to match the average H-K color of faint galaxies. In the UDS field deep Y-band images have also been acquired. They are an essential complement to the CANDELS data set, since neither Y098 nor Y105 imaging of this field has been obtained within CANDELS. This release contains deep Y-band images of the UDS field and the extracted source catalogue.
description: This is a dynamic dataset; it is growing as new data is added. The DOI refers to the newest available dataset.
DOI: 10.18727/archive/36
title: INvestigating Stellar Populations and IMF in RElics - 1104.B-0370

description: INSPIRE is based on data obtained as part of the ESO Large Programme ID: 1104.B- 0370, PI: C. Spiniello, which has been awarded 154 hrs of observations on X-Shooter to spectroscopically follow up 52 UCMGs with redshift 0.1
description: This is a dynamic dataset; it is growing as new data is added. The DOI refers to the newest available dataset.
DOI: 10.18727/archive/37
title: KIDS - The Kilo-Degree Survey (VST)

description: KiDS is an ESO public survey carried out with the VLT Survey Telescope and OmegaCAM camera that has imaged 1350 square degrees in four filters (u, g, r, i), in single epochs per filter. KiDS was designed as a weak lensing shear tomography survey, and its core science drivers are mapping of the large-scale matter distribution in the universe and constraining the equation-of-state of Dark Energy. Additional science cases are manifold and range from galaxy evolution to Milky Way structure, and from detection of white dwarfs to high-redshift quasars.
description: This is a dynamic dataset; it is growing as new data is added. The DOI refers to the newest available dataset.
DOI: 10.18727/archive/38
title: KMOS reduced data obtained by standard ESO pipeline processing

description: This is the release of reduced IFU data cubes from KMOS, the K-band Multi Object Spectrograph. The instrument is located at the VLT UT1 telescope and has 24 image slicer Integral Field Units (IFUs) that can be placed independently in the patrol field of 7.2 arcmin diameter. Five different gratings can be used which are centred at the I+Z, Y+J, H, H+K, and K infrared atmospheric bands thus allowing observations between 0.8 and 2.5 μm. Spectral resolving power depends on the grating and is between 2000 and 4200. This release is an open stream release. It is complete from start of operations on 1st October 2013 until present. Data content is not fixed but grows with time as new data are being acquired and processed (approximately with monthly cadence and with a delay of one to two months). Data reduction is executed first for each IFU containing an object. It includes sky subtraction, flat fielding, wavelength calibration, flux calibration, and cube reconstruction. Telluric absorption features in the individual cube spectra are corrected for.
description: This is a dynamic dataset; it is growing as new data is added. The DOI refers to the newest available dataset.
DOI: 10.18727/archive/39
title: LEGA-C - Large Early Galaxy Astrophysics Census

description: The Large Early Galaxy Astrophysics Census (LEGA-C) is an ESO 130−night public spectroscopic survey conducted with VIMOS on the Very Large Telescope. The survey covers the 1.4 square degrees of the UltraVISTA survey in the COSMOS field (R.A. = 10h00; Dec. = +2 deg). The VIMOS high-resolution red grating is used in combination with the GG475 order separation filter, which results in a typical wavelength range of ∼ 6300Å – 8800Å at a resolution of R = 2500 and a dispersion of 0.6Å per pixel. LEGA-C’s unique combination of sample size and depth enables for the first time to map the stellar content at large look-back time (8 Gigayears), across galaxies of different types and star-formation activity. Core science goals are, among others, to chart the star formation histories of galaxies, quenching of star formation, evolution of galaxy kinematics and other scaling relations. Observations started in December 2014 and were completed by March 2018.
description: This is a dynamic dataset; it is growing as new data is added. The DOI refers to the newest available dataset.
DOI: 10.18727/archive/40
title: LESS - LABOCA Extended Chandra Deep Field South Submillimetre Survey

description: The LABOCA Extended Chandra Deep Field South (ECDFS) Submillimetre Survey (LESS) is a public legacy survey of the ECDFS at 870 μm using the LABOCA camera (Siringo et al. 2009) on the APEX telescope (Gusten et al. 2006). A full description of the observations, reduction and analysis of the the datasets presented here is given in Weiss et al. (2009, ApJ, 707, 1201).
description: This is a dynamic dataset; it is growing as new data is added. The DOI refers to the newest available dataset.
DOI: 10.18727/archive/41
title: MUSE reduced data obtained by standard ESO pipeline processing

description: This is the release of reduced IFU datacubes from the MUSE spectrograph, taken in the Wide Field Mode. MUSE, the Multi-Unit Spectroscopic Explorer, is an Integral Field Spectrograph located at the VLT UT4 telescope. The instru- ment samples almost the full optical wavelength range with a mean resolution of 3000. In the Wide- Field mode (WFM), it has a 1 squared arcmin field of view (FOV) sampling the sky with 0.2 arcsec- onds spatial pixels. In this mode, observations are carried out under natural seeing (WFM-NOAO) or, since 2017, also assisted by the UT4 AO system (WFM-AO). The Narrow-Field mode (NFM) has a FOV of 7.4”x7.4” and samples with 0.025 arcseconds spatial pixels. It is offered since P103 and is supported by laser tomography, as NFM-AO. This release is an open stream release. It is complete from the begin of operations, 2014-09-13, until present. Data from the Science Verification periods (NOAO in June and August 2014, AO in August and September 2017) are also included. The data content grows with time as new data are being acquired and processed (approximately with monthly cadence and with a delay of 1 or 2 months). The data have most of their instrument signature removed: they have been pre-processed, de-biased, flat- fielded, astrometrically calibrated, sky-subtracted, wavelength-calibrated, and fluxed. Their wave- length scale has been corrected to the barycentric reference system. In the last step they usually have been combined (except for documented cases) and resampled. The sky correction either uses user-defined SKY pointings, or – if not available - the sky is determined from the observations directly, applying a sky model. Errors are propagated throughout the reduction and provided in the final datacube.
description: This is a dynamic dataset; it is growing as new data is added. The DOI refers to the newest available dataset.
DOI: 10.18727/archive/42
title: MUSE reduced data obtained by standard ESO pipeline processing, co-added across multiple observations

description: This is the release of reduced IFU datacubes from the MUSE spectrograph, taken in the Wide Field Mode. MUSE, the Multi-Unit Spectroscopic Explorer, is an Integral Field Spectrograph located at the VLT UT4 telescope. The instru- ment samples almost the full optical wavelength range with a mean resolution of 3000. In the Wide- Field mode (WFM), it has a 1 squared arcmin field of view (FOV) sampling the sky with 0.2 arcsec- onds spatial pixels. In this mode, observations are carried out under natural seeing (WFM-NOAO) or, since 2017, also assisted by the UT4 AO system (WFM-AO). The Narrow-Field mode (NFM) has a FOV of 7.4”x7.4” and samples with 0.025 arcseconds spatial pixels. It is offered since P103 and is supported by laser tomography, as NFM-AO. Where multiple visits of the same target exist, with multiple OBs, the deep datacube combines the input files from these OBs with the goal to reach the maximum possible depth of the observations. There are also many OBs that visit a given target only once, and then no deep datacube exists. Therefore, the MUSE and the MUSE-DEEP releases are generally complementary. This release is an open stream release. The release covers the two MUSE Science Verification periods in June and August 2014, and data from the regular MUSE operations which started in September 2014. Data from the AO Science Verification period in August and September 2017 are also included. Depending on the availability of an end-of-run signal, new data are processed within a month or two after that signal, or with a larger delay in some cases.
description: This is a dynamic dataset; it is growing as new data is added. The DOI refers to the newest available dataset.
DOI: 10.18727/archive/43
title: MUSE library of stellar spectra

description: The dataset comprises a library of 35 high-fidelity MUSE stellar spectra for a subset of the stars part of the X-SHOOTER Spectral Library, covering the Hertzsprung-Russell diagram for both extragalactic and stellar studies. We verified the continuum shape of these spectra with synthetic broad-band colors derived from the spectra. We also report some spectral indices from the Lick system, derived from the new observations. The spectra span the range from ~4800 to ~9300 Angstrom, with a resolving power varying within this limits from 1750 to 3750. The observations were carried out with the MUSE (Multi-Unit Spectroscopic Explorer) integral field unit spectrograph at the VLT in Apr-May 2017 in non-photometric conditions. Each star was observed six times, following the same offset pattern used for MUSE spectrophotometric stan- dards to minimize any systematic effects.
description: This is a dynamic dataset; it is growing as new data is added. The DOI refers to the newest available dataset.
DOI: 10.18727/archive/44
title: Accurate PSF-fitting photometry of 300 sq.deg around the Galactic centre

description: The Milky Way Bulge PSF Photometry provides a comprehensive census of the stellar popula- tions in the inner ~ 300 deg2 of the Galaxy. It is based on observations obtained with the near-IR imager VIRCAM mounted at the VISTA telescope as part of the ESO public survey VISTA Variables in the Via Lactea (VVV, ESO programme 179.B-2002). With a limiting magnitudes Ks~20 and J~21, this new photometric compilation allows to characterize the evolved and un-evolved stellar population of the Milky Way bulge over most its extension. A detailed description of the data reduction and catalogs construction is provided in Surot et al. (2019A&A, 629, 1).
description: This is a dynamic dataset; it is growing as new data is added. The DOI refers to the newest available dataset.
DOI: 10.18727/archive/45
title: The Next Generation Transit Survey

description: The Next-Generation Transit Survey (NGTS) is a ground-based exoplanet survey designed to detect and study Neptune and super-Earth sized planets around bright host stars using the transit method. The project is described by Wheatley et al. (2018, MNRAS, 475, 4476) and the project website is http://ngtransits.org.
description: This is a dynamic dataset; it is growing as new data is added. The DOI refers to the newest available dataset.
DOI: 10.18727/archive/46
title: PESSTO - Spectroscopic Survey of Transient Objects

description: PESSTO (Public ESO Spectroscopic Survey of Transient Objects) began in April 2012 on the New Technology Telescope using the instruments EFOSC2 and SOFI. Supernovae and optical transients brighter than 20.5m were targeted for classification and specific science targets were selected for detailed follow-up. Standard EFOSC2 setups were used providing spectra with resolutions of 13-17Å between 3650-9995Å. A subset of the brighter science targets were selected for SOFI spectroscopy with the blue and red Grisms (resolutions 23-33Å) and imaging with broadband JHKs filters.
description: This is a dynamic dataset; it is growing as new data is added. The DOI refers to the newest available dataset.
DOI: 10.18727/archive/47
title: 3D Mapping of the Dynamic Feedback and Chemistry in the Star Formation Process across Galaxy Disks

description: The PHANGS-MUSE observational programme, is a survey using the MUSE integral field spectrograph at the VLT to map 19 star-forming disk galaxies (Emsellem et al. 2021, arXiv:2110.03708). Together with dedicated ALMA and HST observations delivering exquisite information regarding, e.g., giant molecular clouds and star clusters, the MUSE campaign provides a comprehensive view of the chemo-dynamical evolution of the star formation process across the different environments, addressing timescales associated with star formation, quantifying the importance of stellar feedback, studying the chemical enrichment and mixing, and connecting the local conditions with the large-scale dynamics. Please find additional information, including on data types, in the data Release Description (https://www.eso.org/rm/api/v1/public/releaseDescriptions/184) and in Emsellem et al. 2022 (A&A, 659, 191; https://ui.adsabs.harvard.edu/abs/2022A%26A...659A.191E/abstract).
description: This is a dynamic dataset; it is growing as new data is added. The DOI refers to the newest available dataset.
DOI: 10.18727/archive/48
title: PIONIER reduced data obtained by IPAG pipeline processing

description: This is a release of processed data from the PIONIER interferometric instrument at ESO's VLTI. The instrument modes covered are all modes offered for service, currently including modes FREE_H and GRISM_H. The data are processed by IPAG with the PNDRS pipeline (Le Bouquin, J.- B., Berger, J.-P., Lazareff, B., et al. 2011, AAP 535, AA67) and calibrated using stars listed in the JSDC catalog (Lafrasse, S., Guillaume, M., Bonneau, et al. 2010, Proceedings of the SPIE, Vol. 7734, 4E). The calibrated data can be used to fit models of stellar sources, including stellar diameters and shapes, disks and companions, to name a few. Larger data sets for individual targets may also be used to produce maps independent of specific source models (image reconstruction). This release is an open stream release.
description: This is a dynamic dataset; it is growing as new data is added. The DOI refers to the newest available dataset.
DOI: 10.18727/archive/49
title: SUPER: a SINFONI Survey for Unveiling the Physics and the Effect of Radiative feedback

description: SUPER (http://www.super-survey.org) is an ESO Large Programme (196.A-0377) using SINFONI in Seeing-Enhancer mode to study Active Galactic Nuclei at z=2-2.5. The AO assisted observations reach a PSF of 0.2 arcsec in H band. This first data release concerns the Type-1 AGN, which roughly corresponds to half of the survey sample (20/39). We release flux calibrated H (or H+K) band cubes, which at those redshifts cover the Halpha and [OIII]5007 lines.
description: This is a dynamic dataset; it is growing as new data is added. The DOI refers to the newest available dataset.
DOI: 10.18727/archive/52
title: UltraVISTA - Ultra Deep Survey with VISTA

description: UltraVISTA is an ultra-deep near-infrared survey of the central region of the COSMOS field.
description: This is a dynamic dataset; it is growing as new data is added. The DOI refers to the newest available dataset.