cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.18727/archive/53
title: VANDELS - A deep VIMOS survey of the CANDELS UDS and CDFS fields

description: The VANDELS survey used the VIMOS spectrograph on ESO’s VLT to obtain ultra-deep, medium resolution, optical spectra of galaxies within the UKIDSS Ultra Deep Survey (UDS) and Chandra Deep Field South (CDFS) survey fields (0.2 sq. degree total area). Using robust photometric redshift pre-selection, VANDELS targeted ~2100 galaxies in the redshift interval 1.0 &lt; z &lt; 7.0, with 85% of its targets selected to be at a redshift greater than 3. In addition, VANDELS targeted a substantial number of passive galaxies in the redshift interval 1.0 &lt; z &lt; 2.5. Exploiting the red sensitivity of the refurbished VIMOS spectrograph, the survey obtained ultra-deep optical spectroscopy with the VIMOS MR grism and GG475 order-sorting filter, which covers the wavelength range 4800-10000Å at a dispersion of 2.5 Å/pix and a spectral resolution of R~600. Each galaxy received between a minimum of 20-hours and a maximum of 80-hours of on-source integration time. The fundamental aim of the survey was to provide the high signal-to-noise spectra necessary to measure key physical properties such as stellar population ages, metallicities and outflow velocities from detailed absorption-line studies. By targeting two extra-galactic survey fields with superb multi-wavelength imaging data, VANDELS was designed to produce a unique legacy dataset for exploring the physics underpinning high-redshift galaxy evolution.
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/54
title: VST survey of Early-type GAlaxieS (VEGAS)

description: VEGAS is a deep multi-band (u’g’r’i’) imaging survey, carried out with the ESO VLT Survey Tele- scope (VST). VST is a 2.6-m wide-field optical survey telescope, located at ESO Paranal Observatory (Chile). First VEGAS observations started in October 2011 (former PI: M. Capaccioli,). Later the program was approved for an extension to the period 2016-2021 (PI: E. Iodice). The whole VEGAS sample is made by selecting groups and clusters of galaxies with an early-type galaxy in the core brighter than MB = −21 mag, in the local volume within 54 Mpc/h, mainly located in the Southern hemisphere.
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/55
title: VEILS - The VISTA Extragalactic Infrared Legacy Survey

description: The VISTA Extragalactic Infrared Legacy Survey (VEILS; Program ID:198.A-2005) is a deep J and Ks-band transient and wide-field survey being conducted using the VIRCAM camera with the primary goals of understanding the epoch of reionisation, the build-up of massive galaxies, and constraining the cosmological equation of state using both Type 1a supernovae and AGN dust lag measurements. VEILS is covering 9 sq-deg of the extragalactic sky over three fields: ES1 (RA=00h30m, Dec=-43d00m), CDFS (RA=03h36m, Dec=-28d00m) and XMM-LSS (RA=02h22m, Dec=-06d00m). Each field requires two separate pointings of the camera to image. A total of 14-16 epochs are required per year per field for the transient science and by the end of the survey we expect around 30-40 epochs of observations per field.
description: This is a dynamic dataset; it is growing as new data is added. The DOI refers to the newest available dataset.
DOI: 10.18727/archive/58
title: VIDEO - VISTA Deep Extragalactic Observations Survey

description: VIDEO is a deep near-­infrared survey which targets ~12 square degrees over the ELAIS-­‐S1, XMMLSS, and ECDFS extragalactic fields. We recommend using only those sources with Ks&lt;23.5 for most studies as this gives a completeness of ~90 per cent (Jarvis et al. 2013, MNRAS, 428, 1281).
description: This is a dynamic dataset; it is growing as new data is added. The DOI refers to the newest available dataset.
DOI: 10.5203/nwfd-2n12
title: fortwhyte-alive-model-watershed-project
DOI: 10.18727/archive/59
title: VIKING - VISTA Kilo-degree Infrared Galaxy Survey

description: The VIKING survey with VISTA (ESO programme ID 179.A-2004) is a wide area (covering a final area of 1350 sq.degrees), intermediate-depth (5-sigma detection limit J∼21 on Vega system) near-infrared imaging survey, in the five broadband filters Z, Y, J, H, Ks.The sky coverage is at high galactic latitudes, and includes two main stripes ∼ 70 × 10◦ each: one in the South Galactic cap near Dec∼ −30◦, and one near Dec∼0◦ in the North galactic cap; in addition, there are two smaller outrigger patches called GAMA09 and CFHLS-W1. Science goals include z &gt;6.5 quasars, extreme brown dwarfs, and multiwavelength coverage and identifications for a range of other imaging surveys, notably VST-KiDS and Herschel-ATLAS.
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/60
title: VIMOS reduced data obtained by standard ESO pipeline processing

description: This is the release of reduced data from the VIMOS imager from the beginning of regular operation (April 2003) until the instrument decommissioning (March 2018). This data set contains all of the science observations done using the VIMOS instrument in imaging mode. These are not part of a single self-contained project or survey. Rather they contain observations from many different projects and surveys, using various filters and observing methods. The distribution of fields is obviously governed by the time of year in which the observations were taken.
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/61
title: VINROUGE - VIsta Near-infraRed Observations Unveiling Gravitational wave Events

description: The data released here were obtained with the VIRCAM instrument on VISTA under programme 198.D-2010. They consist of Y, J & Ks band imaging, and their associated object catalogues, of portions of the error regions for gravitational wave events found during the second LIGO/Virgo science run, O2. Specifically, the events triggered on were the binary black hole mergers GW170809 (~17 sq-deg), GW170814 (~27 sq-deg) and the binary neutron star merger GW170817 (~3.5 sq- deg). For the latter case, the kilonova counterpart of the merger was identified in the second field observed on the first night, and thereafter this field was re-observed for 14 further epochs over the subsequent ~3 weeks. The primary goals of the VINROUGE survey are to locate and characterize the electromagnetic counterparts of gravitational wave discovered events. This is achieved through wide field, multi-filter imaging of the error regions with VIRCAM on VISTA.
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/62
title: VIPERS - The VIMOS Public Extragalactic Redshift Survey

description: The VIPERS redshift survey is the result of a Large Programme (182.A-0886). This data release includes the final redshift catalogue, corresponding to 91,507 spectroscopic measurements, of which 86,775 are galaxies, distributed over two equato- rial areas of sky centered around RA=22 hrs and RA=2 hrs. The data provide an unprecedented sampling (in terms of volume and statistics) of galaxies and large-scale structure at 0.5 &lt; z &lt; 1.2. The PDR-2 is the first data release hosted by ESO; a partial set of VIPERS data (PDR-1) has been distributed in 2013 only trough the VIPERS website (http://vipers.inaf.it).
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/64
title: VMC - VISTA Magellanic Survey

description: Observations were obtained with the VISTA telescope as part of the VISTA survey of the Magellanic Cloud system (VMC; ESO program 179.B-2003) in three filters: Y, J and Ks. The main goals of the VMC survey are the determination of the spatially resolved star formation history and the three- dimensional geometry of the Magellanic system. The sensitivity of the data is designed to reach sources below the oldest main-sequence turn off point of the stellar population and the multi-epochs to measure accurate Ks mean magnitudes for pulsating variable stars, e.g. RR Lyrae stars and Cepheids.
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/65
title: VPHAS+ - VST Photometric H-a Survey of the Southern Galactic Plane

description: The primary goal of the VST Photometric Halpha Survey of the Southern Galactic Plane and Bulge (VPHAS+) was to collect single-epoch ugri broad-band and Ha narrow-band photometry across the southern Galactic Plane within the latitude range -5 &lt; b &lt; +5 deg, down to point source magnitudes of ~21 or better. For reasons of resource limitations, the survey terminated in August 2018, omitting some parts of the 4th Galactic quadrant. The VPHAS+ footprint expands to include the inner Galactic Bulge, defined as a 20 x 20 deg2 box around the Galactic Centre. For all massive OBA stars this survey is deep enough to explore all but the most heavily obscured locations of the southern Plane, reaching up to 10 kpc from the Sun. The narrowband data yield a uniform view of southern emission line stars, giving more robust statistics on important scarce object types. The wide-area broadband photometry obtained can facilitate stellar population studies, tracing structure over much of the southern Plane. VPHAS+ data are also suited to trawling the star-formation history of the Galaxy as seen in stellar remnants of all types. More information on the four VPHAS+ data releases can be obtained from https://www.vphasplus.org/data.shtml. Releases 1, 2 and 4 at the ESO archive contain CASU-processed files, while release 3 includes tiles generated by WFAU, Edinburgh.
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/66
title: The VST Atlas Survey

description: The ATLAS survey is particularly aimed at survey cosmology but can be exploited for many other branches of extragalactic and Galactic astron- omy. Its wide wavelength coverage from the u to the z bands complements the VISTA Hemisphere and VIKING Surveys in the YJHK bands. A full description of the ATLAS survey is given by Shanks et al (2015, MNRAS, 451, 4238). The passbands covered are the SDSS u,g,r,i,z bands reaching ap- proximately the same depth (r~22.5) as the SDSS survey in the Northern Hemisphere. Median FWHM seeing ranges from 0.8arcsec in i,z to 1.1arcsec in u.
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/67
title: VVV - VISTA Variables in the Via Lactea Survey

description: Vista Variables in the Via Lactea (VVV) is a public IR variability survey of the Milky Way bulge and an adjacent section of the mid-plane where star formation activity is high. It performed wide FOV multi-epoch observations of the Galaxy’s bulge and part of the disk, providing the astronomical public community with a high resolution 3-D (or 4-D if you include the time dimension) map of the bulge.
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/69
title: Quasars and their absorption lines: a legacy survey of the high-redshift universe (XQ-100)

description: The Large Programme “Quasars and their absorption lines: a legacy survey of the high-redshift universe with VLT/XSHOOTER” (ID 189.A-0424, hereafter ‘XQ-100’) has produced a homogeneous and high-quality sample of echelle spectra of 100 QSOs at redshifts z ~ 3.5–4.5 observed with full spectral coverage from 315 to 2500 nm. XQ-100 is the largest spectroscopic survey to date of high-redshift QSOs with simultaneous rest-frame UV/optical coverage, and as such enables a wide range of extra- galactic research, from cosmology and galaxy evolution to AGN astrophysics (López et al. 2016, A&A, 594, 91L).
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/70
title: XSGRB afterglow sample

description: This release is the XS-GRB sample of Gamma-Ray Burst (GRB) afterglows. It consists of spectra of 103 individual afterglows observed within 48 hours of the GRB trigger and a few late-time host observations, included for completeness. Redshifts have been measured for 97 per cent of these, covering a redshift range from 0.059 to 7.84. These X-shooter spectra have been taken during a period of eight years corresponding to the ESO observing periods P84 through P98. This dataset provides a unique resource to study the ISM across cosmic time, from the local progenitor surroundings to the intervening universe. The data and scope are described in Selsing et al. (2019, A&A, 623, 92S).
description: This is a dynamic dataset; it is growing as new data is added. The DOI refers to the newest available dataset.
DOI: 10.6084/m9.figshare.19780153
title: Dataset_Sadovy de Mitcheson et al 2022_mandarinfish

description: Dataset from "<strong>Mating system in a small pelagic spawner: field case study of the mandarinfish, </strong><em><strong>Synchiropus splendidus", </strong></em>de Mitcheson et al. 2022.
DOI: 10.6084/m9.figshare.19780153.v1
title: Dataset_Sadovy de Mitcheson et al 2022_mandarinfish

description: Dataset from "<strong>Mating system in a small pelagic spawner: field case study of the mandarinfish, </strong><em><strong>Synchiropus splendidus", </strong></em>de Mitcheson et al. 2022.
DOI: 10.18727/archive/71
title: XSHOOTER ECHELLE pipeline-reduced spectroscopic data

description: This is the release of reduced 1D spectra from the XSHOOTER spectrograph, ECHELLE (SLIT) mode (as opposed to the IFU mode which is not included). All spectra have been reduced under the assumption of point-like sources. This release is an open stream release, it includes so far archived XSHOOTER data and will be continued into the future. The processing scheme is as homogeneous as possible. The selected data cover the vast majority of the entire XSHOOTER data archive, from the begin of operations in October 2009 until present.
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/72
title: X-Shooter Spectral Library (XSL)

description: The XSL (X-shooter Spectral Library) project aims to build a new, moderate-resolution stellar spectral library for use in stellar population modelling. The spectra are flux-calibrated and telluric-corrected. The wavelength coverage, spectral resolution, and spectral type of this library make it well suited to stellar population synthesis of galaxies and clusters, kinematics investigation of stellar systems, and the study of the physics of cool stars.
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/73
title: zCOSMOS Spectroscopic Redshift Survey

description: zCOSMOS (P.I. Simon Lilly) is a large redshift survey undertaken in the COSMOS field using the VIMOS spectrograph mounted at the Melipal Unit Telescope of the VLT at ESO's Cerro Paranal Observatory, Chile. The zCOSMOS redshift survey has been designed to efficiently utilize VIMOS by splitting the sur- vey into two parts. The first, zCOSMOS-bright, which is the subject of DR3, aims to produce a red- shift survey of approximately 20,000 I-band selected galaxies at redshifts z &lt; 1.2. Covering the approximately 1.7 deg2 of the COSMOS field (essentially the full ACS-covered area), the trans- verse dimension at z ~ 1 is 75 Mpc. The second part, zCOSMOS-deep, observed a smaller number of galaxies selected to mostly lie at higher redshifts, 1.5 &lt; z &lt; 3.0. The full set of extracted 1-dimensional spectra are being released, plus a catalogue in which for each target the 1-D spectra filenames, the I-band magnitude used for the selection are given, as well as the measured redshift and confidence class. A full description of the survey can be found in Lilly et al. 2007, ApJS, 172, 70, and Lilly et al. 2009, ApJS, 184, 218.
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/74
title: Swift Burst Alert Telescope AGN survey of molecular gas fueling in powerful nearby AGN

description: This data collection contains APEX/SHFI CO(2-1) spectra from a sample of nearby (0.01 &lt; z &lt; 0.05) hard X-ray selected AGN galaxies. The main science goal of the survey was to determine the molecular gas content of these AGN-selected galaxies, and compare them with similar CO(2-1) galaxies from field samples. While this programme was mainly aiming at a statistical sample, many of the galaxies observed are well-known galaxies, and these phase 3 data can provide a valuable total power measurement of the CO(2-1) which can be combined with interferometric observations obtained with ALMA.
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/75
title: SHARKS - Southern H-ATLAS Regions Ks-band Survey

description: SHARKS is a deep Ks-band survey of ~300 square degrees covering large parts of the South Galactic Plane (SGP), GAMA-12h (G12) and GAMA-15h (G15) fields from the H-ATLAS survey, the largest Herschel program. These regions are covered by several optical and near-infrared surveys, including VIKING, HSC and DES, among others, as well as by the future LSST and Euclid. The aim is to reach a 5 sigma magnitude limit of Ks~22.7 mag (AB), for example, to match ~90% of the H-ATLAS sources up to redshift 3.
description: This is a dynamic dataset; it is growing as new data is added. The DOI refers to the newest available dataset.
DOI: 10.5203/xz97-we22
title: government-of-north-dakota-boundaries-from-north-dakota-gis-hub-data-portal
DOI: 10.5517/ccdc.csd.cczjk67
title: CCDC 909639: Experimental Crystal Structure Determination

description: Related Article: Pei-Pei He, Qiao-Yan Xu, Shao-Heng Li, Su-Mu Wei, Hao-Hong Li|2022|CrystEngComm|24|3556|doi:10.1039/D2CE00368F
DOI: 10.5517/ccdc.csd.ccztjq0
title: CCDC 918273: Experimental Crystal Structure Determination

description: Related Article: Pei-Pei He, Qiao-Yan Xu, Shao-Heng Li, Su-Mu Wei, Hao-Hong Li|2022|CrystEngComm|24|3556|doi:10.1039/D2CE00368F
DOI: 10.5517/ccdc.csd.cc2b71j5
title: CCDC 2151726: Experimental Crystal Structure Determination

description: Related Article: Qiling Guo, Tuo Fang, Qian Liu, Liyang Zhu, Suliang Yang, Guoxin Tian|2022|Dalton Trans.|51|7416|doi:10.1039/D2DT00625A
DOI: 10.5517/ccdc.csd.cc2blqth
title: CCDC 2162957: Experimental Crystal Structure Determination

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DOI: 10.5517/ccdc.csd.cc233spq
title: CCDC 1940063: Experimental Crystal Structure Determination

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DOI: 10.5517/ccdc.csd.cc2blqwk
title: CCDC 2162959: Experimental Crystal Structure Determination

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DOI: 10.5517/ccdc.csd.cc233s56
title: CCDC 1940047: Experimental Crystal Structure Determination

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DOI: 10.5517/ccdc.csd.cc233s67
title: CCDC 1940048: Experimental Crystal Structure Determination

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DOI: 10.5517/ccdc.csd.cc233sgh
title: CCDC 1940056: Experimental Crystal Structure Determination

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DOI: 10.5517/ccdc.csd.cc274pdh
title: CCDC 2060086: Experimental Crystal Structure Determination

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DOI: 10.5517/ccdc.csd.cc274pgk
title: CCDC 2060088: Experimental Crystal Structure Determination

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DOI: 10.5517/ccdc.csd.cc274pwz
title: CCDC 2060101: Experimental Crystal Structure Determination

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DOI: 10.5517/ccdc.csd.cc274py1
title: CCDC 2060103: Experimental Crystal Structure Determination

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DOI: 10.5517/ccdc.csd.cc2b7gy0
title: CCDC 2152142: Experimental Crystal Structure Determination

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title: CCDC 2152463: Experimental Crystal Structure Determination

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DOI: 10.5517/ccdc.csd.cc274pcg
title: CCDC 2060085: Experimental Crystal Structure Determination

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title: CCDC 2060110: Experimental Crystal Structure Determination

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title: CCDC 2060104: Experimental Crystal Structure Determination

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title: CCDC 2164215: Experimental Crystal Structure Determination

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title: CCDC 2164266: Experimental Crystal Structure Determination

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title: CCDC 2060098: Experimental Crystal Structure Determination

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title: CCDC 2060084: Experimental Crystal Structure Determination

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