cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.18727/archive/7
title: Ultra-Deep Ks-band imaging of the HST Frontier Fields (KIFF)

description: This release provides reduced Ks–band mosaics from the “KIFF” project: Ks-band Imaging of the Hubble Frontier Fields. The first two fields, Abell 2744 and MACS-0416, were observed with HAWK-I on UT4 in P92 (092.A-0472) and the second two fields, Abell S1063, and Abell 370, were observed in P95 (095.A-0533). The quality of the final mosaics are quite uniform between all of the survey fields, reaching point source limiting magnitudes of Ks~26.0 (AB, 5σ) and with superb image quality, FWHM~0.”4 for point sources. This data release also includes the two northern Frontier Fields clusters, MACS-0717 and MACS- 1149, which were observed with shorter integrations with the Keck/MOSFIRE instrument in 2015 and 2016. The final mosaics of the 0717 and 1149 fields have image quality ~0.”4 and 0.”5 and reach limiting depths Ks=25.5 and 25.1, respectively. The Ks -band at 2.2 μm crucially fills the gap between the reddest HST filter (1.6 μm ∼ H band) and the Spitzer/IRAC 3.6 μm passband. The deep Ks-band images provide important constraints on both the redshifts and the stellar population properties of galaxies extending well below the characteristic stellar mass across most of the age of the universe, down to, and including, the redshifts of the targeted galaxy clusters (z ~ 0.5).
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/8
title: Kinematics of local thick discs

description: The observing programmes 096.B-0054(A) and 097.B-0041(A) aimed at obtaining deep observations (almost three hours) of eight edge-on nearby galaxies with MUSE with the goal of studying the thick disc chemo-dynamics. Here, the science-ready datacubes are released. The steps of the reduction are 1) reduction of the individual exposures using the standard ESO pipeline, 2) manual alignment of the exposures, and 3) usage of ZAP to remove sky residuals. Details on the observ- ing programme and the data processing can be found at Comerón et al. (2019, A&A, 623, A89).
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/10
title: Dissecting GAs Stripping Phenomena in galaxies with MUSE (GASP)

description: GASP (Gas Stripping Phenomena in galaxies) is an ESO Large Program (196.B-0578) using MUSE in wide-field mode with natural seeing to study a sample of 144 galaxies at z=0.04-0.07 in different environments. The release includes reduced data cubes and fits images with maps of Hα and Hβ emission-line fluxes, Hα radial velocity, average star formation rate in four age bins, luminosity-weighted stellar age and stellar mass density, as well as the integrated 1D spectrum of each galaxy.
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/11
title: The EREBOS project - Studying the influence of substellar objects on late stellar evolution

description: The EREBOS (Eclipsing Reflection Effect Binaries from the OGLE Survey) project is an ESO Large Programme (196.D-0214) using FORS2 in long-slit mode. The sample includes several post-common envelope eclipsing binaries with a hot subdwarf primary and a cool, low-mass companion using time-resolved spectroscopy to derive their radial velocity curve and the atmospheric parameters. The goal of this project is to study the interactions of low-mass stellar and sub-stellar companions with low-mass stars. All targets were selected photometrically from the Optical Gravitational Lensing Experiment (OGLE) survey as eclipsing binaries showing a prominent reflection effect and short orbital periods around 0.1 d. We observed all targets with grism GRIS_1200B+97, which covers a wavelength range from 366-511 nm. We always used a 1’’ slit, which results in a resolution R = 1420. In this data release 1 we publish a target catalogue with the coordinates, magnitudes and orbital periods derived from the OGLE survey together with the reduced 1D spectra. Additionally, also the reduced 2D spectra and finding charts of each target are attached as auxiliary files. A catalogue of all individual spectra including the epochs of the observations in HJD and the corresponding orbital phases is released as well.
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/12
title: A MUSE survey of the dense halo gas in z~3 galaxies near optically-thick absorbers

description: This is data release is concerned with MUSE cubes obtained in quasar fields at z~3-4.5 as part of the Large Programme ID 197.A-0384, aimed at studying the distribution of gas around galaxies. For each field, we release the final coadded data cubes totaling ~4 hours of on source observations using the extended wavelength mode. Data have been reduced with the ESO/MUSE pipeline via the Esorex Recipe Execution Tool and are released jointly with the associated white-light images.
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/13
title: Near-IR Imaging of the Galaxy Cluster XMMU J2235.3-2557

description: Deep HAWK-I J and Ks imaging of the X-ray luminous galaxy cluster XMMU J2235.3-2557. The observations consisted of a mosaic of four pointings in two filters, with the centre of the cluster imaged in the four extreme corners of the HAWK-I detector mosaic. The fully processed images contiguously cover a 13’ by 13’ region at a pixel scale of 0.1065”. The image quality varies from 0.3” to 0.7” depending on filter and location. Data were taken under ESO programme ID 60.A-9284(H) as part of the first HAWK-I science verification run from 05-10-2007 to 15-10-2007.
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/14
title: MUSE view of the Seyfert galaxy NGC 7130

description: The release consists of MUSE datacube taken during commissioning and science verification on NGC 7130. The observing programmes are 60.A-9100(K) and 60.A-9493(A), respectively. All the exposures for which the angular resolution was better than 0.2 arcsec were included. The steps of the reduction are 1) reduction of the individual exposures using the standard ESO pipeline, and 2) manual alignment of the exposures. Details on the observing programme and the data processing can be found at Comerón et al. (2021, accepted in A&A, arXiv:2011.02937).
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/15
title: Accretion Discs in Halpha with OmegaCam

description: This describes the released ADHOC images and source catalogues. This release includes reduced images and single-band source lists of the star forming regions Orion A and Gamma Vel. The scientific goal of the ADHOC project is to study the star formation history of the several star forming regions using homogeneous wide fields multi band data, including u, g, r, i and Halpha.
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/16
title: APEX Low-redshift Legacy Survey of MOlecular Gas

description: The APEX Low-redshift Legacy Survey for MOlecular Gas (ALLSMOG) is a survey of CO J=2-1 (rest frame frequency, 230.538 GHz) line emission in a sample of 88 galaxies in the local Universe (programme no. E-192.A- 0359). This sample is well characterized in terms of several derived and measured physical properties (star- formation rates, stellar masses, gas-phase metallicities, and atomic HI gas masses). The primary goal of ALLSMOG is to add information on the cold molecular gas content of these galaxies derived from the low-J CO line emission in order to determine the impact of the gas content on the inferred galaxy properties. The programme lasted for five semesters (P92 to P96) and consumed 327 hours of APEX observing time. The goal of the survey was to reach a CO J=2-1 line peak-to-rms ratio of, S/N&gt;3 for the detections, and an uniform rms of 0.8 mK (31.2 mJy) per 50 km/s channel for the non-detections. Multi-epoch observations of the same source were merged together to produce a single CO J=2-1 spectrum for each target. This document describes the data release of the final reduced ALLSMOG dataset, including both detections and non-detections. <br><br> The data release and analysis is described in more detail in Cicone et al. (2017, A&A, 604, 53; https://ui.adsabs.harvard.edu/abs/2017A%26A...604A..53C/abstract) and Bothwell et al (2014, MNRAS, 445, 2599, https://ui.adsabs.harvard.edu/abs/2014MNRAS.445.2599B/abstract).
description: This is a dynamic dataset; it is growing as new data is added. The DOI refers to the newest available dataset.
DOI: 10.34740/kaggle/dsv/3651804
title: Character
DOI: 10.18727/archive/17
title: AMAZE - Assessing the Mass-Abundance redshift Evolution

description: AMAZE (Assessing the Mass-Abundance redshift[-Z] Evolution) is an ESO large program aimed at determining the mass-metallicity relation and galaxy dynamics in the redshift range 3&lt; z &lt; 5. Observations have been performed with SINFONI, the near-IR integral field spectrometer at VLT, for a total of 180 h, distributed in three semesters under the program ID 178.B-0838 (A) (B) (C), PI: R. Maiolino. SINFONI was used in seeing-limited mode, with the 0.125"x0.25" pixel scale and the H+K grism, yielding a spectral resolution R ∼1500 over the spectral range 1.45 − 2.41 μm. The two-dimensional spectroscopic capabilities of SINFONI are exploited to map the emission lines. The main goal of the SINFONI observations is to determine the gas metallicities by means of a combination of strong line diagnostics based on Hβ and [OIII]5007 redshifted into the K band, as well as [OII]3727 and [NeIII]3870 redshifted into the H band for sources at 3 &lt; z &lt; 4. At 4 &lt; z &gt; 5.2 we only rely on the [OII]/[NeIII] ratio observed in the K band. The spectral resolution is also high enough to trace galaxy kinematics in most 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/19
title: APEX legacy data processed by the APEX science operations team

description: The APEX-SciOps Phase 3 collection is a project that starts from public observations and, by applying a standard calibration process, delivers science ready APEX data to the community via the ESO Archive.
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/20
title: ATLASGAL - APEX Large Area Survey of the Galaxy

description: The APEX Telescope Large Area Survey of the Galaxy (ATLASGAL) is an imaging survey covering 420 sq. deg. of the inner Galactic plane at a wavelength of 870 μm. The observations were carried out between 2007 and 2010, using the LABOCA bolometer array at the APEX telescope, located at 5100m in Llano de Chajnantor, in the Atacama desert. The noise level reached is typically 60 mJy/beam, with an angular resolution of 19''. In total, this survey required more than 400 hours of telescope time. The continuum emission detected at this wavelength mostly originates from cold interstellar dust. These data reveal thousands of compact, dusty clumps, as well as the large-scale structure of the interstellar medium. The current release consists of emission maps covering the full area surveyed, split in 3x3 sq. deg. tiles. A second set of images, where the LABOCA data have been combined with the results of the Planck satellite, is also available. In addition, two compact source catalogs, extracted with two different methods, are provided.
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/21
title: ESPRESSO reduced data obtained by standard ESO pipeline processing

description: This is the release of reduced spectra from the high-resolution echelle spectrograph ESPRESSO. This release is an open stream release. It is complete from start of operations on 24th October 2018 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 have been reduced using the ESPRESSO pipeline version 2.2.1 or higher. It includes extraction of the spectrum, flat fielding, wavelength calibration, and flux calibration. Sky subtraction is only performed if fibre B is placed on sky. If the science target is not a QSO then an automated cross correlation with a stellar reference mask is executed in order to calculate the radial velocity (RV) of the observed object. Please note that systematic shifts of the RV values can occur between different versions of the pipeline. It is highly recommended to use only products from the same pipeline version for RV studies.
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/22
title: ESSENCE/FORS1 High-z Type Ia Supernovae

description: The ESSENCE Survey was initiated to determine the nature of the "dark energy" that causes the accelerated expansion of the universe by determining its equation-of-state parameter, w. It aims to answer a simple, but very important, question: is the dark energy of the universe consistent with a cosmological constant (w=-1)? If not, this means the dark energy must be a more general energy field such as "quintessence." Over the six-year period of the survey (2002-2007) we have discovered and followed-up ~200 Type Ia supernovae (SNe Ia) over a large redshift range (out to z~0.8). To properly identify these SNe Ia and determine their redshift, we have carried out optical long-slit spectroscopy using the FORS1 instrument of the VLT at ESO's Cerro Paranal Observatory, Chile.
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/23
title: Fornax Deep Survey

description: We present the catalog of ugri-bands photometry and morphometry for ∼1.7 million sources over the ∼21 square degree area of the Fornax deep survey (FDS) centered on the bright central galaxy NGC 1399. For a wider area, of ∼27 square degrees extending in the direction of NGC 1316, we provide gri photometry for ∼3.1 million sources. FDS is a survey carried out with the OMegaCAM camera on the VST telescope, and is a joint project that used the GTO time of NOVA (PI. R.F. Peletier) and the INAF survey VEGAS (PI. M. Capaccioli & E. Iodice). To improve the morphological characterization of sources, we generated multi-band image stacks by coadding the best-seeing gri-band single exposures with a cut at full width at half maximum FWHM≤0.9 arcsec. The final catalog contains: (i) source identification and position from the multi-band stacks; (ii) the calibrated and aperture corrected AB magnitudes derived from PSF photometry in all available bands; (iii) the uncorrected aperture and Kron-like magnitudes in all bands; (iv) the morphometric parameters (FWHM, CLASS_STAR, concentration index, flux radius, elongation and sharpness) for the multi- band stacks, as well as the latter for all other available bands. In addition to the photometry for the data available in the FDS image repository, the present release contains images and weight maps for the FDS field n. 8. The reference publication, with all the required details on the present catalog, is Cantiello et al. (2020, A&A 639, A136).
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/24
title: FEROS reduced data obtained by standard ESO pipeline processing

description: This is the release of reduced 1-D spectra from the FEROS (Fibre-fed Extended Range Optical Spectrograph) at the ESO La Silla 2.2m telescope. The products were generated with FEROS pipeline run in a fully automated, unsupervised way. The release covers practically all FEROS science data since November 2003 (ESO Period 72).
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/25
title: Gaia-ESO spectroscopic survey

description: Gaia-ESO is a large public spectroscopic survey carried out with FLAMES, targeting ≥ 105,000 stars, systematically covering all major components of the Milky Way, from halo to star-forming regions, providing the first homogeneous overview of the distributions of kinematics and elemental abundances. The MW targets survey the Bulge, Halo, Thick Disc and Thin Disc populations of the Milky Way. Three primary instrumental setups were used for these observations: UVES 580 for brighter objects and Giraffe HR10 and HR21 for fainter ones. For the Bulge survey observations of K giants were carried out for the brighter objects (GK stars) using UVES 580, otherwise Giraffe HR10 and/or HR21 were used. For the Halo/Thick disc survey, the primary targets are F+G stars, where bluer fainter F stars probe the halo, and brighter F/G stars probe the thick disc. The outer thick disc is probed using distant F/G stars, as well as K giants to sample the far outer disc. For the solar neighbourhood, G stars were observed using UVES 580 only.
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/26
title: GCAV - Galaxy Clusters At Vircam

description: The GCAV Programme aims at observing 20 massive galaxy clusters which have also been observed in many ground based and spaced based programs (e.g. CLASH, RELICS, HFF/ BUFFALO).
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/27
title: GIRAFFE/MEDUSA reduced data obtained by standard ESO pipeline processing

description: This is the release of reduced 1D spectra from the FLAMES/GIRAFFE1 spectrograph, taken in the MEDUSA mode. It is an open stream release, it includes the so far observed GIRAFFE MEDUSA data and will be continued into the future operational lifetime. The data content will grow with time as new data are being acquired and processed (approximately with monthly cadence and with a short delay of 1 or 2 months). The processing scheme is as homogeneous as possible. The release covers all GIRAFFE MEDUSA data starting from the begin of operations, 2003-04-13, until now.
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.6555628
title: Dataset für Präsentation: Baur (2022) Retter in der Not? Die Rolle der Naturhistorischen Museen bei der universitären Vermittlung von Artenkenntnissen am Beispiel von Bern

description: Tabelle mit allen Kursen für das Frühlings- und Herbstsemester 2022 an der Universität Bern in den Fächern Biologie, Ökologie und Evolution sowie Pflanzenwissenschaften. Die Tabelle ist sowohl im Excel XLSX Format als auch im CSV Format verfügbar und diente als Grundlage für die folgende Präsentation: Baur, Hannes. (2022, May 13). Retter in der Not? Die Rolle der Naturhistorischen Museen bei der universitären Vermittlung von Artenkenntnissen am Beispiel von Bern. Zenodo. https://doi.org/10.5281/zenodo.6557500 (sehen Sie auch unten in der Sektion 'References'). <strong>Zitierung</strong><br> Benutzen Sie die vorgeschlagene Zitierung (auf dieser Webseite). <strong>Kontakt</strong><br> Hannes Baur
description: {"references": ["Baur H (2022) Retter in der Not? Die Rolle der Naturhistorischen Museen bei der universit\u00e4ren Vermittlung von Artenkenntnissen am Beispiel von Bern. https://doi.org/10.5281/zenodo.6554280"]}
DOI: 10.5281/zenodo.6555627
title: Dataset für Präsentation: Baur (2022) Retter in der Not? Die Rolle der Naturhistorischen Museen bei der universitären Vermittlung von Artenkenntnissen am Beispiel von Bern

description: Tabelle mit allen Kursen für das Frühlings- und Herbstsemester 2022 an der Universität Bern in den Fächern Biologie, Ökologie und Evolution sowie Pflanzenwissenschaften. Die Tabelle ist sowohl im Excel XLSX Format als auch im CSV Format verfügbar und diente als Grundlage für die folgende Präsentation: Baur, Hannes. (2022, May 13). Retter in der Not? Die Rolle der Naturhistorischen Museen bei der universitären Vermittlung von Artenkenntnissen am Beispiel von Bern. Zenodo. https://doi.org/10.5281/zenodo.6557500 (sehen Sie auch unten in der Sektion 'References'). <strong>Zitierung</strong><br> Benutzen Sie die vorgeschlagene Zitierung (auf dieser Webseite). <strong>Kontakt</strong><br> Hannes Baur
description: {"references": ["Baur H (2022) Retter in der Not? Die Rolle der Naturhistorischen Museen bei der universit\u00e4ren Vermittlung von Artenkenntnissen am Beispiel von Bern. https://doi.org/10.5281/zenodo.6554280"]}
DOI: 10.18727/archive/28
title: The Great Observatories Origins Deep Survey - VLT/FORS2 Spectroscopy

description: As part of the Great Observatories Origins Deep Survey (GOODS), multi-object, optical to NIR spectroscopy in the Chandra Deep Field South (CDF-S) has been carried out, using the FORS2 instrument mounted at the Kueyen Unit Telescope of the VLT at ESO's Cerro Paranal Observatory, Chile. This release accumulates 1715 spectra of 1225 unique targets which have been obtained with the FORS2 spectrograph between September 2002 and October 2006, providing in total 1165 redshift measurements. The average of the redshift distribution (z&gt;0) is z=1.666 (median z=1.158). The typical error in the redshift determination (of course it depends on the S/N of the spectrum) is in general +/-0.001 as we calculated in the paper II (A&A 454, 423-435 (2006)) by comparing the redshift of sources in common with other spectroscopic surveys. This release provides the full set of extracted 1-dimensional fits spectra in the GOODS/FORS2 survey and associated spectral previews and colour image cutouts (5"x5") for each target. Furthermore, a catalogue is provided where we give for each target the basic ACS image information such as magnitude (in the AB system) and colours as well as the measured redshift and associated comments.
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/29
title: The Great Observatories Origins Deep Survey - VLT/ISAAC NIR imaging

description: As part of the Great Observatories Origins Deep Survey (GOODS), near-infrared imaging observations of the Chandra Deep Field South (CDF-S) were carried out in J, H, Ks bands, using the ISAAC instrument mounted at the Antu Unit Telescope of the VLT at ESO's Cerro Paranal Observatory, Chile. This data release includes 26 fully reduced and calibrated VLT/ISAAC fields in J and Ks bands, and 24 fields in H band, covering 172.4, 159.6, and 173.1 arcmin2 of the GOODS/CDF-S region, respectively, as well as three mosaics in J, H and Ks. More than 50% of the images reach a 5-sigma depth for point sources of at least 25.2 mag (J), 24.7 mag (H and Ks) in the AB system ("median depth").
description: This is a dynamic dataset; it is growing as new data is added. The DOI refers to the newest available dataset.