cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.25574/csc2.stk.acisfj1624227m455454_001
title: Chandra X-ray Observatory Stack acisfJ1624227m455454_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25919/58by-et19
title: Parkes observations for project P1345 semester 2024OCTS_12

description: This proposal aims to obtain timing solutions and constrain burst rates and spin down properties of a sample of new rotating radio transients (RRATs) discovered with the ASKAP CRAFT Coherent upgrade (CRACO) system. 
 In the last 6-months of commissioning, CRACO discovered and localised 10 new RRATs, identified by their sporadic pulses with dispersion measures (DM) consistent with Galactic objects. 
 
 We request 15h of Parkes time split into three 30min observations spanning 6-months for each target. 
 This will allow us to constrain phase-coherent timing solutions given that we already have arcsec-precision interferometric localisations. 
 Our main science goals are: 
 1) to measure their burst rates, periods, and spin-down properties; 
 2) to assess their nulling fraction and emission mechanism
 3) to determine if the CRACO RRATs are different to the known RRATs population.
DOI: 10.25919/e3a9-2a55
title: Parkes observations for project P1054 semester 2024OCTS_11

description: With this proposal we ask time to continue our timing follow-up campaign of pulsars discovered with the MeerKAT telescope. Thirtysix sources have been discovered in targeted observations of Fermi unidentified point sources, two in association with a Supernova Remnant, 14 in the Magellanic Clouds, 94 in Globular Clusters and 81 in a survey of the Galactic plane. A large fraction of the new discoveries are recycled pulsars (including at least one double neutron star system and several 'spider' binaries), or young pulsars. Timing observations have an essential role in exploiting the full potential of any pulsar discovery, allowing the precise measurement of rotational, astrometric and orbital parameters which, in turn, give us powerful tools to improve our understanding of the physics in extreme environments as well as of the population of neutron stars as a whole. The UWL receiver of the Parkes telescope is a sensitive, versatile instrument that is allowing us to successfully time these new sources, in the bright-end of TRAPUM discoveries.
DOI: 10.25919/twt0-1g40
title: Parkes observations for project P1345 semester 2024OCTS_11

description: This proposal aims to obtain timing solutions and constrain burst rates and spin down properties of a sample of new rotating radio transients (RRATs) discovered with the ASKAP CRAFT Coherent upgrade (CRACO) system. 
 In the last 6-months of commissioning, CRACO discovered and localised 10 new RRATs, identified by their sporadic pulses with dispersion measures (DM) consistent with Galactic objects. 
 
 We request 15h of Parkes time split into three 30min observations spanning 6-months for each target. 
 This will allow us to constrain phase-coherent timing solutions given that we already have arcsec-precision interferometric localisations. 
 Our main science goals are: 
 1) to measure their burst rates, periods, and spin-down properties; 
 2) to assess their nulling fraction and emission mechanism
 3) to determine if the CRACO RRATs are different to the known RRATs population.
DOI: 10.25574/csc2.stk.acisfj1624548p375814_001
title: Chandra X-ray Observatory Stack acisfJ1624548p375814_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1625124p154632_001
title: Chandra X-ray Observatory Stack acisfJ1625124p154632_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1613096p543338_001
title: Chandra X-ray Observatory Stack acisfJ1613096p543338_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1625311m242519_001
title: Chandra X-ray Observatory Stack acisfJ1625311m242519_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1612436m522538_001
title: Chandra X-ray Observatory Stack acisfJ1612436m522538_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1613056p540938_001
title: Chandra X-ray Observatory Stack acisfJ1613056p540938_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1639096p282455_001
title: Chandra X-ray Observatory Stack acisfJ1639096p282455_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1614096m630651_001
title: Chandra X-ray Observatory Stack acisfJ1614096m630651_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1522547p253158_001
title: Chandra X-ray Observatory Stack acisfJ1522547p253158_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1627179m243424_001
title: Chandra X-ray Observatory Stack acisfJ1627179m243424_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1517409m242251_001
title: Chandra X-ray Observatory Stack acisfJ1517409m242251_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1626551p551339_001
title: Chandra X-ray Observatory Stack acisfJ1626551p551339_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1626354m515622_001
title: Chandra X-ray Observatory Stack acisfJ1626354m515622_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1641419p362741_001
title: Chandra X-ray Observatory Stack acisfJ1641419p362741_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1504596p260139_001
title: Chandra X-ray Observatory Stack acisfJ1504596p260139_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1506022p013829_001
title: Chandra X-ray Observatory Stack acisfJ1506022p013829_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1614196m190643_001
title: Chandra X-ray Observatory Stack acisfJ1614196m190643_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1627510m593652_001
title: Chandra X-ray Observatory Stack acisfJ1627510m593652_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1630188m124031_001
title: Chandra X-ray Observatory Stack acisfJ1630188m124031_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1641286m490015_001
title: Chandra X-ray Observatory Stack acisfJ1641286m490015_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1627514m291648_001
title: Chandra X-ray Observatory Stack acisfJ1627514m291648_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1635071m473419_001
title: Chandra X-ray Observatory Stack acisfJ1635071m473419_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1628255m243248_001
title: Chandra X-ray Observatory Stack acisfJ1628255m243248_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1635532p661504_001
title: Chandra X-ray Observatory Stack acisfJ1635532p661504_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1643491p410248_001
title: Chandra X-ray Observatory Stack acisfJ1643491p410248_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1657078m040552_001
title: Chandra X-ray Observatory Stack acisfJ1657078m040552_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1628296p115425_001
title: Chandra X-ray Observatory Stack acisfJ1628296p115425_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1522238p274034_001
title: Chandra X-ray Observatory Stack acisfJ1522238p274034_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1631593p243757_001
title: Chandra X-ray Observatory Stack acisfJ1631593p243757_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1635533m473452_001
title: Chandra X-ray Observatory Stack acisfJ1635533m473452_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1726551p855355_001
title: Chandra X-ray Observatory Stack acisfJ1726551p855355_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1618129m505821_001
title: Chandra X-ray Observatory Stack acisfJ1618129m505821_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1709302m443049_001
title: Chandra X-ray Observatory Stack acisfJ1709302m443049_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1628587p400741_001
title: Chandra X-ray Observatory Stack acisfJ1628587p400741_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1647193p322752_001
title: Chandra X-ray Observatory Stack acisfJ1647193p322752_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1628413m352238_001
title: Chandra X-ray Observatory Stack acisfJ1628413m352238_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1636020m474835_001
title: Chandra X-ray Observatory Stack acisfJ1636020m474835_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25318/3410023401-fra
title: Propriétaires publics dont le système de traitement des eaux usées doit être amélioré pour satisfaire aux normes de qualité des effluents du Règlement fédéral sur les effluents des systèmes d’assainissement des eaux uses, Infrastructure Canada, inactif

description: Propriétaires publics dont le système de traitement des eaux usées doit être amélioré. Les données sont disponibles pour toutes les provinces et territoires. Les données sont présentées pour 2016. Les données sont présentées en nombres et pourcentages.
DOI: 10.25574/csc2.stk.acisfj1636379m465938_001
title: Chandra X-ray Observatory Stack acisfJ1636379m465938_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1640432m464846_001
title: Chandra X-ray Observatory Stack acisfJ1640432m464846_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1620045m200355_001
title: Chandra X-ray Observatory Stack acisfJ1620045m200355_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1638097p115114_001
title: Chandra X-ray Observatory Stack acisfJ1638097p115114_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1521001p505330_001
title: Chandra X-ray Observatory Stack acisfJ1521001p505330_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1630233p243555_001
title: Chandra X-ray Observatory Stack acisfJ1630233p243555_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1507597m162427_001
title: Chandra X-ray Observatory Stack acisfJ1507597m162427_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1524137m315309_001
title: Chandra X-ray Observatory Stack acisfJ1524137m315309_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1617360m510927_001
title: Chandra X-ray Observatory Stack acisfJ1617360m510927_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1639563m465757_001
title: Chandra X-ray Observatory Stack acisfJ1639563m465757_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1508418p332745_001
title: Chandra X-ray Observatory Stack acisfJ1508418p332745_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1649205p510136_001
title: Chandra X-ray Observatory Stack acisfJ1649205p510136_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1633181p352005_001
title: Chandra X-ray Observatory Stack acisfJ1633181p352005_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1509238m585151_002
title: Chandra X-ray Observatory Stack acisfJ1509238m585151_002

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.stk.acisfj1617309m505532_001
title: Chandra X-ray Observatory Stack acisfJ1617309m505532_001

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".