cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.25582/data.2023-03.2758964/2318151
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2758869/2318152
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2759876/2318153
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2759972/2318154
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2760394/2318155
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2758848/2318156
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2758923/2318157
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25919/5c76457234b08
title: Southern Galactic Plane Survey (SGPS) - 1.4GHz Continuum Observations

description: The Southern Galactic Plane Survey (SGPS) was a large-scale project to image at arcminute resolution the H I spectral line and 21 cm continuum emission in parts of the plane of the Milky Way. The survey covered Galactic longitudes 253 deg &lt;= l &lt;= 358 deg and latitudes |b|&lt;=1.5d (SGPS I). The survey combines data from the Australia Telescope Compact Array and the Parkes Radio Telescope for sensitivity to angular scales ranging from 2' to several degrees. The combined data cover 325 deg2 and have an rms sensitivity of 1.6 K. This data set provides an unprecedented view of the neutral component of interstellar hydrogen in the inner Milky Way.

Available here are SGPS continuum images of Stokes I, Q, & U for the region of Galactic longitude, l=253 deg to l=358 deg covering Galactic latitude |b| &lt;= 1.5 deg
DOI: 10.25582/data.2023-03.2760219/2318158
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2760313/2318159
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2760069/2318160
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2760033/2318161
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2759591/2318162
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2759869/2318163
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2758915/2318164
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2759994/2318165
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2758842/2318166
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2760070/2318167
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2760106/2318168
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2758967/2318169
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2758969/2318170
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25919/hb3c-p376
title: ASKAP Data Products for Project AS110 (The Rapid ASKAP Continuum Survey): images and visibilities

description: This observatory led project will cover the whole southern sky to +40 deg Declination with ASKAP. The survey parameters will be such that observations for the entire region should take of order one week, with a target RMS of roughly ~0.25 mJy/beam. Multiple passes will be done to cover ASKAP’s full frequency range and additional epochs of the survey are planned to search for transient sources. This survey will provide a unique opportunity to study the radio sky and radio populations, in particular AGN and their role in galaxy evolution. RACS will produce a global sky model for ASKAP, and test operations from data collection and reduction to release.
DOI: 10.25582/data.2023-03.2758979/2318171
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2758671/2318172
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2759877/2318173
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2759940/2318174
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2758708/2318175
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2759592/2318176
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2760036/2318177
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2758909/2318178
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2760218/2318179
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2759942/2318180
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2758636/2318181
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2759898/2318182
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2758861/2318183
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2759943/2318184
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25919/6mr6-rd83
title: ASKAP Data Products for Project AS110 (The Rapid ASKAP Continuum Survey): images and visibilities

description: This observatory led project will cover the whole southern sky to +40 deg Declination with ASKAP. The survey parameters will be such that observations for the entire region should take of order one week, with a target RMS of roughly ~0.25 mJy/beam. Multiple passes will be done to cover ASKAP’s full frequency range and additional epochs of the survey are planned to search for transient sources. This survey will provide a unique opportunity to study the radio sky and radio populations, in particular AGN and their role in galaxy evolution. RACS will produce a global sky model for ASKAP, and test operations from data collection and reduction to release.
DOI: 10.25582/data.2023-03.2759871/2318185
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2758914/2318186
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2759853/2318187
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2758970/2318188
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2759852/2318189
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2758829/2318190
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2758889/2318191
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2758672/2318192
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2759134/2318193
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25919/njck-8w13
title: ASKAP Data Products for Project AS109 (ASKAP Pilot Survey for FLASH): images and visibilities

description: These observations will form part of the ASKAP pilot survey program. This is a joint exercise between CASS and the ASKAP Survey Science Teams to conduct a series of observations to learn how to conduct large-scale surveys using the full capabilities of this new telescope. The key goal of the pilot survey program is to establish readiness for full survey operations, including determining and testing observing and processing strategies, and data validation and release. The observations collected here are primarily for FLASH
DOI: 10.25582/data.2023-03.2759934/2318194
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25919/2424-6m26
title: ASKAP Data Products for Project AS104 (ASKAP Pilot Survey for DINGO): images and visibilities

description: These observations will form part of the ASKAP pilot survey program. This is a joint exercise between CASS and the ASKAP Survey Science Teams to conduct a series of observations to learn how to conduct large-scale surveys using the full capabilities of this new telescope. The key goal of the pilot survey program is to establish readiness for full survey operations, including determining and testing observing and processing strategies, and data validation and release. The observations collected here are primarily for DINGO.
DOI: 10.25582/data.2023-03.2759432/2318195
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2758852/2318196
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25582/data.2023-03.2759909/2318197
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25919/5d6547a602619
title: ASKAP Data Products for Project AS111 (ASKAP Pilot Survey for Gravitational Wave Counterparts): images and visibilities

description: This survey is designed to test and develop ASKAP’s capability to rapidly follow up on gravitational wave detections. When observatories such as LIGO issue event notifications, they will be assessed for the likelihood of a radio counterpart and a target of opportunity event triggered if the chance of detection is high (e.g. in the case of a double neutron star merger). Gravitational wave events often have a large angular uncertainty in their direction of origin, so ASKAP’s wide field of view makes it extremely effective at following up these events. Data processing strategies are similar to those of the VAST survey.
DOI: 10.25582/data.2023-03.2759956/2318198
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25919/b9e3-gh43
title: ASKAP Data Products for Project AS111 (ASKAP Pilot Survey for Gravitational Wave Counterparts): images and visibilities

description: This survey is designed to test and develop ASKAP’s capability to rapidly follow up on gravitational wave detections. When observatories such as LIGO issue event notifications, they will be assessed for the likelihood of a radio counterpart and a target of opportunity event triggered if the chance of detection is high (e.g. in the case of a double neutron star merger). Gravitational wave events often have a large angular uncertainty in their direction of origin, so ASKAP’s wide field of view makes it extremely effective at following up these events. Data processing strategies are similar to those of the VAST survey.
DOI: 10.25919/vf5n-kq09
title: ASKAP Data Products for Project AS111 (ASKAP Pilot Survey for Gravitational Wave Counterparts): images and visibilities

description: This survey is designed to test and develop ASKAP’s capability to rapidly follow up on gravitational wave detections. When observatories such as LIGO issue event notifications, they will be assessed for the likelihood of a radio counterpart and a target of opportunity event triggered if the chance of detection is high (e.g. in the case of a double neutron star merger). Gravitational wave events often have a large angular uncertainty in their direction of origin, so ASKAP’s wide field of view makes it extremely effective at following up these events. Data processing strategies are similar to those of the VAST survey.
DOI: 10.48597/xy93-5jay
title: Measurement of Particle_number_size_distribution at Hohenpeissenberg

description: Measurement of Particle_number_size_distribution at Hohenpeissenberg
DOI: 10.48597/y2ch-tmy7
title: Measurement of pH at Irafoss

description: Measurement of pH at Irafoss
DOI: 10.25582/data.2023-03.2759967/2318199
title: Data for EMSL Project 51287 from March 2023
DOI: 10.48597/y6zy-nmq6
title: Measurement of pH at Irafoss

description: Measurement of pH at Irafoss
DOI: 10.25919/5e5d13ed1d33a
title: ASKAP Data Products for Project AS111 (ASKAP Pilot Survey for Gravitational Wave Counterparts): images and visibilities

description: This survey is designed to test and develop ASKAP’s capability to rapidly follow up on gravitational wave detections. When observatories such as LIGO issue event notifications, they will be assessed for the likelihood of a radio counterpart and a target of opportunity event triggered if the chance of detection is high (e.g. in the case of a double neutron star merger). Gravitational wave events often have a large angular uncertainty in their direction of origin, so ASKAP’s wide field of view makes it extremely effective at following up these events. Data processing strategies are similar to those of the VAST survey.
DOI: 10.48597/ygbk-9hqm
title: Measurement of Inorganics in precipitation at Irafoss

description: Measurement of Inorganics in precipitation at Irafoss
DOI: 10.48597/ymkx-b79y
title: Measurement of Inorganics in air and particle phase at Montelibretti

description: Measurement of Inorganics in air and particle phase at Montelibretti
DOI: 10.25582/data.2023-03.2758830/2318200
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25919/5d5eb010176be
title: ASKAP Data Products for Project AS111 (ASKAP Pilot Survey for Gravitational Wave Counterparts): images and visibilities

description: This survey is designed to test and develop ASKAP’s capability to rapidly follow up on gravitational wave detections. When observatories such as LIGO issue event notifications, they will be assessed for the likelihood of a radio counterpart and a target of opportunity event triggered if the chance of detection is high (e.g. in the case of a double neutron star merger). Gravitational wave events often have a large angular uncertainty in their direction of origin, so ASKAP’s wide field of view makes it extremely effective at following up these events. Data processing strategies are similar to those of the VAST survey.
DOI: 10.48597/yrh5-2bh8
title: Measurement of Inorganics in precipitation at Irafoss

description: Measurement of Inorganics in precipitation at Irafoss
DOI: 10.48597/yuvf-gyzq
title: Measurement of Inorganics in air and particle phase at Montelibretti

description: Measurement of Inorganics in air and particle phase at Montelibretti
DOI: 10.25919/5d7a603b88ecd
title: ASKAP Data Products for Project AS111 (ASKAP Pilot Survey for Gravitational Wave Counterparts): images and visibilities

description: This survey is designed to test and develop ASKAP’s capability to rapidly follow up on gravitational wave detections. When observatories such as LIGO issue event notifications, they will be assessed for the likelihood of a radio counterpart and a target of opportunity event triggered if the chance of detection is high (e.g. in the case of a double neutron star merger). Gravitational wave events often have a large angular uncertainty in their direction of origin, so ASKAP’s wide field of view makes it extremely effective at following up these events. Data processing strategies are similar to those of the VAST survey.
DOI: 10.48597/z9s7-ssb6
title: Measurement of pH at Irafoss

description: Measurement of pH at Irafoss
DOI: 10.25582/data.2023-03.2759969/2318201
title: Data for EMSL Project 51287 from March 2023
DOI: 10.25919/5dadbc4814c98
title: ASKAP Data Products for Project AS111 (ASKAP Pilot Survey for Gravitational Wave Counterparts): images and visibilities

description: This survey is designed to test and develop ASKAP’s capability to rapidly follow up on gravitational wave detections. When observatories such as LIGO issue event notifications, they will be assessed for the likelihood of a radio counterpart and a target of opportunity event triggered if the chance of detection is high (e.g. in the case of a double neutron star merger). Gravitational wave events often have a large angular uncertainty in their direction of origin, so ASKAP’s wide field of view makes it extremely effective at following up these events. Data processing strategies are similar to those of the VAST survey.
DOI: 10.48597/zd77-ffr4
title: Measurement of Particle_number_size_distribution at Leipzig-Eisenbahnstrasse

description: Measurement of Particle_number_size_distribution at Leipzig-Eisenbahnstrasse
DOI: 10.48597/zmrx-mqd5
title: Measurement of pH at Irafoss

description: Measurement of pH at Irafoss
DOI: 10.25919/wavj-y889
title: ASKAP Data Products for Project AS111 (ASKAP Pilot Survey for Gravitational Wave Counterparts): images and visibilities

description: This survey is designed to test and develop ASKAP’s capability to rapidly follow up on gravitational wave detections. When observatories such as LIGO issue event notifications, they will be assessed for the likelihood of a radio counterpart and a target of opportunity event triggered if the chance of detection is high (e.g. in the case of a double neutron star merger). Gravitational wave events often have a large angular uncertainty in their direction of origin, so ASKAP’s wide field of view makes it extremely effective at following up these events. Data processing strategies are similar to those of the VAST survey.
DOI: 10.48597/zype-mcpt
title: Measurement of Particle_number_size_distribution at Leipzig-Eisenbahnstrasse

description: Measurement of Particle_number_size_distribution at Leipzig-Eisenbahnstrasse
DOI: 10.48597/zzby-d2am
title: Measurement of Particle_number_size_distribution at Hohenpeissenberg

description: Measurement of Particle_number_size_distribution at Hohenpeissenberg
DOI: 10.25582/data.2023-03.2760255/2318202
title: Data for EMSL Project 51287 from March 2023
DOI: 10.48597/283g-ncg2
title: Measurement of Pm25_mass at Ispra

description: Measurement of Pm25_mass at Ispra
DOI: 10.48597/2gvn-kfa5
title: Measurement of Nitrate at Yarner Wood

description: Measurement of Nitrate at Yarner Wood
DOI: 10.48597/2qcp-r2ss
title: Measurement of Nitrogen oxides at Ispra

description: Measurement of Nitrogen oxides at Ispra
DOI: 10.25582/data.2023-03.2758949/2318203
title: Data for EMSL Project 51287 from March 2023
DOI: 10.48597/3r4u-zhsu
title: Measurement of Ammonium at Eskdalemuir

description: Measurement of Ammonium at Eskdalemuir
DOI: 10.25582/data.2023-03.2758579/2318204
title: Data for EMSL Project 51287 from March 2023
DOI: 10.48597/4gdk-park
title: Measurement of Chloride at Yarner Wood

description: Measurement of Chloride at Yarner Wood
DOI: 10.4225/08/5729853e7687b
title: ASKAP Data Products for Project AS031 (BETA Science Observations): catalogues

description: The Boolardy Engineering Test Array (BETA; Hotan et al. 2014) is a six-antenna prototype of the Australian SKA Pathnder (ASKAP) telescope. The ASKAP Commissioning and Early Science team will use BETA for a limited number of science observations that will exploit the unique wide-eld capabilities of BETA between 700 and 1800 MHz.
DOI: 10.48597/54vb-rgeg
title: Measurement of Wind_speed at Harwell

description: Measurement of Wind_speed at Harwell
DOI: 10.25582/data.2023-03.2758828/2318205
title: Data for EMSL Project 51287 from March 2023
DOI: 10.48597/5ev4-2adf
title: Measurement of Conductivity at Strath Vaich Dam

description: Measurement of Conductivity at Strath Vaich Dam
DOI: 10.25919/c6bh-2717
title: ASKAP Data Products for Project AS103 (ASKAP Pilot Survey for POSSUM): catalogues

description: These observations will form part of the ASKAP pilot survey program. This is a joint exercise between CASS and the ASKAP Survey Science Teams to conduct a series of observations to learn how to conduct large-scale surveys using the full capabilities of this new telescope. The key goal of the pilot survey program is to establish readiness for full survey operations, including determining and testing observing and processing strategies, and data validation and release. The observations collected here are primarily for POSSUM.
DOI: 10.48597/5x5v-u8nf
title: Measurement of Nitrate at Strath Vaich Dam

description: Measurement of Nitrate at Strath Vaich Dam
DOI: 10.48597/64ye-547w
title: Measurement of Precipitation_amount at Lough Navar

description: Measurement of Precipitation_amount at Lough Navar
DOI: 10.25582/data.2023-03.2759142/2318206
title: Data for EMSL Project 51287 from March 2023
DOI: 10.48597/6qr9-wjzy
title: Measurement of Precipitation_amount at High Muffles

description: Measurement of Precipitation_amount at High Muffles
DOI: 10.48597/73c2-dbnf
title: Measurement of pH at Lough Navar

description: Measurement of pH at Lough Navar
DOI: 10.25582/data.2023-03.2758907/2318207
title: Data for EMSL Project 51287 from March 2023
DOI: 10.48597/79dm-ed9n
title: Measurement of pH at High Muffles

description: Measurement of pH at High Muffles
DOI: 10.25919/44sn-2x47
title: ASKAP Data Products for Project AS034 (ASKAP Early Science Broadband Survey): derived data products

description: This collection contains Stokes I Taylor 0 and Taylor 1 images of the Abell S1136 galaxy cluster. The images are comprised of 33 ASKAP beams, at a centre frequency of 888 MHz, a 240 MHz bandwidth, and 240 x 1MHz channels. The synthesised beam is 12.60’’ x 10.04’’. This data is presented in Macgregor et al. (2021).
DOI: 10.48597/7r3v-rt73
title: Measurement of Nitrate at Lough Navar

description: Measurement of Nitrate at Lough Navar
DOI: 10.25582/data.2023-03.2758871/2318208
title: Data for EMSL Project 51287 from March 2023
DOI: 10.48597/9ban-4s5m
title: Measurement of Nitrate at High Muffles

description: Measurement of Nitrate at High Muffles
DOI: 10.48597/9wc7-de6b
title: Measurement of Potassium at Eskdalemuir

description: Measurement of Potassium at Eskdalemuir
DOI: 10.48597/9yja-fgad
title: Measurement of Inorganics in air and particle phase at Ispra

description: Measurement of Inorganics in air and particle phase at Ispra
DOI: 10.25582/data.2023-03.2758926/2318209
title: Data for EMSL Project 51287 from March 2023
DOI: 10.48597/9yrb-sf7t
title: Measurement of Calcium at Strath Vaich Dam

description: Measurement of Calcium at Strath Vaich Dam
DOI: 10.25919/5d1ed28479f82
title: ASKAP Data Products for Project AS035 (ASKAP Early Science Widefield HI Survey): derived images

description: A mosaicked spectral image cube of IC 5201 and its satellites. The cube is comprised of 4 ASKAP beams, consisting of 650 channels that span 12 MHz (1408.5 - 1420.5) of bandwidth, with a resolution of 18.5 kHz. The cube is ~ 2.2 x 2.2 deg, with IC 5021 located near the centre. This spectral image cube is presented in Kleiner et al. (2019), with a detailed description of the data processing in Section 5.
DOI: 10.25919/p524-xb81
title: ASKAP Project AS110 - The Rapid ASKAP Continuum Survey: cataloguing the sky at 1367.5 MHz and the second data release of RACS-mid

description: Data products associated with the release of the Stokes I catalogue (Duchesne+2023b) from the Rapid ASKAP Continuum Survey (RACS) at 1367.5 MHz (RACS-mid). This work took the images of the tiles associated with RACS-mid survey (see Duchesne+2023a) at 1367.5 MHz (144 MHz bandwidth), convolved them to a common resolution, and mosaicked them with neighbouring images to obtain near-uniform sensitivity images covering the sky up to declination +49 degrees. Released are the 1493 Stokes I images constructed in this manner, and the resulting source and component catalogue covering the region. Catalogues were made by running PyBDSF (see Mohan and Rafferty: 2015ascl.soft02007M) over each mosaiced tile image. These tile catalogues were combined together and duplicates removed. An additional set of images are produced at a fixed resolution of 25" times 25", to match the RACS catalogue at 887.5 MHz (RACS-low, Hale+2021) with coverage up to declination +30 degrees. An auxiliary catalogue is produced with these 25" images intended for simple cross-matching to the RACS-low catalogue or for users who required a position-independent resolution. See Duchesne+2023b for details on the individual catalogues.
DOI: 10.48597/a5gv-hna5
title: Measurement of Potassium at Yarner Wood

description: Measurement of Potassium at Yarner Wood
DOI: 10.48597/a8sr-sqwd
title: Measurement of Dewpoint_temperature at Harwell

description: Measurement of Dewpoint_temperature at Harwell
DOI: 10.25582/data.2023-03.2758657/2318210
title: Data for EMSL Project 51287 from March 2023
DOI: 10.48597/apkg-k2wj
title: Measurement of Propanone at Lahemaa

description: Measurement of Propanone at Lahemaa
DOI: 10.48597/bevu-my58
title: Measurement of Potassium at Lough Navar

description: Measurement of Potassium at Lough Navar
DOI: 10.48597/c4xm-rr33
title: Measurement of Sodium at Lough Navar

description: Measurement of Sodium at Lough Navar
DOI: 10.25582/data.2023-03.2760155/2318211
title: Data for EMSL Project 51287 from March 2023