cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.6084/m9.figshare.30889556
title: Responses of seven tested models for real clinical questions

description: This dataset contains 14 files, each corresponding to the model responses to 14 question groups, two of which belong to the AE (accident and emergency) specialty, and the other 12 belonging to 12 separate specialties (from cardiology to rare diseases).Each file (in JSON format) contains dozens of items, each corresponding to responses for a specific clinical question. Each question has a unique ID (QID) and is one of two question types, OSCE or realCases. The "modelResponses" field typically is a dictionary with seven keys pointing to seven responses.The seven keys, which is in the format of 6-letter random alphabet followed by a four-letter suffix, represent the seven models tested. The key suffices help identify the models that produced the responses, with explanations below:CG4L: ChatGPT-4oL (first released May 13, 2024)<br>QM212: QwenMAX (Release Date [API Availability]: January 29, 2025)<br>RDS3: DS32B (DeepSeek-R1-Distill-Qwen-32B, Released January 20, 2025)<br>G2FT: Gemini2F (gemini-2.0-flash-thinking-exp-01-21, Released January 21, 2025)<br>Q3B: Qwen32B (Qwen3 32B or QwQ-32B, March 6, 2025)<br>SR67: DS-r1 671B ( Released January 20, 2025)<br>R17: DeS70B (DeepSeek-R1-Distill-Llama-70B, January 20, 2025)<br><br>hallu-sept-4-2025.xlsx contains the 40 alleged hallucinations.
DOI: 10.25574/20103
title: Chandra X-ray Observatory ObsId 20103

description: An X-ray Census of YSOs in Infrared Dark Clouds. II. Star Cluster Formation from a Massive Filament
DOI: 10.6084/m9.figshare.30889556.v1
title: Responses of seven tested models for real clinical questions

description: This dataset contains 14 files, each corresponding to the model responses to 14 question groups, two of which belong to the AE (accident and emergency) specialty, and the other 12 belonging to 12 separate specialties (from cardiology to rare diseases).Each file (in JSON format) contains dozens of items, each corresponding to responses for a specific clinical question. Each question has a unique ID (QID) and is one of two question types, OSCE or realCases. The "modelResponses" field typically is a dictionary with seven keys pointing to seven responses. The seven keys, which is in the format of 6-letter random alphabet followed by a four-letter suffix, represent the seven models tested. The key suffices help identify the models that produced the responses, with explanations below:CG4L: ChatGPT-4oL (first released May 13, 2024)<br>QM212: QwenMAX (Release Date [API Availability]: January 29, 2025)<br>RDS3: DS32B (DeepSeek-R1-Distill-Qwen-32B, Released January 20, 2025)<br>G2FT: Gemini2F (gemini-2.0-flash-thinking-exp-01-21, Released January 21, 2025)<br>Q3B: Qwen32B (Qwen3 32B or QwQ-32B, March 6, 2025)<br>SR67: DS-r1 671B ( Released January 20, 2025)<br>R17: DeS70B (DeepSeek-R1-Distill-Llama-70B, January 20, 2025)<br>
DOI: 10.6084/m9.figshare.30889556.v2
title: Responses of seven tested models for real clinical questions

description: This dataset contains 14 files, each corresponding to the model responses to 14 question groups, two of which belong to the AE (accident and emergency) specialty, and the other 12 belonging to 12 separate specialties (from cardiology to rare diseases).Each file (in JSON format) contains dozens of items, each corresponding to responses for a specific clinical question. Each question has a unique ID (QID) and is one of two question types, OSCE or realCases. The "modelResponses" field typically is a dictionary with seven keys pointing to seven responses.The seven keys, which is in the format of 6-letter random alphabet followed by a four-letter suffix, represent the seven models tested. The key suffices help identify the models that produced the responses, with explanations below:CG4L: ChatGPT-4oL (first released May 13, 2024)<br>QM212: QwenMAX (Release Date [API Availability]: January 29, 2025)<br>RDS3: DS32B (DeepSeek-R1-Distill-Qwen-32B, Released January 20, 2025)<br>G2FT: Gemini2F (gemini-2.0-flash-thinking-exp-01-21, Released January 21, 2025)<br>Q3B: Qwen32B (Qwen3 32B or QwQ-32B, March 6, 2025)<br>SR67: DS-r1 671B ( Released January 20, 2025)<br>R17: DeS70B (DeepSeek-R1-Distill-Llama-70B, January 20, 2025)<br><br>hallu-sept-4-2025.xlsx contains the 40 alleged hallucinations.
DOI: 10.25574/20104
title: Chandra X-ray Observatory ObsId 20104

description: Cavities, shocks and stripping in a high-velocity group-group merger: NGC 6338
DOI: 10.25574/20108
title: Chandra X-ray Observatory ObsId 20108

description: Using the sharp Chandra's eyes to find a neutron star lurking in the wind of WR124
DOI: 10.25574/20109
title: Chandra X-ray Observatory ObsId 20109

description: Using the sharp Chandra's eyes to find a neutron star lurking in the wind of WR124
DOI: 10.25574/20110
title: Chandra X-ray Observatory ObsId 20110

description: Using the sharp Chandra's eyes to find a neutron star lurking in the wind of WR124
DOI: 10.6084/m9.figshare.30899276
title: Landslide inventories

description: Reasonable landslide susceptibility mapping (LSM) is helpful to avoid damage caused by landslides. At present, it is not clear which screening method can yield the optimal combination of causative factors. Moreover, the "black box" nature of machine learning models limits understanding of their internal mechanisms and the driving roles of causative factors in the landslide development process. In this work, GeoDetector, information gain (IG), and Gini index (Gini) were used to select the optimal combination of causative factors to explore the most effective method. The Random Forest (RF_GeoDetector, RF_IG, and RF_Gini), Support Vector Machine (SVM_GeoDetector, SVM_IG, and SVM_Gini), and eXtreme Gradient Boosting (XGBoost_GeoDetector, XGBoost_IG, and XGBoost_Gini) were constructed for LSM.Furthermore, the SHapley Additive exPlanation (SHAP) algorithm was applied to quantify the marginal contribution of each causative factor to the landslide susceptibility. The conclusion showed that (1) Giniis superior to GeoDetector and IG in screening the optimal combination of causative factors. (2) The SHAP revealed that proximity to roads was the most significant contributor to landslide occurrence, followed by lithology and annual average precipitation of March-July. It highlights the coupling effect of natural and anthropogenic factors on landslide susceptibility. (3) For LSM, the XGBoost_Ginimodel achieves the optimum performance. A reasonable LSM provides better technical support and more accurate disaster prevention.
DOI: 10.6084/m9.figshare.30899276.v1
title: Landslide inventories

description: Reasonable landslide susceptibility mapping (LSM) is helpful to avoid damage caused by landslides. At present, it is not clear which screening method can yield the optimal combination of causative factors. Moreover, the "black box" nature of machine learning models limits understanding of their internal mechanisms and the driving roles of causative factors in the landslide development process. In this work, GeoDetector, information gain (IG), and Gini index (Gini) were used to select the optimal combination of causative factors to explore the most effective method. The Random Forest (RF_GeoDetector, RF_IG, and RF_Gini), Support Vector Machine (SVM_GeoDetector, SVM_IG, and SVM_Gini), and eXtreme Gradient Boosting (XGBoost_GeoDetector, XGBoost_IG, and XGBoost_Gini) were constructed for LSM.Furthermore, the SHapley Additive exPlanation (SHAP) algorithm was applied to quantify the marginal contribution of each causative factor to the landslide susceptibility. The conclusion showed that (1) Giniis superior to GeoDetector and IG in screening the optimal combination of causative factors. (2) The SHAP revealed that proximity to roads was the most significant contributor to landslide occurrence, followed by lithology and annual average precipitation of March-July. It highlights the coupling effect of natural and anthropogenic factors on landslide susceptibility. (3) For LSM, the XGBoost_Ginimodel achieves the optimum performance. A reasonable LSM provides better technical support and more accurate disaster prevention.
DOI: 10.25574/20111
title: Chandra X-ray Observatory ObsId 20111

description: A Magnetic X-ray Filament near the Galactic Center: Seeking the Energy Source
DOI: 10.25574/20112
title: Chandra X-ray Observatory ObsId 20112

description: Cavities, shocks and stripping in a high-velocity group-group merger: NGC 6338
DOI: 10.25574/20113
title: Chandra X-ray Observatory ObsId 20113

description: Cavities, shocks and stripping in a high-velocity group-group merger: NGC 6338
DOI: 10.25574/20114
title: Chandra X-ray Observatory ObsId 20114

description: X-ray confirmation of two intermediate mass black hole candidates
DOI: 10.17026/ar/zbrh2q
title: PAN-00179475 - three-ribbed La Tène bracelet variant H6a

description: &lt;p&gt;This find is registered at Portable Antiquities of the Netherlands with number PAN-00179475&lt;/p&gt;
description: Modified: 2025-09-09T10:11:55+02:00
DOI: 10.25574/20115
title: Chandra X-ray Observatory ObsId 20115

description: X-ray confirmation of two intermediate mass black hole candidates
DOI: 10.25574/20116
title: Chandra X-ray Observatory ObsId 20116

description: Mysterious ejecta from a high-mass gamma-ray binary
DOI: 10.25574/20117
title: Chandra X-ray Observatory ObsId 20117

description: Cavities, shocks and stripping in a high-velocity group-group merger: NGC 6338
DOI: 10.25574/20120
title: Chandra X-ray Observatory ObsId 20120

description: X-raying the Bones of the Milky Way
DOI: 10.25574/20121
title: Chandra X-ray Observatory ObsId 20121

description: The Faint CVs and MSPs of the Globular Cluster NGC 6752
DOI: 10.25574/20122
title: Chandra X-ray Observatory ObsId 20122

description: The Faint CVs and MSPs of the Globular Cluster NGC 6752
DOI: 10.25574/20123
title: Chandra X-ray Observatory ObsId 20123

description: The Faint CVs and MSPs of the Globular Cluster NGC 6752
DOI: 10.25574/20124
title: Chandra X-ray Observatory ObsId 20124

description: The X-rays of a bright QSO well within the epoch of reionization at z=7.54
DOI: 10.25574/20127
title: Chandra X-ray Observatory ObsId 20127

description: Long-Term Multi-wavelength Monitoring of a Stellar Tidal Disruption at Only 90 Mpc
DOI: 10.25574/20128
title: Chandra X-ray Observatory ObsId 20128

description: Long-Term Multi-wavelength Monitoring of a Stellar Tidal Disruption at Only 90 Mpc
DOI: 10.25574/20129
title: Chandra X-ray Observatory ObsId 20129

description: Probing the Physics of the ICM in the Most Violent Mergers at High Redshift
DOI: 10.25574/20133
title: Chandra X-ray Observatory ObsId 20133

description: Probing the X-ray Emission from the Massive Star Cluster Westerlund 2
DOI: 10.25574/20134
title: Chandra X-ray Observatory ObsId 20134

description: Probing the X-ray Emission from the Massive Star Cluster Westerlund 2
DOI: 10.25574/20135
title: Chandra X-ray Observatory ObsId 20135

description: Resolving the Double FU Orionis System RNO 1B/1C With Chandra
DOI: 10.25574/20136
title: Chandra X-ray Observatory ObsId 20136

description: A Comprehensive Search for X-ray Emission from the Coolest Magnetically Active Brown Dwarfs
DOI: 10.6084/m9.figshare.30899297
title: Nocardiopsis bonnevillensis DSM 118115 genome

description: <i>Nocardiopsis bonnevillensis </i>DSM 118115 was isolated from sediment collected in July 2021 along the shoreline of Farmington Bay, Great Salt Lake (41° 3′ 58″ N, 112° 13′ 48″ W), within Antelope Island State Park, Utah. To obtain a whole-genome sequence of <i>N. bonnevillensis </i>DSM 118115, genomic DNA was extracted using an MP Biomedicals FastDNA SPIN Kit according to the manufacturer’s instructions and sequenced by Plasmidsaurus using Oxford Nanopore. CheckM analysis of the assembled genome indicated 100.0% completeness and 0.5% contamination. The 6.1 Mb genome was assembled into six contigs with an average coverage depth of 29x.
DOI: 10.6084/m9.figshare.30899297.v1
title: Nocardiopsis bonnevillensis DSM 118115 genome

description: <i>Nocardiopsis bonnevillensis </i>DSM 118115 was isolated from sediment collected in July 2021 along the shoreline of Farmington Bay, Great Salt Lake (41° 3′ 58″ N, 112° 13′ 48″ W), within Antelope Island State Park, Utah. To obtain a whole-genome sequence of <i>N. bonnevillensis </i>DSM 118115, genomic DNA was extracted using an MP Biomedicals FastDNA SPIN Kit according to the manufacturer’s instructions and sequenced by Plasmidsaurus using Oxford Nanopore. CheckM analysis of the assembled genome indicated 100.0% completeness and 0.5% contamination. The 6.1 Mb genome was assembled into six contigs with an average coverage depth of 29x.
DOI: 10.25574/20137
title: Chandra X-ray Observatory ObsId 20137

description: A Comprehensive Search for X-ray Emission from the Coolest Magnetically Active Brown Dwarfs
DOI: 10.25574/20138
title: Chandra X-ray Observatory ObsId 20138

description: A Comprehensive Search for X-ray Emission from the Coolest Magnetically Active Brown Dwarfs
DOI: 10.25574/20139
title: Chandra X-ray Observatory ObsId 20139

description: A Comprehensive Search for X-ray Emission from the Coolest Magnetically Active Brown Dwarfs
DOI: 10.25574/20140
title: Chandra X-ray Observatory ObsId 20140

description: A Comprehensive Search for X-ray Emission from the Coolest Magnetically Active Brown Dwarfs
DOI: 10.25574/20141
title: Chandra X-ray Observatory ObsId 20141

description: A Comprehensive Search for X-ray Emission from the Coolest Magnetically Active Brown Dwarfs
DOI: 10.25574/20142
title: Chandra X-ray Observatory ObsId 20142

description: LONG-OVERDUE X-RAY OBSERVATIONS OF THE EXTRAORDINARY MASSIVE ECLIPSING BINARY RY SCUTI
DOI: 10.25574/20143
title: Chandra X-ray Observatory ObsId 20143

description: LONG-OVERDUE X-RAY OBSERVATIONS OF THE EXTRAORDINARY MASSIVE ECLIPSING BINARY RY SCUTI
DOI: 10.25574/20144
title: Chandra X-ray Observatory ObsId 20144

description: LONG-OVERDUE X-RAY OBSERVATIONS OF THE EXTRAORDINARY MASSIVE ECLIPSING BINARY RY SCUTI
DOI: 10.25574/20145
title: Chandra X-ray Observatory ObsId 20145

description: Catching an FUor in the Act: Chandra ToO Observations of Extreme Accretion onto Young S
DOI: 10.25574/20146
title: Chandra X-ray Observatory ObsId 20146

description: Catching an FUor in the Act: Chandra ToO Observations of Extreme Accretion onto Young S
DOI: 10.25574/20147
title: Chandra X-ray Observatory ObsId 20147

description: Catching an FUor in the Act: Chandra ToO Observations of Extreme Accretion onto Young S
DOI: 10.25574/20148
title: Chandra X-ray Observatory ObsId 20148

description: Tracking changes in the magnetosphere of HD148937
DOI: 10.25574/20149
title: Chandra X-ray Observatory ObsId 20149

description: Cepheids: A New Class of X-Ray Variable: Part I: l Car
DOI: 10.25574/20150
title: Chandra X-ray Observatory ObsId 20150

description: Secret Lives of Cepheids: beta Dor as a Test of Cepheid X-ray Heating Mechanisms
DOI: 10.25574/20151
title: Chandra X-ray Observatory ObsId 20151

description: Secret Lives of Cepheids: beta Dor as a Test of Cepheid X-ray Heating Mechanisms
DOI: 10.25574/20152
title: Chandra X-ray Observatory ObsId 20152

description: A unique opportunity to observe the extreme massive binary HD 93129A near periastron passage
DOI: 10.25574/20153
title: Chandra X-ray Observatory ObsId 20153

description: A unique opportunity to observe the extreme massive binary HD 93129A near periastron passage
DOI: 10.25574/20162
title: Chandra X-ray Observatory ObsId 20162

description: Beyond Proxima b: Characterizing the X-ray Environments of the Next Three Nearest Potentially Habitable Exoplanets
DOI: 10.25574/20163
title: Chandra X-ray Observatory ObsId 20163

description: Beyond Proxima b: Characterizing the X-ray Environments of the Next Three Nearest Potentially Habitable Exoplanets
DOI: 10.25574/20164
title: Chandra X-ray Observatory ObsId 20164

description: Beyond Proxima b: Characterizing the X-ray Environments of the Next Three Nearest Potentially Habitable Exoplanets
DOI: 10.25574/20180
title: Chandra X-ray Observatory ObsId 20180

description: The Late-time X-ray Behavior of Short Gamma-ray Bursts: Implications for Energetics and Rates
DOI: 10.25574/20181
title: Chandra X-ray Observatory ObsId 20181

description: The Late-time X-ray Behavior of Short Gamma-ray Bursts: Implications for Energetics and Rates
DOI: 10.25574/20195
title: Chandra X-ray Observatory ObsId 20195

description: Transient LMXBs in Globular Clusters
DOI: 10.25574/20197
title: Chandra X-ray Observatory ObsId 20197

description: The Nature of INTEGRAL Sources in the Galactic Plane
DOI: 10.25574/20198
title: Chandra X-ray Observatory ObsId 20198

description: The Nature of INTEGRAL Sources in the Galactic Plane
DOI: 10.17026/ar/tavldt
title: PAN-00149827 - roof lead

description: &lt;p&gt;This find is registered at Portable Antiquities of the Netherlands with number PAN-00149827&lt;/p&gt;
description: Modified: 2025-10-20T16:19:24+02:00
DOI: 10.25574/20199
title: Chandra X-ray Observatory ObsId 20199

description: The Nature of INTEGRAL Sources in the Galactic Plane
DOI: 10.25574/20200
title: Chandra X-ray Observatory ObsId 20200

description: The Nature of INTEGRAL Sources in the Galactic Plane
DOI: 10.25574/20201
title: Chandra X-ray Observatory ObsId 20201

description: The Nature of INTEGRAL Sources in the Galactic Plane
DOI: 10.25574/20202
title: Chandra X-ray Observatory ObsId 20202

description: Studying the very cold neutron star in HETE J1900.1-2455
DOI: 10.25574/20207
title: Chandra X-ray Observatory ObsId 20207

description: X-Ray Jets in Microquasars
DOI: 10.25574/20208
title: Chandra X-ray Observatory ObsId 20208

description: X-Ray Jets in Microquasars
DOI: 10.25574/20267
title: Chandra X-ray Observatory ObsId 20267

description: Searching for Obscured ULX in LIRGS: a Deep Observation of NGC7552
DOI: 10.25574/20268
title: Chandra X-ray Observatory ObsId 20268

description: Searching for Obscured ULX in LIRGS: a Deep Observation of NGC7552
DOI: 10.5255/ukda-sn-6739-1
title: Food and You Survey, 2010
title: Food and You Surveys, 2010-2018, and Food and You 2, 2020-

description: &lt;p&gt;The &lt;span style="font-style: italic;"&gt;Food and You Surveys&lt;/span&gt; (2010-2018), and &lt;span style="font-style: italic;"&gt;Food and You 2&lt;/span&gt; (2020- ) are bi-annual, cross-sectional surveys of adults aged 16 years and over living in England, Wales and Northern Ireland,  commissioned by the Food Standards Agency (FSA). &lt;span style="font-style: italic;"&gt;Food and You&lt;/span&gt; provides data about the prevalence of different attitudes, reported behaviour and knowledge about ways in which food is purchased, stored, prepared and eaten.&lt;/p&gt;&lt;p&gt;&lt;span style="font-weight: bold;"&gt;Food and You, 2010-2018&lt;/span&gt;&lt;br&gt;From 2010, &lt;span style="font-style: italic;"&gt;Food and You&lt;/span&gt; became the FSA’s flagship social survey. In addition, the FSA conducted regular tracking surveys including the bi-annual Public Attitudes Tracker and the annual Food Hygiene Rating Scheme (FHRS) Consumer Attitudes Tracker (these studies are not held at UKDS). From Wave 4, &lt;span style="font-style: italic;"&gt;Food and You&lt;/span&gt; included new questions to cover the affordability of food, choice, security and sustainability.&lt;/p&gt;&lt;p&gt;&lt;span style="font-weight: bold;"&gt;Food and You 2, 2020-&lt;/span&gt;&lt;br&gt;In 2018, the FSA’s Advisory Committee for Social Science (ACSS) recommended that Food and You and the Public Attitudes Tracker be replaced with a new ‘push-to-web’ survey, &lt;span style="font-style: italic;"&gt;Food and You 2&lt;/span&gt;, which was commissioned in 2019 with data collection commencing in July 2020. Due to differences in the survey methodologies, comparisons cannot be made between the earlier &lt;span style="font-style: italic;"&gt;Food and You&lt;/span&gt; surveys, or the Public Attitudes Tracker, and &lt;span style="font-style: italic;"&gt;Food and You 2&lt;/span&gt;. Therefore &lt;span style="font-style: italic;"&gt;Food and You 2&lt;/span&gt;, 2020 is the start of a new data time series. Data will be collected through Food and You 2 on a bi-annual basis. Unlike the previous surveys, as well as the standard End User Licence (EUL) study for &lt;span style="font-style: italic;"&gt;Food and You 2&lt;/span&gt; the UKDS also holds additional variables under Special Licence (see SN 8815).&lt;/p&gt;&lt;p&gt; Further information may be found on the FSA's &lt;a title="Food and You Survey" href="https://www.food.gov.uk/research/food-and-you"&gt;Food and You Survey&lt;/a&gt; webpage.&lt;br&gt;
&lt;/p&gt;
DOI: 10.25574/20269
title: Chandra X-ray Observatory ObsId 20269

description: X-RAY IMAGING OF THE HIGH-MASS GAMMA-RAY BINARY HESS J0632+057
DOI: 10.25574/20276
title: Chandra X-ray Observatory ObsId 20276

description: Investigating the Current State of V1535 Sco
DOI: 10.25574/20278
title: Chandra X-ray Observatory ObsId 20278

description: Late-time X-rays to map the Zoo of Engine-driven Stellar Explosions
DOI: 10.25574/20279
title: Chandra X-ray Observatory ObsId 20279

description: Late-time X-rays to map the Zoo of Engine-driven Stellar Explosions
DOI: 10.25574/20280
title: Chandra X-ray Observatory ObsId 20280

description: Rapid Observations of Short-Duration Gamma-Ray Bursts: Accurate Positions Hold the Key to the Progenitor Population
DOI: 10.25574/20281
title: Chandra X-ray Observatory ObsId 20281

description: Where Have All the Central Compact Objects Gone?
DOI: 10.25574/20282
title: Chandra X-ray Observatory ObsId 20282

description: Where Have All the Central Compact Objects Gone?
DOI: 10.25574/20283
title: Chandra X-ray Observatory ObsId 20283

description: Where Have All the Central Compact Objects Gone?
DOI: 10.25574/20284
title: Chandra X-ray Observatory ObsId 20284

description: Where Have All the Central Compact Objects Gone?
DOI: 10.15468/dl.353yp5
title: Occurrence Download

description: A dataset containing 32 species occurrences available in GBIF matching the query:
{
 "and" : [
 "TaxonKey is Pitcairnia geyskesii",
 "HasCoordinate is true",
 "HasGeospatialIssue is false"
 ]
}

 The dataset includes 32 records from 13 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0055545-251120083545085/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.25574/20285
title: Chandra X-ray Observatory ObsId 20285

description: Where Have All the Central Compact Objects Gone?
DOI: 10.25574/20286
title: Chandra X-ray Observatory ObsId 20286

description: Where Have All the Central Compact Objects Gone?
DOI: 10.25574/20287
title: Chandra X-ray Observatory ObsId 20287

description: Where Have All the Central Compact Objects Gone?
DOI: 10.25574/20288
title: Chandra X-ray Observatory ObsId 20288

description: Where Have All the Central Compact Objects Gone?
DOI: 10.25574/20289
title: Chandra X-ray Observatory ObsId 20289

description: Source of Energy and pre-explosion progenitor evolution of Super-luminous Supernovae
DOI: 10.25574/20290
title: Chandra X-ray Observatory ObsId 20290

description: Source of Energy and pre-explosion progenitor evolution of Super-luminous Supernovae
DOI: 10.25574/20291
title: Chandra X-ray Observatory ObsId 20291

description: Source of Energy and pre-explosion progenitor evolution of Super-luminous Supernovae
DOI: 10.25574/20292
title: Chandra X-ray Observatory ObsId 20292

description: Uncovering a new population of soft gamma-ray pulsars with Chandra
DOI: 10.25574/20293
title: Chandra X-ray Observatory ObsId 20293

description: Uncovering a new population of soft gamma-ray pulsars with Chandra
DOI: 10.25574/20294
title: Chandra X-ray Observatory ObsId 20294

description: Uncovering a new population of soft gamma-ray pulsars with Chandra
DOI: 10.25574/20295
title: Chandra X-ray Observatory ObsId 20295

description: Uncovering a new population of soft gamma-ray pulsars with Chandra
DOI: 10.25574/20296
title: Chandra X-ray Observatory ObsId 20296

description: Uncovering a new population of soft gamma-ray pulsars with Chandra