cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.25574/csc2.obs.08622
title: Chandra X-ray Observatory ObsId 08622

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.obs.23220
title: Chandra X-ray Observatory ObsId 23220

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: 10.15468/dl.m4qa7q
title: Occurrence Download

description: A dataset containing 45 species occurrences available in GBIF matching the query:
{
 "and" : [
 "BasisOfRecord is Specimen",
 "TaxonKey is Annona insignis R.E.Fr."
 ]
}

 The dataset includes 45 records from 19 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0010461-250127130748423/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.25574/csc2.obs.07715
title: Chandra X-ray Observatory ObsId 07715

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: 10.48577/jpl.el4ema
title: Upcycling titanium-based bulk metallic glass scrap feedstock through compositional steering

description: Bulk metallic glasses (BMGs) are an emerging commercial material with applications in consumer electronics, fasteners, watches, and precision gears, among other uses. Mass-production of hardware using BMGs requires the production of feedstock material using conventional foundry techniques, normally comprising rods, thin sheets, and powder. Due to the unique amorphous nature and highly designed compositions of BMGs, recycling and upcycling waste products are challenging because the properties of BMGs are highly dependent on their chemical composition and impurity content. In this work, an off-composition, scrap titanium-based BMG feedstock material is upcycled into usable material through the novel use of a correction ingot to steer the composition into either a better glass-forming alloy or an alloy that exhibits improved mechanical performance. In one example, the feedstock, initially with exceptionally poor mechanical properties and low glass-forming-ability, can be compositionally steered into a 3.5-mm thick BMG by mixing it with as little as 25% by mass of a designed alloy.
DOI: 10.25574/csc2.obs.07861
title: Chandra X-ray Observatory ObsId 07861

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.obs.13289
title: Chandra X-ray Observatory ObsId 13289

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.obs.19312
title: Chandra X-ray Observatory ObsId 19312

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.obs.08273
title: Chandra X-ray Observatory ObsId 08273

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.obs.19947
title: Chandra X-ray Observatory ObsId 19947

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.obs.07131
title: Chandra X-ray Observatory ObsId 07131

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.obs.12096
title: Chandra X-ray Observatory ObsId 12096

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.obs.12262
title: Chandra X-ray Observatory ObsId 12262

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.obs.21275
title: Chandra X-ray Observatory ObsId 21275

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: 10.48577/jpl.wdxevl
title: Maneuver Design Techniques for Deploying and Maintaining the SunRISE Constellation

description: The Sun Radio Interferometer Space Experiment (SunRISE) mission will employ a constellation of 6 CubeSats in an orbit 300 km above geostationary to study the transport and acceleration of solar energetic particles associated with coronal mass ejections. While the spacecraft are capable of executing maneuvers anywhere within the orbit, selecting the time of the OTM may minimize the DeltaV, ensure that DeltaV constraints are met, and minimize the chance of close approaches within the constellation during transfers. The present paper focuses on the maneuver design process for deploying and maintaining the constellation in a loose, repeating formation to create the first spaceborne imaging interferometer.
DOI: 10.25574/csc2.obs.02309
title: Chandra X-ray Observatory ObsId 02309

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: 10.48577/jpl.9d0blm
title: Superconducting nanowire single-photon detector arrays for optical communication, astronomy, and single-photon imaging

description: No abstract available.
DOI: 10.25574/csc2.obs.08464
title: Chandra X-ray Observatory ObsId 08464

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.obs.21853
title: Chandra X-ray Observatory ObsId 21853

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.obs.20306
title: Chandra X-ray Observatory ObsId 20306

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: 10.48577/jpl.j1ngpi
title: Psyche’s Thruster Checkouts:Design, Navigation Strategy, and Results

description: No abstract available.
DOI: 10.25574/csc2.obs.18092
title: Chandra X-ray Observatory ObsId 18092

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.obs.23076
title: Chandra X-ray Observatory ObsId 23076

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.obs.00344
title: Chandra X-ray Observatory ObsId 00344

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.obs.09392
title: Chandra X-ray Observatory ObsId 09392

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.obs.23217
title: Chandra X-ray Observatory ObsId 23217

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: 10.48577/jpl.9d5xjt
title: Machine Learning for Frequency Stability Estimation of High Precision Oscillators

description: No abstract available.
DOI: 10.25574/csc2.obs.12988
title: Chandra X-ray Observatory ObsId 12988

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.obs.02339
title: Chandra X-ray Observatory ObsId 02339

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: 10.48577/jpl.6dq6dp
title: Superconducting nanowire single-photon detector arrays for deep space optical communication ground receivers

description: No abstract available.
DOI: 10.25574/csc2.obs.11613
title: Chandra X-ray Observatory ObsId 11613

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.obs.04993
title: Chandra X-ray Observatory ObsId 04993

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.obs.13403
title: Chandra X-ray Observatory ObsId 13403

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.obs.18635
title: Chandra X-ray Observatory ObsId 18635

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.obs.02157
title: Chandra X-ray Observatory ObsId 02157

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.obs.05910
title: Chandra X-ray Observatory ObsId 05910

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.obs.15573
title: Chandra X-ray Observatory ObsId 15573

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.obs.21546
title: Chandra X-ray Observatory ObsId 21546

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.obs.24837
title: Chandra X-ray Observatory ObsId 24837

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: 10.48577/jpl.ynytjt
title: GUIDANCE, NAVIGATION, AND CONTROL FOR THE DEEP SPACE OPTICAL COMMUNICATION MISSION

description: NASA’s Deep Space Optical Communication (DSOC) mission is currently operating on-board the PSYCHE spacecraft and has demonstrated the first optical communication link from beyond the Earth-Moon system. The opti- cal link requires micro-radian level pointing stability which DSOC achieves through a combination of passive isolation, to reject high frequency distur- bances from the spacecraft, and active pointing control, to track the uplink and downlink stations. The passive isolation is enabled by a floating platform that is tethered to the main spacecraft with soft cables. The floating platform holds a telescope assembly for both receiving the uplink and transmitting the dowlink signals. The floating platform is actively controlled to both reject disturbances from the main spacecraft and to track an uplink signal, which is in turn used as a reference for downlink pointing. In this architecture, down- link pointing control is only used to track the slowly varying drift between the uplink and downlink directions; all pointing isolation is provided by the floating platform control. This allows the dowlink pointing to operate at a nearly fixed point which improves the calibration of the dowlink pointing bias between operational activities. Current experience confirms that the softness and strain in the tethering cables are key design parameters. Furthermore, idiosyncrasies in the sensors used for platform control have, in some instances, hampered pointing performance, which could be resolved in future missions.
DOI: 10.25574/csc2.obs.07116
title: Chandra X-ray Observatory ObsId 07116

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.obs.16524
title: Chandra X-ray Observatory ObsId 16524

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.obs.04802
title: Chandra X-ray Observatory ObsId 04802

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.obs.19313
title: Chandra X-ray Observatory ObsId 19313

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.obs.26201
title: Chandra X-ray Observatory ObsId 26201

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.obs.00875
title: Chandra X-ray Observatory ObsId 00875

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: 10.48577/jpl.7vun7l
title: Psyche's Thruster Checkouts: Design, Navigation Strategy, and Results

description: Psyche, a low-thrust solar electric propulsion spacecraft, is currently on its way to the main- belt asteroid (16) Psyche. The sole source of propulsion is a set of four Hall effect thrusters, a technology which had never flown beyond cislunar space prior to this mission. In order to ac- curately design thrust maneuvers and predict the trajectory of the spacecraft while thrusting, the thrusters needed to be characterized and calibrated during the initial checkout phase. We detail here the design of these calibration activities, the navigation strategy and filter setup for estimating the actual thrust, and the results obtained for the Psyche mission.
DOI: 10.25574/csc2.obs.05244
title: Chandra X-ray Observatory ObsId 05244

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.obs.11355
title: Chandra X-ray Observatory ObsId 11355

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.obs.11358
title: Chandra X-ray Observatory ObsId 11358

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.obs.09516
title: Chandra X-ray Observatory ObsId 09516

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.obs.06585
title: Chandra X-ray Observatory ObsId 06585

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: 10.48577/jpl.ryd2ro
title: Motion Primitive Approach to Spacecraft Trajectory Design in the Neptune-Triton System

description: No abstract available.
DOI: 10.25574/csc2.obs.07133
title: Chandra X-ray Observatory ObsId 07133

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.obs.18715
title: Chandra X-ray Observatory ObsId 18715

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.obs.07374
title: Chandra X-ray Observatory ObsId 07374

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: 10.48577/jpl.ahalat
title: NEO Surveyor: Balancing Desats and Solar Pressure with Gravity

description: No abstract available.
DOI: 10.25574/csc2.obs.01611
title: Chandra X-ray Observatory ObsId 01611

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.obs.23677
title: Chandra X-ray Observatory ObsId 23677

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.obs.08198
title: Chandra X-ray Observatory ObsId 08198

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.obs.17059
title: Chandra X-ray Observatory ObsId 17059

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.obs.17234
title: Chandra X-ray Observatory ObsId 17234

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.obs.17032
title: Chandra X-ray Observatory ObsId 17032

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".