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21 results for “Psyche”
Spherical harmonic models of the shape of asteroid (16) Psyche
<p>This archive contains spherical harmonic models of the shape of asteroid (16) Psyche.</p> <p><strong>Psyche-Shepard2017.sh</strong></p> <p>This is a degree and order 29 spherical harmonic model of the shape of Psyche that was constructed from the shape model of Shepard et al. (2017). The spherical harmonic coefficients were obtained from a least squares inversion that made use of the vertex coordinates from the file <code>psyche.v.final.mod.mod</code>. The least squares inversion was performed using the pyshtools routine <code>SHCoeffs.from_least_squares()</code> and tests show that the power spectrum is stable for maximum degrees up to, and including, 29. The coefficients are in meters and should be used with 4-pi normalized spherical harmonic functions.</p> <p><strong>Psyche-Shepard2021.sh</strong></p> <p>This is a degree and order 10 spherical harmonic model of the shape of Psyche that was constructed from the shape model of Shepard et al. (2021). The spherical harmonic coefficients were obtained from a least squares inversion that made use of the vertex coordinates from the file <code>psyche.vertex.obj</code>. The least squares inversion was performed using the pyshtools routine <code>SHCoeffs.from_least_squares()</code>, and tests show that the power spectrum decreases dramatically for maximum spherical harmonic degrees beyond 10. The coefficients are in meters and should be used with 4-pi normalized spherical harmonic functions.</p>
Maps of thermal inertia, dielectric constant and brightness temperature of asteroid (16) Psyche derived from ALMA data
<p>These data and results are in support of the findings by Cambioni, S., de Kleer, K. and Shepard, M. in their paper "The Heterogeneous Surface of Asteroid (16) Psyche", Journal of Geophysical Research: Planets, link: https://agupubs.onlinelibrary.wiley.com/doi/abs/10.1029/2021JE007091. </p> <p>If using any of this material, please cite the above article as doi: 10.1029/2021JE007091</p> <p> </p>
Cupid and Psyche
Cupid and Psyche, statue in marble, executed in 1861 by Georg Christian Freund under the supervision of H.W. Bissen, after Thorvaldsen´s original model from 1807 (A27). Thorvaldsen Museum (Copenhagen, Denmark). Made with Memento Beta (Now ReMake) from AutoDesk. After many inhuman ordeals, Psyche has at last found her Cupid again. In her hand she holds a chalice with the elixir of immortality that will render her divine like her lover, so the two can finally marry. For more updates, please follow @GeoffreyMarchal on Twitter. Source: Objaverse 1.0 / Sketchfab
3D Printable Psyche Revived By Cupid
Psyche Revived by Cupid's Kiss at The Louvre, Paris (remix) Removed voids in the model. Now it's correct to slice in Simplify3D. Printed on [3D Printer Lad-1.0](https://3dladnik.wixsite.com/workshop/lad-1-0): Nozzle - 0.3 mm Layer - 100 μm support Colorless ABS  Source: Objaverse 1.0 / Sketchfab
Data for Estimate of water and hydroxyl abundance on asteroid (16) Psyche from JWST data
<p>The data as ASCII files used to produce the figures in the manuscript, " Estimate of water and hydroxyl abundance on asteroid (16) Psyche from JWST data". Almost all the files are ECSV files created from astropy Table. These files have complete metadata headers. Otherwise, the data, where appropriate, include s3d fits IFU data cubes used to produce 1D spectra, the solar spectra output by the Planetary Spectrum Generator, a thermophysical model output, asteroid reflectance measurements, and chondrite reflectance measurements all of which are described in further detail below. </p> <p>The Figures folder contains data behind the figures where data were used.</p> <p>For Figure 2 this corresponds to the NIRSpec and MIRI flux observations with a column for wavelength (in microns), flux (in Jansky), and error (in Jansky). </p> <p>For Figure 3 this corresponds to the normalized reflectance for the NIRSpec observations. The first column in each dataset corresponds to the wavelength in microns, the second column to the normalized reflectance (unitless), the third column to the error (unitless), and in the case of the .txt files the fourth column corresponds to the gaussian fit to the normalized reflectance. </p> <p>For Figure 4 these are the normalized reflectance divided by the continuum of the groups of data along wavelength ranges described in the manuscript for Figure 4. The first column corresponds to the wavelength in microns, the second column to the reflectance, the third column to the continuum fit to the data, the fourth column is the normalized reflectance divided by the continuum, and the error. </p> <p>For Figure 5 these are the data used to produce the 3-micron feature plot with the gaussian fit for each NIRSpec observation. The first column corresponds to the wavelength in microns, second column to the normalized reflectance divided by the continuum (unitless) and subtracted from the mean of the continuum between 3.6 and 3.7 microns such that the average of the continuum would be 0, the fourth column the error (unitless), and the fifth column the gaussian fit to the data. </p> <p>For Figure 6 the only additional data needed to produce this plot beyond what is provided for Figure 5 is the IRTF data which is provided as a text file. The first column corresponds to the wavelength in microns, the second column to the normalized reflectance divided by the continuum (unitless), and the third column to the error (unitless). </p> <p>For Figure 7 the additional data used to produce this plot beyond what is provided for Figure 5 includes laboratory reflectance measurements of various chondrites. The .scl files are the original laboratory measurements where the first column corresponds to the wavelength in microns, the second column to the normalized reflectance (unitless) and the third column to the error to 1 significant digit (unitless). The scaled_lab_reflectance.txt file has all the laboratory reflectance data used to produce the Figure 7 plot that includes the wavelength in microns, the normalized scaled reflectance for the CM chondrite, the normalized scaled reflectance for the CH/CBb chondrite, and the normalized scaled reflectance for the CY chondrite. </p> <p>For Figure 8 the additional data include original normalized reflectance data for asteroids interamnia, themis, bamberga, and europa as .trim files. The columns for these files correspond to wavelength in microns, normalized reflectance (unitless), and the error (unitless). The 'continuumremoved' .txt files correspond to the wavelength in microns and the normalized reflectance divided by the continuum (unitless). </p> <p>For Figure 9 these are the MIRI emissivity data for the two sets of observations. The first column corresponds to the wavelength in microns, the second column to the normalized emission by taking the flux subtracting the solar flux and dividing by a thermophysical model (unitless), the error (unitless), and the gaussian fit to the normalized emission. </p> <p>For the supplemental figures these are the additional fit absorption features that are located in the appendix of the manuscript. For the 1.25 - 4.8 micron text files the columns correspond to the wavelength in microns, the continuum divided normalized reflectance (unitless), the error (unitless), and the gaussian fit. For the 5.74 - 5.98 micron text files the columns correspond to wavelength in microns, normalized emission divided by a linear fit to a region outside any potential features (unitless), the error (unitless), and the gaussian fit to the feature. </p> <p>The MIRI 1D spectra folder contains the ASCII files corresponding to the 1 arcsec aperture summed spectra from the MIRI observations. The columns correspond to wavelength in microns, flux in Jansky, and error in Jansky. </p> <p>The NIRSpec 1D spectra folder contains the ASCII files corresponding to the 1 arcsec aperture summed spectra from the NIRSpec observations. The columns correspond to wavelength in microns, flux in Jansky, and error in Jansky. </p> <p>The Solar Spectra folder contains the solar spectra flux used to reduce the data to produce the reflectance and emission spectra. The lbl text files are equivalent to the files with the same name without the lbl but also include the column information. The first column corresponds to the wavelength in microns, the second column to the total spectral irradiance in Jansky, the third column to the flux from the object in Jansky, the fourth column to the reflected sunlight in Jansky, and the fifth column to the thermal contribution in Jansky. The only column used for the solar reflectance used in the analysis corresponds to the fourth column. </p> <p>The ThermalModel folder contains the ASCII files with the data corresponding to the thermophysical model used to produce the reflectance (by subtracting the thermal contribution) and the emission (by dividing by the thermal contribution). The first column corresponds to the wavelength in microns, the second to the thermal flux in Jansky, the third to the smoothed thermal flux in Jansky, and the fourth column to the normalized thermal flux. Only column two corresponding to the thermal flux in Jansky was used in the analysis associated with the manuscript. </p>
PSYCHE-D: predicting change in depression severity using person-generated health data (DATASET)
<p>This dataset is made available under <a href="https://creativecommons.org/licenses/by-nc/4.0/">Creative Commons Attribution-NonCommercial 4.0 International (CC BY-NC 4.0)</a>. See LICENSE.pdf for details.</p> <p><strong>Dataset description</strong></p> <p>Parquet file, with:</p> <ul> <li>35694 rows</li> <li>154 columns</li> </ul> <p>The file is indexed on [<em>participant</em>]_[<em>month</em>], such that 34_12 means month 12 from participant 34. All participant IDs have been replaced with randomly generated integers and the conversion table deleted.</p> <p>Column names and explanations are included as a separate tab-delimited file. Detailed descriptions of feature engineering are available from the linked publications.</p> <p>File contains aggregated, derived feature matrix describing person-generated health data (PGHD) captured as part of the DiSCover Project (<a href="https://clinicaltrials.gov/ct2/show/NCT03421223">https://clinicaltrials.gov/ct2/show/NCT03421223</a>). This matrix focuses on individual changes in depression status over time, as measured by PHQ-9.</p> <p>The DiSCover Project is a 1-year long longitudinal study consisting of 10,036 individuals in the United States, who wore consumer-grade wearable devices throughout the study and completed monthly surveys about their mental health and/or lifestyle changes, between January 2018 and January 2020.</p> <p>The data subset used in this work comprises the following:</p> <ul> <li>Wearable PGHD: step and sleep data from the participants’ consumer-grade wearable devices (Fitbit) worn throughout the study</li> <li>Screener survey: prior to the study, participants self-reported socio-demographic information, as well as comorbidities</li> <li>Lifestyle and medication changes (LMC) survey: every month, participants were requested to complete a brief survey reporting changes in their lifestyle and medication over the past month</li> <li>Patient Health Questionnaire (PHQ-9) score: every 3 months, participants were requested to complete the PHQ-9, a 9-item questionnaire that has proven to be reliable and valid to measure depression severity</li> </ul> <p>From these input sources we define a range of input features, both static (defined once, remain constant for all samples from a given participant throughout the study, e.g. demographic features) and dynamic (varying with time for a given participant, e.g. behavioral features derived from consumer-grade wearables).</p> <p>The dataset contains a total of 35,694 rows for each month of data collection from the participants. We can generate 3-month long, non-overlapping, independent samples to capture changes in depression status over time with PGHD. We use the notation ‘SM0’ (sample month 0), ‘SM1’, ‘SM2’ and ‘SM3’ to refer to relative time points within each sample. Each 3-month sample consists of: PHQ-9 survey responses at SM0 and SM3, one set of screener survey responses, LMC survey responses at SM3 (as well as SM1, SM2, if available), and wearable PGHD for SM3 (and SM1, SM2, if available). The wearable PGHD includes data collected from 8 to 14 days prior to the PHQ-9 label generation date at SM3. Doing this generates a total of 10,866 samples from 4,036 unique participants.</p>
Recording of Psyche with the Allen Telescope Array shortly after launch (decimated)
<p>This dataset contains an IQ recording of the X-band 8417.7 MHz telemetry signal from the Psyche spacecraft done with the Allen Telescope Array starting only 1 hour 30 minutes after launch. Antennas 1a and 5c from the ATA were used in dual linear polarization (X and Y polarizations).</p><p>The hardware configuration was as follows: the antennas were connected to RFCB LO d, which was tuned to a frequency of 8417 MHz and used an output IF of 512 MHz. A USRP N321 and N320 digitized both polarizations of each antenna. The USRPs used an external 10 MHz reference and PPS coming from the observatory distribution system, and LO sharing was set up among the four channels. The IQ sample rate of the USRPs was 4.096 Msps and a GNU Radio flowgraph was used to record IQ data to disk. The GNU Radio flowgraph stored the IQ data for each channel as 16-bin integers in the <a href="https://wiki.gnuradio.org/index.php/Metadata_Information">GNU Radio metatata file format</a>, with detached headers.</p><p>After recording, the data was downsampled to 128 ksps centered around 8417.525 MHz and formatted using <a href="https://github.com/gnuradio/SigMF">SigMF</a> with the script do_sigmf.py. This reduced bandwidth is sufficient to decode the low data rate (2 kbps) telemetry signal. There is a higher data rate (61.1 kbps) signal, as well as sequential ranging tones, near the end of the recording for which this bandwidth is insufficient. The original 4.096 Msps data for this part of the recording has been published for a single antenna and polarization in 8-bit resolution in the dataset "<a href="https://zenodo.org/records/10023378">Recording of Psyche with the Allen Telescope Array shortly after launch (wideband)</a>".</p>
Recording of Psyche with the Allen Telescope Array shortly after launch (wideband)
<p>This dataset contains an IQ recording of the X-band 8417.7 MHz telemetry signal from the Psyche spacecraft done with the Allen Telescope Array starting only 1 hour 30 minutes after launch. Antennas 1a and 5c from the ATA were used in dual linear polarization (X and Y polarizations).</p> <p>The hardware configuration was as follows: the antennas were connected to RFCB LO d, which was tuned to a frequency of 8417 MHz and used an output IF of 512 MHz. A USRP N321 and N320 digitized both polarizations of each antenna. The USRPs used an external 10 MHz reference and PPS coming from the observatory distribution system, and LO sharing was set up among the four channels. The IQ sample rate of the USRPs was 4.096 Msps and a GNU Radio flowgraph was used to record IQ data to disk. The GNU Radio flowgraph stored the IQ data for each channel as 16-bin integers in the <a href="https://wiki.gnuradio.org/index.php/Metadata_Information">GNU Radio metatata file format</a>, with detached headers.</p> <p>After recording, the data was formatted using <a href="https://github.com/gnuradio/SigMF">SigMF</a> with the script do_sigmf.py. This dataset contains only the last part of the recording in the original 4.096 Msps sample rate, and only one antenna and polarization. During most of the recording the spacecraft signal is a low rate signal (2 kbps) that fits in a much smaller bandwidth, so another dataset "<a href="https://zenodo.org/records/10003647">Recording of Psyche with the Allen Telescope Array shortly after launch (decimated)</a>" has been published with 128 ksps centered at this signal for each antenna and polarization.</p>
Randomized Trial Of Achieving Healthy Lifestyles In Psych Rehabilitation
ClinicalTrials.gov study NCT00902694. IPD Sharing: Not stated. Countries: 1. Publications: 3.
Cupid Revives Psyche - Low Poly
A very low poly version of Geoffrey Marchal's [Cupid Revives Psyche](https://sketchfab.com/models/b856632b62da42ab8468d1169ece5b2c) Source: Objaverse 1.0 / Sketchfab
Cupid (or Amor) and Psyche – Austerlitz
A sculptural group from 1705 depicting a mythological story about Cupid and Psyche. Cupid and Psyche is a story originally from Metamorphoses, written in the 2nd century AD by Lucius Apuleius Madaurensis (or Platonicus). The tale concerns the overcoming of obstacles to the love between Psyche and Cupid (or Amor – "Love"; also Eros and Psyche), and their ultimate union in a sacred marriage. A sculptural group from the workshop of Giovanni Giuliani (1664–1744) was created in 1705 on the order of Count Dominic Andreas von Kaunitz (1655–1705). Today the baroque statue is located in the garden of the Austerlitz Castle (Slavkov u Brna). Material: limestone; height (approx.): 450 cm. _____ *Photo from today's location:*  Source: Objaverse 1.0 / Sketchfab
Data for "The Geologic Impact of 16 Psyche's Surface Temperatures"
<p>This repository contains the data used to create the figures in "The Geologic Impact of 16 Psyche's Surface Temperatures"</p>
PSilocybin for psYCHological and Existential Distress in PALliative Care (PSYCHED-PAL)
ClinicalTrials.gov study NCT04754061. IPD Sharing: NO. Countries: 1. Publications: 14.
Myasthenia Gravis and Psyche
ClinicalTrials.gov study NCT03205306. IPD Sharing: Not stated. Countries: 1. Publications: 1.
Psilocybin Microdose for Psychological and Existential Distress in Palliative Care (PSYCHED-PAL-RCT)
ClinicalTrials.gov study NCT07063862. IPD Sharing: NO. Countries: 1. Publications: 15.
Utilising Psych Arrays for the identification of CNVs and SNPs from Schizophrenia cases and controls from South-India.
GEO Series GSE242813. Homo sapiens. 373 samples. Type: Methylation profiling by array.
Psyche with the jar
Psyche with the jar (1806), (ref A26), Bertel Thorvaldsens, plaster, height: 1,32 m. Thorvaldsens museum (Copenhagen, Denmark). Made with Memento Beta (now ReMake) from AutoDesk. On this plaster, the wings are still not present but will be added on the final sculpture in marble. For more updates, please follow @GeoffreyMarchal on Twitter. Source: Objaverse 1.0 / Sketchfab
Cupid and Psyche: Rodin
A scuplture of Cupid and Psyche created by Auguste Rodin around 1898. **Badly scanned around the top part of the bodies, so needs redoing.** Credit Line: Given to the Victoria and Albert Museum by Rodin in 1914 Museum number: A.49-1914 Gallery location: Sculpture, Room 21, The Dorothy and Michael Hintze Galleries, case FS, shelf WN Source: Objaverse 1.0 / Sketchfab
PSYCHE Cognitive Remediation & Social Recovery Study
ClinicalTrials.gov study NCT06032182. IPD Sharing: YES. Countries: 1. Publications: 0.
PSYCHE (Personalised Monitoring SYstems for Care in Mental Health)
ClinicalTrials.gov study NCT01879982. IPD Sharing: Not stated. Countries: 1. Publications: 0.
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International Brain Laboratory public data
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OpenNeuro
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