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Louvre Artemis

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FIGURE 6 in Zyras (Diaulaconia) artemis sp. n., a new termitophilous species from Taiwan (Coleoptera: Staphylinidae: Aleocharinae: Lomechusini)

FIGURE 6. Variations of tHe spermatHeCa of Zyras (Diaulaconia) artemis sp. n. LoCality of eaCH speCimens: A, Gaupo (Taoyuan Co.); B, Hsilin trail (Hualien Co.); C, DaHasHan (Pingtung Co.); D, E, Dakeng (TaiCHung City); F, Xiaping (Nantou Co.); G, H, LuansHan (Taitung Co.); I, SHeding (Pingtung Co.); J, K, PengHu Islands (PengHu Co.).

FIGURE 5 in Zyras (Diaulaconia) artemis sp. n., a new termitophilous species from Taiwan (Coleoptera: Staphylinidae: Aleocharinae: Lomechusini)

FIGURE 5. Zyras (Diaulaconia) artemis sp. n., female. A, eigHt abdominal tergite, dorsal vieW; B 8th abdominal sternite, ventral vieW; C, spermatHeCa; D, tHe pHotograpH of tHe apiCal part and spermatHeCal gland; E, tHe pHotograpH of tHe inner Wall of apiCal 1/3 of tHe basal part; F, tHe base of tHe basal part and tHe spermatHeCal duCt.

FIGURE 3 in Zyras (Diaulaconia) artemis sp. n., a new termitophilous species from Taiwan (Coleoptera: Staphylinidae: Aleocharinae: Lomechusini)

FIGURE 3. Zyras (Diaulaconia) artemis sp. n. A, male 4th tergite WitH a pair of projeCtions on posterior margin, large individual, dorsal vieW; B, ditto, projeCtion bilobed apiCally, lateral vieW; C, ditto, small individual, dorsal vieW; D, ditto, projeCtion WitH no bilobed apiCally, lateral vieW; E, male 7th tergite WitH apiCal median tuberCle, dorsal vieW; F, ditto, lateral vieW; G, female 7th tergite WitH no small median tuberCle, dorsal vieW.

FIGURE 2 in Zyras (Diaulaconia) artemis sp. n., a new termitophilous species from Taiwan (Coleoptera: Staphylinidae: Aleocharinae: Lomechusini)

FIGURE 2. Zyras (Diaulaconia) artemis sp. n. A, forebody, dorsal vieW; B, rigHt antenna, lateral vieW; C, ditto, dorsal vieW; D, frons of tHe female WitHout granulations; E, frons of tHe male WitH granulations.

FIGURE 4 in Zyras (Diaulaconia) artemis sp. n., a new termitophilous species from Taiwan (Coleoptera: Staphylinidae: Aleocharinae: Lomechusini)

FIGURE 4. Zyras (Diaulaconia) artemis sp. n., male. A, eigHt abdominal tergite, dorsal vieW; B, 8th abdominal sternite, ventral vieW; C, median lobe of aedeagus, ventral vieW; D, ditto, tHe pHotograpH; E, ditto, lateral vieW; F, ditto, tHe pHotograpH.

Recording of Artemis I Orion with the Allen Telescope Array on 2022-11-16 (part 2/2)

This dataset contains an IQ recording of the S-band 2216.5 MHz telemetry signal from the Artemis I Orion Multipurpose Crewed Vehicle. The recording was done on 2022-11-16, about seven hours after launch. Antenna 1a from the Allen Telescope Array was used in dual XY (linear) polarization. The hardware configuration was as follows: the antenna was connected to RFCB LO d, which was tuned to a frequency of 2216.5 MHz and used an output IF of 512 MHz. A USRP N321 was connected to the IF output of the RFCB. The USRP N321 digitized both polarizations of the antenna. The USRP used an external 10 MHz reference and PPS coming from the observatory distribution system, and LO sharing was set up among the two channels. The IQ sample rate of the USRP was 10.24 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. After recording, the data was postprocessed to synthesize the signal polarization (which is expected to be RHCP) by finding and correcting the amplitude and phase offset between the X and Y channels, and adding coherently both channels. The data was converted to 8-bit to reduce the size of the dataset. Finally the dataset was formatted using <a href="https://github.com/gnuradio/SigMF">SigMF</a>. This dataset contains part 2. Part 1, which contains a recording done at an earlier time during the same session can be found <a href="https://zenodo.org/record/7395644">here</a>.

Recording of Artemis I Orion with the Allen Telescope Array on 2022-11-16 (part 1/2)

This dataset contains an IQ recording of the S-band 2216.5 MHz telemetry signal from the Artemis I Orion Multipurpose Crewed Vehicle. The recording was done on 2022-11-16, about seven hours after launch. Antenna 1a from the Allen Telescope Array was used in dual XY (linear) polarization. The hardware configuration was as follows: the antenna was connected to RFCB LO d, which was tuned to a frequency of 2216.5 MHz and used an output IF of 512 MHz. A USRP N321 was connected to the IF output of the RFCB. The USRP N321 digitized both polarizations of the antenna. The USRP used an external 10 MHz reference and PPS coming from the observatory distribution system, and LO sharing was set up among the two channels. The IQ sample rate of the USRP was 10.24 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. After recording, the data was postprocessed to synthesize the signal polarization (which is expected to be RHCP) by finding and correcting the amplitude and phase offset between the X and Y channels, and adding coherently both channels. The data was converted to 8-bit to reduce the size of the dataset. Finally the dataset was formatted using <a href="https://github.com/gnuradio/SigMF">SigMF</a>. This dataset contains part 1. Part 2, which contains a recording done at a later time during the same session can be found <a href="https://zenodo.org/record/7396606">here</a>.

Decoded Artemis I Orion S-band telemetry frames recieved with the Allen Telescope Array on 2022-11-16

This datasets contains the AOS Space Data Link frames obtained by decoding the Artemis I Orion Multipurpose Crewed Vehicle S-band telemetry signal at 2261.5 MHz using some IQ recordings done at the Allen Telescope Array on 2022-11-16, about 7 hours after launch. The 128-byte AOS frames are stored in raw binary files, which contain all the frames concatenated, with no headers or delimiters. The IQ recordings from which these frames have been decoded can be found in the datasets Recording of Artemis I Orion with the <a href="https://zenodo.org/record/7395644">Allen Telescope Array on 2022-11-16 (part 1/2)</a> and <a href="https://zenodo.org/record/7396606">Recording of Artemis I Orion with the Allen Telescope Array on 2022-11-16 (part 2/2)</a>.

Recordings of Artemis I LunaH-Map with the Allen Telescope Array on 2022-11-16

This dataset contains IQ recordings of the X-band 8451.7 MHz MHz telemetry signal from the Artemis I LunaH-Map cubesat. The recording was done on 2022-11-16, about seven hours after launch. Antennas 1a and 5c from the Allen Telescope Array were used in dual XY (linear) polarization. The hardware configuration was as follows: the antennas were connected to RFCB LO d, which was tuned to a frequency of 8451.5 MHz and used an output IF of 512 MHz. A USRP N321 and a USRP N320 were connected to the IF output of the RFCB. The USRP N321 digitized both polarizations of antenna 1a, while the USRP N320 digitized both polarizations of antenna 5c. The USRPs used an external 10 MHz reference and PPS coming from the observatory distribution system, and LO sharing was set up among all the channels. The IQ sample rate of the USRPs was 1.92 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. After recording, the data was converted to <a href="https://github.com/gnuradio/SigMF">SigMF</a> format. The detached headers are also provided in the dataset (they have the .hdr extension). There are two recordings in this dataset. In the first one, LunaH-Map is transmitting a PCM/PM/bi-phase-L signal at approximately 48 kbaud. In the second one, LunaH-Map is transmitting a PCM/PM/NRZ signal at approximately 255 kbaud. Since the second recording doesn't have good enough SNR for error-free decoding with a single antenna, the two antennas were beamformed by determining the correct complex amplitude, delay and frequency offsets for the two antennas, and by correcting these parameters before adding the signals. The beamformed signal is provided in the HMAP_2022-11-16T15:16:06_beamform SigMF dataset. In this dataset, the signal polarization has been synthesized by finding the correct amplitude and phase offset between the X and Y channels of each antenna, and adding coherently both channels before beamforming.

Recording of Artemis I EQUULEUS with the Allen Telescope Array on 2022-11-16

This dataset contains an IQ recording of the X-band 8443.5 MHz MHz telemetry signal from the Artemis I EQUULEUS cubesat. The recording was done on 2022-11-16, about seven hours after launch. Antennas 1a and 5c from the Allen Telescope Array were used in dual XY (linear) polarization. The hardware configuration was as follows: the antennas were connected to RFCB LO d, which was tuned to a frequency of 8443.5 MHz and used an output IF of 512 MHz. A USRP N321 and a USRP N320 were connected to the IF output of the RFCB. The USRP N321 digitized both polarizations of antenna 1a, while the USRP N320 digitized both polarizations of antenna 5c. The USRPs used an external 10 MHz reference and PPS coming from the observatory distribution system, and LO sharing was set up among all the channels. The IQ sample rate of the USRPs was 1.92 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. After recording, the data was converted to <a href="https://github.com/gnuradio/SigMF">SigMF</a> format. The detached headers are also provided in the dataset (they have the .hdr extension).

Recording of Artemis I ArgoMoon with the Allen Telescope Array on 2022-11-16

This dataset contains an IQ recording of the X-band 8475 MHz telemetry signal from the Artemis I ArgoMoon cubesat. The recording was done on 2022-11-16, about seven hours after launch. Antennas 1a and 5c from the Allen Telescope Array were used in dual XY (linear) polarization. The hardware configuration was as follows: the antennas were connected to RFCB LO d, which was tuned to a frequency of 8475 MHz and used an output IF of 512 MHz. A USRP N321 and a USRP N320 were connected to the IF output of the RFCB. The USRP N321 digitized both polarizations of antenna 1a, while the USRP N320 digitized both polarizations of antenna 5c. The USRPs used an external 10 MHz reference and PPS coming from the observatory distribution system, and LO sharing was set up among all the channels. The IQ sample rate of the USRPs was 1.92 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. After recording, the data was converted to <a href="https://github.com/gnuradio/SigMF">SigMF</a> format. The detached headers are also provided in the dataset (they have the .hdr extension). There are two recordings in this data set. A different modulation and data rate is used by ArgoMoon in each of them.

closedIPD-NOFeb 2026View details →

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ClinicalTrials.gov study NCT05832827. IPD Sharing: NO. Countries: 1. Publications: 29.

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Artemis Sleep Countermeasures

ClinicalTrials.gov study NCT06531733. IPD Sharing: UNDECIDED. Countries: 1. Publications: 24.

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ARTEMIS Synovial Markers in Arthritis Childhood

ClinicalTrials.gov study NCT02505828. IPD Sharing: Not stated. Countries: 1. Publications: 2.

controlledIPD-YESFeb 2026View details →

Autologous Gene Therapy for Artemis-Deficient SCID

ClinicalTrials.gov study NCT03538899. IPD Sharing: YES. Countries: 1. Publications: 53.