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opencc-by-4.0Mar 2020View details →

SUNERGY Kick-off video

SUNERGY Kick-off video. Video from the joint closing event for SUNRISE (www.sunriseaction.eu) and ENERGY-X (www.energy-x.eu) initiatives that served to present SUNERGY.

opencc-by-4.0Nov 2017View details →

SilkFusion_Kick-off_group photo

Attendees at the SilkFusion Kick-off meeting, Palazzo Bellisomi-Vistarino, Pavia, Italy, 23-24th November 2017.

opencc-by-4.0Jun 2021View details →

CIMPA Kick Off Meeting Press Release

Press release at the end of the CIMPA project Kick Off meeting in June 2021

opencc-by-4.0Jun 2024View details →

ImpactX+MADX input and output files for a thin-kick model of the FNAL Booster

Input and output files for a thin-kick model of the Fermilab Booster ring in MAD-X (expressed in SXF format), together with a Python script to parse and run ImpactX using the SXF lattice file.

FIG. 7. — A in The culture collection of cyanobacteria and microalgae at the French National Museum of Natural History: a century old but still alive and kicking! Including in memoriam: Professor Alain Couté

FIG. 7. — A, geographical distribution of cyanobacterial strains isolated around the world; B, strains isolated in the different administrative districts of France (metropolitan and overseas). Number of cyanobacterial strains in black, number of eukaryotic strains in blue. Strains isolated in France represent 58.0 % and 98.4 % of cyanobacterial and eukaryotic strains, respectively, in the collection.

FIG. 10 in The culture collection of cyanobacteria and microalgae at the French National Museum of Natural History: a century old but still alive and kicking! Including in memoriam: Professor Alain Couté

FIG. 10. — Culture of Onychonema filiforme (MNHN-ALCP-0000-086.1): A, from the 1948 catalogue of the algotheca (photo: R. Lami); B, the same culture observed in 2021 (photo: M. Jarno).

FIG. 5 in The culture collection of cyanobacteria and microalgae at the French National Museum of Natural History: a century old but still alive and kicking! Including in memoriam: Professor Alain Couté

FIG. 5. — Relative abundances of the different orders among the 1010 live strains represented in the cyanobacteria collection (left) and of the different phyla among the 345 live strains represented in the eukaryotic microalgae collection (right).

FIG. 6 in The culture collection of cyanobacteria and microalgae at the French National Museum of Natural History: a century old but still alive and kicking! Including in memoriam: Professor Alain Couté

FIG. 6. — Morphological diversity of cyanobacterial strains:A, B, Pseudochroococcus couteii (MNHN-PMC-2014-885); C, D, Planktothrix agardhii (MNHN-PMC-2002-75); E, F, Aphanizomenon gracile (MNHN-PMC-2010-627); G, H, Haloleptolyngbya elongata (MNHN-PMC-2015-895). Abbreviations: ae, aerotope; cc, cross-walls; cy, cyanophycin granules; cw, cell wall; mu, mucilage; r, reserves; s, sheath; tz, transparent zone; t, thylakoids. A, C, E, G: light microscopy; B, D, F, H: TEM micrographs. Scale bars: A, C, E, G, 10 µm; B, D, F, H, 500 nm.

FIG. 4 in The culture collection of cyanobacteria and microalgae at the French National Museum of Natural History: a century old but still alive and kicking! Including in memoriam: Professor Alain Couté

FIG. 4. — Emission spectra produced by Cool Daylight FLUO MAZDA (red) and White LEDs SLV (blue), both at a 85 μmol.m-2.s-1 (PAR) irradiance.

FIG. 1 in The culture collection of cyanobacteria and microalgae at the French National Museum of Natural History: a century old but still alive and kicking! Including in memoriam: Professor Alain Couté

FIG. 1. — From left to right: Pierre Allorge (1891-1944), Marcel Lefèvre (1897-1975) & Pierre Bourrelly (1910-1995).

FIG. 2 in The culture collection of cyanobacteria and microalgae at the French National Museum of Natural History: a century old but still alive and kicking! Including in memoriam: Professor Alain Couté

FIG. 2. — The "algothèque" in the Cryptogamy laboratory of the French National Museum of Natural History in Paris in 1935 and in 2021.

FIG. 3 in The culture collection of cyanobacteria and microalgae at the French National Museum of Natural History: a century old but still alive and kicking! Including in memoriam: Professor Alain Couté

FIG. 3. — Phylogeny of the 265 cyanobacterial strains for which a 16S rRNA sequence was obtained (see Appendix 1 for Genbank accession numbers and PMC identifiers). Phylogenetic reconstruction was based on Maximum likelihood with a GTR+G+I Model (5 categories and invariants) based on 1284 nucleotide positions, values at nodes were based on 100 bootstrap replicates. The number of strains (OTUs) is added when more than a single strain is available.

FIG. 8. — A, B in The culture collection of cyanobacteria and microalgae at the French National Museum of Natural History: a century old but still alive and kicking! Including in memoriam: Professor Alain Couté

FIG. 8. — A, B, Staurastrum polytrichum (MNHN-ALCP-2019-823.2), solitary cells with very deep median constriction (isthmus) dividing the cell into two semicells or hemisomates. SEM images show triangular semicells in apical view with straight sides, broadly rounded angles and many inframarginal spines (sp). Cell surface ornemented with pores. C, D, Cosmarium connatum (MNHN-ALCP-2019-832.1), solitary cells, lateral view with a barely marked isthmus (i) and smooth cell wall with pores. E, F, Synura petersenii (MNHN-ALCP-2019-877.3), colony and scales morphology. SEM images show rows of silica scales around individual cells. Scales with well-developed thorns (t). Ribs (r) running from the thorn to the scale perimeter up to the outer rim. G, H, Micrasterias furcata (MNHN-ALCP-2019-821.5), solitary cells, deeply constricted and dorsiventrally compressed. Semicells dissected into a polar lobe (p) divided into the second order. Lateral lobes (l) themselves divides into second and third order (or many times) ending with two simple spines (s). A, C, E, G: light microscopy; B, D, F, H: SEM micrographs. Scale bars: A, C, E, G, 20 µm; B, D, F, H, 10 µm.

FIG. 9 in The culture collection of cyanobacteria and microalgae at the French National Museum of Natural History: a century old but still alive and kicking! Including in memoriam: Professor Alain Couté

FIG. 9. — Example of morphological diversity among eukaryotic algae strains from ALCP collection: A, Centronella reicheltii (MNHN-ALCP-2020-884.1); B, Euglena gracilis (MNHN-ALCP-0000-006.3); C, Gymnodinium sp. (MNHN-ALCP-2019-879.1); D, Synura petersenii (MNHN-ALCP-2019-877.3); E, Chlorobotrys sp. (MNHN-ALCP-0000-003.1); F, Porphyridium purpureum (MNHN-ALCP-0000-100.2); G, Stigeoclonium sp. (MNHN-ALCP-2019-854.1); H, Oedogonium sp. (MNHN-ALCP-2019-867.1); I, Gonium formosum (MNHN-ALCP-2019-819.1); J, Haematococcus pluvialis (MNHN-ALCP-2019-876.1); K, Kirchneriella lunaris (MNHN-ALCP-0000-073.1); L, Monoraphidium sp. (MNHN-ALCP-2019-822.1); M, Dictyosphaerium pulchellum (MNHN-ALCP-2019-865.1); N, Picocystis salinarum (MNHN-ALCP-2018-144.1); O, Staurastrum sp. (MNHN-ALCP-2019-836.1); P, Spirogyra sp. (MNHN-ALCP-2019-858.1). Scale bars: 20 μm.

FIG. 11 in The culture collection of cyanobacteria and microalgae at the French National Museum of Natural History: a century old but still alive and kicking! Including in memoriam: Professor Alain Couté

FIG. 11. — An "algaegraphie" by the artist Lia Giraud representing one co-author, Claude Yéprémian (curator from 2007 to 2019).

opencc-by-4.0Aug 2021View details →

Dataset from: Binary population synthesis with probabilistic remnant mass and kick prescriptions

This contains the data behind the paper "<a href="https://ui.adsabs.harvard.edu/abs/2021MNRAS.500.1380M">Binary population synthesis with probabilistic remnant mass and kick prescriptions</a>" See<a href="https://github.com/TeamCOMPAS/COMPAS"> https://github.com/TeamCOMPAS/COMPAS</a> for code information and instructions on parsing the data.

opencc-by-4.0Mar 2024View details →

Kick vs Punch

This is a pre-processed version of the dataset saved in numpy format. The original dataset is obtained from <a href="http://mocap.cs.cmu.edu/subjects.php">CMU-MOCAP</a>. The data are 3-dimensional arrays of shape [n_samples, time_steps, n_variables]. The data can be loaded as follows: <pre><code>loaded_data = np.load("KickvsPunch.npz") Xtr = loaded_data['Xtr'] # Training data of shape (16, 841, 62) Ytr = loaded_data['Ytr'] # Training labels of shape (16, 1) Xte = loaded_data['Xte'] # Test data of shape (10, 841, 62) Yte = loaded_data['Yte'] # Test labels of shape (10, 1)</code></pre>

opencc-by-4.0Mar 2024View details →

Neutron Star - White Dwarf Binaries: Probing Formation Pathways and Natal Kicks with LISA

We present supplementary datasets accompanying our publication <a href="https://arxiv.org/abs/2310.06559">Neutron Star - White Dwarf Binaries: Probing Formation Pathways and Natal Kicks with LISA</a>. These catalogues reperesent the Galactic population of double white dwarf (DWD) and neutron star  - white dwarf (NSWD) binaries emitting gravitational waves (GWs) in the Laser Interferometer Space Antenna (LISA) frequency band (0.1 mHz - 1 Hz). The catalogues have been constructed based on binary evolution models <a href="https://arxiv.org/abs/1208.6446">Toonen et al. 2012</a> for DWDs and <a href="https://arxiv.org/abs/1804.01538">Toonen et al. 2018</a> for NSWD binaries, obtained using SeBa binary population synthesis code. Data contents The dataset consists of 12 catalogues representing Galactic populations of NSWD and/or DWD binaries, which are expected to be the most numerous types of binaries amongt LISA's Galactic sources. Each catalogue is distinguished by its model ID, which specifies the presence of NSWD and/or DWD binaries, the CE model used, CE efficiency values, and the NS natal kick prescription applied (see table below). Each catalogue is structured to describe a binary systems with the following attributes: <ul> <li>Name*: binary identifier; this consist of a prefix indicating the binary type (<code>'MW_DWD'</code> for a DWD binary, <code>'MW_NSWD_ecc0'</code> for a circular NSWD bianry, or <code>'MW_NSWD_ecc1'</code> for an eccentric NSWD binary) followed by a unique ID number. For example, <code>'MW_DWD 28713637'</code>.</li> <li>Frequency: present-day GW frequency (Hz).</li> <li>Frequency Derivative: rate of change of GW frequency over time (Hz^2).</li> <li>Ecliptic Latitude: in radians (rad).</li> <li>Ecliptic Longitude: in radians (rad).</li> <li>Amplitude: GW amplitude (dimensionless).</li> <li>Inclination: angle between the binary's orbital plane and our line of sight, in radians (rad).</li> <li>Polarization: Orientation of the GW's polarization, in radians (rad).</li> <li>Initial Phase: initial phase (rad).</li> <li>Eccentricity: orbital eccentricity (dimensionless).</li> </ul> *Note that the Name field for eccentric NS+WD binaries (staring with <code>'MW_NSWD_ecc1'</code>) is not unique because these binaries are represented by multiple harmonics sharing the same name ID. The number of harmonics included varies for each binary to ensure that at least 99% of the binary's total GW power is represented. Thus, for each binary, we added harmonics incrementally until this threshold is reached. <table> <tbody> <tr> <td>Model ID</td> <td>WD+WD</td> <td>NS+WD</td> <td>CE model</td> <td>CE efficiency</td> <td>NS natal kick</td> </tr> <tr> <td>1_0</td> <td>Yes</td> <td>No</td> <td>αα</td> <td>αλ=2.00</td> <td>N/A</td> </tr> <tr> <td>1_1</td> <td>Yes</td> <td>Yes</td> <td>αα</td> <td>αλ=2.00</td> <td>Verbunt</td> </tr> <tr> <td>1_2</td> <td>Yes</td> <td>Yes</td> <td>αα</td> <td>αλ=2.00</td> <td>Arzoumanian</td> </tr> <tr> <td>1_3</td> <td>Yes</td> <td>Yes</td> <td>αα</td> <td>αλ=2.00</td> <td>Hobbs</td> </tr> <tr> <td>1_4</td> <td>Yes</td> <td>Yes</td> <td>αα</td> <td>αλ=2.00</td> <td>Blaauw</td> </tr> <tr> <td>2_0</td> <td>Yes</td> <td>No</td> <td>αα2</td> <td>αλ=0.25</td> <td>N/A</td> </tr> <tr> <td>2_1</td> <td>Yes</td> <td>Yes</td> <td>αα2</td> <td>αλ=0.25</td> <td>Verbunt</td> </tr> <tr> <td>2_2</td> <td>Yes</td> <td>Yes</td> <td>αα2</td> <td>αλ=0.25</td> <td>Arzoumanian</td> </tr> <tr> <td>2_3</td> <td>Yes</td> <td>Yes</td> <td>αα2</td> <td>αλ=0.25</td> <td>Hobbs</td> </tr> <tr> <td>2_4</td> <td>Yes</td> <td>Yes</td> <td>αα2</td> <td>αλ=0.25</td> <td>Blaauw</td> </tr> <tr> <td>3_0</td> <td>Yes</td> <td>No</td> <td>αγ</td> <td>αλ=2.00, γ=1.75</td> <td>N/A</td> </tr> <tr> <td>3_1</td> <td>Yes</td> <td>Yes</td> <td>αγ</td> <td>αλ=2.00, γ=1.75</td> <td>Verbunt</td> </tr> </tbody> </table>   <h4>Citing the Dataset</h4> When utilising these catalogues in your research, please cite <a href="https://arxiv.org/abs/2310.06559">Korol et al. 2024.</a> We also note our companion data-analysis-focused paper <a href="https://arxiv.org/abs/2310.06568">Moore et al. 2024</a>.

opencc-by-4.0Aug 2018View details →

Nano2day kick-off meeting

Nano2day kick-off meeting. Photo of the consortium members.