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<!DOCTYPE HTML>
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<title>TVS Software Contributions</title>
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<h2>TVS In-Kind Software Contributions</h2>
<p>Status as of March 2023. Contributions in bold have been presented at a software workshop.</p>
<p> The updated list of TVS software contributions can be found <a href="taskForces/in_kind_software_task_force.html">here</a>.</p>
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<th>#</th>
<th>ID</th>
<th>Contribution Title</th>
<th>Lead</th>
<th>Category</th>
<th>Primary Collaborator</th>
<th>Benefitting Collaborations</th>
</tr>
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<tr>
<td>1</td>
<td><b>SER-SAG-S1</b></td>
<td><b>Science Pipeline Development for analysis of variability of celestial sources in the LSST AGN and TVS Science Collaboration</b></td>
<td><b>Dr. Andjelka Kovacevic</b></td>
<td><b>4.2 - Directable SW dev</b></td>
<td><b>LSST AGN Science Collaboration</b></td>
<td><b>LSST AGN Science Collaboration, LSST Transients and Variable Stars Science Collaboration</b></td>
</tr>
<tr>
<td>2</td>
<td>UKD-UKD-S10</td>
<td>Science Software development: spectroscopic classification of transients and 4MOST spectra</td>
<td>Prof Mark Sullivan</td>
<td>4.3 - Non-directable SW dev</td>
<td>LSST Dark Energy Science Collaboration</td>
<td>LSST Dark Energy Science Collaboration, LSST Transients and Variable Stars Science Collaboration</td>
</tr>
<tr>
<td>3</td>
<td>ITA-INA-S12</td>
<td>Directable SW contribution for the SMWLV SC: Machine Learning tools for the characterization of stellar populations</td>
<td>Dr. Sara Lucatello</td>
<td>4.2 - Directable SW dev</td>
<td>LSST Stars Milky Way and Local Volume Science Collaboration</td>
<td>LSST Stars Milky Way and Local Volume Science Collaboration, LSST Transients and Variable Stars Science Collaboration</td>
</tr>
<tr>
<td>4</td>
<td>CAN-CAN-S4</td>
<td>Science Pipeline Development in the LSST Transient and Variable Star Science Collaboration</td>
<td>Dr. Maria Drout</td>
<td>4.2 - Directable SW dev</td>
<td>LSST Transients and Variable Stars Science Collaboration</td>
<td>LSST Transients and Variable Stars Science Collaboration</td>
</tr>
<tr>
<td>5</td>
<td><b>CRO-RBI-S1</b></td>
<td><b>Science Analysis Infrastructure Effort</b></td>
<td><b>Dr. Lovro Palaversa</b></td>
<td><b>4.2 - Directable SW dev</b></td>
<td><b>LSST Transients and Variable Stars Science Collaboration</b></td>
<td><b>LSST Transients and Variable Stars Science Collaboration, Rubin International Program Coordinator (Software Development)</b></td>
</tr>
<tr>
<td>6</td>
<td><b>GER-ARI-S1</b></td>
<td><b>Target and Observations Management (TOM) system Development in the LSST TVS Science Collaboration</b></td>
<td><b>Dr. Yiannis Tsapras</b></td>
<td><b>4.2 - Directable SW dev</b></td>
<td><b>LSST Transients and Variable Stars Science Collaboration</b></td>
<td><b>LSST Transients and Variable Stars Science Collaboration</b></td>
</tr>
<tr>
<td>7</td>
<td><b>HUN-KON-S2</b></td>
<td><b>Directable Effort in the General Area of Machine Learning Classification and Associated Infrastructure Software</b></td>
<td><b>Dr. Róbert Szabó (Konkoly Observatory)</b></td>
<td><b>4.2 - Directable SW dev</b></td>
<td><b>LSST Transients and Variable Stars Science Collaboration</b></td>
<td><b>LSST Transients and Variable Stars Science Collaboration</b></td>
</tr>
<tr>
<td>8</td>
<td>IND-IUC-S3</td>
<td>Science Pipeline Development in the LSST Transients and Variable stars Science Collaboration</td>
<td>Dr. Sukanta Bose</td>
<td>4.2 - Directable SW dev</td>
<td>LSST Transients and Variable Stars Science Collaboration</td>
<td>LSST Transients and Variable Stars Science Collaboration</td>
</tr>
<tr>
<td>9</td>
<td><b>ITA-INA-S3</b></td>
<td><b>Directable SW contribution for the TVS SC: Development of a software to classify variable stars</b></td>
<td><b>Rosaria Bonito</b></td>
<td><b>4.2 - Directable SW dev</b></td>
<td><b>LSST Transients and Variable Stars Science Collaboration</b></td>
<td><b>LSST Transients and Variable Stars Science Collaboration</b></td>
</tr>
<tr>
<td>10</td>
<td><b>ITA-INA-S8</b></td>
<td><b>Tools for the simulation of Pulsating Stars</b></td>
<td><b>Ilaria Musella</b></td>
<td><b>4.2 - Directable SW dev</b></td>
<td><b>LSST Transients and Variable Stars Science Collaboration</b></td>
<td><b>LSST Transients and Variable Stars Science Collaboration</b></td>
</tr>
<tr>
<td>11</td>
<td><b>ITA-INA-S10</b></td>
<td><b>Directable SW contribution for the SMWLV and TVS SCs: Software Tools for</b></td>
<td><b>Dr. Massimo Dall’Ora</b></td>
<td><b>4.2 - Directable SW dev</b></td>
<td><b>LSST Transients and Variable Stars Science Collaboration</b></td>
<td><b>LSST Transients and Variable Stars Science Collaboration, LSST Stars Milky Way and Local Volume Science Collaboration, Rubin Crowded Field Coordination Group</b></td>
</tr>
<tr>
<td>12</td>
<td>ITA-INA-S15</td>
<td>Tools for classification, full characterization and validation of variable sources</td>
<td>Dr. Gisella Clementini</td>
<td>4.2 - Directable SW dev</td>
<td>LSST Transients and Variable Stars Science Collaboration</td>
<td>LSST Transients and Variable Stars Science Collaboration</td>
</tr>
<tr>
<td>13</td>
<td>ITA-INA-S26</td>
<td>Non-Directable SW contribution for the TVS SC: A Bridge from Gamma to Optical</td>
<td>L.A. Antonelli</td>
<td>4.3 - Non-directable SW dev</td>
<td>LSST Transients and Variable Stars Science Collaboration</td>
<td>LSST Transients and Variable Stars Science Collaboration, LSST Stars Milky Way and Local Volume Science Collaboration</td>
</tr>
<tr>
<td>14</td>
<td>MAL-ISS-S1</td>
<td>Science Pipeline Development in the LSST TVS Science Collaboration and support for ISSC</td>
<td>Dr. Kristian Zarb-Adami</td>
<td>4.2 - Directable SW dev</td>
<td>LSST Transients and Variable Stars Science Collaboration</td>
<td>LSST Transients and Variable Stars Science Collaboration</td>
</tr>
<tr>
<td>15</td>
<td>NED-UTR-S4</td>
<td>Multi-Messenger Astronomy Science Pipeline Development in the</td>
<td>Dr. S Nissanke</td>
<td>4.2 - Directable SW dev</td>
<td>LSST Transients and Variable Stars Science Collaboration</td>
<td>LSST Transients and Variable Stars Science Collaboration, LSST Dark Energy Science Collaboration</td>
</tr>
<tr>
<td>16</td>
<td>NED-UTR-S5</td>
<td>Construction and maintenance of AGN catalogs to enable early science with LSST alerts</td>
<td>Dr. Sjoert van Velzen</td>
<td>4.3 - Non-directable SW dev</td>
<td>LSST Transients and Variable Stars Science Collaboration</td>
<td>LSST Transients and Variable Stars Science Collaboration, NOIRLab CSDC</td>
</tr>
<tr>
<td>17</td>
<td><b>SLO-UNG-S2</b></td>
<td><b>Science Pipeline Development in the LSST TVS Science Collaboration</b></td>
<td><b>Dr. Andreja Gomboc</b></td>
<td><b>4.2 - Directable SW dev</b></td>
<td><b>LSST Transients and Variable Stars Science Collaboration</b></td>
<td><b>LSST Transients and Variable Stars Science Collaboration</b></td>
</tr>
<tr>
<td>18</td>
<td><b>UKD-UKD-S9</b></td>
<td><b>Science Software development: Cross-matching</b></td>
<td><b>Prof. Tim Naylor.</b></td>
<td><b>4.3 - Non-directable SW dev</b></td>
<td><b>LSST Transients and Variable Stars Science Collaboration</b></td>
<td><b>LSST Transients and Variable Stars Science Collaboration, LSST Stars Milky Way and Local Volume Science Collaboration</b></td>
</tr>
</tbody>
</table>
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<h2>About</h2>
<p>TVS is a <a href="https://rubinobservatory.org">Vera C. Rubin Observatory</a> Legacy Survey of Space and Time <a href="https://www.lsstcorporation.org/science-collaborations">Science Collaboration</a> (SC). Our SC is a group focused on preparing to study the transient and variable sky with the revolutionary Legacy Survey of Space and Time (LSST).</p>
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