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<style type="text/css">.ritz .waffle a { color: inherit; }.ritz .waffle .s0{background-color:#eef7e3;text-align:left;color:#000000;font-family:'docs-docs-Source Sans Pro',Arial;font-size:10pt;vertical-align:bottom;white-space:normal;overflow:hidden;word-wrap:break-word;direction:ltr;padding:2px 3px 2px 3px;}.ritz .waffle .s2{border-bottom:1px SOLID #26000000;border-right:1px SOLID #26000000;background-color:#ffffff;text-align:left;color:#000000;font-family:'docs-docs-Source Sans Pro',Arial;font-size:10pt;vertical-align:bottom;white-space:normal;overflow:hidden;word-wrap:break-word;direction:ltr;padding:2px 3px 2px 3px;}.ritz .waffle .s1{border-bottom:1px SOLID #26000000;border-right:1px SOLID #26000000;background-color:#ffffff;text-align:left;font-weight:bold;color:#000000;font-family:'docs-docs-Source Sans Pro',Arial;font-size:10pt;vertical-align:bottom;white-space:normal;overflow:hidden;word-wrap:break-word;direction:ltr;padding:2px 3px 2px 3px;}</style><div class="ritz grid-container" dir="ltr"><table class="waffle" cellspacing="0" cellpadding="0"><thead><tr><th class="row-header freezebar-origin-ltr"></th><th id="1996106432C0" style="width:100px;" class="column-headers-background">A</th><th id="1996106432C1" style="width:185px;" class="column-headers-background">B</th><th id="1996106432C2" style="width:130px;" class="column-headers-background">C</th><th id="1996106432C3" style="width:223px;" class="column-headers-background">D</th><th id="1996106432C4" style="width:274px;" class="column-headers-background">E</th><th id="1996106432C5" style="width:352px;" class="column-headers-background">F</th></tr></thead><tbody><tr style="height: 20px"><th id="1996106432R0" style="height: 20px;" class="row-headers-background"><div class="row-header-wrapper" style="line-height: 20px">1</div></th><td class="s0" dir="ltr" colspan="6"><span style="font-size:14pt;font-family:Source Sans Pro,Arial;font-weight:bold;">TVS In-Kind software contributions - march 2023 </span><span style="font-size:14pt;font-family:Source Sans Pro,Arial;">contributions in bold have been presented at a software workshop</span></td></tr><tr style="height: 20px"><th id="1996106432R1" style="height: 20px;" class="row-headers-background"><div class="row-header-wrapper" style="line-height: 20px">2</div></th><td class="s1" dir="ltr">SER-SAG-S1</td><td class="s1" dir="ltr">Science Pipeline Development for analysis of variability of celestial sources in the LSST AGN and TVS Science Collaboration</td><td class="s1" dir="ltr">Dr. Andjelka Kovacevic</td><td class="s1" dir="ltr">4.2 - Directable SW dev</td><td class="s1" dir="ltr">LSST AGN Science Collaboration</td><td class="s1" dir="ltr">LSST AGN Science Collaboration, LSST Transients and Variable Stars Science Collaboration</td></tr><tr style="height: 20px"><th id="1996106432R2" style="height: 20px;" class="row-headers-background"><div class="row-header-wrapper" style="line-height: 20px">3</div></th><td class="s2" dir="ltr">UKD-UKD-S10</td><td class="s2" dir="ltr">Science Software development: spectroscopic classification of transients and 4MOST spectra</td><td class="s2" dir="ltr">Prof Mark Sullivan</td><td class="s2" dir="ltr">4.3 - Non-directable SW dev</td><td class="s2" dir="ltr">LSST Dark Energy Science Collaboration</td><td class="s2" dir="ltr">LSST Dark Energy Science Collaboration, LSST Transients and Variable Stars Science Collaboration</td></tr><tr style="height: 20px"><th id="1996106432R3" style="height: 20px;" class="row-headers-background"><div class="row-header-wrapper" style="line-height: 20px">4</div></th><td class="s2" dir="ltr">ITA-INA-S12</td><td class="s2" dir="ltr">Directable SW contribution for the SMWLV SC: Machine Learning tools for the characterization of stellar populations</td><td class="s2" dir="ltr">Dr. Sara Lucatello</td><td class="s2" dir="ltr">4.2 - Directable SW dev</td><td class="s2" dir="ltr">LSST Stars Milky Way and Local Volume Science Collaboration</td><td class="s2" dir="ltr">LSST Stars Milky Way and Local Volume Science Collaboration, LSST Transients and Variable Stars Science Collaboration</td></tr><tr style="height: 20px"><th id="1996106432R4" style="height: 20px;" class="row-headers-background"><div class="row-header-wrapper" style="line-height: 20px">5</div></th><td class="s2" dir="ltr">CAN-CAN-S4</td><td class="s2" dir="ltr">Science Pipeline Development in the LSST Transient and Variable Star Science Collaboration</td><td class="s2" dir="ltr">Dr. Maria Drout</td><td class="s2" dir="ltr">4.2 - Directable SW dev</td><td class="s2" dir="ltr">LSST Transients and Variable Stars Science Collaboration</td><td class="s2" dir="ltr">LSST Transients and Variable Stars Science Collaboration</td></tr><tr style="height: 20px"><th id="1996106432R5" style="height: 20px;" class="row-headers-background"><div class="row-header-wrapper" style="line-height: 20px">6</div></th><td class="s1" dir="ltr">CRO-RBI-S1</td><td class="s1" dir="ltr">Science Analysis Infrastructure Effort</td><td class="s1" dir="ltr">Dr. Lovro Palaversa</td><td class="s1" dir="ltr">4.2 - Directable SW dev</td><td class="s1" dir="ltr">LSST Transients and Variable Stars Science Collaboration</td><td class="s1" dir="ltr">LSST Transients and Variable Stars Science Collaboration, Rubin International Program Coordinator (Software Development)</td></tr><tr style="height: 20px"><th id="1996106432R6" style="height: 20px;" class="row-headers-background"><div class="row-header-wrapper" style="line-height: 20px">7</div></th><td class="s1" dir="ltr">GER-ARI-S1</td><td class="s1" dir="ltr">Target and Observations Management (TOM) system Development in the LSST TVS Science Collaboration</td><td class="s1" dir="ltr">Dr. Yiannis Tsapras</td><td class="s1" dir="ltr">4.2 - Directable SW dev</td><td class="s1" dir="ltr">LSST Transients and Variable Stars Science Collaboration</td><td class="s1" dir="ltr">LSST Transients and Variable Stars Science Collaboration</td></tr><tr style="height: 20px"><th id="1996106432R7" style="height: 20px;" class="row-headers-background"><div class="row-header-wrapper" style="line-height: 20px">8</div></th><td class="s1" dir="ltr">HUN-KON-S2</td><td class="s1" dir="ltr">Directable Effort in the General Area of Machine Learning Classification and Associated Infrastructure Software</td><td class="s1" dir="ltr">Dr. Róbert Szabó (Konkoly Observatory)</td><td class="s1" dir="ltr">4.2 - Directable SW dev</td><td class="s1" dir="ltr">LSST Transients and Variable Stars Science Collaboration</td><td class="s1" dir="ltr">LSST Transients and Variable Stars Science Collaboration</td></tr><tr style="height: 20px"><th id="1996106432R8" style="height: 20px;" class="row-headers-background"><div class="row-header-wrapper" style="line-height: 20px">9</div></th><td class="s2" dir="ltr">IND-IUC-S3</td><td class="s2" dir="ltr">Science Pipeline Development in the LSST Transients and Variable stars Science Collaboration</td><td class="s2" dir="ltr">Dr. Sukanta Bose</td><td class="s2" dir="ltr">4.2 - Directable SW dev</td><td class="s2" dir="ltr">LSST Transients and Variable Stars Science Collaboration</td><td class="s2" dir="ltr">LSST Transients and Variable Stars Science Collaboration</td></tr><tr style="height: 20px"><th id="1996106432R9" style="height: 20px;" class="row-headers-background"><div class="row-header-wrapper" style="line-height: 20px">10</div></th><td class="s1" dir="ltr">ITA-INA-S3</td><td class="s1" dir="ltr">Directable SW contribution for the TVS SC: Development of a software to classify variable stars</td><td class="s1" dir="ltr">Rosaria Bonito</td><td class="s1" dir="ltr">4.2 - Directable SW dev</td><td class="s1" dir="ltr">LSST Transients and Variable Stars Science Collaboration</td><td class="s1" dir="ltr">LSST Transients and Variable Stars Science Collaboration</td></tr><tr style="height: 20px"><th id="1996106432R10" style="height: 20px;" class="row-headers-background"><div class="row-header-wrapper" style="line-height: 20px">11</div></th><td class="s1" dir="ltr">ITA-INA-S8</td><td class="s1" dir="ltr">Tools for the simulation of Pulsating Stars</td><td class="s1" dir="ltr">Ilaria Musella</td><td class="s1" dir="ltr">4.2 - Directable SW dev</td><td class="s1" dir="ltr">LSST Transients and Variable Stars Science Collaboration</td><td class="s1" dir="ltr">LSST Transients and Variable Stars Science Collaboration</td></tr><tr style="height: 20px"><th id="1996106432R11" style="height: 20px;" class="row-headers-background"><div class="row-header-wrapper" style="line-height: 20px">12</div></th><td class="s1" dir="ltr">ITA-INA-S10</td><td class="s1" dir="ltr">Directable SW contribution for the SMWLV and TVS SCs: Software Tools for</td><td class="s1" dir="ltr">Dr. Massimo Dall’Ora</td><td class="s1" dir="ltr">4.2 - Directable SW dev</td><td class="s1" dir="ltr">LSST Transients and Variable Stars Science Collaboration</td><td class="s1" dir="ltr">LSST Transients and Variable Stars Science Collaboration, LSST Stars Milky Way and Local Volume Science Collaboration, Rubin Crowded Field Coordination Group</td></tr><tr style="height: 20px"><th id="1996106432R12" style="height: 20px;" class="row-headers-background"><div class="row-header-wrapper" style="line-height: 20px">13</div></th><td class="s2" dir="ltr">ITA-INA-S15</td><td class="s2" dir="ltr">Tools for classification, full characterization and validation of variable sources</td><td class="s2" dir="ltr">Dr. Gisella Clementini</td><td class="s2" dir="ltr">4.2 - Directable SW dev</td><td class="s2" dir="ltr">LSST Transients and Variable Stars Science Collaboration</td><td class="s2" dir="ltr">LSST Transients and Variable Stars Science Collaboration</td></tr><tr style="height: 20px"><th id="1996106432R13" style="height: 20px;" class="row-headers-background"><div class="row-header-wrapper" style="line-height: 20px">14</div></th><td class="s2" dir="ltr">ITA-INA-S26</td><td class="s2" dir="ltr">Non-Directable SW contribution for the TVS SC: A Bridge from Gamma to Optical</td><td class="s2" dir="ltr">L.A. Antonelli</td><td class="s2" dir="ltr">4.3 - Non-directable SW dev</td><td class="s2" dir="ltr">LSST Transients and Variable Stars Science Collaboration</td><td class="s2" dir="ltr">LSST Transients and Variable Stars Science Collaboration, LSST Stars Milky Way and Local Volume Science Collaboration</td></tr><tr style="height: 20px"><th id="1996106432R14" style="height: 20px;" class="row-headers-background"><div class="row-header-wrapper" style="line-height: 20px">15</div></th><td class="s2" dir="ltr">MAL-ISS-S1</td><td class="s2" dir="ltr">Science Pipeline Development in the LSST TVS Science Collaboration and support for ISSC</td><td class="s2" dir="ltr">Dr. Kristian Zarb-Adami</td><td class="s2" dir="ltr">4.2 - Directable SW dev</td><td class="s2" dir="ltr">LSST Transients and Variable Stars Science Collaboration</td><td class="s2" dir="ltr">LSST Transients and Variable Stars Science Collaboration</td></tr><tr style="height: 20px"><th id="1996106432R15" style="height: 20px;" class="row-headers-background"><div class="row-header-wrapper" style="line-height: 20px">16</div></th><td class="s2" dir="ltr">NED-UTR-S4</td><td class="s2" dir="ltr">Multi-Messenger Astronomy Science Pipeline Development in the</td><td class="s2" dir="ltr">Dr. S Nissanke</td><td class="s2" dir="ltr">4.2 - Directable SW dev</td><td class="s2" dir="ltr">LSST Transients and Variable Stars Science Collaboration</td><td class="s2" dir="ltr">LSST Transients and Variable Stars Science Collaboration, LSST Dark Energy Science Collaboration</td></tr><tr style="height: 20px"><th id="1996106432R16" style="height: 20px;" class="row-headers-background"><div class="row-header-wrapper" style="line-height: 20px">17</div></th><td class="s2" dir="ltr">NED-UTR-S5</td><td class="s2" dir="ltr">Construction and maintenance of AGN catalogs to enable early science with LSST alerts</td><td class="s2" dir="ltr">Dr. Sjoert van Velzen</td><td class="s2" dir="ltr">4.3 - Non-directable SW dev</td><td class="s2" dir="ltr">LSST Transients and Variable Stars Science Collaboration</td><td class="s2" dir="ltr">LSST Transients and Variable Stars Science Collaboration, NOIRLab CSDC</td></tr><tr style="height: 20px"><th id="1996106432R17" style="height: 20px;" class="row-headers-background"><div class="row-header-wrapper" style="line-height: 20px">18</div></th><td class="s1" dir="ltr">SLO-UNG-S2</td><td class="s1" dir="ltr">Science Pipeline Development in the LSST TVS Science Collaboration</td><td class="s1" dir="ltr">Dr. Andreja Gomboc</td><td class="s1" dir="ltr">4.2 - Directable SW dev</td><td class="s1" dir="ltr">LSST Transients and Variable Stars Science Collaboration</td><td class="s1" dir="ltr">LSST Transients and Variable Stars Science Collaboration</td></tr><tr style="height: 20px"><th id="1996106432R18" style="height: 20px;" class="row-headers-background"><div class="row-header-wrapper" style="line-height: 20px">19</div></th><td class="s1" dir="ltr">UKD-UKD-S9</td><td class="s1" dir="ltr">Science Software development: Cross-matching</td><td class="s1" dir="ltr">Prof. Tim Naylor.</td><td class="s1" dir="ltr">4.3 - Non-directable SW dev</td><td class="s1" dir="ltr">LSST Transients and Variable Stars Science Collaboration</td><td class="s1" dir="ltr">LSST Transients and Variable Stars Science Collaboration, LSST Stars Milky Way and Local Volume Science Collaboration</td></tr></tbody></table></div>