SOAR/Goodman Spectroscopic Assessment of Candidate Counterparts of the LIGO-Virgo Event GW190814

On 2019 August 14 at 21:10:39 UTC, the LIGO/Virgo Collaboration (LVC) detected a possible neutron star-black hole merger (NSBH), the first ever identified. An extensive search for an optical counterpart of this event, designated GW190814, was undertaken using the Dark Energy Camera (DECam) on the 4m...

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Veröffentlicht in:arXiv.org 2022-06
Hauptverfasser: Tucker, Douglas, Allam, Sahar, Soares-Santos, Marcelle, Clecio de Bom, Butner, Melissa, Garcia, Alyssa, Morgan, Robert, Palmese, Antonella, Santana-Silva, Luidhy, Shrivastava, Anushka, Kilpatrick, Charles, Sherman, Nora, Amara, Adam, Lin, Huan, Smith, Mathew, Swann, Elizabeth, Bachmann, Tristan, Bechtol, Keith, Berlfein, Federico, Briceno, Cesar, Butler, Bobby, Cartier, Regis, Casares, Jorge, Hsin-Yu, Chen, Conselice, Christopher, Cooke, Jeff, Dage, Kristen, D'Andrea, Chris, Davis, Tamara, de Carvalho, Reinaldo, Diehl, Tom, Doctor, Zoheyr, Drout, Maria, Farr, Ben, Foley, Ryan, Frieman, Josh, Frohmaier, Christopher, Gruendl, Robert, Holz, Daniel, Kessler, Richard, Kuropatkin, Nikolay, Lahav, Ofer, Lundquist, Michael, Mann, Andrew, Marshall, Jennifer, Martinez-Vazquez, Clara, McCully, Curtis, Menanteau, Felipe, Meza, Nico, Narayan, Gautham, Neilsen, Eric, Nicolaou, Constantina, Pineda, Jonathan, Points, Sean, Quirola-Vasquez, Jonathan, Rest, Armin, Rodriguez, Osmar, Sako, Masao, Salim, Samir, Scolnic, Daniel, Smith, J Allyn, Sullivan, Mark, Thomas, Daniel, Walker, Alistair, Weller, Jochen, Wood, Mackenna, Aguena, Michel, Andrade-Oliveira, Felipe, Bertin, Emmanuel, Brooks, David, Burke, David, Aurelio Carnero Rosell, Carretero, Jorge, Costanzi, Matteo, da Costa, Luiz, De Vicente, Juan, Desai, Shantanu, Spencer, Everett, Ferrero, Ismael, Flaugher, Brenna, Gerdes, David, Gschwend, Julia, Gutierrez, Gaston, Hollowood, Devon L, Honscheid, Klaus, James, David, Maia, Marcio, Miquel, Ramon, Ogando, Ricardo, Pieres, Adriano, Rodriguez-Monroy, Martin, Sanchez, Eusebio, Scarpine, Vic, Schubnell, Michael, Serrano, Santiago, Sevilla-Noarbe, Ignacio, Suchyta, Eric, Tarle, Gregory, Chun-Hao To, Zhang, Yuanyuan
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container_title arXiv.org
container_volume
creator Tucker, Douglas
Allam, Sahar
Soares-Santos, Marcelle
Clecio de Bom
Butner, Melissa
Garcia, Alyssa
Morgan, Robert
Palmese, Antonella
Santana-Silva, Luidhy
Shrivastava, Anushka
Kilpatrick, Charles
Sherman, Nora
Amara, Adam
Lin, Huan
Smith, Mathew
Swann, Elizabeth
Bachmann, Tristan
Bechtol, Keith
Berlfein, Federico
Briceno, Cesar
Butler, Bobby
Cartier, Regis
Casares, Jorge
Hsin-Yu, Chen
Conselice, Christopher
Cooke, Jeff
Dage, Kristen
D'Andrea, Chris
Davis, Tamara
de Carvalho, Reinaldo
Diehl, Tom
Doctor, Zoheyr
Drout, Maria
Farr, Ben
Foley, Ryan
Frieman, Josh
Frohmaier, Christopher
Gruendl, Robert
Holz, Daniel
Kessler, Richard
Kuropatkin, Nikolay
Lahav, Ofer
Lundquist, Michael
Mann, Andrew
Marshall, Jennifer
Martinez-Vazquez, Clara
McCully, Curtis
Menanteau, Felipe
Meza, Nico
Narayan, Gautham
Neilsen, Eric
Nicolaou, Constantina
Pineda, Jonathan
Points, Sean
Quirola-Vasquez, Jonathan
Rest, Armin
Rodriguez, Osmar
Sako, Masao
Salim, Samir
Scolnic, Daniel
Smith, J Allyn
Sullivan, Mark
Thomas, Daniel
Walker, Alistair
Weller, Jochen
Wood, Mackenna
Aguena, Michel
Andrade-Oliveira, Felipe
Bertin, Emmanuel
Brooks, David
Burke, David
Aurelio Carnero Rosell
Carretero, Jorge
Costanzi, Matteo
da Costa, Luiz
De Vicente, Juan
Desai, Shantanu
Spencer, Everett
Ferrero, Ismael
Flaugher, Brenna
Gerdes, David
Gschwend, Julia
Gutierrez, Gaston
Hollowood, Devon L
Honscheid, Klaus
James, David
Maia, Marcio
Miquel, Ramon
Ogando, Ricardo
Pieres, Adriano
Rodriguez-Monroy, Martin
Sanchez, Eusebio
Scarpine, Vic
Schubnell, Michael
Serrano, Santiago
Sevilla-Noarbe, Ignacio
Suchyta, Eric
Tarle, Gregory
Chun-Hao To
Zhang, Yuanyuan
description On 2019 August 14 at 21:10:39 UTC, the LIGO/Virgo Collaboration (LVC) detected a possible neutron star-black hole merger (NSBH), the first ever identified. An extensive search for an optical counterpart of this event, designated GW190814, was undertaken using the Dark Energy Camera (DECam) on the 4m Victor M. Blanco Telescope at the Cerro Tololo Inter-American Observatory. Target of Opportunity interrupts were issued on 8 separate nights to observe 11 candidates using the 4.1m Southern Astrophysical Research (SOAR) telescope's Goodman High Throughput Spectrograph in order to assess whether any of these transients was likely to be an optical counterpart of the possible NSBH merger. Here, we describe the process of observing with SOAR, the analysis of our spectra, our spectroscopic typing methodology, and our resultant conclusion that none of the candidates corresponded to the gravitational wave merger event but were all instead other transients. Finally, we describe the lessons learned from this effort. Application of these lessons will be critical for a successful community spectroscopic follow-up program for LVC observing run 4 (O4) and beyond.
doi_str_mv 10.48550/arxiv.2109.13351
format Article
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An extensive search for an optical counterpart of this event, designated GW190814, was undertaken using the Dark Energy Camera (DECam) on the 4m Victor M. Blanco Telescope at the Cerro Tololo Inter-American Observatory. Target of Opportunity interrupts were issued on 8 separate nights to observe 11 candidates using the 4.1m Southern Astrophysical Research (SOAR) telescope's Goodman High Throughput Spectrograph in order to assess whether any of these transients was likely to be an optical counterpart of the possible NSBH merger. Here, we describe the process of observing with SOAR, the analysis of our spectra, our spectroscopic typing methodology, and our resultant conclusion that none of the candidates corresponded to the gravitational wave merger event but were all instead other transients. Finally, we describe the lessons learned from this effort. Application of these lessons will be critical for a successful community spectroscopic follow-up program for LVC observing run 4 (O4) and beyond.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.2109.13351</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Black holes ; Neutron stars ; Neutrons ; Optical counterparts (astronomy) ; Physics - High Energy Astrophysical Phenomena</subject><ispartof>arXiv.org, 2022-06</ispartof><rights>2022. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><rights>http://creativecommons.org/licenses/by/4.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,782,786,887,27934</link.rule.ids><backlink>$$Uhttps://doi.org/10.3847/1538-4357/ac5b60$$DView published paper (Access to full text may be restricted)$$Hfree_for_read</backlink><backlink>$$Uhttps://doi.org/10.48550/arXiv.2109.13351$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Tucker, Douglas</creatorcontrib><creatorcontrib>Allam, Sahar</creatorcontrib><creatorcontrib>Soares-Santos, Marcelle</creatorcontrib><creatorcontrib>Clecio de Bom</creatorcontrib><creatorcontrib>Butner, 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Jochen</creatorcontrib><creatorcontrib>Wood, Mackenna</creatorcontrib><creatorcontrib>Aguena, Michel</creatorcontrib><creatorcontrib>Andrade-Oliveira, Felipe</creatorcontrib><creatorcontrib>Bertin, Emmanuel</creatorcontrib><creatorcontrib>Brooks, David</creatorcontrib><creatorcontrib>Burke, David</creatorcontrib><creatorcontrib>Aurelio Carnero Rosell</creatorcontrib><creatorcontrib>Carretero, Jorge</creatorcontrib><creatorcontrib>Costanzi, Matteo</creatorcontrib><creatorcontrib>da Costa, Luiz</creatorcontrib><creatorcontrib>De Vicente, Juan</creatorcontrib><creatorcontrib>Desai, Shantanu</creatorcontrib><creatorcontrib>Spencer, Everett</creatorcontrib><creatorcontrib>Ferrero, Ismael</creatorcontrib><creatorcontrib>Flaugher, Brenna</creatorcontrib><creatorcontrib>Gerdes, David</creatorcontrib><creatorcontrib>Gschwend, Julia</creatorcontrib><creatorcontrib>Gutierrez, Gaston</creatorcontrib><creatorcontrib>Hollowood, Devon L</creatorcontrib><creatorcontrib>Honscheid, Klaus</creatorcontrib><creatorcontrib>James, David</creatorcontrib><creatorcontrib>Maia, Marcio</creatorcontrib><creatorcontrib>Miquel, Ramon</creatorcontrib><creatorcontrib>Ogando, Ricardo</creatorcontrib><creatorcontrib>Pieres, Adriano</creatorcontrib><creatorcontrib>Rodriguez-Monroy, Martin</creatorcontrib><creatorcontrib>Sanchez, Eusebio</creatorcontrib><creatorcontrib>Scarpine, Vic</creatorcontrib><creatorcontrib>Schubnell, Michael</creatorcontrib><creatorcontrib>Serrano, Santiago</creatorcontrib><creatorcontrib>Sevilla-Noarbe, Ignacio</creatorcontrib><creatorcontrib>Suchyta, Eric</creatorcontrib><creatorcontrib>Tarle, Gregory</creatorcontrib><creatorcontrib>Chun-Hao To</creatorcontrib><creatorcontrib>Zhang, Yuanyuan</creatorcontrib><title>SOAR/Goodman Spectroscopic Assessment of Candidate Counterparts of the LIGO-Virgo Event GW190814</title><title>arXiv.org</title><description>On 2019 August 14 at 21:10:39 UTC, the LIGO/Virgo Collaboration (LVC) detected a possible neutron star-black hole merger (NSBH), the first ever identified. An extensive search for an optical counterpart of this event, designated GW190814, was undertaken using the Dark Energy Camera (DECam) on the 4m Victor M. Blanco Telescope at the Cerro Tololo Inter-American Observatory. Target of Opportunity interrupts were issued on 8 separate nights to observe 11 candidates using the 4.1m Southern Astrophysical Research (SOAR) telescope's Goodman High Throughput Spectrograph in order to assess whether any of these transients was likely to be an optical counterpart of the possible NSBH merger. Here, we describe the process of observing with SOAR, the analysis of our spectra, our spectroscopic typing methodology, and our resultant conclusion that none of the candidates corresponded to the gravitational wave merger event but were all instead other transients. Finally, we describe the lessons learned from this effort. Application of these lessons will be critical for a successful community spectroscopic follow-up program for LVC observing run 4 (O4) and beyond.</description><subject>Black holes</subject><subject>Neutron stars</subject><subject>Neutrons</subject><subject>Optical counterparts (astronomy)</subject><subject>Physics - High Energy Astrophysical 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; Garcia, Alyssa ; Morgan, Robert ; Palmese, Antonella ; Santana-Silva, Luidhy ; Shrivastava, Anushka ; Kilpatrick, Charles ; Sherman, Nora ; Amara, Adam ; Lin, Huan ; Smith, Mathew ; Swann, Elizabeth ; Bachmann, Tristan ; Bechtol, Keith ; Berlfein, Federico ; Briceno, Cesar ; Butler, Bobby ; Cartier, Regis ; Casares, Jorge ; Hsin-Yu, Chen ; Conselice, Christopher ; Cooke, Jeff ; Dage, Kristen ; D'Andrea, Chris ; Davis, Tamara ; de Carvalho, Reinaldo ; Diehl, Tom ; Doctor, Zoheyr ; Drout, Maria ; Farr, Ben ; Foley, Ryan ; Frieman, Josh ; Frohmaier, Christopher ; Gruendl, Robert ; Holz, Daniel ; Kessler, Richard ; Kuropatkin, Nikolay ; Lahav, Ofer ; Lundquist, Michael ; Mann, Andrew ; Marshall, Jennifer ; Martinez-Vazquez, Clara ; McCully, Curtis ; Menanteau, Felipe ; Meza, Nico ; Narayan, Gautham ; Neilsen, Eric ; Nicolaou, Constantina ; Pineda, Jonathan ; Points, Sean ; Quirola-Vasquez, Jonathan ; Rest, Armin ; Rodriguez, Osmar ; Sako, Masao ; Salim, Samir ; Scolnic, Daniel ; Smith, J Allyn ; Sullivan, Mark ; Thomas, Daniel ; Walker, Alistair ; Weller, Jochen ; Wood, Mackenna ; Aguena, Michel ; Andrade-Oliveira, Felipe ; Bertin, Emmanuel ; Brooks, David ; Burke, David ; Aurelio Carnero Rosell ; Carretero, Jorge ; Costanzi, Matteo ; da Costa, Luiz ; De Vicente, Juan ; Desai, Shantanu ; Spencer, Everett ; Ferrero, Ismael ; Flaugher, Brenna ; Gerdes, David ; Gschwend, Julia ; Gutierrez, Gaston ; Hollowood, Devon L ; Honscheid, Klaus ; James, David ; Maia, Marcio ; Miquel, Ramon ; Ogando, Ricardo ; Pieres, Adriano ; Rodriguez-Monroy, Martin ; Sanchez, Eusebio ; Scarpine, Vic ; Schubnell, Michael ; Serrano, Santiago ; Sevilla-Noarbe, Ignacio ; Suchyta, Eric ; Tarle, Gregory ; Chun-Hao To ; Zhang, 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Adam</au><au>Lin, Huan</au><au>Smith, Mathew</au><au>Swann, Elizabeth</au><au>Bachmann, Tristan</au><au>Bechtol, Keith</au><au>Berlfein, Federico</au><au>Briceno, Cesar</au><au>Butler, Bobby</au><au>Cartier, Regis</au><au>Casares, Jorge</au><au>Hsin-Yu, Chen</au><au>Conselice, Christopher</au><au>Cooke, Jeff</au><au>Dage, Kristen</au><au>D'Andrea, Chris</au><au>Davis, Tamara</au><au>de Carvalho, Reinaldo</au><au>Diehl, Tom</au><au>Doctor, Zoheyr</au><au>Drout, Maria</au><au>Farr, Ben</au><au>Foley, Ryan</au><au>Frieman, Josh</au><au>Frohmaier, Christopher</au><au>Gruendl, Robert</au><au>Holz, Daniel</au><au>Kessler, Richard</au><au>Kuropatkin, Nikolay</au><au>Lahav, Ofer</au><au>Lundquist, Michael</au><au>Mann, Andrew</au><au>Marshall, Jennifer</au><au>Martinez-Vazquez, Clara</au><au>McCully, Curtis</au><au>Menanteau, Felipe</au><au>Meza, Nico</au><au>Narayan, Gautham</au><au>Neilsen, Eric</au><au>Nicolaou, Constantina</au><au>Pineda, Jonathan</au><au>Points, Sean</au><au>Quirola-Vasquez, Jonathan</au><au>Rest, Armin</au><au>Rodriguez, Osmar</au><au>Sako, Masao</au><au>Salim, Samir</au><au>Scolnic, Daniel</au><au>Smith, J Allyn</au><au>Sullivan, Mark</au><au>Thomas, Daniel</au><au>Walker, Alistair</au><au>Weller, Jochen</au><au>Wood, Mackenna</au><au>Aguena, Michel</au><au>Andrade-Oliveira, Felipe</au><au>Bertin, Emmanuel</au><au>Brooks, David</au><au>Burke, David</au><au>Aurelio Carnero Rosell</au><au>Carretero, Jorge</au><au>Costanzi, Matteo</au><au>da Costa, Luiz</au><au>De Vicente, Juan</au><au>Desai, Shantanu</au><au>Spencer, Everett</au><au>Ferrero, Ismael</au><au>Flaugher, Brenna</au><au>Gerdes, David</au><au>Gschwend, Julia</au><au>Gutierrez, Gaston</au><au>Hollowood, Devon L</au><au>Honscheid, Klaus</au><au>James, David</au><au>Maia, Marcio</au><au>Miquel, Ramon</au><au>Ogando, Ricardo</au><au>Pieres, Adriano</au><au>Rodriguez-Monroy, Martin</au><au>Sanchez, Eusebio</au><au>Scarpine, Vic</au><au>Schubnell, Michael</au><au>Serrano, Santiago</au><au>Sevilla-Noarbe, Ignacio</au><au>Suchyta, Eric</au><au>Tarle, Gregory</au><au>Chun-Hao To</au><au>Zhang, Yuanyuan</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>SOAR/Goodman Spectroscopic Assessment of Candidate Counterparts of the LIGO-Virgo Event GW190814</atitle><jtitle>arXiv.org</jtitle><date>2022-06-02</date><risdate>2022</risdate><eissn>2331-8422</eissn><abstract>On 2019 August 14 at 21:10:39 UTC, the LIGO/Virgo Collaboration (LVC) detected a possible neutron star-black hole merger (NSBH), the first ever identified. An extensive search for an optical counterpart of this event, designated GW190814, was undertaken using the Dark Energy Camera (DECam) on the 4m Victor M. Blanco Telescope at the Cerro Tololo Inter-American Observatory. Target of Opportunity interrupts were issued on 8 separate nights to observe 11 candidates using the 4.1m Southern Astrophysical Research (SOAR) telescope's Goodman High Throughput Spectrograph in order to assess whether any of these transients was likely to be an optical counterpart of the possible NSBH merger. Here, we describe the process of observing with SOAR, the analysis of our spectra, our spectroscopic typing methodology, and our resultant conclusion that none of the candidates corresponded to the gravitational wave merger event but were all instead other transients. Finally, we describe the lessons learned from this effort. Application of these lessons will be critical for a successful community spectroscopic follow-up program for LVC observing run 4 (O4) and beyond.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.2109.13351</doi><oa>free_for_read</oa></addata></record>
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subjects Black holes
Neutron stars
Neutrons
Optical counterparts (astronomy)
Physics - High Energy Astrophysical Phenomena
title SOAR/Goodman Spectroscopic Assessment of Candidate Counterparts of the LIGO-Virgo Event GW190814
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