CaltechAUTHORS
  A Caltech Library Service

A Systematic Search for Outbursting AM CVn Systems with the Zwicky Transient Facility

van Roestel, Jan and Creter, Leah and Kupfer, Thomas and Szkody, Paula and Fuller, Jim and Green, Matthew J. and Rich, R. Michael and Sepikas, John and Burdge, Kevin and Caiazzo, Ilaria and Mróz, Przemek and Prince, Thomas A. and Duev, Dmitry A. and Graham, Matthew J. and Shupe, David L. and Laher, Russ R. and Mahabal, Ashish A. and Masci, Frank J. (2021) A Systematic Search for Outbursting AM CVn Systems with the Zwicky Transient Facility. Astronomical Journal, 162 (3). Art. No. 113. ISSN 0004-6256. doi:10.3847/1538-3881/ac0622. https://resolver.caltech.edu/CaltechAUTHORS:20210526-152342697

[img] PDF - Published Version
See Usage Policy.

4MB
[img] PDF - Submitted Version
Creative Commons Attribution.

3MB

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20210526-152342697

Abstract

AM CVn systems are a rare type of accreting binary that consists of a white dwarf and a helium-rich, degenerate donor star. Using the Zwicky Transient Facility (ZTF), we searched for new AM CVn systems by focusing on blue, outbursting stars. We first selected outbursting stars using the ZTF alerts. We cross matched the candidates with Gaia and Pan-STARRS catalogs. The initial selection of candidates based on the Gaia BP-RP contains 1751 unknown objects. We used the Pan-STARRS g-r and r-i color in combination with the Gaia color to identify 59 strong AM CVn candidates. We obtained identification spectra of 35 sources, of which 18 are high-priority candidates, and discovered nine new AM CVn systems and one magnetic CV that shows only He-ii lines. Using the outburst recurrence time, we estimate the orbital periods of the nine new AM CVn systems that are in the range of 29–50 minutes. We conclude that targeted follow up of blue, outbursting sources is an efficient method to find new AM CVn systems and we plan to follow up all candidates we identified to systematically study the population of outbursting AM CVn systems.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.3847/1538-3881/ac0622DOIArticle
https://arxiv.org/abs/2105.02261arXivDiscussion Paper
ORCID:
AuthorORCID
van Roestel, Jan0000-0002-2626-2872
Kupfer, Thomas0000-0002-6540-1484
Szkody, Paula0000-0003-4373-7777
Fuller, Jim0000-0002-4544-0750
Green, Matthew J.0000-0002-0948-4801
Rich, R. Michael0000-0003-0427-8387
Burdge, Kevin0000-0002-7226-836X
Caiazzo, Ilaria0000-0002-4770-5388
Mróz, Przemek0000-0001-7016-1692
Prince, Thomas A.0000-0002-8850-3627
Duev, Dmitry A.0000-0001-5060-8733
Graham, Matthew J.0000-0002-3168-0139
Shupe, David L.0000-0003-4401-0430
Laher, Russ R.0000-0003-2451-5482
Mahabal, Ashish A.0000-0003-2242-0244
Masci, Frank J.0000-0002-8532-9395
Additional Information:© 2021. The American Astronomical Society. Received 2021 May 8; revised 2021 May 24; accepted 2021 May 26; published 2021 August 19. This paper is dedicated in part to the memory of Dr. Bill Whitney who was above all a great teacher and educator. For over 68 yr from Caltech to MIT to JPL and back to Caltech, Bill has guided and nurtured both students and faculty from across the country and world, with a love of physics, science, and education. Bill was one of the founders of the Caltech Summer Undergraduate Research Fellowship (SURF) in 1979 under the principle that undergraduates can productively contribute to research, which was considered very novel at the time. Since then, the SURF undergraduate model has been replicated by many leading universities benefiting many thousands of students and faculty alike. Bill's deep recognition for the efficacy of multigenerational science education is reflected in this paper as contributing author and SURF student Leah Creter is the student of also contributing author Dr. John Sepikas who in turn was the student of Dr. Bill Whitney. Nothing would have made Dr. Whitney more proud. J.v.R. is partially supported by NASA-LISA grant 80NSSC19K0325. Based on observations obtained with the Samuel Oschin Telescope 48 inch at the Palomar Observatory as part of the Zwicky Transient Facility project. Z.T.F. is supported by the National Science Foundation under grant No. AST-1440341 and a collaboration including Caltech, IPAC, the Weizmann Institute for Science, the Oskar Klein Center at Stockholm University, the University of Maryland, the University of Washington, Deutsches Elektronen-Synchrotron and Humboldt University, Los Alamos National Laboratories, the TANGO Consortium of Taiwan, the University of Wisconsin at Milwaukee, and Lawrence Berkeley National Laboratories. Operations are conducted by COO, IPAC, and UW. This research has made use of the SIMBAD database, operated at CDS, Strasbourg, France; Astroquery (Ginsburg et al. 2019); and Astropy, a community-developed core Python package for Astronomy (Astropy Collaboration et al. 2013, 2018). Some of the data presented herein were obtained at the W.M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California, and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W.M. Keck Foundation. Based on observations made with the William Herchel Telescope (WHT) operated on the island of La Palma by the Isaac Newton Group in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofsica de Canarias. This work has made use of data from the European Space Agency (ESA) mission Gaia (https://www.cosmos.esa.int/gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC, https://www.cosmos.esa.int/web/gaia/dpac/consortium). Funding for the DPAC has been provided by national institutions, in particular, the institutions participating in the Gaia Multilateral Agreement. The Pan-STARRS1 Surveys (PS1) have been made possible through contributions of the Institute for Astronomy, the University of Hawaii, the Pan-STARRS Project Office, the Max-Planck Society and its participating institutes, the Max Planck Institute for Astronomy, Heidelberg, and the Max Planck Institute for Extraterrestrial Physics, Garching, The Johns Hopkins University, Durham University, the University of Edinburgh, Queen's University Belfast, the Harvard-Smithsonian Center for Astrophysics, the Las Cumbres Observatory Global Telescope Network Incorporated, the National Central University of Taiwan, the Space Telescope Science Institute, the National Aeronautics and Space Administration under Grant No. NNX08AR22G issued through the Planetary Science Division of the NASA Science Mission Directorate, the National Science Foundation under grant No. AST-1238877, the University of Maryland, and Eotvos Lorand University (ELTE). Facilities: P48(ZTF) - , WHT:4.2 m (ACAM) - , Keck II:10 m (LRIS&DEIMOS) - , P200:5.0 m (CHIMERA) - , Shane:3.0 m (Kast) - . Software: penquins, astropy & astroquery (Astropy Collaboration et al. 2013, 2018), Lpipe (Perley 2019), PypeIt (Prochaska et al. 2020).
Group:Astronomy Department, Infrared Processing and Analysis Center (IPAC), Zwicky Transient Facility
Funders:
Funding AgencyGrant Number
Caltech Summer Undergraduate Research Fellowship (SURF)UNSPECIFIED
NASA80NSSC19K0325
NSFAST-1440341
ZTF partner institutionsUNSPECIFIED
W. M. Keck FoundationUNSPECIFIED
Gaia Multilateral AgreementUNSPECIFIED
NASANNX08AR22G
NSFAST-1238877
Subject Keywords:AM Canum Venaticorum stars; Cataclysmic variable stars; Sky surveys
Issue or Number:3
Classification Code:Unified Astronomy Thesaurus concepts: AM Canum Venaticorum stars (31); Cataclysmic variable stars (203); Sky surveys (1464)
DOI:10.3847/1538-3881/ac0622
Record Number:CaltechAUTHORS:20210526-152342697
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20210526-152342697
Official Citation:Jan van Roestel et al 2021 AJ 162 113
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:109259
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:26 May 2021 23:03
Last Modified:20 Aug 2021 18:44

Repository Staff Only: item control page