The JCMT Transient Survey: Single-epoch Transients and Variability of Faint Sources

• Published in: The Astrophysical journal Vol. 937; no. 1; pp. 6 - 17
• Main Authors: Johnstone, Doug, Lalchand, Bhavana, Mairs, Steve, Shang, Hsien, Chen, Wen Ping, Bower, Geoffrey C., Herczeg, Gregory J., Lee, Jeong-Eun, Forbrich, Jan, Chen, Bo-Yan, Contreras Peña, Carlos, Lee, Yong-Hee, Park, Wooseok, Broughton, Colton, Plovie, Spencer
• Format: Journal Article
• Language: English
• Published: Philadelphia The American Astronomical Society 01.09.2022; IOP Publishing
• Subjects: Astrophysics; Binary stars; Complications; Cosmology; Flares; Magnetic reconnection; Star formation; Stellar flares; Submillimeter astronomy; Surveys; Variability; Variable stars; Wavelengths; Young stellar objects
• ISSN: 0004-637X; 1538-4357
• DOI: 10.3847/1538-4357/ac8a48

Abstract Short-duration flares at millimeter wavelengths provide unique insights into the strongest magnetic reconnection events in stellar coronae and combine with longer-term variability to introduce complications to next-generation cosmology surveys. We analyze 5.5 yr of JCMT Transient Survey 850 μ m submillimeter monitoring observations toward eight Gould Belt star-forming regions to search for evidence of transient events or long-duration variability from faint sources. The eight regions (30′ diameter fields), including ∼1200 infrared-selected YSOs, have been observed on average 47 times with integrations of approximately half an hour, or one day total, spread over 5.5 yr. Within this large data set, only two robust faint source detections are recovered: JW 566 in OMC 2/3 and MGM12 2864 in NGC 2023. JW 566, a Class II T Tauri binary system previously identified as an extraordinary submillimeter flare, remains unique, the only clear single-epoch transient detection in this sample with a flare eight times bright than our ∼4.5 σ detection threshold of 55 mJy beam −1 . The lack of additional recovered flares intermediate between JW 566 and our detection limit is puzzling if smaller events are more common than larger events. In contrast, the other submillimeter variable identified in our analysis, Source 2864, is highly variable on all observed timescales. Although Source 2864 is occasionally classified as a YSO, the source is most likely a blazar. The degree of variability across the electromagnetic spectrum may be used to aid source classification.