monitoring of the tess sectors by the zwicky transient facility · 2019-08-05 · sectors by the...

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Monitoring of the TESS sectors by the Zwicky Transient Facility As a service to the astronomical community, the Zwicky Transient Facility (ZTF) will conduct a nightly public survey of all 13 TESS northern sectors in 2019-2020. ZTF will observe the portions of the TESS sector visible from Palomar each night. Each ZTF pointing will have one exposure each with g and r filters, totaling two images per night. The observations of the first northern sector, Sector 14, have begun on July 18, 2019. Data release: Any optical variability detected by ZTF (‘alerts’) will be published nightly, allowing rapid ground-based follow-up observations by the community. All ZTF-alerts are already crossmatched to external catalogs, including Gaia, Pan-STARRS, 2MASS and others. Lightcurves for all objects will be made available within one month of the end of the TESS observing campaign. Full coverage 1-day cadence g&R colours Limiting mag >20.5 1 arcsec pixels Publicly available Fast data-release TESS 21 arcsec pixels ZTF 1 arcsec pixels Jan van Roestel

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Page 1: Monitoring of the TESS sectors by the Zwicky Transient Facility · 2019-08-05 · sectors by the Zwicky Transient Facility As a service to the astronomical community, the Zwicky Transient

Monitoring of the TESS sectors by the Zwicky

Transient FacilityAs a service to the astronomical community, the Zwicky Transient Facility (ZTF) will conduct a nightly public survey of all 13 TESS northern sectors in 2019-2020. ZTF will observe the portions of the TESS sector visible from Palomar each night. Each ZTF pointing will have one exposure each with g and r filters, totaling two images per night. The observations of the first northern sector, Sector 14, have begun on July 18, 2019.

Data release:Any optical variability detected by ZTF (‘alerts’) will be published nightly, allowing rapid ground-based follow-up observations by the community. All ZTF-alerts are already crossmatched to external catalogs, including Gaia, Pan-STARRS, 2MASS and others. Lightcurves for all objects will be made available within one month of the end of the TESS observing campaign.

✓ Full coverage ✓ 1-day cadence✓ g&R colours✓ Limiting mag >20.5✓ 1 arcsec pixels✓ Publicly available✓ Fast data-release

TESS 21 arcsec pixelsZTF 1 arcsec pixels

Jan van Roestel