Difference: SSWGProjects (11 vs. 12)

Revision 122022-09-13 - MichaelKelley

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META TOPICPARENT name="SolarSystemWorkingGroup"
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General Projects

NEOZTF

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Projects

 
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Lead: Quanzhi Ye
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Asteroidal phase curves

 
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Abstract: searching for near-Earth objects (NEOs) in all ZTF datasets.
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Derive asteroidal phase curves for a large set of objects, and use the results to interpret the physical properties of the asteroidal population.
 
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NEOZTF Scanning Instructions

Comet Outburst Discovery and Follow-Up

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Team: Zhong-Yi Lin, Wing Ip

Deliverables: Refereed paper

 
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Leads: Mike Kelley, Dennis Bodewits
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Spectroscopic studies of Themis family asteroids with SEDM

 
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Abstract: We examine all ZTF observations of known comets to measure their brightness and morphologies. We are looking for deviations from their baseline activity trends in order to discover outbursts, and identify events for follow-up studies.
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Study reflectance spectra of Themis family asteroids at different orbital phases, to investigate the potential presence of water ice and its variability with heliocentric distance.
 
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We use the ZChecker ( UMD, Caltech) software for outburst discovery (user: ztf, password: enckeekcne).

Active Asteroid Warning System

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Team: Zhong-Yi, Wing Ip, Josiah Purdum
 
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Lead: Quanzhi Ye
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Deliverables: Refereed paper
 
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Abstract: early alert of potential active asteroids.

Super-fast Rotator and rotation period Survey

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Solar system object follow-up and monitoring with Nieves Observatory

 
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Lead: Chan-Kao Chang
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At Soka University of America, in Aliso Viejo CA (near Irvine) we have a robotic/programmable 0.3-meter system which includes a FLI CDK14 telescope and mount, and an FLI Proline CCD camera. We call it the Nieves Observatory at Soka University of America: https://sites.soka.edu/SUO/
 
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Abstract: TBD

Twilight Survey

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We have been monitoring a selection of Near-Earth asteroids and comets, and welcome suggestions for new monitoring campaigns.
 
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Lead: Bryce Bolin
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Team: Bryan Penprase, and students
 
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Abstract: constraining the population of Atira and 'Ayló'chaxnim asteroids with ZTF Twilight observations.
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C/2022 E3 (ZTF)

 
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TNO Survey
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Targeted follow-up spectroscopy and photometry of this potentially bright comet.
 
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Leads: Rich Dekany, Mike Brown
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Team: Dennis Bodewits, Josiah Purdum, Zhong-Yi Lin, Mike Kelley
 
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Abstract: TBD
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Deliverables: Refereed papers
 
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Specific Projects

Synthetic Tracking Experiment

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NEO and small body discoveries with ZTF

 
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Lead: Quanzhi Ye, Chengxing Zhai
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Identify, discovery, and measure astrometry of near-Earth objects, objects interior to Earth/Venus orbit, interstellar objects. Exploit ZTF surveys with ZStreaks, DeepStreaks, ZMODE, and Tails.
 
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Abstract: testing the synthetic tracking technique.

Sparse/Long-term lightcurve fitting

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NEOZTF Scanning Instructions
 
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Lead: Lynne Jones (there is overlap with projects by Rex Chang, and Daniela Huppenkothen is the lead for the Gaussian Processes portion of the project, which includes non-ZTF experiments and data too).
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Team: George Helou, Tom Prince, Kumar Venkataramani, Quanzhi Ye, with contributions from students and follow-up observers
 
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Abstract: We are attempting to understand best methods for fitting rotation curves, and (next-up) phase curves, for known asteroids detected by ZTF. Currently we are using the alert photometry, but hope to extend this to using matchfile photometry. One area of investigation is fitting the rotational light curve with simple two-component Fourier models; another area is fitting lightcurves with Gaussian Processes.
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Deliverables: Astrometry to the Minor Planet Center
 
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Thesis Projects

Rotation period using sparse lightcurve

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NEO co-discovery with Sierra Remote Observatory

 
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PhD student: Ting-Shuo Yeh
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Goal is to execute rapid automated follow-up of fast moving candidate NEO tracklets found in ZTF data with SRO.
 
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Supervisor: Chan-Kao Chang (Rex)
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Team: Tom Prince, George Helou, Kumar Vekataramani, JPL
 
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I have conducted a rotation period survey using CNEOST (China) and KMTNet (Korea) for my master thesis. I would like to continue this work using sparse lightcurve obtained by ZTF. The fitting method includes Fourier series and HG.

Tracklet-less Heliocentric Orbit Recovery (THOR) on ZTF

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Deliverables: Astrometry to the Minor Planet Center
 
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PhD student: Joachim Moeyens
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Prompt cometary outburst discovery and follow-up

 
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Supervisor: Mario Juric
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We examine all ZTF observations of known comets to measure their brightness and morphologies. We are looking for deviations from their baseline activity trends in order to discover outbursts, and identify events for follow-up studies.
 
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We have built a minor planet detection linking algorithm capable of discovering moving objects at high completeness without the need to build or observe tracklets. We have run it on two weeks of ZTF detections (finding 97% of all known moving objects with at least 5 detections) and are now working on running it on all of ZTF's detections.
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We use the ZChecker software to process ZTF data nightly. Online interface at zbrowser2.mkelley.dev, contact Mike Kelley for access.
 
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Rotation period of TNOs using ZTF sparse lightcurves

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Team: Mike Kelley, and any interested follow-up observer
 
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Master student: HanJie Tan
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Deliverables: Public announcements via telegrams
 
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Supervisor: Chan-Kao Chang (Rex)
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Archival cometary outburst search and summary

 
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The rotation periods of TNOs are very limited. We have extracted the light curves of TNOs from ZTF archive PSF source catalogs and are analyzing thier rotation periods and phase curve. We hope to add some reliable rotation periods of TNOs to the current inventory.
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Identify all cometary outbursts in ZTF data. Analyze results as a statistical data set, and investigate individual events on a case-by-case basis.
 
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Postdoc Projects

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Team: Mike Kelley, Quanzhi Ye, Dennis Bodewits
 
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N/A
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Deliverables: Refereed papers
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