Author
Listed:
- David C. Seith
- Siyanbade Adegoke
- Camisha Burchett
- Ryan Kennedy
Abstract
In this letter to the editor, we compare six different event history models to estimate which eligible families participated in a subsidized rental housing program and when . Answering these questions can inform efforts to improve program marketing and outreach, staffing and budgeting, triage, bias identification, as well as benchmarking and evaluation. One of six specifications clearly outperforms the others and understanding how will inform similar research pursuits. Although decision-relevant participation patterns are available in state administrative records, deciphering them is difficult for several well-known reasons. Participants enter and exit the eligible risk pool at different times, for different reasons, and at different rates. To answer our questions of when and whom , we restructure the data from calendar to relative months and then employ event history models designed to accurately estimate a complete hypothetical risk trajectory from observed spells of varying lengths, many of which ended before families took up the rental subsidy, (i.e., censored observation spells). We find that eligible parents most likely to take up the subsidy live in high-rent counties, have relatively strong recent work history, short prior adult lifetime TANF receipt, and medium-size families. Program take-up fell substantially during the COVID-19 pandemic. Contrasting the application of six parallel specifications, we find that a Royston-Parmar proportional hazard model achieves an exceptional balance between the descriptive accuracy of discrete time approaches and the elegance of Cox regression.
Suggested Citation
David C. Seith & Siyanbade Adegoke & Camisha Burchett & Ryan Kennedy, 2025.
"Time to Take a Chance: The Promise of Royston-Parmar Proportional Hazard Models for Understanding Caseload Transitions,"
Evaluation Review, , vol. 49(4), pages 773-796, August.
Handle:
RePEc:sae:evarev:v:49:y:2025:i:4:p:773-796
DOI: 10.1177/0193841X241305869
Download full text from publisher
Corrections
All material on this site has been provided by the respective publishers and authors. You can help correct errors and omissions. When requesting a correction, please mention this item's handle: RePEc:sae:evarev:v:49:y:2025:i:4:p:773-796. See general information about how to correct material in RePEc.
If you have authored this item and are not yet registered with RePEc, we encourage you to do it here. This allows to link your profile to this item. It also allows you to accept potential citations to this item that we are uncertain about.
We have no bibliographic references for this item. You can help adding them by using this form .
If you know of missing items citing this one, you can help us creating those links by adding the relevant references in the same way as above, for each refering item. If you are a registered author of this item, you may also want to check the "citations" tab in your RePEc Author Service profile, as there may be some citations waiting for confirmation.
For technical questions regarding this item, or to correct its authors, title, abstract, bibliographic or download information, contact: SAGE Publications (email available below). General contact details of provider: .
Please note that corrections may take a couple of weeks to filter through
the various RePEc services.