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META TOPICPARENT |
name="CosmoTelecons" |
ZTF Ia Phone-con: 2021-May-05
Meeting Agenda:
1. SNe of the week [Joel J]
2. How are we going to measure photometry [Mickael R]
3. AOB / Close
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Participants (14):
- Mat, Estelle, Jakob, Joel, Joel, Martin, Maxime C, Maxime D, Mattia, Melissa, Mickael, Suhail, Philippe, Valery, Young-Lo
Notes:
Transients of the Week:
- Table sorting is still slow
- ZTF21aarguvb: pre-detection bump? Not real.
- ZTF21aaxwytv: pre-detection excess? AGN?
- ZTF21aaxwytv: early, fast rising.
- ZTF21aaxwnlr: early; redenned.
- ZTF21aavsbkt: in interacting galaxy.
- ZTF21aaxuywf: pretty :). Could do with another spectrum. Not a convincing SNIFS classification.
- Maxime: getting maximum light spectra of all Ia's within 100Mpc.
Measuring Photometry:
- What are we going to use for photometry for our next data release?
- The current pipeline (Suhail) uses ZUDS.
- This makes individual references (swarp) and then HOTPANTS for subtraction.
- We want to update parts of this:
- HOTPANTS -> ZOGY as this is used in LSST.
- There are examples for Meerlicht
- + interface PSF pipeline with it: ZIFF
- There is now a working version of this.
- Critical as this isn't corrected now.
- But we probably keep ZUDS for making references.
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- So we need to incorporate ZUDS references with ZOGY and then combine ZOGY with ZIFF.
- (Scene-modelling is a longer term problem. End of this year probably).
- Questions:
- Suhail: should we go to HOTPANTS? DES + PS1 use this.
- Consensus: no: the overall normalisation will fall out.
- How are we going to keep track of everything?
- Answer: a database. postgres probably. This is a 2nd order problem
- Should we use the IPAC sandbox:
- This is great, but isn't going to allow us to run everything, so no ;).
- Miscellaneous:
- There might be a student in Stockholm (Hiranya's) who can help in ZOGY+ZIFF
- The Plan:
- The key is to extract the source code for making references from ZUDS (basically swarp) and format it for ZOGY.
- Mickael + Suhail to get together next week for this step
- After that, we'll see. Small steps easily go to big steps. Volunteers welcome.
Closing Remarks: |