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META TOPICPARENT |
name="CosmoTelecons" |
ZTF Ia Phone-con: 2021-Mar-10 |
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1. SNe of the week [Joel J] |
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< < | 2. TARDIS Modelling of early SNIa Spectra [Luke] |
> > | 2. TARDIS Modelling of early SNIa Spectra [Luke H] |
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< < | 3. Measuring the thickness of the ZTF CCD [Philippe] |
> > | 3. Measuring the thickness of the ZTF CCD [Philippe R] |
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< < | 4. Proposal planning [Mat] |
> > | 4. Proposal planning [Mat S] |
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5. AOB / Close |
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< < | Participants ():
- Mickael R, Mat S, Jeremy L, Martin B (Lyon), Joel J, Ariel G, Suhail D, Mattia B, Ana S-C (Stockholm), Jakob N, Valery B, Simeon R (Berlin), Kate M, Jacco T (Trinity), Melissa A, Philippe R (Cleremont), Benjamin R, Bastien C, Julian B (Marseille)
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> > | Participants (20):
- Mickael R, Mat S, Young-Lo K, Martin B (Lyon), Joel J, Ariel G, Suhail D, Mattia B, Ana S-C(Stockholm), Kate M, Jacco T, Luke H, Maxime D, Mark M (Trinity), Melissa A, Philippe R, Manu G (Cleremont), Bastien C, Benjamin R(Marseille), Nicolas R (Paris)
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| Notes:
Transients of the Week: |
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- ZTF21aaomuka: young and discovered by POISE (CSP group) @ z=0.07.
- ZTF21aamnngb: strong early time Calcium. Going in to the LT queue. z=0.016.
- RCF are going to automate classifications to TNS. Using SNIa score: aka Ia/non-Ia.
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| Luke on early time spectral modelling: |
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- Using the 2018 cosmology sample: objects with early and peak spectra: 50. 8 objects after S/N and coverage cuts cuts.
- TARDIS is a 1D spectral synthesis code.
- ZTF18abfhryc is the current focus: have fits to both spectra, and is trying to reconcile the two profiles.
- Velocity profile moves from 30,000 km/s at early times to 20,000 km/s around peak.
- Lots to come from this project!
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| Philippe on CCD thickness: |
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- Trying to predict the sensor contribution to the PSF.
- Using the methodology of Medford, Goldstein, Nugent+ used to deduce fringing.
- Tried to use the fringe pattern to estimate thickness profile: failed!
- New idea: silicon absorption varies as a function of wavelength => use flat fields to estimate thickness.
- The ratio of two flat fields (at different wavelengths) should match the thickness profile.
- Implemented a forward modelling approach with physics! Test against fringe maps.
- Have to think about higher order issues: reflection within the camera. Use filterless flat field.
- Use sky spectrum (over assuming a flat spectrum). This is old and needs to be improved.
- Overall the fit is good, but there are issues: it's not great on small scales.
- It works!
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| Mat on Proposals: |
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- Two upcoming deadlines:
- ESO (1st Oct - 31st March): deadline is 25th March
- Gemini (1st Aug - 31st Jan): deadline is 31st March
- Plans within the group:
- Lensing: MUSE+HAWKI (as currently; lead by Ariel); INT (to weed out contaminents; Suhail)
- Early-time: X-SHOOTER (2-3 triggers; lead by Mattia B)
- Gemini LLP (all transient classes, but esp. long lived events; lead by Adam M)
- Local: HST (2-3 events to get TRGB of ZTF; Proof of Concept; organised by Suhail)
- Hosts: MUSE (neary events ~10; pulled together by Mat).
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| Closing Remarks: |