Difference: CosmoTelecon2021mar03 (1 vs. 2)

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META TOPICPARENT name="CosmoTelecons"

ZTF Ia Phone-con: 2021-Mar-03

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  5. AOB / Close
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Participants ():
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Participants (19):
  • 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)
 

Notes:

Transients of the Week:
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  • ZTF21aambvzd: highly redenned nearby Ia.
  • ZTF21aamsiqk: Ia, caught early. Close to galactic plane (Ag=3). Ideal to test galactic extinction maps + R_V along this line-of-sight.
    • This is at max: target this for NIR follow-up.
  • + a couple of other ambiguous classifications caused by the moon. Someone needs to look at this.
 
Jeremy on SEDm spectral modelling:
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  • Hyperspectral modelling in SEDm.
  • Using photometric measurements from PS1 to infer a spectral host model. By convolving this with the SEDm resolution (and correcting for ADR effects), he can find the underlying host contamination in an SEDm spectrum.
    • Working at the pixel level for PS1. Resampling the images to SEDm spaxels. SED fitting (LePhare) to get a virtual IFU for every pixel with S/N>4 (otherwise there's nothing to fit ;)).
    • Precise astrometry in SEDm is an issue.
  • It works! It could be better, but the SN is clearly visible when before it wasn't ;). It takes about 15 mins per object.
  • Not so great for objects in the core of hosts: the SED model is important.
  • Improvements to be made in the fitting assumptions, photometric catalogue, PSF modelling and time taken.
    • Could use existing spectra (SDSS) of the host to constrain the model.
  • Can be used as a model for the host of the SNe: it's basically an IFU of the field.
  • Code is available on GitHub.
  • Help for implementing extensions would be appreciated smile
 
Mat on DEBASS:
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Joel on SNeIa in the NIR:
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  • This is a survey with DECAM to get griz measurements of low redshift SN.
    • The aim is to anchor the Hubble diagram with the same filter set as at high-z.
  • Primary target feeder is likely to be ZTF/SEDm with probably ATLAS on the side.
  • What shall we do about this? This is a bigger scale question than can be summed up in some notes.
 
Closing Remarks:
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  • Sign up for a talk!
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Revision 12021-03-03 - MathewSmith

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META TOPICPARENT name="CosmoTelecons"

ZTF Ia Phone-con: 2021-Mar-03

Meeting Agenda:

1. SNe of the week [Joel J]

2. SEDm host modelling [Jeremy L]

3. The DEBASS survey [Mat S]

4. SNe in the NIR [Joel J]

5. AOB / Close

Participants ():

Notes:

Transients of the Week:
Jeremy on SEDm spectral modelling:
Mat on DEBASS:
Joel on SNeIa in the NIR:
Closing Remarks:
*
 
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