Difference: CosmologyWorkingGroup (1 vs. 31)

Revision 312023-12-20 - MickaelRigault

Line: 1 to 1
 
META TOPICPARENT name="ScienceWorkingGroups"

ZTF Cosmology with SNIa, gravitational lensing and SNIa physics Working Group

Line: 17 to 17
  Phone-cons: Wednesdays @ 16:00 CET (15:00 UK/Ireland)

Ongoing papers

Changed:
<
<

data : https://github.com/ZwickyTransientFacility/ztfcosmoidr (need access)

Tools to play with the data: https://github.com/MickaelRigault/ztfidr

>
>

data : https://github.com/ZwickyTransientFacility/ztfcosmoidr (need access)

ZTF Cosmo DR2 paper authorlist

Tools to play with the data: https://github.com/MickaelRigault/ztfidr

 
  • Data release “<dec 2020)”:

    • General overview | Rigault et al.

    • W-letter (based on volume limited) | Smith et al.

Revision 302022-05-18 - MickaelRigault

Line: 1 to 1
 
META TOPICPARENT name="ScienceWorkingGroups"

ZTF Cosmology with SNIa, gravitational lensing and SNIa physics Working Group

Line: 15 to 15
  Slack: ztfia.slack.com [contact Mickael to get an invitation]
Changed:
<
<
Phone-cons: https://stockholmuniversity.zoom.us/j/69477874064 Wednesdays @ 15:00 CET (14:00 UK/Ireland)
>
>
Phone-cons: Wednesdays @ 16:00 CET (15:00 UK/Ireland)
 

Ongoing papers

data : https://github.com/ZwickyTransientFacility/ztfcosmoidr (need access)

Tools to play with the data: https://github.com/MickaelRigault/ztfidr

  • Data release “<dec 2020)”:

Revision 292022-05-18 - KateMaguire2

Line: 1 to 1
 
META TOPICPARENT name="ScienceWorkingGroups"

ZTF Cosmology with SNIa, gravitational lensing and SNIa physics Working Group

Line: 91 to 91
 
  • Georgios Dimitriadis
  • Luke Harvey
  • Kate Maguire
Deleted:
<
<
  • Mark Magee
 
  • Jacco Terwel
Added:
>
>
  • Umut Burgaz
 
IN2P3 (Clermont)
  • Melissa Amenouche
  • Manu Gangler
Line: 119 to 119
 
  • Uli Feindt (Stockholm)
  • Laura Hangard (Stockholm)
  • Seméli Papadogiannakis (Stockholm)
Added:
>
>
  • Mark Magee (Dublin)
 

Ongoing Projects:

(really needs updating)

Revision 282022-05-18 - MickaelRigault

Line: 1 to 1
 
META TOPICPARENT name="ScienceWorkingGroups"

ZTF Cosmology with SNIa, gravitational lensing and SNIa physics Working Group

Line: 7 to 7
 Lots of mostly-outdated material may be found on the previous CosmoSNIa (2018-2020), or SNeIa (2016-2018) page.

Contact information:

Changed:
<
<
Coordinators: Mickael Rigault (Lyon; Coordinator); Joel Johannson (Stockholm; co-lead); Mat Smith (Lyon; co-lead)
>
>
Coordinators: Mickael Rigault (Lyon; Coordinator); Joel Johannson (Stockholm; co-lead); Mat Smith (Lyon; co-lead),
Georgios Dimitriadis (Dublin ; co-lead)
  thanks to Suhail Dhawan, OKC, Jakob Nordin, HU for their previous leadership.
Line: 16 to 16
 Slack: ztfia.slack.com [contact Mickael to get an invitation]

Phone-cons: https://stockholmuniversity.zoom.us/j/69477874064 Wednesdays @ 15:00 CET (14:00 UK/Ireland)

Changed:
<
<

Minutes:

>
>

Ongoing papers

data : https://github.com/ZwickyTransientFacility/ztfcosmoidr (need access)

Tools to play with the data: https://github.com/MickaelRigault/ztfidr

  • Data release “<dec 2020)”:

    • General overview | Rigault et al.

    • W-letter (based on volume limited) | Smith et al.

  • Calibration (general supervision, Regnault)

    • Ubercal | Racine et al.

    • Flats | Rosnet et al.

    • SMP | Lacroix et al.

  • Volume Limited (has distances, z<0.055)

    • BS20+J21 claim seen by ZTF | Smith et al.

    • Photo SN X Photo host correlations | Ginolin, Smith et al.

  • SNe Ia in Clusters | Ruppin, Rigault et al.

  • SNe Ia Diversities (What are Jacco’s and Luke’s paper for DR2 ?)

    • Subtyping and rates | Dimitriadis et al.

    • Super Chandra | ???

    • Ia-CSM

    • Iax

    • minimal metallicity SNe Ia (non crazy hostless) | Umut et al.

    • Host-less for crazy Dark Matter | Goobar et al.

  • Early and Late LC residual studies | Miller (?) t al.

  • Spectral properties | Johansson et al.

  • Siblings | (Joel+Suhail et al.)

  • Reddening | c>0.3 (Stockholm et al)

  • Strong lensing search (more than DR2) | Sagués-Carracedo et al.

  • Sample Simulation | Amenouche et al.

  • Fs8 and co estimations

    • TensorFlow (fvflow)| Robert et al.

    • Likelihood & impact of bias | Carreres et al.

    • Generalized Cosmography | Dhawan et al.

  • Second bump “ i band”:

    • Helps standardisation - subtypes | Sommer et al.

    • For the progenitor physics | Deckers et al.

  • Phototyping (stating for DR3, Alice and Mat)




Minutes:

  Telecon minutes can be found here.

Science Projects:

Line: 32 to 67
 
    • Obtain ZTF data from Growth / Fritz marshall and SEDm
  • A quick start guide to ZTF photometry pipelines: here. (borrowed from Kate)

Members:

Changed:
<
<
OKC (Stockholm)
>
>
OKC (Stockholm)
 
  • Rahul Biswas
  • Mattia Bulla
  • Ana Sagués Carracedo
  • Suhail Dhawan (recently moved to Cambridge, UK)
  • Ariel Goobar
  • Joel Johansson
Changed:
<
<
HU/DESY (Berlin)
>
>
HU/DESY (Berlin)
 
  • Valéry Brinnel
  • Jakob Nordin
  • Simeon Reusch
  • Nicolas Miranda
Changed:
<
<
IN2P3 (Lyon)
>
>
IN2P3 (Lyon)
 
  • Yannick Copin
  • Young-Lo Kim (recently moved to Lancaster, UK)
  • Jeremy Lezey
  • Mickael Rigault
  • Estelle Robert
  • Mathew Smith
Changed:
<
<
Trinity (Dublin)
>
>
Trinity (Dublin)
 
  • Maxime Deckers
  • Georgios Dimitriadis
  • Luke Harvey
  • Kate Maguire
  • Mark Magee
  • Jacco Terwel
Changed:
<
<
IN2P3 (Clermont)
>
>
IN2P3 (Clermont)
 
  • Melissa Amenouche
  • Manu Gangler
  • Philippe Rosnet
Changed:
<
<
IN2P3 (Marseille)
>
>
IN2P3 (Marseille)
 
  • Julian Bautista
  • Bastien Carreres
  • Fabrice Feinstein
  • Dominique Fouchez
  • Benjamin Racine
Changed:
<
<
IN2P3 (Paris)
>
>
IN2P3 (Paris)
 
  • Nicolas Regault
Changed:
<
<
Northwestern
>
>
Northwestern
 
  • Adam Miller
Changed:
<
<
Caltech (California)
>
>
Caltech (California)
 
  • Abigail Poli
Changed:
<
<
Past Members:
>
>
Past Members:
 
  • Martin Briday (IN2P3: Lyon)
  • Danny Goldstein (Berkeley)

Revision 272021-10-29 - MathewSmith

Line: 1 to 1
 
META TOPICPARENT name="ScienceWorkingGroups"

ZTF Cosmology with SNIa, gravitational lensing and SNIa physics Working Group

Line: 25 to 25
 

Useful Links:

Changed:
<
<
>
>
 
Line: 35 to 36
 
  • Rahul Biswas
  • Mattia Bulla
  • Ana Sagués Carracedo
Changed:
<
<
  • Suhail Dhawan
>
>
  • Suhail Dhawan (recently moved to Cambridge, UK)
 
  • Ariel Goobar
  • Joel Johansson
HU/DESY (Berlin)
Line: 44 to 45
 
  • Simeon Reusch
  • Nicolas Miranda
IN2P3 (Lyon)
Deleted:
<
<
  • Martin Briday
 
  • Yannick Copin
Changed:
<
<
  • Young-Lo Kim
>
>
  • Young-Lo Kim (recently moved to Lancaster, UK)
 
  • Jeremy Lezey
  • Mickael Rigault
Added:
>
>
  • Estelle Robert
 
  • Mathew Smith
Trinity (Dublin)
  • Maxime Deckers
Added:
>
>
  • Georgios Dimitriadis
 
  • Luke Harvey
  • Kate Maguire
  • Mark Magee
Line: 68 to 70
 
  • Benjamin Racine
IN2P3 (Paris)
  • Nicolas Regault
Added:
>
>
Northwestern
  • Adam Miller
 
Caltech (California)
  • Abigail Poli
Past Members:
Added:
>
>
  • Martin Briday (IN2P3: Lyon)
 
  • Danny Goldstein (Berkeley)
  • Peter Nugent (Berkeley: come back Peter!)
  • Matteo Giomi (Berlin)

Revision 262021-03-17 - MathewSmith

Line: 1 to 1
 
META TOPICPARENT name="ScienceWorkingGroups"

ZTF Cosmology with SNIa, gravitational lensing and SNIa physics Working Group

Line: 42 to 42
 
  • Valéry Brinnel
  • Jakob Nordin
  • Simeon Reusch
Added:
>
>
  • Nicolas Miranda
 
IN2P3 (Lyon)
  • Martin Briday
  • Yannick Copin
Line: 53 to 54
 
  • Maxime Deckers
  • Luke Harvey
  • Kate Maguire
Added:
>
>
  • Mark Magee
 
  • Jacco Terwel
IN2P3 (Clermont)
  • Melissa Amenouche

Revision 252021-03-17 - MathewSmith

Line: 1 to 1
 
META TOPICPARENT name="ScienceWorkingGroups"

ZTF Cosmology with SNIa, gravitational lensing and SNIa physics Working Group

Line: 51 to 51
 
  • Mathew Smith
Trinity (Dublin)
  • Maxime Deckers
Added:
>
>
  • Luke Harvey
 
  • Kate Maguire
  • Jacco Terwel
IN2P3 (Clermont)

Revision 242021-02-24 - MathewSmith

Line: 1 to 1
 
META TOPICPARENT name="ScienceWorkingGroups"

ZTF Cosmology with SNIa, gravitational lensing and SNIa physics Working Group

Line: 50 to 50
 
  • Mickael Rigault
  • Mathew Smith
Trinity (Dublin)
Added:
>
>
  • Maxime Deckers
 
  • Kate Maguire
  • Jacco Terwel
IN2P3 (Clermont)

Revision 232021-02-11 - MathewSmith

Line: 1 to 1
 
META TOPICPARENT name="ScienceWorkingGroups"

ZTF Cosmology with SNIa, gravitational lensing and SNIa physics Working Group

Line: 34 to 34
 
OKC (Stockholm)
  • Rahul Biswas
  • Mattia Bulla
Added:
>
>
  • Ana Sagués Carracedo
 
  • Suhail Dhawan
  • Ariel Goobar
  • Joel Johansson
Line: 42 to 43
 
  • Jakob Nordin
  • Simeon Reusch
IN2P3 (Lyon)
Changed:
<
<
  • Mickael Rigault
  • Mathew Smith
  • Young-Lo Kim
>
>
  • Martin Briday
 
  • Yannick Copin
Added:
>
>
  • Young-Lo Kim
 
  • Jeremy Lezey
Changed:
<
<
  • Martin Briday
>
>
  • Mickael Rigault
  • Mathew Smith
 
Trinity (Dublin)
  • Kate Maguire
Changed:
<
<
    • and team...
>
>
  • Jacco Terwel
 
IN2P3 (Clermont)
Deleted:
<
<
  • Philippe Rosnet
 
  • Melissa Amenouche
Added:
>
>
  • Manu Gangler
  • Philippe Rosnet
 
IN2P3 (Marseille)
Deleted:
<
<
  • Benjamin Racine
 
  • Julian Bautista
Deleted:
<
<
  • Fabrice Feinstein
 
  • Bastien Carreres
Added:
>
>
  • Fabrice Feinstein
  • Dominique Fouchez
  • Benjamin Racine
 
IN2P3 (Paris)
  • Nicolas Regault
Caltech (California)

Revision 222021-02-04 - MathewSmith

Line: 1 to 1
 
META TOPICPARENT name="ScienceWorkingGroups"

ZTF Cosmology with SNIa, gravitational lensing and SNIa physics Working Group

Line: 29 to 29
 
Changed:
<
<
  • A quick start guide to ZTF photometry pipelines: here. (borrowed from Kate)
>
>
  • A quick start guide to ZTF photometry pipelines: here. (borrowed from Kate)
 

Members:

OKC (Stockholm)
  • Rahul Biswas
Line: 40 to 40
 
HU/DESY (Berlin)
  • Valéry Brinnel
  • Jakob Nordin
Added:
>
>
  • Simeon Reusch
 
IN2P3 (Lyon)
  • Mickael Rigault
  • Mathew Smith

Revision 212021-02-04 - MathewSmith

Line: 1 to 1
 
META TOPICPARENT name="ScienceWorkingGroups"

ZTF Cosmology with SNIa, gravitational lensing and SNIa physics Working Group

Line: 29 to 29
 
Added:
>
>
  • A quick start guide to ZTF photometry pipelines: here. (borrowed from Kate)
 

Members:

OKC (Stockholm)
  • Rahul Biswas
Line: 48 to 49
 
  • Martin Briday
Trinity (Dublin)
  • Kate Maguire
Changed:
<
<
  • ...
IN2P3 (Claremont)
>
>
    • and team...
IN2P3 (Clermont)
 
  • Philippe Rosnet
  • Melissa Amenouche
IN2P3 (Marseille)
Line: 59 to 60
 
  • Bastien Carreres
IN2P3 (Paris)
  • Nicolas Regault
Changed:
<
<
Caltech
>
>
Caltech (California)
 
  • Abigail Poli
Past Members:
  • Danny Goldstein (Berkeley)
Line: 71 to 72
 
  • Seméli Papadogiannakis (Stockholm)

Ongoing Projects:

Changed:
<
<
(needs updating)
>
>
(really needs updating)
 

Revision 202021-02-03 - MathewSmith

Line: 1 to 1
 
META TOPICPARENT name="ScienceWorkingGroups"
Changed:
<
<

ZTF Cosmology with SNe and gravitational lensing Working Group

>
>

ZTF Cosmology with SNIa, gravitational lensing and SNIa physics Working Group

  This is the Wiki page for the ZTF Working Group on cosmology with SNe and gravitational lensing.
Changed:
<
<
Some material may be found on the previous SNeIa page.
>
>
Lots of mostly-outdated material may be found on the previous CosmoSNIa (2018-2020), or SNeIa (2016-2018) page.

Contact information:

 
Changed:
<
<

Contact information:

>
>
Coordinators: Mickael Rigault (Lyon; Coordinator); Joel Johannson (Stockholm; co-lead); Mat Smith (Lyon; co-lead)
 
Changed:
<
<
coordinators: Suhail Dhawan, OKC (Coordinator), Jakob Nordin, HU (Deputy Coordinator)
>
>
thanks to Suhail Dhawan, OKC, Jakob Nordin, HU for their previous leadership.
 
Changed:
<
<
mailing list: ztfia@lists.astro.caltech.edu sign up here
>
>
Mailing list: ztfia@lists.astro.caltech.edu sign up here
 
Changed:
<
<
slack organization: ztfia.slack.com [contact Uli to get an invitation]
>
>
Slack: ztfia.slack.com [contact Mickael to get an invitation]
 
Changed:
<
<
meeting time: Alternating between Wednesdays 14:00 CET and Wednesdays 17:00 CET

Minutes:

>
>
Phone-cons: https://stockholmuniversity.zoom.us/j/69477874064 Wednesdays @ 15:00 CET (14:00 UK/Ireland)

Minutes:

  Telecon minutes can be found here.
Added:
>
>

Science Projects:

 
Changed:
<
<

October 2018 spectroscopic campaign:

This will run for approximately 20 days with the combined goals of investigating how deep an effective ZTF SNIa search can go and what spectroscopic resources this would require/warrant.

Cosmology tasklist Summer 2018

The ZTF camera is great. The raw calibration is better than expected. SEDM works. We find roughly the right order of transients. ZTF could really do ground-breaking cosmology.

But, this requires 2000 (4000+) spectroscopically confirmed and calibrated SNe Ia. Need to get the program running and convince the collaboratoin that its cool. No excuses.

  • Draft outline group for ZTF cosmology project. Ariel, Mickael, Jakob, Uli, Peter, …
  • Show observed rate agrees with simulations. Uli
  • Isolate subset of SNe with minimal/flat host contribution. Script to download PS photometry at coordinate, fit the background with some metric (plane?) and record outcome. Combined with visual confirmation? Ariel
  • Isolate subset of SNe with spectroscopic host redshifts. To what extend can we trust marshal notes? Probably at least want to complement with something slightly more complex. Match with SDSS and NED, calculate confusion metric. CLU matches probably only available throuch Caltech. OKC – Lauras code?
  • Maintain our list of typed SNe Ia, routines for classification (SNID) and subclassification. Are there cases that are ambigous? Semeli/Uli writeup of current.
  • Fit floating SNIa lightcurves to everything in AMPEL - did we miss anything looking like a Ia? JN
  • Trigger instructions for LCO. They have a nice visual tool, but we probably need a script to gather the necessary information. Done frequently by the SN group so they might already have this.
  • TNS submission manual. For single entries there is a convenient web form, Christoffer also has a python script. Probably need to gather some information like what candidates do we want to / should we submit and eg what acknowledgments are used.
  • Figure out how to use the SNCOSMO data (include other templates?, peak fit?, floating offset? upper limits?). I am sure there are cases where the fit is not representative, typically when post-peak data is missing. Mickael
  • AGN rejection in AMPEL. Core distance, catalog matching and variability. Previous variability rejection in AMPEL. Through 30day history and/or PTF. Peter, Nadia, Matteo
  • Maintain updated hubble diagram with diagnostics. Blinding!?! Flag SNe with offset. Ampel
  • SNIFS trigger script: For a given SN, incorporate finding chart into the SNIFS observing database. Mickael.
  • SNIFS training and shifting. We should be ~8 shifters to make this a trivial task (~ a few hoursslac each month) Uli, Mickael, Daniel, Mattia, Jakob, Suhail
  • Immediate SNIFS target selection (for monday, so, today).
  • ePESSTO. Ampel slack note for potential targets (Uli/Jakob).
  • SN cosmoloy program coordination (RCF, ePESSTO, LCO, SNIFS program combination and priority, monitoring). When should what be triggered? Successfull?
  • Web DB interface to coordinate observation. Peter, Uli
  • Organize Marshal Scanning: as partners of ZTF, to verify our filters and/or to make candidate selections. This is also an excellent way to interact with the SN group,= and work eg on early SNIa.
  • I-band fringing. We will be expected to be able to say how well the I-band works before getting more time. Regenerative networks. Peter / Mickael
  • Flatfield (multiple subcomoponents). Matteo
  • RFC comparison vs HU clean - would we have missed anything, found anything extra? Matteo / JN
  • AMPEL/Marshal interaction: Implement that candidates saved in a marshal program is not submitted again. JN

- Shifting scheduler and TODO list: Jakob/Uli

SWG task chairs: So how much of this gets done?

These are intended to distribute live survey work, and each require 10-20% time commitment. In case this is exceeded a task is to be split, or distribute work to the SWG (could be scanning/shifting). The first step will be to determine the tools and procedures that should be used.

  • Candidate selection. (PI: Uli) Are candidates selected as expected? Ingestion of external transients. Scanning evaluation/comparison/organization.
  • Ranking. (PI: Ariel) Is the current transient ranking reasonable? What can be done to improve this?
  • Follow-up trigger. (PI: Mickael) Interface to eg NOT, SNIFS, LCO, SEDM. Tools for telescope availability and finding charts.
  • Telescope shifting. (PI: Daniel -Berlin-) SNIFS + possibly other facilities require shifting
  • Data evaluation. (PI: Suhail) Do we have the spectra? Is the quality sufficient? What is the (sub)type?
  • Photometry review. (PI: Jakob, C-I on commissioning: Matteo ) What is the current lightcurve quality, what are the limiting factors?
  • Program progress. (PI: Uli) Are we on track for publication? Long term follow-up need and proposals?

Projects:

Members:

OKC

>
>
A list of ongoing science projects can be found here. To be expanded shortly.

Useful Links:

Members:

OKC (Stockholm)
 
  • Rahul Biswas
  • Mattia Bulla
  • Suhail Dhawan
Deleted:
<
<
  • Uli Feindt
 
  • Ariel Goobar
Changed:
<
<
  • Laura Hangard
  • Seméli Papadogiannakis

HU/DESY

>
>
  • Joel Johansson
HU/DESY (Berlin)
 
  • Valéry Brinnel
Deleted:
<
<
  • Matteo Giomi
 
  • Jakob Nordin
Changed:
<
<
  • Marek Kowalski

In2p3

>
>
IN2P3 (Lyon)
 
  • Mickael Rigault
Added:
>
>
  • Mathew Smith
  • Young-Lo Kim
  • Yannick Copin
  • Jeremy Lezey
  • Martin Briday
Trinity (Dublin)
  • Kate Maguire
  • ...
IN2P3 (Claremont)
  • Philippe Rosnet
  • Melissa Amenouche
IN2P3 (Marseille)
  • Benjamin Racine
  • Julian Bautista
  • Fabrice Feinstein
  • Bastien Carreres
IN2P3 (Paris)
  • Nicolas Regault
Caltech
  • Abigail Poli
Past Members:
  • Danny Goldstein (Berkeley)
  • Peter Nugent (Berkeley: come back Peter!)
  • Matteo Giomi (Berlin)
  • Marek Kowalski (Berlin)
  • Uli Feindt (Stockholm)
  • Laura Hangard (Stockholm)
  • Seméli Papadogiannakis (Stockholm)

Ongoing Projects:

 
Deleted:
<
<

Berkeley

  • Danny Goldstein
  • Peter Nugent
 \ No newline at end of file
Added:
>
>
(needs updating)

Revision 192019-11-01 - SuhailDhawan

Line: 1 to 1
 
META TOPICPARENT name="ScienceWorkingGroups"

ZTF Cosmology with SNe and gravitational lensing Working Group

Line: 8 to 8
 

Contact information:

Changed:
<
<
coordinators: Uli Feindt, OKC (Coordinator), Jakob Nordin, HU (Deputy Coordinator)
>
>
coordinators: Suhail Dhawan, OKC (Coordinator), Jakob Nordin, HU (Deputy Coordinator)
  mailing list: ztfia@lists.astro.caltech.edu sign up here

slack organization: ztfia.slack.com [contact Uli to get an invitation]

Changed:
<
<
meeting time: Alternating between Wednesdays 14:00 CET (even weeks) and Tuesdays 19:00 CET (odd weeks)
>
>
meeting time: Alternating between Wednesdays 14:00 CET and Wednesdays 17:00 CET
 

Minutes:

Added:
>
>
 Telecon minutes can be found here.

October 2018 spectroscopic campaign:

Line: 30 to 32
 The ZTF camera is great. The raw calibration is better than expected. SEDM works. We find roughly the right order of transients. ZTF could really do ground-breaking cosmology.

But, this requires 2000 (4000+) spectroscopically confirmed and calibrated SNe Ia. Need to get the program running and convince the collaboratoin that its cool. No excuses.

Changed:
<
<
  • Draft outline group for ZTF cosmology project. Ariel, Mickael, Jakob, Uli, Peter, …
>
>
  • Draft outline group for ZTF cosmology project. Ariel, Mickael, Jakob, Uli, Peter, …
 
  • Show observed rate agrees with simulations. Uli
  • Isolate subset of SNe with minimal/flat host contribution. Script to download PS photometry at coordinate, fit the background with some metric (plane?) and record outcome. Combined with visual confirmation? Ariel
Changed:
<
<
  • Isolate subset of SNe with spectroscopic host redshifts. To what extend can we trust marshal notes? Probably at least want to complement with something slightly more complex. Match with SDSS and NED, calculate confusion metric. CLU matches probably only available throuch Caltech. OKC – Lauras code?
>
>
  • Isolate subset of SNe with spectroscopic host redshifts. To what extend can we trust marshal notes? Probably at least want to complement with something slightly more complex. Match with SDSS and NED, calculate confusion metric. CLU matches probably only available throuch Caltech. OKC – Lauras code?
 
  • Maintain our list of typed SNe Ia, routines for classification (SNID) and subclassification. Are there cases that are ambigous? Semeli/Uli writeup of current.
  • Fit floating SNIa lightcurves to everything in AMPEL - did we miss anything looking like a Ia? JN
  • Trigger instructions for LCO. They have a nice visual tool, but we probably need a script to gather the necessary information. Done frequently by the SN group so they might already have this.

Revision 182018-09-05 - JakobNordin

Line: 1 to 1
 
META TOPICPARENT name="ScienceWorkingGroups"

ZTF Cosmology with SNe and gravitational lensing Working Group

Line: 19 to 19
 

Minutes:

Telecon minutes can be found here.
Changed:
<
<

Upcoming Deadlines and Stuff:

>
>

October 2018 spectroscopic campaign:

This will run for approximately 20 days with the combined goals of investigating how deep an effective ZTF SNIa search can go and what spectroscopic resources this would require/warrant.

 

Cosmology tasklist Summer 2018

The ZTF camera is great. The raw calibration is better than expected. SEDM works. We find roughly the right order of transients. ZTF could really do ground-breaking cosmology.

Revision 172018-08-21 - UlrichFeindt

Line: 1 to 1
 
META TOPICPARENT name="ScienceWorkingGroups"

ZTF Cosmology with SNe and gravitational lensing Working Group

Line: 14 to 14
  slack organization: ztfia.slack.com [contact Uli to get an invitation]
Changed:
<
<
meeting time: Every other Wednesday 16:00 CET
>
>
meeting time: Alternating between Wednesdays 14:00 CET (even weeks) and Tuesdays 19:00 CET (odd weeks)
 

Minutes:

Telecon minutes can be found here.

Revision 162018-08-10 - JakobNordin

Line: 1 to 1
 
META TOPICPARENT name="ScienceWorkingGroups"

ZTF Cosmology with SNe and gravitational lensing Working Group

Line: 25 to 25
 
  • Ampel Coding Days (Dec 12/13th)
  • NOT deadlines?
Added:
>
>

Cosmology tasklist Summer 2018

The ZTF camera is great. The raw calibration is better than expected. SEDM works. We find roughly the right order of transients. ZTF could really do ground-breaking cosmology.
 
Changed:
<
<

SWG task chairs:

>
>
But, this requires 2000 (4000+) spectroscopically confirmed and calibrated SNe Ia. Need to get the program running and convince the collaboratoin that its cool. No excuses. * Draft outline group for ZTF cosmology project. Ariel, Mickael, Jakob, Uli, Peter, … * Show observed rate agrees with simulations. Uli * Isolate subset of SNe with minimal/flat host contribution. Script to download PS photometry at coordinate, fit the background with some metric (plane?) and record outcome. Combined with visual confirmation? Ariel * Isolate subset of SNe with spectroscopic host redshifts. To what extend can we trust marshal notes? Probably at least want to complement with something slightly more complex. Match with SDSS and NED, calculate confusion metric. CLU matches probably only available throuch Caltech. OKC – Lauras code? * Maintain our list of typed SNe Ia, routines for classification (SNID) and subclassification. Are there cases that are ambigous? Semeli/Uli writeup of current. * Fit floating SNIa lightcurves to everything in AMPEL - did we miss anything looking like a Ia? JN * Trigger instructions for LCO. They have a nice visual tool, but we probably need a script to gather the necessary information. Done frequently by the SN group so they might already have this. * TNS submission manual. For single entries there is a convenient web form, Christoffer also has a python script. Probably need to gather some information like what candidates do we want to / should we submit and eg what acknowledgments are used. * Figure out how to use the SNCOSMO data (include other templates?, peak fit?, floating offset? upper limits?). I am sure there are cases where the fit is not representative, typically when post-peak data is missing. Mickael * AGN rejection in AMPEL. Core distance, catalog matching and variability. Previous variability rejection in AMPEL. Through 30day history and/or PTF. Peter, Nadia, Matteo * Maintain updated hubble diagram with diagnostics. Blinding!?! Flag SNe with offset. Ampel * SNIFS trigger script: For a given SN, incorporate finding chart into the SNIFS observing database. Mickael. * SNIFS training and shifting. We should be ~8 shifters to make this a trivial task (~ a few hoursslac each month) Uli, Mickael, Daniel, Mattia, Jakob, Suhail * Immediate SNIFS target selection (for monday, so, today). * ePESSTO. Ampel slack note for potential targets (Uli/Jakob). * SN cosmoloy program coordination (RCF, ePESSTO, LCO, SNIFS program combination and priority, monitoring). When should what be triggered? Successfull? * Web DB interface to coordinate observation. Peter, Uli * Organize Marshal Scanning: as partners of ZTF, to verify our filters and/or to make candidate selections. This is also an excellent way to interact with the SN group,= and work eg on early SNIa. * I-band fringing. We will be expected to be able to say how well the I-band works before getting more time. Regenerative networks. Peter / Mickael * Flatfield (multiple subcomoponents). Matteo * RFC comparison vs HU clean - would we have missed anything, found anything extra? Matteo / JN * AMPEL/Marshal interaction: Implement that candidates saved in a marshal program is not submitted again. JN

- Shifting scheduler and TODO list: Jakob/Uli

SWG task chairs: So how much of this gets done?

 These are intended to distribute live survey work, and each require 10-20% time commitment. In case this is exceeded a task is to be split, or distribute work to the SWG (could be scanning/shifting). The first step will be to determine the tools and procedures that should be used.
  • Candidate selection. (PI: Uli) Are candidates selected as expected? Ingestion of external transients. Scanning evaluation/comparison/organization.
  • Ranking. (PI: Ariel) Is the current transient ranking reasonable? What can be done to improve this?

Revision 152018-06-14 - UlrichFeindt

Line: 1 to 1
 
META TOPICPARENT name="ScienceWorkingGroups"

ZTF Cosmology with SNe and gravitational lensing Working Group

Line: 44 to 44
 
Changed:
<
<
>
>
 

Members:

OKC

Revision 142018-06-07 - UlrichFeindt

Line: 1 to 1
 
META TOPICPARENT name="ScienceWorkingGroups"

ZTF Cosmology with SNe and gravitational lensing Working Group

Line: 44 to 44
 
Changed:
<
<
  • ...
>
>
 

Members:

OKC

Revision 132018-05-11 - UlrichFeindt

Line: 1 to 1
 
META TOPICPARENT name="ScienceWorkingGroups"

ZTF Cosmology with SNe and gravitational lensing Working Group

Line: 14 to 14
  slack organization: ztfia.slack.com [contact Uli to get an invitation]
Changed:
<
<
meeting time: Every other Thursday 16:30 CET
>
>
meeting time: Every other Wednesday 16:00 CET
 

Minutes:

Telecon minutes can be found here.

Revision 122017-11-23 - MickaelRigault

Line: 1 to 1
 
META TOPICPARENT name="ScienceWorkingGroups"

ZTF Cosmology with SNe and gravitational lensing Working Group

Line: 28 to 28
 

SWG task chairs:

These are intended to distribute live survey work, and each require 10-20% time commitment. In case this is exceeded a task is to be split, or distribute work to the SWG (could be scanning/shifting). The first step will be to determine the tools and procedures that should be used.
Changed:
<
<
  • Candidate selection. Are candidates selected as expected? Ingestion of external transients. Scanning evaluation/comparison/organization.
  • Ranking. Is the current transient ranking reasonable? What can be done to improve this?
  • Follow-up trigger. Interface to eg NOT, SNIFS, LCO, SEDM. Tools for telescope availability and finding charts.
  • Telescope shifting. SNIFS + possibly other facilities require shifting
  • Data evaluation. Do we have the spectra? Is the quality sufficient? What is the (sub)type?
  • Photometry review. What is the current lightcurve quality, what are the limiting factors?
  • Program progress. Are we on track for publication? Long term follow-up need and proposals?
>
>
  • Candidate selection. (PI: Uli) Are candidates selected as expected? Ingestion of external transients. Scanning evaluation/comparison/organization.
  • Ranking. (PI: Ariel) Is the current transient ranking reasonable? What can be done to improve this?
  • Follow-up trigger. (PI: Mickael) Interface to eg NOT, SNIFS, LCO, SEDM. Tools for telescope availability and finding charts.
  • Telescope shifting. (PI: Daniel -Berlin-) SNIFS + possibly other facilities require shifting
  • Data evaluation. (PI: Suhail) Do we have the spectra? Is the quality sufficient? What is the (sub)type?
  • Photometry review. (PI: Jakob, C-I on commissioning: Matteo ) What is the current lightcurve quality, what are the limiting factors?
  • Program progress. (PI: Uli) Are we on track for publication? Long term follow-up need and proposals?
 

Revision 112017-11-14 - JakobNordin

Line: 1 to 1
 
META TOPICPARENT name="ScienceWorkingGroups"

ZTF Cosmology with SNe and gravitational lensing Working Group

Line: 19 to 19
 

Minutes:

Telecon minutes can be found here.
Added:
>
>

Upcoming Deadlines and Stuff:

 

SWG task chairs:

These are intended to distribute live survey work, and each require 10-20% time commitment. In case this is exceeded a task is to be split, or distribute work to the SWG (could be scanning/shifting). The first step will be to determine the tools and procedures that should be used.
Line: 31 to 37
 
  • Program progress. Are we on track for publication? Long term follow-up need and proposals?
Deleted:
<
<

Tasks:

 

Projects:

Revision 102017-11-14 - JakobNordin

Line: 1 to 1
 
META TOPICPARENT name="ScienceWorkingGroups"

ZTF Cosmology with SNe and gravitational lensing Working Group

Line: 26 to 26
 
  • Ranking. Is the current transient ranking reasonable? What can be done to improve this?
  • Follow-up trigger. Interface to eg NOT, SNIFS, LCO, SEDM. Tools for telescope availability and finding charts.
  • Telescope shifting. SNIFS + possibly other facilities require shifting
Changed:
<
<
  • Spectroscopic evaluation. Do we have the data? Is the quality sufficient? What is the (sub)type?
  • Photometry/calibration review. What is the current lightcurve quality, what are the limiting factors?
  • Analysis progress. Are we on track for publication?
>
>
  • Data evaluation. Do we have the spectra? Is the quality sufficient? What is the (sub)type?
  • Photometry review. What is the current lightcurve quality, what are the limiting factors?
  • Program progress. Are we on track for publication? Long term follow-up need and proposals?
 

Tasks:

Revision 92017-11-13 - JakobNordin

Line: 1 to 1
 
META TOPICPARENT name="ScienceWorkingGroups"

ZTF Cosmology with SNe and gravitational lensing Working Group

Line: 22 to 22
 

SWG task chairs:

These are intended to distribute live survey work, and each require 10-20% time commitment. In case this is exceeded a task is to be split, or distribute work to the SWG (could be scanning/shifting). The first step will be to determine the tools and procedures that should be used.
Changed:
<
<
  • Candidate selection. Are candidates selected as expected? Ingestion of external transients. Scanning evaluation/comparison/organization.
  • Ranking. Is the current transient ranking reasonable? What can be done to improve this?
  • Follow-up trigger. Interface to eg NOT, SNIFS, LCO, SEDM. Tools for telescope availability and finding charts.
  • SNIFS shifting.
>
>
  • Candidate selection. Are candidates selected as expected? Ingestion of external transients. Scanning evaluation/comparison/organization.
  • Ranking. Is the current transient ranking reasonable? What can be done to improve this?
  • Follow-up trigger. Interface to eg NOT, SNIFS, LCO, SEDM. Tools for telescope availability and finding charts.
  • Telescope shifting. SNIFS + possibly other facilities require shifting
 
  • Spectroscopic evaluation. Do we have the data? Is the quality sufficient? What is the (sub)type?
  • Photometry/calibration review. What is the current lightcurve quality, what are the limiting factors?
  • Analysis progress. Are we on track for publication?

Revision 82017-11-09 - MickaelRigault

Line: 1 to 1
 
META TOPICPARENT name="ScienceWorkingGroups"

ZTF Cosmology with SNe and gravitational lensing Working Group

Line: 57 to 57
 
  • Valéry Brinnel
  • Matteo Giomi
  • Jakob Nordin
Changed:
<
<

Lyon

>
>
  • Marek Kowalski

In2p3

 
  • Mickael Rigault
Added:
>
>
 

Berkeley

  • Danny Goldstein
  • Peter Nugent

Revision 72017-11-09 - JakobNordin

Line: 1 to 1
 
META TOPICPARENT name="ScienceWorkingGroups"

ZTF Cosmology with SNe and gravitational lensing Working Group

Line: 21 to 21
 

SWG task chairs:

Added:
>
>
These are intended to distribute live survey work, and each require 10-20% time commitment. In case this is exceeded a task is to be split, or distribute work to the SWG (could be scanning/shifting). The first step will be to determine the tools and procedures that should be used.
 
  • Candidate selection. Are candidates selected as expected? Ingestion of external transients. Scanning evaluation/comparison/organization.
  • Ranking. Is the current transient ranking reasonable? What can be done to improve this?
  • Follow-up trigger. Interface to eg NOT, SNIFS, LCO, SEDM. Tools for telescope availability and finding charts.

Revision 62017-11-08 - JakobNordin

Line: 1 to 1
 
META TOPICPARENT name="ScienceWorkingGroups"

ZTF Cosmology with SNe and gravitational lensing Working Group

Line: 19 to 19
 

Minutes:

Telecon minutes can be found here.
Added:
>
>

SWG task chairs:

  • Candidate selection. Are candidates selected as expected? Ingestion of external transients. Scanning evaluation/comparison/organization.
  • Ranking. Is the current transient ranking reasonable? What can be done to improve this?
  • Follow-up trigger. Interface to eg NOT, SNIFS, LCO, SEDM. Tools for telescope availability and finding charts.
  • SNIFS shifting.
  • Spectroscopic evaluation. Do we have the data? Is the quality sufficient? What is the (sub)type?
  • Photometry/calibration review. What is the current lightcurve quality, what are the limiting factors?
  • Analysis progress. Are we on track for publication?
 

Tasks:

Revision 52017-11-06 - UlrichFeindt

Line: 1 to 1
 
META TOPICPARENT name="ScienceWorkingGroups"

ZTF Cosmology with SNe and gravitational lensing Working Group

Line: 16 to 16
  meeting time: Every other Thursday 16:30 CET
Added:
>
>

Minutes:

Telecon minutes can be found here.

Tasks:

Projects:

 

Members:

OKC

  • Rahul Biswas
Line: 34 to 49
 

Berkeley

  • Danny Goldstein
  • Peter Nugent
Deleted:
<
<

Minutes:

Projects

Revision 42017-11-03 - UlrichFeindt

Line: 1 to 1
 
META TOPICPARENT name="ScienceWorkingGroups"

ZTF Cosmology with SNe and gravitational lensing Working Group

Line: 6 to 6
  Some material may be found on the previous SNeIa page.
Changed:
<
<
Contact informations:
>
>

Contact information:

 
Changed:
<
<
coordinators:
>
>
coordinators: Uli Feindt, OKC (Coordinator), Jakob Nordin, HU (Deputy Coordinator)
  mailing list: ztfia@lists.astro.caltech.edu sign up here
Changed:
<
<
meeting time:
>
>
slack organization: ztfia.slack.com [contact Uli to get an invitation]
 
Changed:
<
<
Members:
>
>
meeting time: Every other Thursday 16:30 CET
 
Changed:
<
<
Minutes:
>
>

Members:

OKC

  • Rahul Biswas
  • Mattia Bulla
  • Suhail Dhawan
  • Uli Feindt
  • Ariel Goobar
  • Laura Hangard
  • Seméli Papadogiannakis

HU/DESY

  • Valéry Brinnel
  • Matteo Giomi
  • Jakob Nordin

Lyon

  • Mickael Rigault

Berkeley

  • Danny Goldstein
  • Peter Nugent
 
Changed:
<
<
Projects
>
>

Minutes:

Projects

Revision 32017-10-25 - MaayaneSoumagnac

Line: 1 to 1
 
META TOPICPARENT name="ScienceWorkingGroups"

ZTF Cosmology with SNe and gravitational lensing Working Group

This is the Wiki page for the ZTF Working Group on cosmology with SNe and gravitational lensing.

Some material may be found on the previous SNeIa page.

Added:
>
>
Contact informations:

coordinators:

mailing list: ztfia@lists.astro.caltech.edu sign up here

meeting time:

Members:

Minutes:

Projects

Revision 22017-10-02 - EricBellm

Line: 1 to 1
 
META TOPICPARENT name="ScienceWorkingGroups"

ZTF Cosmology with SNe and gravitational lensing Working Group

This is the Wiki page for the ZTF Working Group on cosmology with SNe and gravitational lensing.

Changed:
<
<
-- MatthewGraham - 02 Oct 2017
>
>
Some material may be found on the previous SNeIa page.

Revision 12017-10-02 - MatthewGraham

Line: 1 to 1
Added:
>
>
META TOPICPARENT name="ScienceWorkingGroups"

ZTF Cosmology with SNe and gravitational lensing Working Group

This is the Wiki page for the ZTF Working Group on cosmology with SNe and gravitational lensing.

-- MatthewGraham - 02 Oct 2017

 
This site is powered by the TWiki collaboration platform Powered by PerlCopyright © 2008-2025 by the contributing authors. All material on this collaboration platform is the property of the contributing authors.
Ideas, requests, problems regarding TWiki? Send feedback