Difference: TransientWGProjects (1 vs. 40)
Revision 402024-04-16 - ChangLiu
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 55 to 55 | ||||||||
| 12) Classifying SNe based on spectral time-series using unsupervised learning algorithm (presentation). Student: Ofek Bengiat Supervisor: Avishay Gal-Yam 13) Identifying all He-shell detonations in ZTF spectroscopically, Student: Peter Scherbak, Advisor: Mansi Kasliwal, co-advisor: Abi Polin | ||||||||
| Added: | ||||||||
| > > | 14) Connecting ZTF early light curves with late time spectroscopy to understand SN Ia explosion channels. Student: Chang Liu; Advisor: Adam Miller | |||||||
SLSN related papers1) The First set of SLSNe discovered by ZTF --- leading: Lunnan | ||||||||
Revision 392022-04-11 - TuomasKangas
Revision 382022-02-14 - MansiKasliwal
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 53 to 53 | ||||||||
| 11) CSM interaction in normal SNe Ia Student: Jacco Terwel Supervisor: Kate Maguire 12) Classifying SNe based on spectral time-series using unsupervised learning algorithm (presentation). Student: Ofek Bengiat Supervisor: Avishay Gal-Yam | ||||||||
| Added: | ||||||||
| > > | 13) Identifying all He-shell detonations in ZTF spectroscopically, Student: Peter Scherbak, Advisor: Mansi Kasliwal, co-advisor: Abi Polin | |||||||
SLSN related papers1) The First set of SLSNe discovered by ZTF --- leading: Lunnan | ||||||||
Revision 372021-10-21 - JesperSollerman
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 13 to 13 | ||||||||
| 1) Polarimetry of young SNe: Spectro- and imaging polarimetry of young SNe (VLT program and Liverpool Telescope, proposals submitted) Lead: Yi Yang (Weizmann Institute) | ||||||||
| Changed: | ||||||||
| < < | 2) Stripped-envelope supernovae from ZTF. Lead: C. Barbarino, F. Taddia, L. Tartaglia. Photometric and spectral characterisation of the various samples of stripped-envelope supernovae from ZTF, including supernovae Ib, Ic, Ic-bL (and IIb?). | |||||||
| > > | 2) Stripped-envelope supernovae from ZTF. Lead: S. Yang, T. Schweyer. Photometric and spectral characterisation of the various samples of stripped-envelope supernovae from ZTF, including supernovae Ib, Ic, Ic-bL (and IIb?). | |||||||
| Changed: | ||||||||
| < < | 3) Unusual stripped-envelope supernovae with broad-light curves from ZTF. Lead: F. Taddia. Discovering, following and investigating a rare subclass of broad-light curve SE SNe (first discovered by iPTF) which may come from massive single progenitor stars or from lower-mass stellar progenitors powered by magnetar (e.g., iPTF15dtg). | |||||||
| > > | 3) Unusual stripped-envelope supernovae with broad-light curves from ZTF. Lead: T Schweyer . Discovering, following and investigating a rare subclass of broad-light curve SE SNe (first discovered by iPTF) which may come from massive single progenitor stars or from lower-mass stellar progenitors powered by magnetar (e.g., iPTF15dtg). | |||||||
| 4) A UV&optical survey of ZTF type IIn supernovae. Lead: Maayane Soumagnac. A survey of ~10 type IIn SNe brighter than -19. The idea is to obtain UV monitoring with Swift during the rise time, compute the temperature and radii from multiband photometry and answer the question: "what is the percentage of events involving non-spherical CSM?" (lower limit, following the methodology by Soumagnac et al 2018, in preparation). 5) rapid spectroscopic evolution of SN 2018dfi during day 1: lead, Yi Yang (WIS) | ||||||||
| Deleted: | ||||||||
| < < | 6) very early evolution of UV+optical emission from SN 2018fif, lead Maayane Soumagnac. | |||||||
| 7) Double humped non-interacting SNe II, lead O. Yaron, objects: SN2018efj, SN2018egh | ||||||||
| Deleted: | ||||||||
| < < | 8) Sample of ZTF SNe IIn followed up in the UV, for CSM geometry analysis. Lead: Maayane Soumagnac | |||||||
| 9) Spectroscopic study of Type Ia Supernovae and correlation between spectral feature and SN lightcurve and Host properties. Lead: Mickael Rigault 10) Search for precursor explosions prior to SNe of different types. Lead: Nora Linn Strotjohann 11) Modelling of early Type Ia supernova light curves and spectra. Lead: Mark Magee | ||||||||
| Deleted: | ||||||||
| < < | 12) Population characterization of Type Ia SNe: Lead Rahul Biswas | |||||||
13) Relativistic explosions (afterglows & fast blue optical transients): Anna Ho (UC Berkeley)
Thesis projects | ||||||||
| Line: 76 to 70 | ||||||||
| 7) ZTF sample of type II SLSNe with no narrow lines -- leading: Kangas, Yan 8) Single object study of SN2020znr (joined ZTF and ePESSTO+ data) -- leading: Janet, Sheng | ||||||||
| Deleted: | ||||||||
| < < | Young Ia papers1) 2018 partnership light curve sample ---- leading: Yuhan Yao 2) early color evolution of 2018 sample ---- leading: Mattia Bhulla 3) early rise of 2018 sample ---- leading: Adam Miller | |||||||
| ||||||||
Revision 362021-10-18 - JanetTingWanChen
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 74 to 74 | ||||||||
| 6) Occurance rate of CSM shells around SLSNe -- leading: Lunnan. VLT program underway. 7) ZTF sample of type II SLSNe with no narrow lines -- leading: Kangas, Yan | ||||||||
| Added: | ||||||||
| > > | 8) Single object study of SN2020znr (joined ZTF and ePESSTO+ data) -- leading: Janet, Sheng | |||||||
Young Ia papers1) 2018 partnership light curve sample ---- leading: Yuhan Yao | ||||||||
Revision 352021-05-02 - OfekBengiat
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 58 to 58 | ||||||||
|
11) CSM interaction in normal SNe Ia Student: Jacco Terwel Supervisor: Kate Maguire | ||||||||
| Added: | ||||||||
| > > | 12) Classifying SNe based on spectral time-series using unsupervised learning algorithm (presentation). Student: Ofek Bengiat Supervisor: Avishay Gal-Yam | |||||||
SLSN related papers1) The First set of SLSNe discovered by ZTF --- leading: Lunnan | ||||||||
Revision 342021-02-15 - AnnaHo
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 35 to 35 | ||||||||
| 12) Population characterization of Type Ia SNe: Lead Rahul Biswas | ||||||||
| Changed: | ||||||||
| < < | 13) Relativistic explosions & fast blue optical transients: Anna Ho (UC Berkeley) | |||||||
| > > | 13) Relativistic explosions (afterglows & fast blue optical transients): Anna Ho (UC Berkeley) | |||||||
Thesis projects1) UV observations of SNe (in the context of ULTRASAT and previous work with GALEX) Plan is to pursue a sample of SNe observed early on with ground + Swift UV. Goal is statistics of UV signals (strength, duration) and demographics of progenitors (radii, explosion energies, CSM?). First object is SN 2018dfi. \n Student: Noam Ganot Supervisor: Avishay Gal-Yam (Weizmann Institute) | ||||||||
Revision 332020-11-27 - TuomasKangas
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 71 to 71 | ||||||||
| 5) The candidate pair-instability SLSN SN2018ibb --- leading: Steve Schulze 6) Occurance rate of CSM shells around SLSNe -- leading: Lunnan. VLT program underway. | ||||||||
| Added: | ||||||||
| > > | 7) ZTF sample of type II SLSNe with no narrow lines -- leading: Kangas, Yan | |||||||
Young Ia papers1) 2018 partnership light curve sample ---- leading: Yuhan Yao | ||||||||
Revision 322020-11-26 - AnnaHo
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 66 to 66 | ||||||||
| 3) Estimates of SLSN rates from the first year of ZTF data -- Yan, Lunnan, Perley et al. | ||||||||
| Changed: | ||||||||
| < < | 4) From the most luminous SE SNe to SLSNe -- interested people: Yan, Fremling + .... | |||||||
| > > | 4) From the most luminous SE SNe to SLSNe (ZTF20abevcoo, ZTF20achvlbs, ZTF18achdidy) -- interested people: Yan, Fremling, Ho + .... | |||||||
| 5) The candidate pair-instability SLSN SN2018ibb --- leading: Steve Schulze | ||||||||
Revision 312020-11-24 - AnnaHo
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
Marshal Science Programs & Corresponding Filters | ||||||||
| Changed: | ||||||||
| < < | 1) Fast Transients, Rapidly Evolving Transients (i.e. afterglows, 18cow-like events; contact: Anna Ho) | |||||||
| > > | 1) Fast Transients, Rapidly Evolving Transients (i.e. afterglows, 18cow-like events; contact: Yuhan Yao & Anna Ho) | |||||||
| 2) Superluminous Supernovae (contact: Lin Yan) | ||||||||
| Line: 34 to 34 | ||||||||
| 11) Modelling of early Type Ia supernova light curves and spectra. Lead: Mark Magee 12) Population characterization of Type Ia SNe: Lead Rahul Biswas | ||||||||
| Added: | ||||||||
| > > | 13) Relativistic explosions & fast blue optical transients: Anna Ho (UC Berkeley) | |||||||
Thesis projects1) UV observations of SNe (in the context of ULTRASAT and previous work with GALEX) Plan is to pursue a sample of SNe observed early on with ground + Swift UV. Goal is statistics of UV signals (strength, duration) and demographics of progenitors (radii, explosion energies, CSM?). First object is SN 2018dfi. \n Student: Noam Ganot Supervisor: Avishay Gal-Yam (Weizmann Institute) 2) Rapid spectroscopy Supervisor: Avishay Gal-Yam (Weizmann Institute) | ||||||||
| Changed: | ||||||||
| < < | 3) Afterglows of Relativistic Explosions Student: Anna Ho Supervisor: Shri Kulkarni 4) Type Ic-BL supernovae Student: Shreya Anand Supervisor: Mansi Kasliwal | |||||||
| > > | 4) Type Ic-BL supernovae Student: Shreya Anand Supervisor: Mansi Kasliwal | |||||||
|
5) Gap Transients (e.g. Calcium-rich, Ultra-stripped events) Student: Kishalay De Supervisor: Mansi Kasliwal | ||||||||
Revision 302020-11-23 - RagnhildLunnan
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 69 to 69 | ||||||||
| 4) From the most luminous SE SNe to SLSNe -- interested people: Yan, Fremling + .... 5) The candidate pair-instability SLSN SN2018ibb --- leading: Steve Schulze | ||||||||
| Added: | ||||||||
| > > | 6) Occurance rate of CSM shells around SLSNe -- leading: Lunnan. VLT program underway. | |||||||
Young Ia papers1) 2018 partnership light curve sample ---- leading: Yuhan Yao | ||||||||
Revision 292020-09-25 - MansiKasliwal
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 42 to 42 | ||||||||
|
3) Afterglows of Relativistic Explosions Student: Anna Ho Supervisor: Shri Kulkarni | ||||||||
| Changed: | ||||||||
| < < | 4) Obscured Supernovae Student: Jacob Jencson Supervisor: Mansi Kasliwal | |||||||
| > > | 4) Type Ic-BL supernovae Student: Shreya Anand Supervisor: Mansi Kasliwal | |||||||
|
5) Gap Transients (e.g. Calcium-rich, Ultra-stripped events) Student: Kishalay De Supervisor: Mansi Kasliwal | ||||||||
Revision 282020-09-25 - KateMaguire2
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 54 to 54 | ||||||||
|
9) Early light curve modelling of SNe Ia Student: Maxime Deckers Supervisor: Kate Maguire | ||||||||
| Added: | ||||||||
| > > | 10) Constraining the spectra of SNe Ia using ZTF Student: Luke Harvey Supervisor: Kate Maguire 11) CSM interaction in normal SNe Ia Student: Jacco Terwel Supervisor: Kate Maguire | |||||||
SLSN related papers1) The First set of SLSNe discovered by ZTF --- leading: Lunnan | ||||||||
Revision 272020-06-30 - RahulBiswas
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 32 to 32 | ||||||||
| 10) Search for precursor explosions prior to SNe of different types. Lead: Nora Linn Strotjohann 11) Modelling of early Type Ia supernova light curves and spectra. Lead: Mark Magee | ||||||||
| Added: | ||||||||
| > > | 12) Population characterization of Type Ia SNe: Lead Rahul Biswas | |||||||
Thesis projects1) UV observations of SNe (in the context of ULTRASAT and previous work with GALEX) Plan is to pursue a sample of SNe observed early on with ground + Swift UV. Goal is statistics of UV signals (strength, duration) and demographics of progenitors (radii, explosion energies, CSM?). First object is SN 2018dfi. \n Student: Noam Ganot Supervisor: Avishay Gal-Yam (Weizmann Institute) | ||||||||
Revision 262020-02-21 - KateMaguire2
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 8 to 8 | ||||||||
| 3) Infant Supernovae (contact: Avishay Gal-Yam) | ||||||||
| Changed: | ||||||||
| < < | 4) Early Observations of SNe Ia (contact: Adam Miller) | |||||||
| > > | 4) Early Observations of SNe Ia (contact: Kate Maguire, Adam Miller) | |||||||
Postdoc projects1) Polarimetry of young SNe: Spectro- and imaging polarimetry of young SNe (VLT program and Liverpool Telescope, proposals submitted) Lead: Yi Yang (Weizmann Institute) | ||||||||
| Line: 30 to 30 | ||||||||
| 9) Spectroscopic study of Type Ia Supernovae and correlation between spectral feature and SN lightcurve and Host properties. Lead: Mickael Rigault 10) Search for precursor explosions prior to SNe of different types. Lead: Nora Linn Strotjohann | ||||||||
| Added: | ||||||||
| > > | 11) Modelling of early Type Ia supernova light curves and spectra. Lead: Mark Magee | |||||||
Thesis projects1) UV observations of SNe (in the context of ULTRASAT and previous work with GALEX) Plan is to pursue a sample of SNe observed early on with ground + Swift UV. Goal is statistics of UV signals (strength, duration) and demographics of progenitors (radii, explosion energies, CSM?). First object is SN 2018dfi. \n Student: Noam Ganot Supervisor: Avishay Gal-Yam (Weizmann Institute) | ||||||||
| Line: 48 to 50 | ||||||||
|
8) Early light curve modeling of CCSNe Student: Ido Irani Supervisor: Avishay Gal-Yam | ||||||||
| Added: | ||||||||
| > > | 9) Early light curve modelling of SNe Ia Student: Maxime Deckers Supervisor: Kate Maguire | |||||||
SLSN related papers1) The First set of SLSNe discovered by ZTF --- leading: Lunnan | ||||||||
Revision 252019-12-01 - NoraLinnStrotjohann
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 28 to 28 | ||||||||
| 8) Sample of ZTF SNe IIn followed up in the UV, for CSM geometry analysis. Lead: Maayane Soumagnac 9) Spectroscopic study of Type Ia Supernovae and correlation between spectral feature and SN lightcurve and Host properties. Lead: Mickael Rigault | ||||||||
| Added: | ||||||||
| > > | 10) Search for precursor explosions prior to SNe of different types. Lead: Nora Linn Strotjohann | |||||||
Thesis projects1) UV observations of SNe (in the context of ULTRASAT and previous work with GALEX) Plan is to pursue a sample of SNe observed early on with ground + Swift UV. Goal is statistics of UV signals (strength, duration) and demographics of progenitors (radii, explosion energies, CSM?). First object is SN 2018dfi. \n Student: Noam Ganot Supervisor: Avishay Gal-Yam (Weizmann Institute) | ||||||||
Revision 242019-11-28 - SteveSchulze
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
Marshal Science Programs & Corresponding Filters | ||||||||
Revision 232019-09-01 - MickaelRigault
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 27 to 27 | ||||||||
| 8) Sample of ZTF SNe IIn followed up in the UV, for CSM geometry analysis. Lead: Maayane Soumagnac | ||||||||
| Added: | ||||||||
| > > | 9) Spectroscopic study of Type Ia Supernovae and correlation between spectral feature and SN lightcurve and Host properties. Lead: Mickael Rigault | |||||||
Thesis projects1) UV observations of SNe (in the context of ULTRASAT and previous work with GALEX) Plan is to pursue a sample of SNe observed early on with ground + Swift UV. Goal is statistics of UV signals (strength, duration) and demographics of progenitors (radii, explosion energies, CSM?). First object is SN 2018dfi. \n Student: Noam Ganot Supervisor: Avishay Gal-Yam (Weizmann Institute) | ||||||||
Revision 222019-08-18 - AnnaHo
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
Marshal Science Programs & Corresponding Filters | ||||||||
| Changed: | ||||||||
| < < | 1) Fast Transients (contact: Anna Ho) | |||||||
| > > | 1) Fast Transients, Rapidly Evolving Transients (i.e. afterglows, 18cow-like events; contact: Anna Ho) | |||||||
| 2) Superluminous Supernovae (contact: Lin Yan) | ||||||||
Revision 212019-08-14 - IdoIrani
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 41 to 41 | ||||||||
|
6) Study of a sample of Type II SNe from ZTF: flash spectroscopy fraction, light curve morphology (see slides 2,3 in presentation below) Student: Rachel Bruch Advisor: Avishay Gal-Yam
| ||||||||
| Added: | ||||||||
| > > | 7) CCSNe in Early type galaxies Student: Ido Irani Supervisor: Avishay Gal-Yam 8) Early light curve modeling of CCSNe Student: Ido Irani Supervisor: Avishay Gal-Yam | |||||||
SLSN related papers1) The First set of SLSNe discovered by ZTF --- leading: Lunnan | ||||||||
Revision 202019-08-12 - MaayaneSoumagnac
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 25 to 25 | ||||||||
| 7) Double humped non-interacting SNe II, lead O. Yaron, objects: SN2018efj, SN2018egh | ||||||||
| Added: | ||||||||
| > > | 8) Sample of ZTF SNe IIn followed up in the UV, for CSM geometry analysis. Lead: Maayane Soumagnac | |||||||
Thesis projects1) UV observations of SNe (in the context of ULTRASAT and previous work with GALEX) Plan is to pursue a sample of SNe observed early on with ground + Swift UV. Goal is statistics of UV signals (strength, duration) and demographics of progenitors (radii, explosion energies, CSM?). First object is SN 2018dfi. \n Student: Noam Ganot Supervisor: Avishay Gal-Yam (Weizmann Institute) | ||||||||
Revision 192019-02-16 - SteveSchulze
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 41 to 41 | ||||||||
SLSN related papers | ||||||||
| Changed: | ||||||||
| < < | 1) The First set of SLSNe discovered by ZTF --- leading: Lunnan 2) LC modeling of a sample of SLSNe, including late-time photometry --- Yan et al. 3) Estimates of SLSN rates from the first year of ZTF data -- Yan, Lunnan, Perley et al. 4) From the most luminous SE SNe to SLSNe -- interested people: Yan, Fremling + .... | |||||||
| > > | 1) The First set of SLSNe discovered by ZTF --- leading: Lunnan 2) LC modeling of a sample of SLSNe, including late-time photometry --- Yan et al. 3) Estimates of SLSN rates from the first year of ZTF data -- Yan, Lunnan, Perley et al. 4) From the most luminous SE SNe to SLSNe -- interested people: Yan, Fremling + .... 5) The candidate pair-instability SLSN SN2018ibb --- leading: Steve Schulze | |||||||
Young Ia papers1) 2018 partnership light curve sample ---- leading: Yuhan Yao | ||||||||
Revision 182019-01-22 - AdamMiller
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 8 to 8 | ||||||||
| 3) Infant Supernovae (contact: Avishay Gal-Yam) | ||||||||
| Added: | ||||||||
| > > | 4) Early Observations of SNe Ia (contact: Adam Miller) | |||||||
Postdoc projects1) Polarimetry of young SNe: Spectro- and imaging polarimetry of young SNe (VLT program and Liverpool Telescope, proposals submitted) Lead: Yi Yang (Weizmann Institute) | ||||||||
| Line: 41 to 42 | ||||||||
SLSN related papers1) The First set of SLSNe discovered by ZTF --- leading: Lunnan2) LC modeling of a sample of SLSNe, including late-time photometry --- Yan et al. 3) Estimates of SLSN rates from the first year of ZTF data -- Yan, Lunnan, Perley et al. 4) From the most luminous SE SNe to SLSNe -- interested people: Yan, Fremling + .... | ||||||||
| Added: | ||||||||
| > > | Young Ia papers | |||||||
| Changed: | ||||||||
| < < | * | |||||||
| > > | 1) 2018 partnership light curve sample ---- leading: Yuhan Yao 2) early color evolution of 2018 sample ---- leading: Mattia Bhulla 3) early rise of 2018 sample ---- leading: Adam Miller | |||||||
| ||||||||
Revision 172018-11-01 - AvishayyGalyam
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 10 to 10 | ||||||||
Postdoc projects | ||||||||
| Changed: | ||||||||
| < < | 1) Polarimetry of young SNe: Spectro- and imaging polarimetry of young SNe (VLT program and Liverpool Telescope, proposals submitted) Lead: Yi Yang (Weizmann Institute) | |||||||
| > > | 1) Polarimetry of young SNe: Spectro- and imaging polarimetry of young SNe (VLT program and Liverpool Telescope, proposals submitted) Lead: Yi Yang (Weizmann Institute) | |||||||
| Changed: | ||||||||
| < < | 2) Stripped-envelope supernovae from ZTF. Lead: C. Barbarino, F. Taddia, L. Tartaglia. Photometric and spectral characterisation of the various samples of stripped-envelope supernovae from ZTF, including supernovae Ib, Ic, Ic-bL (and IIb?). | |||||||
| > > | 2) Stripped-envelope supernovae from ZTF. Lead: C. Barbarino, F. Taddia, L. Tartaglia. Photometric and spectral characterisation of the various samples of stripped-envelope supernovae from ZTF, including supernovae Ib, Ic, Ic-bL (and IIb?). | |||||||
| Changed: | ||||||||
| < < | 3) Unusual stripped-envelope supernovae with broad-light curves from ZTF. Lead: F. Taddia. Discovering, following and investigating a rare subclass of broad-light curve SE SNe (first discovered by iPTF) which may come from massive single progenitor stars or from lower-mass stellar progenitors powered by magnetar (e.g., iPTF15dtg). | |||||||
| > > | 3) Unusual stripped-envelope supernovae with broad-light curves from ZTF. Lead: F. Taddia. Discovering, following and investigating a rare subclass of broad-light curve SE SNe (first discovered by iPTF) which may come from massive single progenitor stars or from lower-mass stellar progenitors powered by magnetar (e.g., iPTF15dtg). | |||||||
| Changed: | ||||||||
| < < | 4) A UV&optical survey of ZTF type IIn supernovae. Lead: Maayane Soumagnac. A survey of ~10 type IIn SNe brighter than -19. The idea is to obtain UV monitoring with Swift during the rise time, compute the temperature and radii from multiband photometry and answer the question: "what is the percentage of events involving non-spherical CSM?" (lower limit, following the methodology by Soumagnac et al 2018, in preparation). | |||||||
| > > | 4) A UV&optical survey of ZTF type IIn supernovae. Lead: Maayane Soumagnac. A survey of ~10 type IIn SNe brighter than -19. The idea is to obtain UV monitoring with Swift during the rise time, compute the temperature and radii from multiband photometry and answer the question: "what is the percentage of events involving non-spherical CSM?" (lower limit, following the methodology by Soumagnac et al 2018, in preparation). 5) rapid spectroscopic evolution of SN 2018dfi during day 1: lead, Yi Yang (WIS) 6) very early evolution of UV+optical emission from SN 2018fif, lead Maayane Soumagnac. 7) Double humped non-interacting SNe II, lead O. Yaron, objects: SN2018efj, SN2018egh | |||||||
Thesis projects | ||||||||
| Changed: | ||||||||
| < < | 1) UV observations of SNe (in the context of ULTRASAT and previous work with GALEX)
Plan is to pursue a sample of SNe observed early on with ground + Swift UV. Goal is statistics of UV signals (strength, duration) and demographics of progenitors (radii, explosion energies, CSM?)\n
Student: Noam Ganot
Supervisor: Avishay Gal-Yam (Weizmann Institute)
2) Rapid spectroscopy
Supervisor: Avishay Gal-Yam (Weizmann Institute)
3) Afterglows of Relativistic Explosions Student: Anna Ho Supervisor: Shri Kulkarni 4) Obscured Supernovae Student: Jacob Jencson Supervisor: Mansi Kasliwal 5) Gap Transients (e.g. Calcium-rich, Ultra-stripped events) Student: Kishalay De Supervisor: Mansi Kasliwal | |||||||
| > > | 1) UV observations of SNe (in the context of ULTRASAT and previous work with GALEX) Plan is to pursue a sample of SNe observed early on with ground + Swift UV. Goal is statistics of UV signals (strength, duration) and demographics of progenitors (radii, explosion energies, CSM?). First object is SN 2018dfi. \n Student: Noam Ganot Supervisor: Avishay Gal-Yam (Weizmann Institute) 2) Rapid spectroscopy Supervisor: Avishay Gal-Yam (Weizmann Institute) | |||||||
| Added: | ||||||||
| > > | 3) Afterglows of Relativistic Explosions Student: Anna Ho Supervisor: Shri Kulkarni 4) Obscured Supernovae Student: Jacob Jencson Supervisor: Mansi Kasliwal 5) Gap Transients (e.g. Calcium-rich, Ultra-stripped events) Student: Kishalay De Supervisor: Mansi Kasliwal 6) Study of a sample of Type II SNe from ZTF: flash spectroscopy fraction, light curve morphology (see slides 2,3 in presentation below) Student: Rachel Bruch Advisor: Avishay Gal-Yam
| |||||||
SLSN related papers | ||||||||
| Changed: | ||||||||
| < < | 1) The First set of SLSNe discovered by ZTF --- leading: Lunnan 2) LC modeling of a sample of SLSNe, including late-time photometry --- Yan et al. 3) Estimates of SLSN rates from the first year of ZTF data -- Yan, Lunnan, Perley et al. 4) From the most luminous SE SNe to SLSNe -- interested people: Yan, Fremling + .... | |||||||
| > > | 1) The First set of SLSNe discovered by ZTF --- leading: Lunnan 2) LC modeling of a sample of SLSNe, including late-time photometry --- Yan et al. 3) Estimates of SLSN rates from the first year of ZTF data -- Yan, Lunnan, Perley et al. 4) From the most luminous SE SNe to SLSNe -- interested people: Yan, Fremling + .... * | |||||||
| ||||||||
| Added: | ||||||||
| > > |
| |||||||
Revision 162018-09-22 - DanielPerley
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 52 to 52 | ||||||||
| 3) Estimates of SLSN rates from the first year of ZTF data -- Yan, Lunnan, Perley et al. 4) From the most luminous SE SNe to SLSNe -- interested people: Yan, Fremling + .... | ||||||||
| Changed: | ||||||||
| < < |
| |||||||
| > > |
| |||||||
Revision 152018-09-22 - DanielPerley
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 51 to 51 | ||||||||
| 2) LC modeling of a sample of SLSNe, including late-time photometry --- Yan et al. 3) Estimates of SLSN rates from the first year of ZTF data -- Yan, Lunnan, Perley et al. 4) From the most luminous SE SNe to SLSNe -- interested people: Yan, Fremling + .... \ No newline at end of file | ||||||||
| Added: | ||||||||
| > > |
| |||||||
Revision 142018-08-22 - MansiKasliwal
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 41 to 41 | ||||||||
| Student: Jacob Jencson Supervisor: Mansi Kasliwal | ||||||||
| Added: | ||||||||
| > > | 5) Gap Transients (e.g. Calcium-rich, Ultra-stripped events) Student: Kishalay De Supervisor: Mansi Kasliwal | |||||||
SLSN related papers1) The First set of SLSNe discovered by ZTF --- leading: Lunnan | ||||||||
Revision 132018-08-08 - LinYan
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 40 to 40 | ||||||||
| 4) Obscured Supernovae Student: Jacob Jencson Supervisor: Mansi Kasliwal | ||||||||
| Added: | ||||||||
| > > |
SLSN related papers1) The First set of SLSNe discovered by ZTF --- leading: Lunnan2) LC modeling of a sample of SLSNe, including late-time photometry --- Yan et al. 3) Estimates of SLSN rates from the first year of ZTF data -- Yan, Lunnan, Perley et al. 4) From the most luminous SE SNe to SLSNe -- interested people: Yan, Fremling + .... | |||||||
Revision 122018-06-28 - MaayaneSoumagnac
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 20 to 20 | ||||||||
| 3) Unusual stripped-envelope supernovae with broad-light curves from ZTF. Lead: F. Taddia. Discovering, following and investigating a rare subclass of broad-light curve SE SNe (first discovered by iPTF) which may come from massive single progenitor stars or from lower-mass stellar progenitors powered by magnetar (e.g., iPTF15dtg). | ||||||||
| Added: | ||||||||
| > > | 4) A UV&optical survey of ZTF type IIn supernovae. Lead: Maayane Soumagnac. A survey of ~10 type IIn SNe brighter than -19. The idea is to obtain UV monitoring with Swift during the rise time, compute the temperature and radii from multiband photometry and answer the question: "what is the percentage of events involving non-spherical CSM?" (lower limit, following the methodology by Soumagnac et al 2018, in preparation). | |||||||
Thesis projects1) UV observations of SNe (in the context of ULTRASAT and previous work with GALEX) | ||||||||
Revision 112018-06-28 - AvishayGalyam
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 6 to 6 | ||||||||
| 2) Superluminous Supernovae (contact: Lin Yan) | ||||||||
| Changed: | ||||||||
| < < | 3) Infant Supernovae (contact: ??) | |||||||
| > > | 3) Infant Supernovae (contact: Avishay Gal-Yam) | |||||||
Postdoc projects | ||||||||
Revision 102018-02-21 - RagnhildLunnan
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
| ||||||||
| Changed: | ||||||||
| < < | Science Programs & Corresponding Filters | |||||||
| > > | Marshal Science Programs & Corresponding Filters | |||||||
| 1) Fast Transients (contact: Anna Ho) | ||||||||
| Added: | ||||||||
| > > | 2) Superluminous Supernovae (contact: Lin Yan) 3) Infant Supernovae (contact: ??) | |||||||
Postdoc projects | ||||||||
Revision 92018-02-14 - AnnaHo
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
| ||||||||
| Added: | ||||||||
| > > | Science Programs & Corresponding Filters1) Fast Transients (contact: Anna Ho) | |||||||
Postdoc projects1) Polarimetry of young SNe: | ||||||||
Revision 82017-11-15 - MansiKasliwal
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
Postdoc projects | ||||||||
| Line: 26 to 26 | ||||||||
| Student: Anna Ho Supervisor: Shri Kulkarni | ||||||||
| Changed: | ||||||||
| < < | -- SteveSchulze - 08 Nov 2017 | |||||||
| > > | 4) Obscured Supernovae Student: Jacob Jencson Supervisor: Mansi Kasliwal | |||||||
Revision 72017-11-15 - BradCenko
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
Postdoc projects | ||||||||
Revision 62017-11-15 - YiYang
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
Postdoc projects1) Polarimetry of young SNe: | ||||||||
| Changed: | ||||||||
| < < | Spectro- and imaging polarimetry and of young SNe (VLT program and Liverpool Telescope, proposals submitted) | |||||||
| > > | Spectro- and imaging polarimetry of young SNe (VLT program and Liverpool Telescope, proposals submitted) | |||||||
| Lead: Yi Yang (Weizmann Institute) 2) Stripped-envelope supernovae from ZTF. Lead: C. Barbarino, F. Taddia, L. Tartaglia. | ||||||||
Revision 52017-11-15 - YiYang
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
Postdoc projects | ||||||||
| Changed: | ||||||||
| < < | 1) Polarimetry of young CCSNe Spectro- and imaging polarimetry and of young SNe (VLT program) | |||||||
| > > | 1) Polarimetry of young SNe: Spectro- and imaging polarimetry and of young SNe (VLT program and Liverpool Telescope, proposals submitted) | |||||||
| Lead: Yi Yang (Weizmann Institute) 2) Stripped-envelope supernovae from ZTF. Lead: C. Barbarino, F. Taddia, L. Tartaglia. | ||||||||
Revision 42017-11-15 - FrancescoTaddia
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
Postdoc projects | ||||||||
| Line: 6 to 6 | ||||||||
| Spectro- and imaging polarimetry and of young SNe (VLT program) Lead: Yi Yang (Weizmann Institute) | ||||||||
| Changed: | ||||||||
| < < | 2) Stripped-envelope supernovae from ZTF. Lead: C. Barbarino, F. Taddia L. Tartaglia. | |||||||
| > > | 2) Stripped-envelope supernovae from ZTF. Lead: C. Barbarino, F. Taddia, L. Tartaglia. | |||||||
| Photometric and spectral characterisation of the various samples of stripped-envelope supernovae from ZTF, including supernovae Ib, Ic, Ic-bL (and IIb?). 3) Unusual stripped-envelope supernovae with broad-light curves from ZTF. Lead: F. Taddia. | ||||||||
Revision 32017-11-13 - FrancescoTaddia
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
Postdoc projects | ||||||||
| Line: 6 to 6 | ||||||||
| Spectro- and imaging polarimetry and of young SNe (VLT program) Lead: Yi Yang (Weizmann Institute) | ||||||||
| Added: | ||||||||
| > > | 2) Stripped-envelope supernovae from ZTF. Lead: C. Barbarino, F. Taddia L. Tartaglia. Photometric and spectral characterisation of the various samples of stripped-envelope supernovae from ZTF, including supernovae Ib, Ic, Ic-bL (and IIb?). 3) Unusual stripped-envelope supernovae with broad-light curves from ZTF. Lead: F. Taddia. Discovering, following and investigating a rare subclass of broad-light curve SE SNe (first discovered by iPTF) which may come from massive single progenitor stars or from lower-mass stellar progenitors powered by magnetar (e.g., iPTF15dtg). | |||||||
Thesis projects1) UV observations of SNe (in the context of ULTRASAT and previous work with GALEX) | ||||||||
Revision 22017-11-08 - AnnaHo
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
| ||||||||
| Deleted: | ||||||||
| < < | ||||||||
Postdoc projects1) Polarimetry of young CCSNe | ||||||||
| Line: 17 to 16 | ||||||||
| 2) Rapid spectroscopy Supervisor: Avishay Gal-Yam (Weizmann Institute) | ||||||||
| Added: | ||||||||
| > > | 3) Afterglows of Relativistic Explosions Student: Anna Ho Supervisor: Shri Kulkarni | |||||||
| -- SteveSchulze - 08 Nov 2017 | ||||||||
Revision 12017-11-08 - SteveSchulze
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
| Added: | ||||||||
| > > |
Postdoc projects1) Polarimetry of young CCSNe Spectro- and imaging polarimetry and of young SNe (VLT program) Lead: Yi Yang (Weizmann Institute)Thesis projects1) UV observations of SNe (in the context of ULTRASAT and previous work with GALEX) Plan is to pursue a sample of SNe observed early on with ground + Swift UV. Goal is statistics of UV signals (strength, duration) and demographics of progenitors (radii, explosion energies, CSM?)\n Student: Noam Ganot Supervisor: Avishay Gal-Yam (Weizmann Institute) 2) Rapid spectroscopy Supervisor: Avishay Gal-Yam (Weizmann Institute) -- SteveSchulze - 08 Nov 2017 | |||||||
View topic | History: r40 < r39 < r38 < r37 | More topic actions...
Copyright © 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