
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
FRITZ Marshal Corresponding Filters | ||||||||
| Line: 38 to 38 | ||||||||
Characterizing Cataclysmic Variables | ||||||||
| Changed: | ||||||||
| < < |
| |||||||
| > > |
| |||||||
Close binaries at the centre of planetary nebulae
| ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
FRITZ Marshal Corresponding Filters | ||||||||
| Line: 70 to 70 | ||||||||
| ||||||||
| Changed: | ||||||||
| < < | White dwarf with transiting debris
| |||||||
| > > | White dwarfs with transiting planetary debris
| |||||||
LISA Gravitational Wave Sources in ZTF
| ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
FRITZ Marshal Corresponding Filters | ||||||||
| Line: 34 to 34 | ||||||||
Calibration of period-luminosity relations using ZTF observed globular clusters
| ||||||||
| Changed: | ||||||||
| < < |
| |||||||
| > > |
| |||||||
| ||||||||
| Changed: | ||||||||
| < < |
| |||||||
| > > |
| |||||||
Characterizing Cataclysmic Variables
| ||||||||
| Line: 55 to 55 | ||||||||
Student Thesis projects | ||||||||
| Added: | ||||||||
| > > |
| |||||||
| ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
FRITZ Marshal Corresponding Filters | ||||||||
| Line: 49 to 49 | ||||||||
| ||||||||
| Changed: | ||||||||
| < < | ||||||||
| > > | Searches for self-lensing compact object binaries with ZTF
| |||||||
Student Thesis projects
| ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
FRITZ Marshal Corresponding Filters | ||||||||
| Line: 41 to 41 | ||||||||
| ||||||||
| Added: | ||||||||
| > > | Close binaries at the centre of planetary nebulae
Identification of AR Sco type objects with ZTF
| |||||||
| Deleted: | ||||||||
| < < | ||||||||
Student Thesis projects
| ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
FRITZ Marshal Corresponding Filters | ||||||||
| Line: 6 to 6 | ||||||||
| CVs/dwarf novae outbursts (Szkody/vanRoestel) | ||||||||
| Changed: | ||||||||
| < < | Xrays sources watchlist (Bellm) | |||||||
| > > | X-ray sources watchlist (Bellm/Kong) | |||||||
| Dippers (Mahabal) | ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
| ||||||||
| Changed: | ||||||||
| < < | GROWTH Marshal Science Programs & Corresponding Filters | |||||||
| > > | FRITZ Marshal Corresponding Filters | |||||||
| Young stellar objects (Hillenbrand/Kuhn) | ||||||||
| Changed: | ||||||||
| < < | CVs/dwarf novae outbursts (Szkody/Kupfer) M31 (Kupfer/Prince) | |||||||
| > > | CVs/dwarf novae outbursts (Szkody/vanRoestel) | |||||||
| Xrays sources watchlist (Bellm) | ||||||||
| Changed: | ||||||||
| < < | O'Connell binaries (Graham, Drake)
(ML) Classification of variable objects | |||||||
| > > | Dippers (Mahabal) | |||||||
| Changed: | ||||||||
| < < |
| |||||||
| > > | AM CVn (vanRoestel/Szkody)
'Dippers'
Searching for Boyajian's Star Analogs
O'Connol binaries
(ML) Classification of variable objects
| |||||||
Searches for state-changing X-ray binaries
| ||||||||
| Deleted: | ||||||||
| < < | Searches for counterparts to Fermi unassociated sources
Stellar flare occurance rates
| |||||||
Calibration of period-luminosity relations using ZTF observed globular clusters | ||||||||
| Deleted: | ||||||||
| < < | ||||||||
| ||||||||
| Line: 35 to 38 | ||||||||
Characterizing Cataclysmic Variables | ||||||||
| Changed: | ||||||||
| < < |
| |||||||
| > > |
| |||||||
| ||||||||
| Changed: | ||||||||
| < < |
Searching for Boyajian's Star Analogs
| |||||||
| > > |
| |||||||
Student Thesis projects | ||||||||
| Line: 49 to 49 | ||||||||
| ||||||||
| Deleted: | ||||||||
| < < | LISA Gravitational Wave Sources in ZTF
| |||||||
A search for compact objects with ZTF
Postdoc projects | ||||||||
| Added: | ||||||||
| > > | Searches for counterparts to Fermi unassociated sources
White dwarf with transiting debris
LISA Gravitational Wave Sources in ZTF
| |||||||
The population of short period hot subdwarfs/helium stars using ZTF lightcurves | ||||||||
| Deleted: | ||||||||
| < < | ||||||||
| ||||||||
| Line: 68 to 74 | ||||||||
| ||||||||
| Changed: | ||||||||
| < < | The population of eclipsing white dwarfs (dWD, WD+MS) | |||||||
| > > | The population of eclipsing white dwarfs (dWD, WD+RD/BD) | |||||||
| ||||||||
| Changed: | ||||||||
| < < | A search for eclipsing planetisimals around white dwarfs
RR Lyrae Discovery in ALert Stream and Lightcurve ~ (photometric) metallicity Relation
| |||||||
| > > | AMCVn binaries
| |||||||
Radial velocity followup of PS1 RR Lyrae
| ||||||||
| Line: 98 to 100 | ||||||||
| ||||||||
| Added: | ||||||||
| > > | Microlensing events
OLD PROJECTSStellar flare occurance rates
RR Lyrae Discovery in ALert Stream and Lightcurve ~ (photometric) metallicity Relation
A search for eclipsing planetisimals around white dwarfs
| |||||||
| ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
GROWTH Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 16 to 16 | ||||||||
| ||||||||
| Deleted: | ||||||||
| < < | (ML) Alert Stream Classification
| |||||||
Searches for state-changing X-ray binaries
Searches for counterparts to Fermi unassociated sources | ||||||||
| Changed: | ||||||||
| < < |
| |||||||
| > > |
| |||||||
Stellar flare occurance rates | ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
GROWTH Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 21 to 21 | ||||||||
Searches for state-changing X-ray binaries | ||||||||
| Changed: | ||||||||
| < < |
| |||||||
| > > |
| |||||||
Searches for counterparts to Fermi unassociated sources | ||||||||
| Line: 98 to 98 | ||||||||
| ||||||||
| Changed: | ||||||||
| < < |
-- ThomasKupfer - 10 Apr 2018
| |||||||
| > > | Stochastic Variability of Galactic XRBs
| |||||||
| ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
GROWTH Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 37 to 37 | ||||||||
| ||||||||
| Added: | ||||||||
| > > |
| |||||||
Characterizing Cataclysmic Variables
| ||||||||
| Line: 49 to 50 | ||||||||
Student Thesis projects
| ||||||||
| Added: | ||||||||
| > > |
| |||||||
LISA Gravitational Wave Sources in ZTF | ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
GROWTH Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 10 to 10 | ||||||||
| Xrays sources watchlist (Bellm) | ||||||||
| Added: | ||||||||
| > > | O'Connell binaries (Graham, Drake) | |||||||
(ML) Classification of variable objects
| ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
GROWTH Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 31 to 31 | ||||||||
| ||||||||
| Changed: | ||||||||
| < < | Calibration of RR Lyrae period-luminosity relations using ZTF observed globular clusters | |||||||
| > > | Calibration of period-luminosity relations using ZTF observed globular clusters | |||||||
| ||||||||
| Changed: | ||||||||
| < < |
| |||||||
| > > |
| |||||||
Characterizing Cataclysmic Variables
| ||||||||
| Line: 47 to 47 | ||||||||
Student Thesis projects | ||||||||
| Changed: | ||||||||
| < < |
| |||||||
| > > |
| |||||||
LISA Gravitational Wave Sources in ZTF | ||||||||
| Line: 88 to 87 | ||||||||
| ||||||||
| Deleted: | ||||||||
| < < |
Be stars Variability
| |||||||
Searching and Characterising Pulsar Binaries
| ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
GROWTH Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 40 to 40 | ||||||||
| ||||||||
| Deleted: | ||||||||
| < < |
Searching and Characterising Pulsar Binaries
| |||||||
Searching for Boyajian's Star Analogs
| ||||||||
| Line: 100 to 94 | ||||||||
| ||||||||
| Changed: | ||||||||
| < < | ||||||||
| > > | Searching and Characterising Pulsar Binaries
| |||||||
Cepheids
| ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
GROWTH Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 63 to 63 | ||||||||
| ||||||||
| Added: | ||||||||
| > > | A search for compact objects with ZTF
| |||||||
Postdoc projectsThe population of short period hot subdwarfs/helium stars using ZTF lightcurves | ||||||||
| Line: 80 to 85 | ||||||||
| ||||||||
| Deleted: | ||||||||
| < < |
A search for compact objects with ZTF
| |||||||
RR Lyrae Discovery in ALert Stream and Lightcurve ~ (photometric) metallicity Relation
| ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
GROWTH Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 60 to 60 | ||||||||
LISA Gravitational Wave Sources in ZTF
| ||||||||
| Changed: | ||||||||
| < < |
| |||||||
| > > |
| |||||||
Postdoc projects | ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
GROWTH Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 41 to 41 | ||||||||
| ||||||||
| Added: | ||||||||
| > > | Searching and Characterising Pulsar Binaries
| |||||||
Searching for Boyajian's Star Analogs
| ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
GROWTH Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 97 to 97 | ||||||||
| ||||||||
| Added: | ||||||||
| > > | Cepheids
| |||||||
| -- ThomasKupfer - 10 Apr 2018 | ||||||||
| Changed: | ||||||||
| < < |
| |||||||
| > > |
| |||||||
| ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
GROWTH Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 98 to 98 | ||||||||
| ||||||||
| Added: | ||||||||
| > > |
| |||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
GROWTH Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 41 to 41 | ||||||||
| ||||||||
| Added: | ||||||||
| > > | Searching for Boyajian's Star Analogs
| |||||||
Student Thesis projects
| ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
GROWTH Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 43 to 43 | ||||||||
Student Thesis projects | ||||||||
| Changed: | ||||||||
| < < |
| |||||||
| > > |
| |||||||
| ||||||||
| Deleted: | ||||||||
| < < |
| |||||||
LISA Gravitational Wave Sources in ZTF | ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
GROWTH Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 63 to 63 | ||||||||
The population of eclipsing white dwarfs (dWD, WD+MS) | ||||||||
| Changed: | ||||||||
| < < |
| |||||||
| > > |
| |||||||
A search for eclipsing planetisimals around white dwarfs
| ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
GROWTH Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 24 to 24 | ||||||||
Searches for counterparts to Fermi unassociated sources | ||||||||
| Changed: | ||||||||
| < < |
| |||||||
| > > |
| |||||||
Stellar flare occurance rates | ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
GROWTH Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 20 to 20 | ||||||||
Searches for state-changing X-ray binaries | ||||||||
| Changed: | ||||||||
| < < |
| |||||||
| > > |
| |||||||
Searches for counterparts to Fermi unassociated sources | ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
GROWTH Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 83 to 84 | ||||||||
| ||||||||
| Added: | ||||||||
| > > | Radial velocity followup of PS1 RR Lyrae
| |||||||
Be stars Variability
| ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
GROWTH Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 15 to 15 | ||||||||
| ||||||||
| Added: | ||||||||
| > > | (ML) Alert Stream Classification
| |||||||
Searches for state-changing X-ray binaries
| ||||||||
| Line: 74 to 78 | ||||||||
| ||||||||
| Changed: | ||||||||
| < < | RR lyrae period-metallicity
| |||||||
| > > | RR Lyrae Discovery in ALert Stream and Lightcurve ~ (photometric) metallicity Relation
| |||||||
Be stars Variability
| ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
GROWTH Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 42 to 42 | ||||||||
| ||||||||
| Changed: | ||||||||
| < < |
| |||||||
| > > |
| |||||||
LISA Gravitational Wave Sources in ZTF | ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
GROWTH Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 10 to 10 | ||||||||
| Xrays sources watchlist (Bellm) | ||||||||
| Deleted: | ||||||||
| < < | General projects/Group projects
| |||||||
(ML) Classification of variable objects
| ||||||||
| Changed: | ||||||||
| < < | ||||||||
| > > | Searches for state-changing X-ray binaries
Searches for counterparts to Fermi unassociated sources
Stellar flare occurance rates
| |||||||
Calibration of RR Lyrae period-luminosity relations using ZTF observed globular clusters
| ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
| ||||||||
| Changed: | ||||||||
| < < | GROWTH Marshal Science Programs & Corresponding Filters | |||||||
| > > | GROWTH Marshal Science Programs & Corresponding Filters | |||||||
| Young stellar objects (Hillenbrand/Kuhn) | ||||||||
| Line: 10 to 10 | ||||||||
| Xrays sources watchlist (Bellm) | ||||||||
| Changed: | ||||||||
| < < | General projects | |||||||
| > > | General projects/Group projects | |||||||
| ||||||||
| Added: | ||||||||
| > > | ||||||||
| ||||||||
| Changed: | ||||||||
| < < |
(ML) Classification of variable objects | |||||||
| > > |
(ML) Classification of variable objects | |||||||
| ||||||||
| Changed: | ||||||||
| < < | Calibration of RR Lyrae period-luminosity relations using ZTF observed globular clusters | |||||||
| > > | Calibration of RR Lyrae period-luminosity relations using ZTF observed globular clusters | |||||||
| ||||||||
| Changed: | ||||||||
| < < | Characterizing Cataclysmic Variables | |||||||
| > > | Characterizing Cataclysmic Variables | |||||||
| ||||||||
| Changed: | ||||||||
| < < | Thesis projects | |||||||
| > > |
Student Thesis projects | |||||||
| ||||||||
| Changed: | ||||||||
| < < | LISA Gravitational Wave Sources in ZTF | |||||||
| > > | LISA Gravitational Wave Sources in ZTF | |||||||
| ||||||||
| Changed: | ||||||||
| < < | Postdoc projects | |||||||
| > > | Postdoc projects | |||||||
| Changed: | ||||||||
| < < | The population of short period hot subdwarfs/helium stars using ZTF lightcurves | |||||||
| > > | The population of short period hot subdwarfs/helium stars using ZTF lightcurves | |||||||
| ||||||||
| Changed: | ||||||||
| < < | The population of eclipsing white dwarf - main sequence/planet(isimals) | |||||||
| > > | The population of eclipsing white dwarfs (dWD, WD+MS) | |||||||
| ||||||||
| Changed: | ||||||||
| < < | A search for compact objects with ZTF | |||||||
| > > | A search for eclipsing planetisimals around white dwarfs
A search for compact objects with ZTF | |||||||
| ||||||||
| Changed: | ||||||||
| < < | Be stars Variability | |||||||
| > > |
RR lyrae period-metallicity
Be stars Variability | |||||||
| ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
GROWTH Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 8 to 8 | ||||||||
| M31 (Kupfer/Prince) | ||||||||
| Added: | ||||||||
| > > | Xrays sources watchlist (Bellm) | |||||||
General projects
| ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
GROWTH Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 13 to 13 | ||||||||
| ||||||||
| Changed: | ||||||||
| < < | (ML) Classification of variable stars | |||||||
| > > | (ML) Classification of variable objects | |||||||
| Changed: | ||||||||
| < < |
| |||||||
| > > |
| |||||||
Calibration of RR Lyrae period-luminosity relations using ZTF observed globular clusters | ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
GROWTH Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 24 to 24 | ||||||||
| ||||||||
| Changed: | ||||||||
| < < | ||||||||
| > > | Characterizing Cataclysmic Variables
| |||||||
Thesis projects
| ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
GROWTH Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 15 to 15 | ||||||||
(ML) Classification of variable stars | ||||||||
| Changed: | ||||||||
| < < |
| |||||||
| > > |
| |||||||
| ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
GROWTH Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 19 to 19 | ||||||||
| ||||||||
| Added: | ||||||||
| > > | Calibration of RR Lyrae period-luminosity relations using ZTF observed globular clusters
| |||||||
Thesis projects
| ||||||||
| Line: 51 to 57 | ||||||||
| ||||||||
| Changed: | ||||||||
| < < | Be stars
| |||||||
| > > | Be stars Variability
| |||||||
| ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
GROWTH Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 16 to 16 | ||||||||
(ML) Classification of variable stars
| ||||||||
| Changed: | ||||||||
| < < |
| |||||||
| > > |
| |||||||
Thesis projects | ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
GROWTH Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 15 to 15 | ||||||||
(ML) Classification of variable stars | ||||||||
| Changed: | ||||||||
| < < |
| |||||||
| > > |
| |||||||
Thesis projects | ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
GROWTH Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 24 to 24 | ||||||||
| ||||||||
| Deleted: | ||||||||
| < < |
| |||||||
| ||||||||
| Added: | ||||||||
| > > | LISA Gravitational Wave Sources in ZTF
| |||||||
Postdoc projectsThe population of short period hot subdwarfs/helium stars using ZTF lightcurves | ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
GROWTH Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 41 to 41 | ||||||||
| ||||||||
| Added: | ||||||||
| > > | A search for compact objects with ZTF
| |||||||
Be stars
| ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
GROWTH Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 16 to 16 | ||||||||
(ML) Classification of variable stars
| ||||||||
| Changed: | ||||||||
| < < |
| |||||||
| > > |
| |||||||
Thesis projects | ||||||||
| Line: 37 to 37 | ||||||||
The population of eclipsing white dwarf - main sequence/planet(isimals) | ||||||||
| Changed: | ||||||||
| < < |
| |||||||
| > > |
| |||||||
Be stars | ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
| ||||||||
| Changed: | ||||||||
| < < | Marshal Science Programs & Corresponding Filters | |||||||
| > > | GROWTH Marshal Science Programs & Corresponding Filters | |||||||
| Young stellar objects (Hillenbrand/Kuhn) | ||||||||
| Line: 13 to 13 | ||||||||
| ||||||||
| Added: | ||||||||
| > > | (ML) Classification of variable stars
| |||||||
Thesis projects | ||||||||
| Line: 34 to 39 | ||||||||
| ||||||||
| Changed: | ||||||||
| < < |
| |||||||
| > > |
| |||||||
Be stars
| ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 30 to 30 | ||||||||
| ||||||||
| Added: | ||||||||
| > > | The population of eclipsing white dwarf - main sequence/planet(isimals)
| |||||||
Be stars
| ||||||||
| Deleted: | ||||||||
| < < |
| |||||||
| ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 8 to 8 | ||||||||
| M31 (Kupfer/Prince) | ||||||||
| Changed: | ||||||||
| < < | General projects | |||||||
| > > | General projects | |||||||
| ||||||||
| Changed: | ||||||||
| < < | Postdoc projects
Thesis projects | |||||||
| > > | Thesis projects | |||||||
| ||||||||
| Line: 28 to 22 | ||||||||
| ||||||||
| Added: | ||||||||
| > > | Postdoc projectsThe population of short period hot subdwarfs/helium stars using ZTF lightcurves
Be stars
| |||||||
| -- ThomasKupfer - 10 Apr 2018 | ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 18 to 18 | ||||||||
| ||||||||
| Changed: | ||||||||
| < < |
| |||||||
| > > |
| |||||||
Thesis projects | ||||||||
| Line: 1 to 1 | ||||||||
|---|---|---|---|---|---|---|---|---|
Marshal Science Programs & Corresponding Filters | ||||||||
| Line: 22 to 22 | ||||||||
Thesis projects | ||||||||
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Marshal Science Programs & Corresponding FiltersYoung stellar objects (Hillenbrand/Kuhn) CVs/dwarf novae outbursts (Szkody/Kupfer)Postdoc projectsThesis projects-- ThomasKupfer - 10 Apr 2018 | |||||||