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 | ||||||||
Changed: | ||||||||
< < |
| |||||||
> > |
| |||||||
|
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
Marshal Science Programs & Corresponding Filters | ||||||||
Line: 17 to 17 | ||||||||
Postdoc projects
| ||||||||
Changed: | ||||||||
< < |
| |||||||
> > |
| |||||||
Thesis projects |
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
Marshal Science Programs & Corresponding Filters | ||||||||
Line: 18 to 17 | ||||||||
Postdoc projects
| ||||||||
Changed: | ||||||||
< < |
| |||||||
> > |
| |||||||
| ||||||||
Deleted: | ||||||||
< < | ||||||||
Thesis projects
|
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
Marshal Science Programs & Corresponding Filters | ||||||||
Line: 25 to 25 | ||||||||
Thesis projects
| ||||||||
Added: | ||||||||
> > |
| |||||||
|
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
Marshal Science Programs & Corresponding Filters | ||||||||
Line: 13 to 13 | ||||||||
| ||||||||
Added: | ||||||||
> > |
| |||||||
Postdoc projects |
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
Marshal Science Programs & Corresponding Filters | ||||||||
Line: 25 to 25 | ||||||||
| ||||||||
Added: | ||||||||
> > |
| |||||||
-- ThomasKupfer - 10 Apr 2018 \ No newline at end of file |
Line: 1 to 1 | ||||||||
---|---|---|---|---|---|---|---|---|
Marshal Science Programs & Corresponding Filters | ||||||||
Line: 11 to 11 | ||||||||
General projects | ||||||||
Added: | ||||||||
> > |
| |||||||
Postdoc 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 |