The ESO proposals are in.
Got two in. Hectic. Of course I had plenty more ideas. Most productive thing I did was kill one off. Straight down. It was technically feasible but I could not fathom a good scientific reason to do it!
This often happens; there is a good project but not a clear scientific reason to do it. Then one should not write the proposal of course.
Now it is back to high-redshift galaxies. And I shaved off the proposal beard.
Friday, March 28, 2014
Tuesday, March 11, 2014
ESO, TOP, ERC and HST applications/proposals
There are some opportunities coming up: TOP grants to get 2-3 years of postdoc funding, European ERC funding for same and then I will need to apply for ESO and HST observing time.
So. gimme cash and gimme time!
quite a number of these new pieces of prose are about occulting galaxies. Matt is pushing me to publish some of this as the white paper on what we'll do with all these overlapping pairs. I just might. A&A? Just plonk it on astro-ph? no idea really.
So. gimme cash and gimme time!
quite a number of these new pieces of prose are about occulting galaxies. Matt is pushing me to publish some of this as the white paper on what we'll do with all these overlapping pairs. I just might. A&A? Just plonk it on astro-ph? no idea really.
Sunday, March 9, 2014
SOFIA in the hangar good/bad?
Part of the NASA FY2015 budget is more priority for WFIRST (yay) and the plan to put SOFIA into a hangar for most of the year following its upgrade this summer (boo?).
I'm still in two minds about this. In some ways SOFIA is deplorably late in getting started. Much of the low-hanging
Plus I would like to see my NHEMESES follow-up program with SOFIA get done.
Preferably with me in the guest observing chair.
But a useful titbit to know is that SOFIA costs about 300k/hour of observing. You can get to space for that. Suddenly rolling it into a hangar and not having it cost this much sounds way more sensible.
However, the NASA budget is not a zero-sum game. And that 300k needs to come down. Maybe the threat of mothballing will get that done.
Also: move over, I want to fly this thing!
Thursday, March 6, 2014
Spring Cleaning of the Hopper
There are still several papers in the Hopper that need to get out. I was very happy that the M-dwarf/BoRG paper appeared. It feels like the last word on star-selection with sextractor in HST imaging. And it might be. Who knows? And the idea-that-went-in-a-drawer-for-years is now a manuscript and off to MNRAS.
But still, there is the S4G morphology paper part II to rewrite, there is a cool paper with Rychard approaching completion, I have a draft(ish) thing for using the M-dwarfs to register JWST imaging, the Dustlanes in GalaxyZoo paper needs a final check and it can go off, the Andromeda Project background galaxies paper needs an update and collaboration feedback, and the NHEMESES and LADUMA survey papers need one final push. Oh and I have a paper on NGC 891. Like you do.
So yeah. those are all at the 90% level. Just need to do the "other" 90% of the effort. Time for some spring cleaning!
But still, there is the S4G morphology paper part II to rewrite, there is a cool paper with Rychard approaching completion, I have a draft(ish) thing for using the M-dwarfs to register JWST imaging, the Dustlanes in GalaxyZoo paper needs a final check and it can go off, the Andromeda Project background galaxies paper needs an update and collaboration feedback, and the NHEMESES and LADUMA survey papers need one final push. Oh and I have a paper on NGC 891. Like you do.
So yeah. those are all at the 90% level. Just need to do the "other" 90% of the effort. Time for some spring cleaning!
Monday, March 3, 2014
The SNIa prior
Finally completed a project I had in the back of my head ever since I heard of the SDSS-II Supernova program. The idea was: can you use the inferred extinction (AV) from SNIa lightcurve fits to probe the dusty ISM of the host galaxies. It is tied to the prior for the AV in those lightcurve fit.
I explored how the AV distribution depends on host galaxy properties and one thing pops out immediately: the host galaxy disk's inclination is IMPORTANT! Other properties not as much.
Well the paper is done. Off the MNRAS. Hope my point is helpful for future supernova work.
In other news: Lorentz Center SED workshop is taking off. hurray!
I explored how the AV distribution depends on host galaxy properties and one thing pops out immediately: the host galaxy disk's inclination is IMPORTANT! Other properties not as much.
Well the paper is done. Off the MNRAS. Hope my point is helpful for future supernova work.
In other news: Lorentz Center SED workshop is taking off. hurray!
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