They say dress for the job you want... so it's a good thing this Princeton T-shirt that I got as a prospective graduate student in 2017 has been a regular in my rotation. I am thrilled to share that I will be joining
@PrincetonPhys
as an Assistant Professor in Fall 2025!
I passed my oral exam and am officially a PhD candidate! Which means I can stop worrying about the opacity of protostars on the Hayashi track and the spectrum of E-modes of the CMB and go back to worrying about gravitational waves!
If you've heard me talk about "secret LIGO work" over the last several months, I'm super excited to finally be able to share the discovery of GW230529: the first observation of a mass-gap object merging with a neutron star!
Image:
@astronerdika
1/7
Excited to finally share that I will be a
@NASA
Einstein fellow
@NUCIERA
in the fall! Grateful for the opportunity to keep listening to the Universe with gravitational waves, and looking forward to meeting the other amazing fellows in my cohort!
@KyleMorgenstein
You actually can’t be on the student subscription for more than four years as I am sadly learning this year! Even with a different university email, as long as it’s associated with the same account ☹️
Any other GW data analysis folks feel like we’re in a weird limbo between physics and astronomy? I’m not really a theorist or experimentalist but also definitely not an observational astronomer in the traditional sense… makes it hard to understand where we fit in
Grateful for the opportunity to represent gravitational waves at
#HEAD20
in Hawaii with my talk on how we can use future observations with
@LISACommunity
to probe tides in double white dwarfs!
1/4
My first first-author paper is on the arXiv today!
With
@sasomao
and
@CJHaster
we investigated how well the chirp mass of binary neutron stars can be determined by low latency gravitational wave searches 1/n
The universe listened to my plea - and gave us an NSBH! Online PE finished in about half an hour and we got the skymap out promptly after that. Sorry for the 25000 deg^2 sky localization 😅
The universe likes to wait until I’m on the PE ROTA to give us potentially EM-bright sources! Check out these classifications and the updated skymap I just sent out:
🚨 An exciting one!
#GravitationalWave
candidate
#S240422ed
If real, the source is probably a neutron star–black hole (could have an electromagnetic counterpart)
False alarm rate 1 in 10^5 yr
GraceDB
GCN
Rating 🍫🎱🥯
#O4IsHere
Today Nobel Laureate Rai Weiss saw me walk into the office with my violin and asked me if I wanted to play the Mozart Violin Sonatas with him on piano. That is all.
Katerina Chatziioannou shares exciting new results from
@LIGO
at
#AAS235
- the detection of the second binary neutron star merger
#GW190425
with the heaviest total mass of any known double neutron star system!
Cheesin hard while presenting my work on gravitational-wave astronomy with
@LIGO
-
@ego_virgo
during my dissertation talk at
#AAS241
including correlations in the binary black hole spin distribution and multimessenger prospects of neutron star-black hole mergers
Do you often find yourself wondering why binary black hole component spins are so hard to measure? Are you despondent about the fact that the spins of LIGO-Virgo black holes seem to be small? Then may be for you!
Excited to be
@astronomy2024
this week in Cape Town (local penguins below)! Catch me tomorrow morning during the 1st plenary session presenting the latest results from
@LIGO
-
@ego_virgo
-
@KAGRA_PR
, and check out the corresponding GW230529 paper now in ApJL:
Kicking off Thursday
@APSMeetings
with an engaging session on Population Inference of Gravitational Wave Sources!
First up,
@ColmMTalbot
presenting an alternative, entropy-based approach to standard hierarchical inference working directly with strain instead of posterior samples
Alas, during O3a I was on the parameter estimation ROTA four times and all my events were either sub-threshold or glitches, and now when I was next up on the ROTA for O3b, the run is suspended... suspicious? 🤔
Choosing which waveform model to use for gravitational-wave data analysis remains a contentious question even after 20 years… as Alessandra Buonanno tells us at the 25th anniversary lecture of the effective one-body approach at the LVK meeting
@LSUphysastro
@LIGO
@ego_virgo
Since
@astronerdika
can’t tweet while she’s presenting, here she is telling us about the best models to use for the binary black hole spin distribution at
#GWPAW22
I had a busy day
@APSMeetings
yesterday, starting with my thesis talk in the Cecilia Payne Gaposchkin Dissertation Award Finalist Session. Check out the summary of my talk in this
@astrobites
article!
My professional website is now up, check it out (especially if you’ve been looking for an easy condor tutorial)!
And if you’ve been needing some encouragement to make your own: you, too, can learn just enough html to edit a website template!
I just sent a GCN circular for an LVK event! It's an updated skymap for last week's BBH event obtained using full parameter estimation. Sort of wild that I have this power...
A team led by Physics grad student Sylvia Biscoveanu has developed a method to tease out the very faint signals of primordial ripples from gravitational-wave data.
@ScienceMIT
@MITKavli
@sylvia_bisco
Nothing like looking back at code you wrote five years ago to find that it’s actually really clever and well commented and you can reuse it for a new project 😌
Apparently at THE
@MIT_ISTnews
there is no native way to set up automatic out of office emails with exceptions for certain addresses… so you heard it here first that I’m taking time off before starting my postdoc in September!
Ciao from Venice 👋
If you’ve ever been curious about the nitty gritty details of the statistical properties of LIGO noise, check out my talk today on the effect of PSD uncertainty on GW parameter estimation at
@ipam_ucla
(recording and slides👇)
Lively discussion on how to access stochastic backgrounds in next-generation ground-based GW detectors like
@CosmicExpGW
in the presence of astrophysical foregrounds at this evening’s session at
#gwpopnext
. We look forward to learning a lot from
@LISACommunity
#teamglobalfit
Excited to share my new paper () with
@ColmMTalbot
@EHThrane
@SuperSymmetric1
because it means I get to do a 🧵 on stochastic gravitational-wave backgrounds, which have the potential to reveal information about the early Universe! 1/n
Lots of interesting talks at the April
@APSMeetings
on gravitational-wave populations! First up,
@EdelmanBruce
telling us about non-parametric inference of the BBH mass distribution.
Quick little thread on a quick little research note that will likely be my last work with my MIT affiliation… Have you been wondering how many gamma-ray bursts come from neutron star-black hole mergers?
1/3
If you like gamma-ray bursts, relativistic jets, neutron stars, gravitational waves, or hierarchical Bayesian inference check out my new paper with Eric Thrane and
@sasomao
! 1/n
New preprint on the arXiv with
@sasomao
,
@CJHaster
, and undergrad Jonathan Davies, investigating how the uncertainty in the gravitational wave detector noise properties affects the parameters we infer for compact binaries observed by
@LIGO
1/n
Excited to finally share a new paper on the kilonova discovery potential of the Wide-field Infrared Transient Explorer (WINTER):
with Danielle Frostig,
@gmo_omg
, Viraj Karambelkar,
@sasomao
and others
@MITKavli
,
@PMACaltech
, and
@IJCLab
1/4
🚨New paper on the arXiv today with
@ColmMTalbot
and
@sasomao
about how you can get the binary neutron star mass distribution wrong with gravitational wave measurements if you mismodel the spin:
Feeling very inspired after three days of discussion on the future of GW astronomy at the PAX workshop! Thanks to SOC
@sasomao
@SuperSymmetric1
& Sarah Caudill for the opportunity to share my vision for a fully Bayesian approach to data analysis in the future with
@CosmicExpGW
!
I will be looking to grow my group over the next couple years. If you are interested in research in gravitational-wave astronomy at Princeton as a student (undergrad or grad) or postdoc, please feel free to reach out!
This is not just the realization of a personal dream of mine, but also of the American dream. My great-great-grandmother took the shoes off her own feet so that my grandfather could go to school in rural Romania. Grateful for the support and inspiration of the
@PDSoros
community.
I led the team of
@LIGO
-
@ego_virgo
-Kagra scientists working on the analysis and paper writing of this event with
@spacedontwait
. Check out his talk
@APSMeetings
at 1:30PM PDT today for more details, or read on for the highlights!
2/7
Likelihood reweighting, aka importance sampling, is quickly becoming an important computational tool in gravitational-wave astronomy. Check out my
#toolsofthetrade
article in
@NatRevPhys
highlighting some neat applications and caveats for this technique
@sasomao
tells us about potential pitfalls in gravitational-wave population inference at
#GWPAW22
, highlighting our working showing that mismodeling the neutron star spin biases the mass inference. Misleading sub-solar mass compact objects, anyone?
Finally, the existence of equal-mass NSBH systems like this one leads to an increase in the inferred rate of NSBH systems detectable with gravitational waves that may have electromagnetic counterparts - good news for our EM observing partners following up public alerts!
7/7
I learned more astrophysics studying for my quals than I did in classes. Yes I was extremely stressed for a semester, but I personally wouldn’t have retained nearly as much with a different format. An opportunity for repeated, extended consolidation I haven’t gotten otherwise
Unpopular opinion, but I learned and reinforced a ton of physics and astrophysics by studying for my quals. It also took me multiple attempts to pass. But ... studying deeply and persevering are valuable research skills
Sylvia from 10 years ago would never have dreamed that she could end up here. I am incredibly grateful to my mentors along the way for their guidance and to my family for their continued and unwavering support.
Last week I started questioning the validity of my entire analysis due to a factor of 2 discrepancy. Turns out I was using a different value for H0 than my collaborator who simulated the data I was trying to analyze 🙃
#troublewithhubble
A tip as we enter faculty campus interview season: take a screenshot of the schedule you’ve been given with the names and room numbers for all your meetings and set it as the Lock Screen for your phone or iPad or whatever you’re carrying around with you.
Check out this awesome highlight of our work identifying a correlation between the width of the binary black hole spin distribution and redshift in
@AASNova
!
A New Spin on Binary Black Hole Evolution
Today's article might leave your head spinning — read on for an investigation into how the spins of binary black holes have changed across cosmic time!
@MITKavli
@FlatironCCA
@SBUResearch
Really excited to be
@yalecuwip
this weekend as a panelist talking about “what I wish I knew about grad school” - and great to see so many future female physicists in one place!
After five years as a student at MIT… I was not allowed to keep my student card for the memories when I went to get an employee ID card 😔 (have a temp position here until my postdoc starts in the fall)
Alas, during O3a I was on the parameter estimation ROTA four times and all my events were either sub-threshold or glitches, and now when I was next up on the ROTA for O3b, the run is suspended... suspicious? 🤔
This week we will suspend observing at
@LIGOWA
,
@LIGOLA
&
@ego_virgo
. We are working to ensure that all preparations are made for a smooth end of run. It is sad to end O3 early, but it has been a tremendously successful run, and we look forward to sharing our discoveries soon.
Do you want to learn the details of gravitational-wave data analysis from a team of experts
@MIT_Physics
? Sign up to attend our GWODW study hub next week on campus!
If you are a student/postdoc/etc in the Boston area and interested in gravitational-wave data analysis, we are organizing one of these at MIT next week. Sign up (place is limited). There is homework to do in advance! Please share!🙏
This advice holds for early career folks on the postdoc job market too. Usually the postdocs are in charge of the early career seminar series in their departments, so ask your postdoc friends/collaborators to invite you!
I have about a year before I lose my own first physics bet… maybe
@NANOGrav
will detect the SMBHB background before then and neither of us will win on a technicality 😅
So, last week I was sitting in a visitor office in the Caltech astronomy department, because one of our
@caltechipac
buildings flooded (😱). The office was in the TAPIR (Theoretical Astrophysics Including Relativity) wing, home of past greats like Roger Blandford and Kip Thorne.
@JordanBHarrod
It adopted an adult cat at the start of the second year of my PhD. I spend about $10 on dry food per month, $15 on wet food, and $15 on litter. The start-up items like carrier, bowls, litter box, food, some toys, treats, etc. cost about $150. So worth it!
@spacedontwait
opens this morning’s session at
#gwpopnext
by roasting population data analysts’ past overly optimistic predictions of our ability to distinguish binary formation channels
Here’s a nice way to visualize the correlation that we find: slices of the binary black hole effective aligned spin distribution get wider at increasing redshifts, while the uncertainty (shaded region) stays roughly the same
New paper on the ArXiv led by
@MITKavli
grad student
@sylvia_bisco
.
We look at the population of observed binary black holes (BBHs) to see if there are any correlations between the spin-mass-redshift properties of the population, and we found something!
Including this event in our analyses of the NSBH population leads to a significant decrease in the inferred minimum mass of black holes in binaries with neutron stars, from ~6 Msun to ~3 Msun!
6/7
Turned in my last assignment of my first year of grad school yesterday and I keep having residual pangs of “I should be studying right now”
#makeitstop
Does this finally resolve the internal conflict I face every time I have to pick a category for my gravitational-wave data analysis conference talks? Am I a theorist? 😲
@astrobel_rs
tells us the recipe for the perfect gravitational-wave catalog-pizza this morning at
#gwpopnext
. Data quality checks ensure it’s tasty, thresholding ensures it’s just the right size
Observations of X-ray binaries have supported the existence of a "lower mass gap" in the compact-object mass spectrum between the most massive neutron stars and least massive black holes in the range of 3-5 Msun.
3/7
This means that GW230529 is the most equal-mass NSBH merger observed to date. We find that systems like this one are at least as common as the more "vanilla" NSBH systems with more massive black holes observed in the previous observing run.
5/7
TLDR: LISA will teach us about tidal physics in white dwarfs! Check out our paper here, which has been updated to include this new section on the inference method.
4/4
Boston friends, come out on Monday to hear me talk about the cosmic symphony of gravitational waves! Currently debating if I should bring my violin for demonstration purposes...
GW230529 represents the strongest evidence for the existence of a compact object in this mass range. We infer that the mass gap object, the heavier of the two in the binary, is likely a black hole, while its companion is a neutron star.
Image:
@astronerdika
4/7
My upstairs neighbors are apparently the type of people that unironically listen to “My Heart Will Go On” on a daily basis... It’s on the same playlist as “Blue (Da Ba Dee)” that basically just loops all day 🙃
@MIT_Physics
@ScienceMIT
@NASA
@SpaceTelescope
Thanks for sharing! It’s worth also noting that another fellow in our cohort, Peter Kosec, is also currently based at MIT as a postdoc in the Kavli Institute for Astrophysics.
@sasomao
reports on evidence for an anticorrelation between the mean of the effective spin distribution and mass ratio and a correlation between the width of the distribution with redshift
Super excited to share a new paper on a topic that’s outside my usual wheelhouse - probing tidal physics with mass transferring double white dwarf binaries with
@LISACommunity
!
With Kyle Kremer and
@EHThrane
1/6
@astronerdika
continues the analogy talking about contamination. Do you want a small but pure pizza-catalog, or a large exotic pizza-catalog that may have some bad wheat-events?
You won’t need to worry about misplacing a physical printout or about pulling it up from your email before each meeting.
(Tip borrowed from wedding planning 😅)
@PotatoAsad
@sasomao
Anarya Ray shares another method to look for correlations using a binned Gaussian process, in his words “a glorified histogram” (work with
@quarkcharmer_
). They find evidence for a different chi_eff distribution for 30-40 Msun black holes compared to the bulk of the population.