Hello World!

I am a Postdoctoral Research Fellow in the First Light research group at University College London (UCL). The main focus of my research is to study the evolution of the physical properties of distant galaxies and supermassive black holes through multi-wavelength observations using state-of-the-art telescopes around the world.

I am interested in studying the nature of high-redshift (distant) galaxies that are in the very early stages of their evolution. As a member of the VANDELS and LACES collaborations, I am currently studying the underlying stellar populations and their ionising outputs in early star-forming galaxies. One of the fundamental challenges of modern astrophysics is to determine when and how the Universe made a phase transition from neutral to ionised (the epoch of reionisation), and my research is aimed at addressing this challenge.

I am also interested in studying distant active galaxies powered by active supermassive black holes in their centres. In addition to spectroscopy, I am using multi-wavelength data ranging from X-rays to radio waves to study the impact that active black holes and exotic stellar systems such as X-ray binaries have on their host galaxies and the surrounding inter-galactic medium.

I am now looking forward to using the revolutionary James Webb Space Telescope to study galaxies and active black holes in the early Universe in unparalleled detail, with two accepted proposals in Cycle 1 observations (one as Co-PI, one as Co-I)!

Research

X-ray binary (XRB) populations in high-redshift star-forming galaxies

There is growing evidence that star-forming galaxies in the early Universe drove the bulk of the reionisation of neutral hydrogen within the first billion years of the Universe's lifetime. However, it is still unclear how many ionising photons were produced by massive stars in these galaxies, and how many of these escaped into the intergalactic medium to drive reionisation. It may also be possible that a class of high-mass binary star systems, which includes a stellar mass black hole accreting material from a companion high mass star, shining brightly at X-ray wavelengths, may play a role in the production and escape of ionising photons.
My recent research has been focused on identifying and constraining the X-ray activity in very distant galaxies powered by these X-ray binary systems in a bid to constrain their overall contribution to the photon production budget of star-forming galaxies, and their eventual impact on the reionisation of the Universe. A preprint reporting the latest results from this work can be found here:
The VANDELS Survey: New constraints on the high-mass X-ray binary populations in normal star-forming galaxies at 3 < z < 5.5, 2021

Physical properties of Helium II emitting galaxies in VANDELS

Galaxies in the early Universe that emit copius amounts of Helium II are likely to be dominated by very massive stars that have very few metals. Such galaxies represent a population of the first galaxies that may have formed in the Universe, and studying large samples can reveal the physics that dominates within the earliest galaxies to appear in the Universe.
The paper reporting the Helium II emitting galaxies from VANDELS can be found here:
The properties of He II λ1640 emitters at z = 2.5-5 from the VANDELS survey, 2020

Our follow-up work has investigated whether the presence of exotic stellar systems, such as interacting black hole and massive star binaries, or X-ray binaries, can power the bulk of He II emission that is observed in distant galaxies. The paper reporting these results can be found here:
X-ray properties of He II λ1640 emitting galaxies in VANDELS, 2020

Discovery of the most distant radio galaxy to date

In June 2018, my research team discovered the most distant radio galaxy observed to date, named TGSS J1530+1049, at a distance of 12.7 billion light years away (redshift = 5.72)! In comparison, the age of the Universe is 13.6 billion years. Therefore, this is a galaxy that was formed within the first 7% of the Universe's lifetime! This discovery broke the distance record for a radio galaxy after almost 20 years. Radio galaxies are some of the most massive galaxies in the Universe and harbour a supermassive black hole in their centres that is actively eating up the gas and dust that surrounds it. Discovering such an object at such a large distance from us poses some interesting challenges about how and when the seeds of this galaxy and the supermassive black hole were sown, and how they evolved to be so massive in such a short period of time after the Big Bang.
The paper reporting this discovery has now been published in the Monthly Notices of the Royal Astronomical Society and can be found here:
Discovery of a radio galaxy at z = 5.72, 2018

In the media:
Astronomy Now: Most distant radio galaxy, host to a voracious black hole, is found
Phys.org: The most distant radio galaxy discovered
Astronomie.nl: Astronomen ontdekken verst verwijderde radiostelsel ooit (Astronomers discover the most distant radio galaxy ever)
BBC Brasil: Radiogaláxia mais distante da Terra é descoberta com participação de brasileiro - e dá mais pistas sobre o Big Bang (Most distant radio galaxy is discovered with Brazilian participation - and gives more clues about the Big Bang)
Media INAF: Scoperta la radiogalassia più lontana (The most distant radio galaxy discovered)

High-redshift extreme spectrum project (HiZESP)

We have started a large campaign to hunt for distant radio galaxies by taking advantage of the new all-sky surveys at low radio frequencies using telescopes such as the Giant Metrewave Radio Telescope (GMRT) in India, the Very Large Array (VLA) in USA and the Low Frequency Array (LOFAR) in the Netherlands and all of Europe. Early results from this project can be found here:
A search for faint high-redshift radio galaxy candidates at 150 MHz, 2018

In addition to studying these sources at radio wavelengths, it is essential to also observe them at optical and infrared wavelengths. As part of this project, we have been awarded observing time on telescopes all over the world to a) obtain spectra and determine redshifts of candidate high-redshift radio galaxies and b) observe our targets at near-infrared wavelengths to study the underlying stellar populations.

The telescopes being used for this project include the Hobby-Eberly Telescope (HET), Gemini North, William Herschel Telescope (WHT) and the Large Binocular Telescope (LBT). The paper reporting these observations has now been accepted for publication in the Monthly Notices of the Royal Astronomical Society and can be found here:
The nature of faint radio galaxies at high redshifts, 2019

Modelling the growth of radio AGN across cosmic time

One of the first projects of my PhD was to build a model capable of tracking the evolution of radio galaxies from first principles, and predicting the luminosity and size distribution of radio sources at any given epoch. This model included recipes for a host of physical phenomenon and the results can be found here:
Modelling the luminosities and sizes of radio sources: radio luminosity function at z = 6, 2017

Other interests

In addition to astronomy, I have had the pleasure to be a part of various activities in and around town. Here you can find some of the things that I care about!

Astronomy on Tap London

Astronomy on Tap (AoT) is a unique concept that combines an astronomy public talk with the joy of drinking beer in the local pub! In 2020, I helped bring AoT to London, although in an innovative online format because of the COVID-19 pandemic. We have had tremendous success so far engaging with audiences from all around the world, and cannot wait to bring AoT London to a pub near UCL! Stay tuned for updates.

Public Engagement

Here at UCL there are several public outreach initiatives underway with the aim of bringing physics and astronomy to the wider public, promoting participation from traditionally underrepresented communities and using science to bridge socio-economic inequalities. I am involved with several of our outreach initiatives, and have enjoyed giving talks about stars, galaxies and black holes in the early Universe at amateur astronomy society meetings in and around London. Follow the link by clicking on the image to find out more!

Leiden International Short Film Experience (LISFE)

The 10th edition of LISFE at the artsy cinema, Het Kijkhuis, was a wrap this spring and it was a huge success! LISFE has grown from a day or two of screening short-films in a student centre in Leiden to one of the biggest national level short-film festivals in The Netherlands! LISFE received over 800 films from 70 countries for the 2018 edition and we are looking forward to expand and grow again this year. Click on the image on the left to know more!

Leiden Football Factory

After achieving the second place in the lower divisions of the Dutch Amateur League, the new football (soccer) season starts again this autumn and we will be back to challenge for the division title! Click on the image on the left to follow updates (hopefully you click only when we've won a few games)!

Short CV

Here you can find a short version of my CV:

Research positions

Postdoctoral Research Fellow, UCL, UK, March 2020 - present
Postdoctoral Researcher, INAF-OA Roma, Italy, Feb 2019 - Feb 2020

Education

PhD Astronomy and Astrophysics, Leiden Observatory, The Netherlands, 2014 - 2019
MSc Astrophysics, University College London, UK, 2014

First author publications

  • X-ray properties of He II λ 1640 emitting galaxies in VANDELS, Saxena, A., et al., Monthly Notices of the Royal Astronomical Society (MNRAS)
  • The properties of He II 1640 emitting galaxies at z ~ 2.5-5 from the VANDELS survey (2020), Saxena A., et al., Astronomy & Astrophysics (A&A)
  • The nature of faint radio galaxies at high redshifts (2019), Saxena A., et al., MNRAS
  • Discovery of a radio galaxy at z = 5.72 (2018), Saxena A., et al., MNRAS
  • A search for faint high-redshift radio galaxy candidates at 150 MHz (2018), Saxena A., et al., MNRAS
  • Modelling the luminosities and sizes of radio sources: radio luminosity function at z = 6 (2017), Saxena A., Röttgering H.J.A., Rigby E.E., MNRAS
  • High-redshift radio galaxies at low frequencies (2018), Saxena A., Rottgering H.J.A., Astronomy in Focus, XXX IAU General Assembly

Some successful observing proposals

  • JWST NIRSpec/IFU (Cycle 1), 2021, Co-PI, 24 hours
  • LUCI MOS (Large Binocular Telescope), 2019/2020, PI, 11 hours
  • MUSE (Very Large Telescope), 2018, PI, 8 hours
  • XSHOOTER (Very Large Telescope), 2017, PI, 4 hours DDT
  • William Herschel Telescope, 2017-2019, PI, 7 dark nights
  • Very Large Array A-configuration, 2016, Co-I/contact person, 9+ hours of priority-A time

Contact Me

Here is where you can find me both physically and online.

Office Address

North-West Wing
University College London
Gower Street, London
WC1E 6BT, UK

Email and phone

Email: aayush [dot] saxena [at] ucl [dot] ac [dot] uk

If you'd like to get in touch, either to find out more about my research or to complain about anything that you did not like on this website, why not send me an email on the address listed above?