Search Publications

The rebrightening of a ROSAT-selected tidal disruption event: repeated weak partial disruption flares from a quiescent galaxy?
DOI: 10.1093/mnras/stad022 Bibcode: 2023MNRAS.520.3549M

Liu, Z.; Buchner, J.; Nandra, K. +11 more

The ROSAT-selected tidal disruption event (TDE) candidate RX J133157.6-324319.7 (J1331) was detected in 1993 as a bright [0.2-2 keV flux of (1.0 ± 0.1) × 10-12 erg s-1 cm-2], ultra-soft (kT = 0.11 ± 0.03 keV) X-ray flare from a quiescent galaxy (z = 0.051 89). During its fifth all-sky survey (eRASS5) in 2022, Spect…

2023 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton 42
Tormund's return: Hints of quasi-periodic eruption features from a recent optical tidal disruption event
DOI: 10.1051/0004-6361/202346440 Bibcode: 2023A&A...675A.152Q

Miniutti, G.; Clerc, N.; Webb, N. A. +8 more

Context. Quasi-periodic eruptions (QPEs) are repeating thermal X-ray bursts associated with accreting massive black holes, the precise underlying physical mechanisms of which are still unclear.
Aims: We present a new candidate QPE source, AT 2019vcb (nicknamed Tormund by the Zwicky Transient Facility Collaboration), which was found during an …

2023 Astronomy and Astrophysics
XMM-Newton 42
From Images to Dark Matter: End-to-end Inference of Substructure from Hundreds of Strong Gravitational Lenses
DOI: 10.3847/1538-4357/aca525 Bibcode: 2023ApJ...942...75W

Marshall, Philip J.; Birrer, Simon; Darragh-Ford, Elise +4 more

Constraining the distribution of small-scale structure in our universe allows us to probe alternatives to the cold dark matter paradigm. Strong gravitational lensing offers a unique window into small dark matter halos (<1010 M ) because these halos impart a gravitational lensing signal even if they do not host luminous ga…

2023 The Astrophysical Journal
eHST 42
On the impact of f(Q) gravity on the large scale structure
DOI: 10.1093/mnras/stad968 Bibcode: 2023MNRAS.522..252S

Sokoliuk, Oleksii; Arora, Simran; Praharaj, Subhrat +2 more

We investigate the exponential f(Q) symmetric teleparallel gravitation, namely $f(Q)=Q+\alpha Q_0(1-e^{-\beta \sqrt{Q/Q_0}})$ using ME-GADGET code to probe the structure formation with box sizes LBox = 10/100 Mpc h-1 and middle resolution $N_p^{1/3}=512$. To reproduce viable cosmology within the aforementioned modified gravit…

2023 Monthly Notices of the Royal Astronomical Society
eHST 42
The Pan-STARRS1 z > 5.6 Quasar Survey. II. Discovery of 55 Quasars at 5.6 < z < 6.5
DOI: 10.3847/1538-4365/acb3c7 Bibcode: 2023ApJS..265...29B

Hennawi, Joseph F.; Noirot, Gaël; Fan, Xiaohui +20 more

The identification of bright quasars at z ≳ 6 enables detailed studies of supermassive black holes, massive galaxies, structure formation, and the state of the intergalactic medium within the first billion years after the Big Bang. We present the spectroscopic confirmation of 55 quasars at redshifts 5.6 < z < 6.5 and UV magnitudes -24.5 <…

2023 The Astrophysical Journal Supplement Series
Gaia 41
Optimized Photometric Redshifts for the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS)
DOI: 10.3847/1538-4357/ac9f12 Bibcode: 2023ApJ...942...36K

Finkelstein, Steven L.; Pérez-González, Pablo G.; Santini, Paola +27 more

We present the first comprehensive release of photometric redshifts (photo- z's) from the Cosmic Assembly Near-Infrared Deep Extragalactic Legacy Survey (CANDELS) team. We use statistics based upon the Quantile-Quantile (Q-Q) plot to identify biases and signatures of underestimated or overestimated errors in photo- z probability density functions …

2023 The Astrophysical Journal
eHST 41
Pegasus IV: Discovery and Spectroscopic Confirmation of an Ultra-faint Dwarf Galaxy in the Constellation Pegasus
DOI: 10.3847/1538-4357/aca1c3 Bibcode: 2023ApJ...942..111C

Zenteno, A.; James, D. J.; Li, T. S. +31 more

We report the discovery of Pegasus IV, an ultra-faint dwarf galaxy found in archival data from the Dark Energy Camera processed by the DECam Local Volume Exploration Survey. Pegasus IV is a compact, ultra-faint stellar system ( ${r}_{1/2}={41}_{-6}^{+8}$ pc; M V = -4.25 ± 0.2 mag) located at a heliocentric distance of ${90}_{-6}^{+4}\…

2023 The Astrophysical Journal
Gaia 41
The VANDELS survey: the ionizing properties of star-forming galaxies at 3 ≤ z ≤ 5 using deep rest-frame ultraviolet spectroscopy
DOI: 10.1093/mnras/stad1283 Bibcode: 2023MNRAS.522.6295S

Chisholm, J.; Schaerer, D.; Cullen, F. +15 more

The physical properties of Epoch of Reionization (EoR) galaxies are still poorly constrained by observations. To better understand the ionizing properties of galaxies in the EoR, we investigate deep, rest-frame ultraviolet (UV) spectra of ≃500 star-forming galaxies at 3 ≤ z ≤ 5 selected from the public ESO-VANDELS spectroscopic survey. The absolut…

2023 Monthly Notices of the Royal Astronomical Society
eHST 41
Variability Catalog of Stars Observed during the TESS Prime Mission
DOI: 10.3847/1538-4365/acdee5 Bibcode: 2023ApJS..268....4F

Kane, Stephen R.; Pepper, Joshua; Huber, Daniel +10 more

During its 2 yr Prime Mission, TESS observed over 232,000 stars at a 2 minute cadence across ~70% of the sky. These data provide a record of photometric variability across a range of astrophysically interesting timescales, probing stellar rotation, stellar binarity, and pulsations. We have analyzed the TESS 2 minute light curves to identify period…

2023 The Astrophysical Journal Supplement Series
Gaia 41
The Fundamental Signature of Star Formation Quenching from AGN Feedback: A Critical Dependence of Quiescence on Supermassive Black Hole Mass, Not Accretion Rate
DOI: 10.3847/1538-4357/acac7c Bibcode: 2023ApJ...944..108B

Maiolino, Roberto; Bluck, Asa F. L.; Piotrowska, Joanna M.

We identify the intrinsic dependence of star formation quenching on a variety of galactic and environmental parameters, utilizing a machine-learning approach with Random Forest classification. We have previously demonstrated the power of this technique to isolate causality, not mere correlation, in complex astronomical data. First, we analyze thre…

2023 The Astrophysical Journal
eHST 41