activity
20092026
most citedSource-intrinsic near-infrared properties of Sgr A*: Total intensity measurements

113 citations · 1.1k across the 46 of their papers we have counts for

collaborators

48 papers

astro-ph.GA2026

Ionization Structure and Metal Enrichment of the Galactic Center Minispiral Observed with JWST

Nicole M Ford, Mayura Balakrishnan, Sebastiano D. von Fellenberg +11

Sagittarius A* (Sgr A*) is the nearest quiescent supermassive black hole, and its proximity offers a unique opportunity to study its surrounding fuel supply. We leverage extensive…

astro-ph.HE2026

Infrared Line Diagnostics Fail to Constrain Sgr A*'s UV Output

Mayura Balakrishnan, Sebastiano D. von Fellenberg, Daryl Haggard +11

Sgr A*, the 4 x supermassive black hole at the Galactic Center, exhibits frequent flaring with X-ray luminosities of erg s, while i…

astro-ph.GA2025★ 1 cited

Photometric Constraints on Intermediate-mass Black Holes in the Galactic Centre

Tamojeet Roychowdhury, Sebastiano D. von Fellenberg, Joseph M. Michail +14

JWST/MIRI observations can place photometric limits on the presence of an intermediate-mass black hole (IMBH) near the Galactic Centre. The stellar complex IRS 13E, a co-moving con…

astro-ph.HE2025

First mid-infrared detection and modeling of a flare from Sgr A*

Sebastiano D. von Fellenberg, Tamojeet Roychowdhury, Joseph M. Michail +24

The time-variable emission from the accretion flow of Sgr A*, the supermassive black hole at the Galactic Center, has long been examined in the radio-to-mm, near-infrared (NIR), an…

astro-ph.GA2024★ 8 cited

The Evaporating Massive Embedded Stellar Cluster IRS 13 Close to Sgr A*. II. Kinematic structure

Florian Peißker, Michal Zajacek, Matus Labaj +8

The existence of two distinct and apparently unrelated populations of dusty stellar objects in the Nuclear Stellar Cluster (NSC) of the Milky Way, namely IRS 13 and the S-cluster,…

astro-ph.IM2024★ 5 cited

The MICADO first light imager for the ELT: off-axis performance of PSF reconstruction

Matteo Simioni, Daniel Jodlbauer, Carmelo Arcidiacono +14

The highest scientific return, for adaptive optics (AO) observations, is achieved with a reliable reconstruction of the PSF. This is especially true for MICADO@ELT. In this present…

astro-ph.GA2023

The Evaporating Massive Embedded Stellar Cluster IRS 13 Close to Sgr A*. I. Detection of a rich population of dusty objects in the IRS 13 cluster

Florian Peißker, Michal Zajaček, Lauritz Thomkins +6

A detailed analysis of the Nuclear Stellar Cluster (NSC) concedes not only the existence of the Scluster with its fast-moving stars and the supermassive black hole (SMBH) Sgr A*. I…

astro-ph.GA2023★ 6 cited

The JWST Galactic Center Survey -- A White Paper

Rainer Schoedel, Steve Longmore, Jonny Henshaw +111

The inner hundred parsecs of the Milky Way hosts the nearest supermassive black hole, largest reservoir of dense gas, greatest stellar density, hundreds of massive main and post ma…

astro-ph.GA2023★ 10 cited

X3: a high-mass Young Stellar Object close to the supermassive black hole Sgr~A*

Florian Peißker, Michal Zajacek, Nadeen B. Sabha +10

To date, the proposed observation of Young Stellar Objects (YSOs) in the Galactic center (GC) still raises the question where and how these objects could have formed due to the vio…

astro-ph.GA2022★ 9 cited

Mid-Infrared studies of dusty sources in the Galactic Center

Harshitha K. Bhat, Nadeen B. Sabha, Michal Zajaček +5

Mid-Infrared (MIR) images of the Galactic center show extended gas and dust features along with bright IRS sources. Some of these dust features are a part of ionized clumpy streame…

astro-ph.GA2021★ 17 cited

The apparent tail of the Galactic center object G2/DSO

Florian Peißker, Michal Zajacek, Andreas Eckart +6

The observations of the near-infrared excess object G2/DSO induced an increased attention towards the Galactic center and its vicinity. The predicted flaring event in 2014 and the…

astro-ph.GA2021★ 15 cited

First observed interaction of the circumstellar envelope of an S-star with the environment of Sgr A*

Florian Peißker, Basel Ali, Michal Zajaček +7

Several publications highlight the importance of the observations of bow shocks to learn more about the surrounding interstellar medium and radiation field. We revisit the most pro…

astro-ph.GA2020★ 18 cited

Constraining the accretion flow density profile near Sgr A* using the -band emission of the S2 star

S. Elaheh Hosseini, Michal Zajaček, Andreas Eckart +2

The density profile of the ambient medium around a supermassive black hole plays an important role in understanding the inflow-outflow mechanisms in the Galactic Centre. We constra…

astro-ph.GA2020★ 20 cited

Near- and mid-infrared observations in the inner tenth of a parsec of the Galactic center -- Detection of proper motion of a filament very close to Sgr~A*

Florian Peißker, Andreas Eckart, Nadeen B. Sabha +2

We analyze the gas and dust emission in the immediate vicinity of the supermassive black hole Sgr~A* at the Galactic center (GC) with the ESO VLT (Paranal/Chile) instruments SINFON…

astro-ph.GA2020★ 28 cited

An astrophysically motivated ranking criterion for low-latency electromagnetic follow-up of gravitational wave events

M. Celeste Artale, Yann Bouffanais, Michela Mapelli +5

We investigate the properties of the host galaxies of compact binary mergers across cosmic time. To this end, we combine population synthesis simulations together with galaxy catal…

astro-ph.SR2020★ 88 cited

Observational constraints on the optical and near-infrared emission from the neutron star-black hole binary merger S190814bv

K. Ackley, L. Amati, C. Barbieri +151

On 2019 August 14, the LIGO and Virgo interferometers detected a high-significance event labelled S190814bv. Preliminary analysis of the GW data suggests that the event was likely…

astro-ph.GA2020★ 21 cited

SOFIA/FORCAST Galactic Center Legacy Survey: Overview

Matthew J. Hankins, Ryan M. Lau, James T. Radomski +12

The Galactic Center contains some of the most extreme conditions for star formation in our Galaxy as well as many other phenomena that are unique to this region. Given our relative…

astro-ph.GA2019★ 3 cited

Observations of the 86 GHz SiO maser sources in the Central Parsec of the Galactic Centre

A. Borkar, A. Eckart, C. Straubmeier +8

We present results of 3 mm observations of SiO maser sources in the Galactic Centre (GC) from observations with the Australia Telescope Compact Array between , along the…

astro-ph.GA2019★ 19 cited

A new bow-shock source with bipolar morphology in the vicinity of Sgr A*

F. Peißker, M. Zajacek, A. Eckart +3

Here we present a new bowshock blue-shifted source in the close vicinity of Sgr A* that we name X8. We use data-sets that are based on SINFONI observations with the Very Large Tele…

astro-ph.GA2019★ 97 cited

Host galaxies of merging compact objects: mass, star formation rate, metallicity and colours

M. Celeste Artale, Michela Mapelli, Nicola Giacobbo +4

Characterizing the properties of the host galaxies of merging compact objects provides essential clues to interpret current and future gravitational-wave detections. Here, we inves…

astro-ph.HE2018

Light and shadow in the Galactic Center - On the detection of the relativistic periastron shift of star S2 in the Galactic Center

A. Eckart, M. Parsa, E. Mossoux +11

We report on the nature of prominent sources of light and shadow in the Galactic Center. With respect to the Bremsstrahlung X-ray emission of the hot plasma in that region the Gala…

astro-ph.HE2018

The Multifrequency Behavior of Sagittarius A*

A. Eckart, M. Zajacek, M. Parsa +15

The Galactic Center is the closest galactic nucleus that allows us to determine the multi-frequency behavior of the supermassive black hole counterpart Sagittarius A* in great deta…

astro-ph.GA2017★ 3 cited

Experimental Indicators of Accretion Processes in Active Galactic Nuclei

A. Eckart, M. Valencia-S., B. Shahzamanian +19

Bright Active Galactic Nuclei are powered by accretion of mass onto the super massive black holes at the centers of the host galaxies. For fainter objects star formation may signif…

astro-ph.GA2017

Nuclear Activity and the Conditions of Star-formation at the Galactic Center

A. Eckart, M. Valencia-S., B. Shahzamanian +15

The Galactic Center is the closest galactic nucleus that can be studied with unprecedented angular resolution and sensitivity. We summarize recent basic observational results on Sa…