papers

Publications (92)

astro-ph.GA2018

Magnification Bias of Distant Galaxies in the Hubble Frontier Fields: Testing Wave vs. Particle Dark Matter Predictions

Enoch Leung, Tom Broadhurst, Jeremy Lim +4

Acting as powerful gravitational lenses, the strong lensing galaxy clusters of the deep Hubble Frontier Fields (HFF) program permit access to lower-luminosity galaxies lying at hig…

astro-ph.CO2026

Gravitational Lensing Predictions from Wave Simulations of Fuzzy Dark Matter

Jiajun Zhou, Zhengxiang Li, Amruth Alfred +3

In the cold dark matter paradigm, ultra-light particles are emerging as strong contenders to conventional massive particles. A unique prediction of dark matter comprising such ultr…

astro-ph2008

Tracing the asymmetry in the envelope around the carbon star CIT 6

Dinh-V-Trung, Jeremy Lim

We present high angular resolution observations of HCN J=5--4 line and 7 mm continumm emission from the extreme carbon star CIT 6. We find that the 7 mm continuum emission is u…

astro-ph.GA2024

Star Formation, Nebulae, and Active Galactic Nuclei in CLASH Brightest Cluster Galaxies. I. Dependence on Core Entropy of Intracluster Medium

Arsen Levitskiy, Jeremy Lim, Youichi Ohyama +2

We set the stage for reassessing how star formation, emission-line nebulae, and active galactic nuclei (AGNs) in brightest cluster galaxies (BCGs) depend on the thermodynamics of t…

astro-ph.GA2020

Sustained formation of progenitor globular clusters in a giant elliptical galaxy

Jeremy Lim, Emily Wong, Youichi Ohyama +2

Globular clusters (GCs) are thought to be ancient relics from the early formative phase of galaxies, although their physical origin remains uncertain. GCs are most numerous around…

astro-ph.CO2012

The Taiwan ECDFS Near-Infrared Survey: Very Bright End of the Luminosity Function at z>7

Bau-Ching Hsieh, Wei-Hao Wang, Haojing Yan +5

The primary goal of the Taiwan ECDFS Near-Infrared Survey (TENIS) is to find well screened galaxy candidates at z>7 (z' dropout) in the Extended Chandra Deep Field-South (ECDFS). T…

astro-ph2007

Radially-Inflowing Molecular Gas in NGC 1275 Deposited by a X-ray Cooling Flow in the Perseus Cluster

Jeremy Lim, YiPing Ao, Dinh-V-Trung

We have imaged in CO(2-1) the molecular gas in NGC 1275 (Perseus A), the cD galaxy at the center of the Perseus Cluster, at a spatial resolution of 1 kpc over a central regio…

astro-ph.CO2014

The Orthogonally Aligned Dark Halo of an Edge-on Lensing Galaxy in the Hubble Frontier Fields: A Challenge for Modified Gravity

Jose M. Diego, Tom Broadhurst, Narciso Benitez +2

We examine a well resolved 8 arcsec lensed image that is symmetrically bent in the middle by an edge-on lenticular galaxy, in the Hubble Frontier Field (HFF) data of MACSJ0416.1-20…

astro-ph.GA2026

Extragalactic microlensing through Ultra Diffuse Galaxies

Sung Kei Li, Thomas Broadhurst, Jose M. Diego +3

Stellar microlensing is a powerful method to constrain compact dark matter models, uncover binary stars, and exoplanets during caustic crossing events. At cosmological distances, {…

astro-ph.GA2017

Spiral Arms, Infall, and Misalignment of the Circumbinary Disk from the Circumstellar Disks in the Protostellar Binary System L1551 NE

Shigehisa Takakuwa, Kazuya Saigo, Tomoaki Matsumoto +5

We report the ALMA Cycle 2 observations of the Class I binary protostellar system L1551 NE in the 0.9-mm continuum, C18O (3-2), 13CO (3-2), SO (7_8-6_7), and the CS (7-6) emission.…

astro-ph2008

The shaping effect of collimated fast outflows in the Egg nebula

Dinh-V-Trung, Jeremy Lim

We present high angular resolution observations of the HCN J=5--4 line from the Egg nebula, which is the archetype of protoplanetary nebulae. We find that the HCN emi…

astro-ph2008

Prevalence of Tidal Interactions among Local Seyfert Galaxies: The Control Experiment

Ya-Wen Tang, Cheng-Yu Kuo, Jeremy Lim +1

We test whether there is a relation between the observed tidal interactions and Seyfert activity by imaging in HI twenty inactive galaxies at the same spatial resolution and detect…

physics.optics2021

Highly efficient terahertz generation using 3D Dirac semimetals

Lu Wang, Jeremy Lim, Liang Jie Wong

We show that 3D Dirac semimetals are promising candidates for highly efficient optical-to-terahertz conversion due to their extreme optical nonlinearities. In particular, we predic…

astro-ph.GA2022

Recent Formation of a Spiral Disk Hosting Progenitor Globular Clusters at the center of the Perseus Brightest Cluster Galaxy: I. Spiral Disk

Michael C. H. Yeung, Youichi Ohyama, Jeremy Lim

We address the nature and origin of a spiral disk at the center of NGC 1275, the giant elliptical galaxy at the center of the Perseus cluster, that spans a radius of $5\,\rm…

astro-ph.CO2019

Evidence of Neutrino Enhanced Clustering in a Complete Sample of Sloan Survey Clusters, Implying eV

Razieh Emami, Tom Broadhurst, Pablo Jimeno +7

The clustering amplitude of 7143 clusters from the Sloan Digital Sky Survey (SDSS) is found to increase with cluster mass, closely agreeing with the Gaussian random field hypothesi…

astro-ph.CO2015

A Free-Form Prediction for the Reappearance of Supernova Refsdal in the Hubble Frontier Fields Cluster MACSJ1149.5+2223

Jose M. Diego, Tom Broadhurst, Cuncheng Chen +7

The massive cluster MACSJ1149.5+2223(z=0.544) displays five very large lensed images of a well resolved spiral galaxy at . It is within one of these images tha…

astro-ph.GA2013

Formation of Dense Molecular Gas and Stars at the Circumnuclear Starburst Ring in the Barred Galaxy NGC 7552

Hsi-An Pan, Jeremy Lim, Satoki Matsushita +2

We present millimeter molecular-line complemented by optical observations, along with a reanalysis of archival centimeter HI and continuum data, to infer the global dynamics and de…

astro-ph.CO2012

The Taiwan ECDFS Near-Infrared Survey: Ultra-deep J and Ks Imaging in the Extended Chandra Deep Field-South

Bau-Ching Hsieh, Wei-Hao Wang, Chih-Chiang Hsieh +4

We present ultra-deep J and Ks imaging observations covering a 30' * 30' area of the Extended Chandra Deep Field-South (ECDFS) carried out by our Taiwan ECDFS Near-Infrared Survey…

astro-ph.GA2023

JWST's PEARLS: TN J1338-1942 -- I. Extreme jet triggered star-formation in a luminous radio galaxy

Kenneth J. Duncan, Rogier A. Windhorst, Anton M. Koekemoer +25

We present the first JWST observations of the luminous radio galaxy TN J1338-1942, obtained as part of the ``Prime Extragalactic Areas for Reionization and Lensing Science…

physics.app-ph2022

Approaching intrinsic threshold breakdown voltage and ultra-high gain in graphite/InSe Schottky photodetector

Zhiyi Zhang, Bin Cheng, Jeremy Lim +10

Realizing both ultra-low breakdown voltage and ultra-high gain has been one of the major challenges in the development of high-performance avalanche photodetector. Here, we report…

astro-ph.CO2021

An analytic model for the sub-galactic matter power spectrum in fuzzy dark matter halos

Hiroki Kawai, Masamune Oguri, Alfred Amruth +2

Fuzzy dark matter (FDM), a scalar particle coupled to the gravitational field without self-interaction whose mass range is , is one of the prom…

astro-ph.GA2025

Explaining JWST counts with galaxy formation models

Giorgio Manzoni, Tom Broadhurst, Jeremy Lim +18

A distinct power-law break is apparent m_AB approximately 21 in the deep Near-Infrared PEARLS-JWST galaxy counts. The break becomes more pronounced at longer wavelengths, with the…

astro-ph.CO2023

Einstein rings modulated by wavelike dark matter from anomalies in gravitationally lensed images

Alfred Amruth, Tom Broadhurst, Jeremy Lim +10

Unveiling the true nature of Dark Matter (DM), which manifests itself only through gravity, is one of the principal quests in physics. Leading candidates for DM are weakly interact…

astro-ph.GA2021

Wave Dark Matter and Ultra Diffuse Galaxies

Alvaro Pozo, Tom Broadhurst, Ivan De Martino +4

Dark matter as a Bose-Einstein condensate, such as the axionic scalar field particles of String Theory, can explain the coldness of dark matter on large scales. Pioneering simulati…

astro-ph.GA2020

Atacama Compact Array Measurements of the Molecular Mass in the NGC 5044 Cooling Flow Group

Gerrit Schellenberger, Laurence P. David, Jan Vrtilek +13

The fate of cooling gas in the centers of galaxy clusters and groups is still not well understood, as is also the case for the complex processes of triggering star formation in cen…

astro-ph.CO2014

Hubble Frontier Field Free-Form Mass Mapping of the Massive Multiple-Merging Cluster MACSJ0717.5+3745

Jose M. Diego, Tom Broadhurst, Adi Zitrin +4

We examine the latest data on the cluster MACSJ0717.5+3745 from the Hubble Frontier Fields campaign. The critically lensed area is the largest known of any lens and very irregular…

astro-ph.SR2014

Angular Momentum Exchange by Gravitational Torques and Infall in the Circumbinary Disk of the Protostellar System L1551 NE

Shigehisa Takakuwa, Masao Saito, Kazuya Saigo +4

We report the ALMA observation of the Class I binary protostellar system L1551 NE in the 0.9-mm continuum, C18O (3-2), and 13CO (3-2) lines at a ~1.6 times higher resolution and a…

astro-ph.GA2022

Webb's PEARLS: Bright 1.5--2.0 micron Dropouts in the Spitzer/IRAC Dark Field

Haojing Yan, Seth H. Cohen, Rogier A. Windhorst +35

Using the first epoch of four-band NIRCam observations obtained by the James Webb Space Telescope (JWST) Prime Extragalactic Areas for Reionization and Lensing Science Program in t…

astro-ph2008

SMA CO(J=6-5) and 435 micron interferometric imaging of the nuclear region of Arp 220

Satoki Matsushita, Daisuke Iono, Glen R. Petitpas +11

We have used the Submillimeter Array (SMA) to make the first interferometric observations (beam size ~1") of the 12CO J=6-5 line and 435 micron (690 GHz) continuum emission toward…

astro-ph2002

Molecular Gas in nearby Early-Type Powerful Classical Radio Galaxies

Stephane Leon, Jeremy Lim, Francoise Combes +1

We report a survey for molecular gas in nearby powerful radio galaxies. Eight of the eighteen radio galaxies observed were detected with molecular masses in the range 10^7--10^9 Ms…

astro-ph.GA2013

Evidence for Infalling Gas of Low Angular Momentum towards the L1551 NE Keplerian Circumbinary Disk

Shigehisa Takakuwa, Masao Saito, Jeremy Lim +1

We report follow-up observations of the Class I binary protostellar system L1551 NE in the C18O (3--2) line with the SMA in its compact and subcompact configurations. Our previous…

astro-ph.GA2012

A Keplerian Circumbinary Disk around the Protobinary System L1551 NE

Shigehisa Takakuwa, Masao Saito, Jeremy Lim +3

We present SubMillimeter-Array observations of a Keplerian disk around the Class I protobinary system L1551 NE in 335 GHz continuum emission and submillimeter line emission in 13CO…

astro-ph2008

Molecular Gas and Star formation in ARP 302

Yiping Ao, Dinh-V-Trung, Jeremy Lim +2

We present the Submillimeter Array observation of the CO J=2-1 transition towards the northern galaxy, ARP 302N, of the early merging system, ARP 302. Our high angular resolution o…

astro-ph.CO2024

Flashlights: Transients among Gravitationally-Lensed Star Clusters in the Dragon Arc. I. Stellar Microlensing vs Stellar Outbursts

Sung Kei Li, Jose M. Diego, Patrick L. Kelly +8

We report the discovery of transients among star clusters in a distant galaxy that is gravitationally lensed by a foreground galaxy cluster, and explore whether these transients co…

astro-ph.GA2024

High-Spectral Resolution Observations of the Optical Filamentary Nebula in NGC 1275

Benjamin Vigneron, Julie Hlavacek-Larrondo, Carter Lee Rhea +18

We present new high-spectral resolution observations (R = = 7000) of the filamentary nebula surrounding NGC 1275, the central galaxy of the Perseus cluster. These observa…

astro-ph2007

Molecular shells in IRC+10216: Evidence for non-isotropic and episodic mass loss enhancement

Dinh-V-Trung, Jeremy Lim

We report high angular-resolution VLA observations of cyanopolyyne molecules HCN and HCN from the carbon rich circumstellar envelope of IRC+10216. The observed low-lying ro…

astro-ph.GA2025

Tidal Disruption of Super Star Clusters as the origin of Bluish Light at the inner region of the Perseus Cluster Central Galaxy

Arsen Levitskiy, Youichi Ohyama, Jeremy Lim

Relatively blue light extends beyond a spiral disk from a radius of ~5 kpc out to ~14 kpc from the center of NGC 1275. Analyses of its spectrum and broadband colors reveal a popula…

astro-ph.GA2020

Circumbinary Disks of the Protostellar Binary Systems in the L1551 Region

Shigehisa Takakuwa, Kazuya Saigo, Tomoaki Matsumoto +6

We report ALMA Cycle 4 observations of the Class I binary protostellar system L1551 IRS 5 in the 0.9-mm continuum emission, C18O (J=3-2), OCS (J=28-27), and four other Band 7 lines…

astro-ph.CO2024

Imaging dark matter at the smallest scales with lensed stars

J. M. Diego, Sung Kei Li, Alfred Amruth +19

Observations of caustic-crossing galaxies at redshift show a wealth of transient events. Most of them are believed to be microlensing events of highly magnified stars. Ea…

astro-ph2009

The Yuan-Tseh Lee Array for Microwave Background Anisotropy

Paul T. P. Ho, Pablo Altamirano, Chia-Hao Chang +52

The Yuan-Tseh Lee Array for Microwave Background Anisotropy (AMiBA) is the first interferometer dedicated to studying the cosmic microwave background (CMB) radiation at 3mm wavelen…

astro-ph.CO2025

Multi-copy Axion Transfer Function and Observational Implications of Effective de Broglie Scales

Jiashuo Zhang, Tom Broadhurst, Jeremy Lim +2

Ultra-light axions are viable fuzzy/wave-like dark matter (DM) candidates generically predicted by the String Axiverse paradigm with multiple particle copies, whereas most of t…

astro-ph.CO2026

Lensed stars in galaxy-galaxy strong lensing -- a JWST prediction for the Cosmic Horseshoe

Sung Kei Li, Luke Weisenbach, Thomas E. Collett +10

We explore for the first time the possibility of detecting lensed star transients in galaxy-galaxy strong lensing systems upon repeated, deep imaging using the {\it James-Webb Spac…

astro-ph.GA2024

On the Evidence for Molecular Outflows in High-redshift Dusty Star-forming Galaxies

James Nianias, Jeremy Lim, Michael Yeung

Galactic-scale outflows of molecular gas from star-forming galaxies constitute the most direct evidence for regulation of star formation. In the early universe (), such ou…

astro-ph.GA2018

A Likely Super Massive Black Hole Revealed by its Einstein Radius in Hubble Frontier Fields Images

Mandy C. Chen, Tom Broadhurst, Jeremy Lim +4

At cosmological distances, gravitational lensing can provide a direct measurement of supermassive black hole (SMBH) masses irrespective of their luminosities. Here, we directly est…

astro-ph.CO2010

TANGO I: ISM in nearby radio galaxies. Molecular gas

Breezy Ocana Flaquer, Stephane Leon, Francoise Combes +1

Powerful radio-AGN are hosted by massive elliptical galaxies which are usually very poor in molecular gas. Nevertheless gas is needed in the very center to feed the nuclear activit…

astro-ph2007

Jet-disturbed molecular gas near the Seyfert 2 nucleus in M51

Satoki Matsushita, Sebastien Muller, Jeremy Lim

Previous molecular gas observations at arcsecond-scale resolution of the Seyfert 2 galaxy M51 suggest the presence of a dense circumnuclear rotating disk, which may be the reservoi…

astro-ph.CO2014

A Rigorous Free-form Lens Model of Abell 2744 to Meet the Hubble Frontier Fields Challenge

Daniel Lam, Tom Broadhurst, Jose M. Diego +4

Hubble Frontier Fields (HFF) imaging of the most powerful lensing clusters provides access to the most magnified distant galaxies. The challenge is to construct lens models capable…

astro-ph.GA2025

Delayed Feedback in High- Starbursts Revealed by Lyman- Profiles and Metal Line Diagnostics

James Nianias, Jeremy Lim, Yik Lok Wong +1

Lyman- emission, which owing to its resonant nature strongly couples the emergent line profile to gas kinematics, is a key observable for probing outflows from star-forming gal…

astro-ph2008

Interferometric 12CO(J=2-1) image of the Nuclear Region of Seyfert 1 Galaxy NGC 1097

Pei-Ying Hsieh, Satoki Matsushita, Jeremy Lim +2

We have mapped the central region of the Seyfert 1 galaxy NGC 1097 in 12CO(J=2-1) with the Submillieter Array (SMA). The 12CO(J=2-1) map shows a central concentration and a surroun…

astro-ph.GA2023

Unscrambling the lensed galaxies in JWST images behind SMACS0723

Massimo Pascale, Brenda L. Frye, Jose Diego +16

The first deep field images from the James Webb Space Telescope (JWST) of the galaxy cluster SMACS~J0723.3-7327 reveal a wealth of new lensed images at uncharted infrared wavelengt…

astro-ph.CO2022

JWST's PEARLS: Prime Extragalactic Areas for Reionization and Lensing Science: Project Overview and First Results

Rogier A. Windhorst, Seth H. Cohen, Rolf A. Jansen +82

We give an overview and describe the rationale, methods, and first results from NIRCam images of the JWST "Prime Extragalactic Areas for Reionization and Lensing Science" ("PEARLS"…

astro-ph.GA2009

Subarcsecond Imaging of the High-Mass Star Forming Region Onsala 1

Yu-Nung Su, Sheng-Yuan Liu, Jeremy Lim

We report subarcsecond images of the high-mass star forming region Onsala 1 (ON 1) made with the Submillimeter Array (SMA) at 0.85 mm and the Very Large Array at 1.3 cm and 3.6 cm.…

astro-ph.CO2026

The Subversive Role of Excessive External Shear in Concealing Lensing Anomalies

Amruth Alfred, Shashpal Singh, Rommulus Francis Lewis +5

To best reproduce observed multiply-lensed lensed images, lens models usually incorporate shear attributed to objects unrelated to the lensing galaxy (i.e., external shear): whethe…

quant-ph2024

Strongly correlated multi-electron bunches from interaction with quantum light

Suraj Kumar, Jeremy Lim, Nicholas Rivera +4

Strongly correlated electron systems are a cornerstone of modern physics, being responsible for groundbreaking phenomena from superconducting magnets to quantum computing. In most…

astro-ph2003

Radio Cores of Bipolar Nebulae: Search for Collimated Winds

Ting-Hui Lee, Jeremy Lim, Sun Kwok

We present results of our search for collimated ionized winds in bipolar nebulae using the Very Large Array (VLA) and the Australia Telescope Compact Array (ATCA). Our search is mo…

astro-ph.CO2022

Flashlights: More than A Dozen High-Significance Microlensing Events of Extremely Magnified Stars in Galaxies at Redshifts z=0.7-1.5

Patrick L. Kelly, Wenlei Chen, Amruth Alfred +23

Once only accessible in nearby galaxies, we can now study individual stars across much of the observable universe aided by galaxy-cluster gravitational lenses. When a star, compact…

astro-ph2006

654 GHz Continuum and C18O (6-5) Observations of G240.31+0.07 with the Submillimeter Array

Huei-Ru Chen, Yu-Nung Su, Sheng-Yuan Liu +7

We report a dual-band observation at 223 and 654 GHz (460 micron) toward an ultracompact (UC) HII region, G240.31+0.07, with the Submillimeter Array. With a beam size of 1"5 X 0"8,…

astro-ph.CO2016

Geometric Corroboration of the Earliest Lensed Galaxy at z~10.8 from Robust Free-Form Modelling

Brian M. Y. Chan, Tom Broadhurst, Jeremy Lim +4

A multiply-lensed galaxy, MACS0647-JD, with a probable photometric redshift of is claimed to constitute one of the very earliest known galaxies, formed…

astro-ph.GA2014

A Geometrically Supported Candidate Multiply-Imaged by the Hubble Frontier Fields Cluster Abell 2744

Adi Zitrin, Wei Zheng, Tom Broadhurst +11

The deflection angles of lensed sources increase with their distance behind a given lens. We utilize this geometric effect to corroborate the photometric redshi…

astro-ph.SR2009

Multiple Bipolar Molecular Outflows in the L1551 IRS5 Protostellar System

Po-Feng Wu, Shigehisa Takakuwa, Jeremy Lim

The multiple protostellar system L1551 IRS5 exhibits a large-scale bipolar molecular outflow. We have studied this outflow within ~4000 AU of its driving source(s) with the SubMill…

astro-ph.CO2025

Transient star B/R ratio and star formation in lensed galaxies

Sung Kei Li, Jose M. Palencia, Jose M. Diego +8

The extreme magnification from galaxy clusters and microlenses therein allows the detection of individual, luminous stars in lensed galaxies as transient events, and hence provides…

astro-ph.CO2025

Constraining the z 1 Initial Mass Function with {\it HST} and {\it JWST} Lensed Stars in MACS J0416.1-2403

Sung Kei Li, Jose M. Diego, Ashish K. Meena +19

Our understanding of galaxy properties and evolution is contingent on knowing the initial mass function (IMF), and yet to date, the IMF is constrained only to local galaxies. Indiv…

physics.optics2021

Propagation-induced limits to high harmonic generation in 3D Dirac semimetals

Jeremy Lim, Yee Sin Ang, Lay Kee Ang +1

3D Dirac semimetals (DSMs) are promising materials for terahertz high harmonic generation (HHG). We show that 3D DSMs' high nonlinearity opens up a regime of nonlinear optics where…

astro-ph2007

Using Fast-Switching Data to Characterize Atmospheric Phase Fluctuations at the Submillimeter Array

Dharam Vir Lal, Satoki Matsushita, Jeremy Lim

For the submillimeter band observations, we have been routinely adopting the calibration cycle time of 20-30 minutes, which is the same as any typical centimeter and millimeter ban…

astro-ph.CO2024

A high-resolution view of the source-plane magnification near cluster caustics in wave dark matter models

Jose M. Diego, Alfred Amruth, Jose M. Palencia +10

We present the highest resolution images to date of caustics formed by wave dark matter (DM) fluctuations near the critical curves of cluster gravitational lenses. We describe…

astro-ph.GA2016

A free-form lensing model of A370 revealing stellar mass dominated BCGs, in Hubble Frontier Fields images

Jose M. Diego, Kasper B. Schmidt, Tom Broadhurst +9

We derive a free-form mass distribution for the unrelaxed cluster A370 (z=0.375), using the latest Hubble Frontier Fields images and GLASS spectroscopy. Starting from a reliable se…

astro-ph2007

Submillimeter Array Observation of the Proto-Planetary Nebula CRL 618 in the CO J=6-5 Line

Jun-ichi Nakashima, David Fong, Tatsuhiko Hasegawa +6

We report on the results of a Submillimeter Array interferometric observation of the proto-planetary nebula CRL 618 in the 12CO J=6-5 line. With the new capability of SMA enabling…

astro-ph.GA2023

BUFFALO/Flashlights: Constraints on the abundance of lensed supergiant stars in the Spock galaxy at redshift 1

Jose M. Diego, Sung Kei Li, Ashish K. Meena +27

We present a constraint on the abundance of supergiant (SG) stars at redshift z approx. 1, based on recent observations of a strongly lensed arc at this redshift. First we derive a…

astro-ph.CO2025

Signatures of Fuzzy Dark Matter Inside Radial Critical Curves

J. M. Palencia, Paloma Morilla, Sung Kei Li +5

We investigate the strong gravitational lensing properties of fuzzy dark matter (FDM) halos, focusing on the magnification properties near radial critical curves (CCs). Using simul…

astro-ph.GA2020

Geometric Support for Dark Matter by an Unaligned Einstein Ring in Abell 3827

Mandy C. Chen, Tom Broadhurst, Jeremy Lim +4

The non-detection of dark matter (DM) particles in increasingly stringent laboratory searches has encouraged alternative gravity theories where gravity is sourced only from visible…

astro-ph.SR2009

Probing the mass loss history of the yellow hypergiant IRC+10420

Dinh-V-Trung, Sebastien Muller, Jeremy Lim +2

We have used the sub-millimeter array to image the molecular envelope around IRC+10420. Our observations reveal a large and clumpy expanding envelope around the star. The molecular…

astro-ph.GA2021

Temporally and Spatially Extended Star Formation in the Brightest Cluster Galaxy of MACS\,J0329.70211 at : Implications for Stellar Growth

Juno Li, Leo W. H. Fung, Jeremy Lim +1

Brightest cluster galaxies (BCGs), particularly those at the centers of cool-core clusters, can exhibit star formation over spatial extents of up to 100\,kpc at inferred r…

astro-ph.GA2014

Resolving the Bright HCN(1-0) Emission toward the Seyfert 2 Nucleus of M51: Shock Enhancement by Radio Jets and Weak Masing by Infrared Pumping?

Satoki Matsushita, Dinh-V-Trung, Frédéric Boone +3

We present high angular resolution observations of the HCN(1-0) emission (at ~1" or ~34 pc), together with CO J = 1-0, 2-1, and 3-2 observations, toward the Seyfert 2 nucleus of M5…

astro-ph2006

Possible Molecular Spiral Arms in the Protoplanetary Disk of AB Aur

Shin-Yi Lin, Nagayoshi Ohashi, Jeremy Lim +3

The circumstellar dust disk of the Herbig Ae star AB Aur has been found to exhibit complex spiral-like structures in the near-IR image obtained with the Subaru Telescope. We presen…

astro-ph.GA2014

Molecular Gas in the X-ray Bright Group NGC 5044 as Revealed by ALMA

Laurence P. David, Jeremy Lim, William Forman +17

A short 30 minute ALMA observation of the early-type galaxy NGC 5044, which resides at the center of an X-ray bright group with a moderate cooling flow, has detected 24 molecular s…

astro-ph.GA2023

A Lens Finder Map to check claimed High-z Galaxies behind SMACS J0723.3-7327

Alex Chow, Sung Kei Li, Tom Broadhurst +5

The first science image released by the JWST reveals numerous galaxies in the distant background of the galaxy cluster SMACS J0723.3-7327. Some have claimed redshifts of up to $z \…

astro-ph.GA2022

Recent Formation of a Spiral Disk Hosting Progenitor Globular Clusters at the center of the Perseus Brightest Cluster Galaxy: II. Progenitor Globular Clusters

Jeremy Lim, Emily Wong, Youichi Ohyama +1

We address the nature and origin of Super Star Clusters (SSCs) discovered by Holtzman et al. (1992) within a radius of from the center of NGC 1275, the giant ell…

astro-ph.SR2016

Rotationally-Driven Fragmentation for the Formation of the Binary Protostellar System L1551 IRS 5

Jeremy Lim, Paul K. H. Yeung, Tomoyuki Hanawa +3

Either bulk rotation or local turbulence is widely invoked to drive fragmentation in collapsing cores so as to produce multiple star systems. Even when the two mechanisms predict d…

astro-ph.GA2017

Role of Electon Excitation and Nature of Molecular Gas in Cluster Central Elliptical Galaxies

Jeremy Lim, Dinh-V-Trung, Jan Vrtilek +2

We present observations in CO(3-2) that, combined with previous observations in CO(2-1), constrain the physical properties of the filamentary molecular gas in the central 6.5…

astro-ph.CO2009

A Multiwavelength Study of a Young, Z-shaped, FR I Radio Galaxy NGC 3801

Ananda Hota, Jeremy Lim, Youichi Ohyama +3

We present preliminary results from a multi-wavelength study of a merger candidate, NGC3801, hosting a young FR I radio galaxy, with a Z-shaped structure. Analysing archival data f…

astro-ph.CO2024

Dark Matter distinguished by skewed microlensing in the "Dragon Arc"

Tom Broadhurst, Sung Kei Li, Amruth Alfred +18

Microlensed stars recently discovered by JWST & HST follow closely the winding critical curve of A370 along all sections of the ``Dragon Arc" traversed by the critical curve. These…

astro-ph.SR2016

Formation of the Unequal-Mass Binary Protostars in L1551 NE by Rotationally-Driven Fragmentation

Jeremy Lim, Tomoyuki Hanawa, Paul K. H. Yeung +3

We present observations at 7 mm that fully resolve the two circumstellar disks, and a reanalyses of archival observations at 3.5 cm that resolve along their major axes the two ioni…

astro-ph2008

First Confirmed Detection of a Bipolar Molecular Outflow from a Young Brown Dwarf

Ngoc Phan-Bao, Basmah Riaz, Chin-Fei Lee +6

Studying the earliest stages in the birth of stars is crucial for understanding how they form. Brown dwarfs with masses between that of stars and planets are not massive enough to…

astro-ph.SR2017

Dense molecular clumps in the envelope of the yellow hypergiant IRC+10420

Dinh-V-Trung, Ka-Tat Wong, Jeremy Lim

The circumstellar envelope of the hypergiant star IRC+10420 has been traced as far out in SiO J=2-1 as in CO J = 1-0 and CO J = 2-1, in dramatic contrast with the centrally condens…

astro-ph.GA2024

Tracing Outflows from Stellar Feedback in the Early Universe with Lyman-

James Nianias, Jeremy Lim, Yik Lok Wong +3

Blind spectroscopy of massive lensing galaxy clusters with MUSE has revealed large numbers of gravitationally-lensed Lyman- emitters exhibiting asymmetric profiles at $ 2.9 \l…

astro-ph.CO2016

A Free-Form mass model of the Hubble Frontier Fields Cluster AS1063 (RXC J2248.7-4431) with over one hundred constraints

Jose M. Diego, Tom Broadhurst, Jess Wong +5

We derive a free-form mass distribution for the massive cluster AS1063 (z=0.348) using the completed optical imaging from the Hubble Frontier Fields programme. Based on a subset of…

astro-ph2008

Prevalence of Tidal Interactions among Local Seyfert Galaxies

Cheng-Yu Kuo, Jeremy Lim, Ya-Wen Tang +1

No mechanisms have hitherto been conclusively demonstrated to be responsible for initiating optically-luminous nuclear (Seyfert) activity in local disk galaxies. Only a small minor…

astro-ph.SR2022

Resolving the collimation zone of an intermediate-mass protostar

Adriana R. Rodríguez-Kamenetzky, Carlos Carrasco-González, Luis Felipe Rodríguez Jorge +12

We report new VLA and e-MERLIN high resolution and sensitivity images of the Triple Radio continuum Source in the Serpens star forming region. These observations allowed us to perf…

astro-ph.GA2025

JWST's PEARLS: A z=6 quasar in a train-wreck galaxy merger system

Madeline A. Marshall, Rogier A. Windhorst, Giovanni Ferrami +35

We present JWST NIRSpec integral field spectroscopy observations of the z=5.89 quasar NDWFS J1425+3254 from 0.6-5.3 microns, covering the rest-frame ultraviolet and optical at a sp…

astro-ph.CO2025

Magnification bias reveals severe contamination in Hubble Frontier Field photo-z catalogs

Jiashuo Zhang, Jeremy Lim, Tom Broadhurst +4

Gravitational lensing by massive galaxy clusters enables faint distant galaxies to be more abundantly detected than in blank fields, thereby allowing one to construct galaxy lumino…

astro-ph.CO2009

Multiple Radial Cool Molecular Filaments in NGC 1275

I-Ting Ho, Jeremy Lim, Dinh-V-Trung

We have extended our previous observation (Lim et al. 2008) of NGC1275 covering a central radius of ~10kpc to the entire main body of cool molecular gas spanning ~14kpc east and we…

astro-ph2002

Molecular Gas Reservoir in low-z Powerful Radio Galaxies

Jeremy Lim, Stephane Leon, Francoise Combes +1

We report a survey for molecular gas in 3C radio galaxies at redshifts z < 0.031. Four of the twenty-three galaxies observed were detected with molecular gas masses in the range 10…