Search Publications

Dracula's Chivito: Discovery of a Large Edge-on Protoplanetary Disk with Pan-STARRS
DOI: 10.3847/2041-8213/ad43e3 Bibcode: 2024ApJ...967L...3B

Drake, Jeremy J.; Bayyari, Ammar; Russell, Ray W. +6 more

We report the serendipitous discovery of a large edge-on protoplanetary disk in Pan-STARRS (PS1) images. PS1 has five broadband filters designated as g P1, r P1, i P1, z P1, and y P1 with mean wavelengths 4866, 6215, 7545, 8679, and 9633 Å, respectively. The disk's apparent size in the PS1 ima…

2024 The Astrophysical Journal
AKARI Gaia 6
AMICO-COSMOS galaxy cluster and group catalogue up to z = 2: Sample properties and X-ray counterparts
DOI: 10.1051/0004-6361/202348832 Bibcode: 2024A&A...687A..56T

Finoguenov, A.; Castignani, G.; Moscardini, L. +2 more


Aims: We present the results of a new galaxy cluster search in the COSMOS field obtained using the Adaptive Matched Identifier of Clustered Objects (AMICO). Our aim was to produce a new cluster and group catalogue up to z = 2 by performing an innovative application of AMICO with respect to previous successful applications to wide-field survey…

2024 Astronomy and Astrophysics
Gaia 6
Improved modelling of SEP event onset within the WSA-Enlil-SEPMOD framework
DOI: 10.1051/swsc/2024001 Bibcode: 2024JSWSC..14....3P

Richardson, Ian G.; Auster, Hans-Ulrich; Palmerio, Erika +14 more

Multi-spacecraft observations of solar energetic particle (SEP) events not only enable a deeper understanding and development of particle acceleration and transport theories but also provide important constraints for model validation efforts. However, because of computational limitations, a given physics-based SEP model is usually best suited to c…

2024 Journal of Space Weather and Space Climate
SOHO SolarOrbiter 6
JWST/NIRCam Imaging of Young Stellar Objects. II. Deep Constraints on Giant Planets and a Planet Candidate Outside of the Spiral Disk Around SAO 206462
DOI: 10.3847/1538-3881/ad1ffc Bibcode: 2024AJ....167..182C

Dong, Ruobing; Wolff, Schuyler G.; Johnstone, Doug +17 more

We present JWST/NIRCam F187N, F200W, F405N, and F410M direct imaging data of the disk surrounding SAO 206462. Previous images show a very structured disk, with a pair of spiral arms thought to be launched by one or more external perturbers. The spiral features are visible in three of the four filters, with the nondetection in F410M due to the larg…

2024 The Astronomical Journal
JWST 6
The Next Step in Galaxy Cluster Strong Lensing: Modeling the Surface Brightness of Multiply Imaged Sources
DOI: 10.3847/1538-4357/ad8343 Bibcode: 2024ApJ...976..110A

Acebron, Ana; Nonino, Mario; Grillo, Claudio +12 more

Overcoming both modeling and computational challenges, we present, for the first time, the extended surface-brightness distribution model of a strongly lensed source in a complex galaxy-cluster-scale system. We exploit the high-resolution Hubble Space Telescope (HST) imaging and extensive Multi Unit Spectroscopic Explorer spectroscopy to build an …

2024 The Astrophysical Journal
eHST 6
The EBLM Project XII. An eccentric, long-period eclipsing binary with a companion near the hydrogen-burning limit
DOI: 10.1093/mnras/stae842 Bibcode: 2024MNRAS.530.2565D

Trifonov, Trifon; Henning, Thomas; Triaud, Amaury H. M. J. +17 more

In the hunt for Earth-like exoplanets, it is crucial to have reliable host star parameters, as they have a direct impact on the accuracy and precision of the inferred parameters for any discovered exoplanet. For stars with masses between 0.35 and 0.5 M, an unexplained radius inflation is observed relative to typical stellar models. How…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 6
Gaia FGK benchmark stars: Fundamental Teff and log g of the third version
DOI: 10.1051/0004-6361/202347136 Bibcode: 2024A&A...682A.145S

Casamiquela, L.; Creevey, O. L.; Soubiran, C. +8 more

Context. Large spectroscopic surveys devoted to the study of the Milky Way, including Gaia, use automated pipelines to determine the atmospheric parameters of millions of stars. The Gaia FGK benchmark stars are reference stars with Teff and log 𝑔 derived through fundamental relations, independently of spectroscopy, to be used as anchors…

2024 Astronomy and Astrophysics
AKARI Gaia 6
AGN feedback in the Local Universe: Multiphase outflow of the Seyfert galaxy NGC 5506
DOI: 10.1051/0004-6361/202449245 Bibcode: 2024A&A...686A..46E

Vallini, Livia; Alonso-Herrero, Almudena; Ricci, Claudio +21 more

We present new optical GTC/MEGARA seeing-limited (0.9″) integral-field observations of NGC 5506, together with ALMA observations of the CO(3 − 2) transition at a 0.2″ (∼25 pc) resolution. NGC 5506 is a luminous (bolometric luminosity of ∼1044 erg s−1) nearby (26 Mpc) Seyfert galaxy, part of the Galaxy Activity, Torus, and Out…

2024 Astronomy and Astrophysics
eHST 6
The Green Monster Hiding in Front of Cas A: JWST Reveals a Dense and Dusty Circumstellar Structure Pockmarked by Ejecta Interactions
DOI: 10.3847/2041-8213/ad855d Bibcode: 2024ApJ...976L...4D

Temim, Tea; Rest, Armin; Blair, William P. +27 more

JWST observations of the young Galactic supernova remnant Cassiopeia A revealed an unexpected structure seen as a green emission feature in colored composite MIRI F1130W and F1280W images—hence dubbed the Green Monster—that stretches across the central parts of the remnant in projection. Combining the kinematic information from NIRSpec and the MIR…

2024 The Astrophysical Journal
eHST JWST 6
X-Ray and Multiwavelength Polarization of Mrk 501 from 2022 to 2023
DOI: 10.3847/1538-4357/ad63a1 Bibcode: 2024ApJ...974...50C

Kaaret, Philip; Wu, Kinwah; Enoto, Teruaki +143 more

We present multiwavelength polarization measurements of the luminous blazar Mrk 501 over a 14 month period. The 2–8 keV X-ray polarization was measured with the Imaging X-ray Polarimetry Explorer (IXPE) with six 100 ks observations spanning from 2022 March to 2023 April. Each IXPE observation was accompanied by simultaneous X-ray data from NuSTAR,…

2024 The Astrophysical Journal
XMM-Newton 6