Search Publications

A photodissociation region (PDR) model grid in planetary nebula paradigm: dependency of C and O fine structure line emission and PDR thermal structure on central star radiation and nebular dust composition
DOI: 10.1093/mnras/stad1129 Bibcode: 2023MNRAS.523..498B

Das, Ramkrishna; Bandyopadhyay, Rahul

We compute a grid of photodissociation region (PDR) models. The varying parameters of the grid include effective temperature (Teff) and luminosity (L) of the radiation source, density (nH) of the nebula, PDR depth from the nebular ionization front (ΔrPDR), and densities of polycyclic aromatic hydrocarbon (PAH) mole…

2023 Monthly Notices of the Royal Astronomical Society
Herschel ISO 0
Variable stars in the field of open cluster NGC 6819
DOI: 10.51194/INASAN.2023.8.3.002 Bibcode: 2023INASR...8..114G

Karimov, R. G.; Gaysin, R. A.

Here we present preliminary results of searching and study of variable stars based on space observation data of the TESS mission in the field of the open star cluster NGC 6819. The light curves of variable stars of various types located in the field of an open cluster are studied. Based on the data from the GAIA DR3 mission, the probable members o…

2023 INASAN Science Reports
Gaia 0
Variation of temperature and non-thermal velocity with height in fan loops
DOI: 10.1093/mnras/stad2359 Bibcode: 2023MNRAS.525.1657S

Tripathi, Durgesh; Sharma, Aishawnnya

We study the variation of temperature and non-thermal velocity with height in fan loops. For this purpose, we have used the observations recorded by the Extreme Ultraviolet Imaging Spectrometer onboard Hinode. We have employed the emission measure (EM)-loci method to estimate the temperatures of different coronal fan loops and then compute the non…

2023 Monthly Notices of the Royal Astronomical Society
Hinode 0
A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km s-1 Mpc-1 Uncertainty from the Hubble Space Telescope and the SH0ES Team
DOI: 10.3847/2041-8213/ac5c5b Bibcode: 2022ApJ...934L...7R

Casertano, Stefano; Filippenko, Alexei V.; Jones, David O. +15 more

We report observations from the Hubble Space Telescope (HST) of Cepheid variables in the host galaxies of 42 Type Ia supernovae (SNe Ia) used to calibrate the Hubble constant (H 0). These include the complete sample of all suitable SNe Ia discovered in the last four decades at redshift z ≤ 0.01, collected and calibrated from ≥1000 HST o…

2022 The Astrophysical Journal
Gaia eHST 1623
The Pantheon+ Analysis: Cosmological Constraints
DOI: 10.3847/1538-4357/ac8e04 Bibcode: 2022ApJ...938..110B

Filippenko, Alexei V.; Coulter, David A.; Foley, Ryan J. +45 more

We present constraints on cosmological parameters from the Pantheon+ analysis of 1701 light curves of 1550 distinct Type Ia supernovae (SNe Ia) ranging in redshift from z = 0.001 to 2.26. This work features an increased sample size from the addition of multiple cross-calibrated photometric systems of SNe covering an increased redshift span, and im…

2022 The Astrophysical Journal
eHST 770
Challenges for ΛCDM: An update
DOI: 10.1016/j.newar.2022.101659 Bibcode: 2022NewAR..9501659P

Perivolaropoulos, L.; Skara, F.

A number of challenges to the standard ΛCDM model have been emerging during the past few years as the accuracy of cosmological observations improves. In this review we discuss in a unified manner many existing signals in cosmological and astrophysical data that appear to be in some tension (2 σ or larger) with the standard ΛCDM model as specified …

2022 New Astronomy Reviews
Gaia 659
The Pantheon+ Analysis: The Full Data Set and Light-curve Release
DOI: 10.3847/1538-4357/ac8b7a Bibcode: 2022ApJ...938..113S

Filippenko, Alexei V.; Kilpatrick, Charles D.; Coulter, David A. +27 more

Here we present 1701 light curves of 1550 unique, spectroscopically confirmed Type Ia supernovae (SNe Ia) that will be used to infer cosmological parameters as part of the Pantheon+ SN analysis and the Supernovae and H 0 for the Equation of State of dark energy distance-ladder analysis. This effort is one part of a series of works that …

2022 The Astrophysical Journal
eHST 517
Euclid preparation. I. The Euclid Wide Survey
DOI: 10.1051/0004-6361/202141938 Bibcode: 2022A&A...662A.112E

Aussel, H.; Cimatti, A.; Schultheis, M. +242 more

Euclid is a mission of the European Space Agency that is designed to constrain the properties of dark energy and gravity via weak gravitational lensing and galaxy clustering. It will carry out a wide area imaging and spectroscopy survey (the Euclid Wide Survey: EWS) in visible and near-infrared bands, covering approximately 15 000 deg2

2022 Astronomy and Astrophysics
Gaia 387
Two Remarkably Luminous Galaxy Candidates at z ≈ 10-12 Revealed by JWST
DOI: 10.3847/2041-8213/ac9b22 Bibcode: 2022ApJ...940L..14N

Strait, Victoria; van Dokkum, Pieter; Conroy, Charlie +22 more

The first few 100 Myr at z > 10 mark the last major uncharted epoch in the history of the universe, where only a single galaxy (GN-z11 at z ≈ 11) is currently spectroscopically confirmed. Here we present a search for luminous z > 10 galaxies with JWST/NIRCam photometry spanning ≈1-5 µm and covering 49 arcmin2 from the public…

2022 The Astrophysical Journal
Gaia eHST JWST 386
The LOFAR Two-metre Sky Survey. V. Second data release
DOI: 10.1051/0004-6361/202142484 Bibcode: 2022A&A...659A...1S

Prandoni, I.; Zhang, X.; Di Gennaro, G. +103 more

In this data release from the ongoing LOw-Frequency ARray (LOFAR) Two-metre Sky Survey we present 120-168 MHz images covering 27% of the northern sky. Our coverage is split into two regions centred at approximately 12h45m +44°30' and 1h00m +28°00' and spanning 4178 and 1457 square degrees respectively. The images were derived from 3451 h (7.6 PB) …

2022 Astronomy and Astrophysics
Gaia 370