We are improving our search experience. To check which content you have full access to, or for advanced search, go back to the old search.

Search

Please fill in this field.
Filters applied:

Search Results

Showing 1-20 of 10,000 results
  1. Iron Line Emission in X-Ray Afterglows

    Recent observations of X-ray afterglows reveal the presence of a redshifted K...
    Davide Lazzati, Gabriele Ghisellini, ... Luigi Stella in Gamma-Ray Bursts in the Afterglow Era
    Conference paper
  2. Line Emission

    Stefanie N. Milam in Encyclopedia of Astrobiology
    Reference work entry 2023
  3. 4.7 μm CO and H2 Line Emission in NGC 2071

    Two lines of the fundamental vibration-rotation band of carbon monoxide at 4.7 μm have been detected in emission in the NGC 2071 IR out.ow region,...
    Dolores M. Walther, Thomas R. Geballe in High Resolution Infrared Spectroscopy in Astronomy
    Conference paper
  4. A Search for Emission Line Galaxies at z = 6.5

    We are carrying out a search for Lyα emitting galaxies at z = 6.5 employing slitless spectroscopy at the VLT. In our 43 arcmin2 field we find three...
    Jaron Kurk, Andrea Cimatti, ... Emanuele Daddi in Multiwavelength Map** of Galaxy Formation and Evolution
    Conference paper
  5. Linear Spectropolarimetry of Young and Other Emission Line Stars

    The aim of this article is to demonstrate the useful role that can be played by spectropolarimetric observations of young and evolved emission line...
    Janet E. Drew, Jorick S. Vink, ... René D. Oudmaijer in High Resolution Infrared Spectroscopy in Astronomy
    Conference paper
  6. Modeling Emission Line Galaxies

    Predicting the emission line signals from galaxies and IGM observed in the future experiments is crucial for their interpretation as well as for...
    Chapter 2022
  7. Analysis of Emission Line Widths of [CII] 158μm

    A study of [CII] 158 μm emission line profiles observed with Herschel PACS for 379 galaxies is presented. Emission line widths are compared to [CII]...

    A. L. Samsonyan in Astrophysics
    Article 01 June 2022
  8. Implementation of Line Search for Parafac Analysis of Fluorescence Excitation–Emission Matrix

    Recovery of fluorophore groups in dissolved organic matter using the PARAFAC canonical tensor decomposition of fluorescence excitation–emission...

    I. N. Krylov, I. V. Seliverstova, T. A. Labutin in Journal of Applied Spectroscopy
    Article 11 March 2023
  9. The Masses of Distant Galaxies from Optical Emission Line Widths

    Promising methods for studying galaxy evolution rely on optical emission line width measurements to compare intermediate-redshift objects to galaxies...
    Elizabeth Barton Gillespie, Liese van Zee in The Mass of Galaxies at Low and High Redshift
    Conference paper
  10. Understanding the long-term evolution of green line coronal emission and its relation to the sunspots

    Significant association between flux emergence and the complexity of the involved processes in the solar corona could be substantial in estimating...

    Jacob Oloketuyi, Yu Liu, ... Linhua Deng in Astrophysics and Space Science
    Article 08 April 2024
  11. Performance evaluation of Littrow lens assembly for Visible Emission Line Corongraph (VELC) on board Aditya-L1 mission

    Visible Emission Line Coronagraph (VELC) is the prime payload among the seven payloads on board Aditya-L1 mission. VELC is a dedicated payload for...

    Venkata Suresh Narra, Vishweshwar Rao Budhiraju, ... Raghavendra Prasad Budihal in Journal of Optics
    Article 02 July 2023
  12. Photoluminescence Spectra and Unusual Temperature Shift of Zero-Phonon Emission Line of V3+ in SrTiO3

    Abstract

    The paper presents the first observation of photoluminescence spectra of V 3+ impurity in SrTiO 3 . The broad band of the observed emission is...

    A. P. Skvortsov, Z. Potuček, ... V. A. Trepakov in Optics and Spectroscopy
    Article 01 March 2023
  13. Visible Emission Line Spectroscopy of the Solar Corona During the 2019 Total Solar Eclipse

    Spectroscopic measurements of the low solar corona are crucial to understanding the mechanisms that heat the corona and accelerate the solar wind,...

    Gabriel D. Muro, Matt Gunn, ... Huw Morgan in Solar Physics
    Article Open access 12 June 2023
  14. The Solar Line Emission Dopplerometer project

    Observations of the dynamics of solar coronal structures are necessary to investigate space weather phenomena and global heating of the corona. The...

    Jean-Marie Malherbe, Pierre Mein, ... Jan Rybák in Experimental Astronomy
    Article 20 October 2021
  15. Emission Measures Demystified

    We review the terms spectral radiance and spectral irradiance, and show how their precise definitions are crucial for interpreting observations made...

    Brian R. Dennis, Kenneth J. H. Phillips in Solar Physics
    Article 16 April 2024
  16. Spectropolarimetry package for visible emission line coronagraph (VELC) on board Aditya-L1 mission

    One of the unique features of Visible Emission Line Coronagraph (VELC) on board Aditya-L1 mission is spectropolarimetric observations in coronal...

    Suresh Venkata, Raghavendra Prasad B, Jagdev Singh in Experimental Astronomy
    Article 12 January 2022
  17. Emission Line Measurements in the Magnified z = 3.357 HII Region Behind a Cluster at z = 0.54

    Emission line spectroscopy of stellar-photoionized nebulae (HII regions/galaxies) at high redshift is crucial for tracking the chemical evolution of...
    R. A. E. Fosbury, A. Humphrey, ... M. Rauch in The Mass of Galaxies at Low and High Redshift
    Conference paper
  18. Course 10: High Energy Emission of AGN

    We present the most commonly accepted scenarios to account for the properties of the high energy emission in Active Galactic Nuclei (AGN). Because of...
    Conference paper
  19. Prompt and Delayed Emission

    The neutrons and gamma rays emitted after fission have been intensely studied ever since its discovery. The excited fragments return to their ground...
    Matthew Devlin, Alf Göök, ... Ramona Vogt in Nuclear Fission
    Chapter 2023
  20. Multiple soft-photon emission at next-to-leading power to all orders

    This paper derives a next-to-leading power (NLP) soft theorem for multi-photon emission to all orders in the electromagnetic coupling constant,...

    Article Open access 01 March 2024
Did you find what you were looking for? Share feedback.