The Cosmic Origins Spectrograph
arXiv:1110.0462 · doi:10.1088/0004-637X/744/1/60
Abstract
The Cosmic Origins Spectrograph (COS) is a moderate-resolution spectrograph with unprecedented sensitivity that was installed into the Hubble Space Telescope (HST) in May 2009, during HST Servicing Mission 4 (STS-125). We present the design philosophy and summarize the key characteristics of the instrument that will be of interest to potential observers. For faint targets, with flux F_lambda ~ 1.0E10-14 ergs/s/cm2/Angstrom, COS can achieve comparable signal to noise (when compared to STIS echelle modes) in 1-2% of the observing time. This has led to a significant increase in the total data volume and data quality available to the community. For example, in the first 20 months of science operation (September 2009 - June 2011) the cumulative redshift pathlength of extragalactic sight lines sampled by COS is 9 times that sampled at moderate resolution in 19 previous years of Hubble observations. COS programs have observed 214 distinct lines of sight suitable for study of the intergalactic medium as of June 2011. COS has measured, for the first time with high reliability, broad Lya absorbers and Ne VIII in the intergalactic medium, and observed the HeII reionization epoch along multiple sightlines. COS has detected the first CO emission and absorption in the UV spectra of low-mass circumstellar disks at the epoch of giant planet formation, and detected multiple ionization states of metals in extra-solar planetary atmospheres. In the coming years, COS will continue its census of intergalactic gas, probe galactic and cosmic structure, and explore physics in our solar system and Galaxy.
17 pages, 15 figures
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- DIISC-I: The Discovery of Kinematically Anomalous HI Clouds in M 100
- Transient obscuration event captured in NGC 3227 IV. Origin of the obscuring cloud variability
- Investigating the Lyman photon escape in local starburst galaxies with the Cosmic Origins Spectrograph
- The MUSE Extremely Deep Field: Classifying the Spectral Shapes of Lya Emitting Galaxies
- DIISC-II: Unveiling the Connections between Star Formation and ISM in the Extended Ultraviolet Disk of NGC 3344
- AGN STORM 2: I. First results: A Change in the Weather of Mrk 817
- FORECASTOR -- I. Finding Optics Requirements and Exposure times for the Cosmological Advanced Survey Telescope for Optical and UV Research mission
- A Detection of Gas Associated with the M 31 Stellar Stream
- Multiwavelength campaign on Mrk 509. XVI. Continued HST/COS monitoring of the far-ultraviolet spectrum
- NGTS and HST insights into the long period modulation in GW Librae
- HeII Ly Transmission Spikes and Absorption Troughs in Eight High-resolution Spectra Probing the End of HeII Reionization
- X-Shooting ULLYSES: Massive Stars at Low Metallicity X. Physical Parameters and Feedback of Massive Stars in the LMC N11 B Star-Forming Region
- Scientific Objectives for UV/Visible Astrophysics Investigations: A Summary of Responses by the Community (2012)
- A half-ring of ionized circumstellar material trapped in the magnetosphere of a white dwarf merger remnant
- Spectroscopic Investigation of Nebular Gas (SING): Instrument Design, Assembly and Calibration
- Multi-wavelength spectroscopic analysis of the ULX Holmberg II X-1 and its nebula suggests the presence of a heavy black hole accreting from a B-type donor
- X-Shooting ULLYSES: Massive stars at low metallicity. XIII. Putting the bi-stability jump to the test in the LMC
- Extremely iron-poor O-type stars in the Magellanic Bridge
- New Gapless COS G140L Mode Proposed for Background-Limited Far-UV Observations
- Identifying the Lens Galaxy B1152+199 as a Ghostly Damped Lyman Alpha System by the Cosmic Origins Spectrograph
- The COS-Holes Survey: Connecting Galaxy Black Hole Mass with the State of the CGM
- Absorption line abundances in the SMC-like galaxy UGC 5282: evidence for ISM dilution from inflows on kiloparsec scales
- Evidence of a Disk-wind Origin for Fluorescent H in Classical T Tauri Stars
- On the Size and Mass of Photo-ionized Clouds in Extended Spiral Galaxy Halos
- zELDA II: reconstruction of galactic Lyman-alpha spectra attenuated by the intergalactic medium using neural networks
- CHESS: an Innovative Concept for High-Resolution, Far-UV Spectroscopy
- Optical design options for Pollux: UV spectropolarimeter project for the Habitable Worlds Observatory
- The igmspec Database of Public Spectra Probing the Intergalactic Medium
- MUSEQuBES: Physical conditions, origins, and multi-element abundances of the circumgalactic medium of an isolated, star-forming dwarf galaxy at z=0.57
- Ultraviolet Spectra of Comets: Rejecting the Detection of Pentacene, Toluene, and Fe+
- Far-UV Fe Emission as Proxy of Eddington Ratios
- Modelling gas around galaxy pairs and groups using the Q0107 quasar triplet
- UV astronomy with small satellites
- The Near Ultraviolet Transient Surveyor (NUTS): An ultraviolet telescope to observe variable sources
- UV counterpart of an X-ray ultra-fast outflow in IRAS 17020+4544
- The Halo21 Absorption Modeling Challenge: Lessons From "Observing" Synthetic Circumgalactic Absorption Spectra
- Spectroscopic Line Modeling of the Fastest Rotating O-type Stars
- Stellar flare-driven evolution of primordial early exo-Earth atmospheres: Insights from a Young M Dwarf Flare model
- Unveiling the faint ultraviolet Universe
- Observations of the Bright Star in the Globular Cluster 47 Tucanae (NGC 104)
- Studying the gaseous outskirts of galaxy groups with coherent Ly alpha absorption patterns