- ID:
- ivo://irsa.ipac/Herschel/Spectra/GOT_Cplus
- Title:
- Galactic Observations of Terahertz C+
- Short Name:
- GOT_Cplus
- Date:
- 04 Oct 2024 00:04:13
- Publisher:
- NASA/IPAC Infrared Science Archive
- Description:
- Herschel data from the 'Galactic Observations of Terahertz C' (GOT Cplus) Open Time Key Program (KPOT_wlanger_1) are available here using spatial and visualization tools. GOT Cplus surveyed the Galactic Plane in the 158 micron (1.9 THz) fine structure transition of [CII] using Herschel's HIFI instrument. GOT Cplus is a sparse survey containing 454 lines of sight throughout the Galactic Disk, plus two position-velocity maps across the Galactic center.
1 - 7 of 7
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- ID:
- ivo://irsa.ipac/SSA
- Title:
- IRSA Simple Spectral Access (SSA) Protocol Service
- Short Name:
- IRSA SSA
- Date:
- 06 May 2021 17:44:00
- Publisher:
- NASA/IPAC Infrared Science Archive
- Description:
- This is IRSA's implementation of the IVOA Simple Spectral Access (SSA) protocol. Our SSA service allows a rich variety of searches against IRSA's varied holdings.
3. SOFIA EXES
- ID:
- ivo://irsa.ipac/SOFIA/Spectra/EXES
- Title:
- SOFIA EXES
- Short Name:
- SOFIA_EXES
- Date:
- 06 Sep 2024 20:25:59
- Publisher:
- NASA/IPAC Infrared Science Archive
- Description:
- EXES operated in the 4.5 - 28.3 um wavelength region, at high (R ~ 50,000 - 100,000), medium (R ~ 5000 - 20,000) and low (R . 1000 - 3000) spectral resolution.
- ID:
- ivo://irsa.ipac/SOFIA/Spectra/FIFI-LS
- Title:
- SOFIA FIFI-LS
- Short Name:
- SOFIA_FIFI-LS
- Date:
- 06 Sep 2024 20:37:21
- Publisher:
- NASA/IPAC Infrared Science Archive
- Description:
- FIFI-LS was an integral field, far-infrared spectrometer. The instrument included two independent grating spectrometers sharing a common field of view (FOV). The short wavelength spectrometer (blue channel) operated in the 51 - 120 um wavelength region, and the long wavelength spectrometer (red channel) covered 115 - 200 um. The spectral resolution ranged from 600 to 2,000 dependent on the observed wavelength, with higher values towards the long wavelength ends of each spectrometer.
- ID:
- ivo://irsa.ipac/SOFIA/Spectra/FLITECAM
- Title:
- SOFIA FLITECAM
- Short Name:
- SOFIA_FLITECAM
- Date:
- 06 Sep 2024 20:30:57
- Publisher:
- NASA/IPAC Infrared Science Archive
- Description:
- FLITECAM was an infrared camera operating in the 1.0 - 5.5 um waveband. It consisted of a 1024x1024 InSb detector with 0.475"x0.475" pixels and used refractive optics to provide an 8' diameter field of view. The instrument had a set of filters for imaging, and grisms for moderate resolution spectroscopy. The filter suite consisted of standard Barr filters used for imaging at J, H, K, L and M in one filter wheel. A second filter wheel held a selection of narrow-band imaging filters including Pa-alpha, Pa-alpha continuum, 3.07 um H2O ice, 3.3 um PAH, L-narrow and M-narrow. Additionally there were order sorting filters for use with the grisms. A selection of three grisms was available to provide medium resolution (R ~ 1500) spectra over the entire wavelength range.
- ID:
- ivo://irsa.ipac/SOFIA/Spectra/FORCAST
- Title:
- SOFIA FORCAST
- Short Name:
- SOFIA_FORCAST
- Date:
- 06 Sep 2024 20:31:04
- Publisher:
- NASA/IPAC Infrared Science Archive
- Description:
- FORCAST was a dual-channel mid-infrared camera and spectrograph sensitive from 5 - 40 um. Spectroscopy was also possible using a suite of grisms, which provided coverage from 5 - 40 um with a low spectral resolution of R ~ 200.
7. SOFIA GREAT
- ID:
- ivo://irsa.ipac/SOFIA/Spectra/GREAT
- Title:
- SOFIA GREAT
- Short Name:
- SOFIA_GREAT
- Date:
- 06 Sep 2024 20:31:14
- Publisher:
- NASA/IPAC Infrared Science Archive
- Description:
- The German REceiver for Astronomy at Terahertz Frequencies (GREAT) was a modular heterodyne instrument with multiple configurations that provided high-resolution spectra (up to R = 1e8) in several frequency windows between 0.4900-4.7448 THz.