Next: Emission-line galaxies Up: The Hamburg/SAO Survey for Previous: Data reduction . ... Among them 128 are new or confirmed emission line galaxies, 6 are quasars (all with redshifts in the range 2.93 to 3.35) and 23 are galaxies without emission lines (only 5 of them have good enough S/N ratio to identify absorption features and to measure redshifts). ... Emission-line galaxies . ... Non emission-line objects . Absorption line galaxies . Stellar objects . Non-classified objects . ...

... Enhancing the Legacy of HST Spectroscopy . ... HST . ... Data . ... Science Blog . ... The Enhancing the Legacy of HST Spectroscopy workshop will take place November 15-16, 2012 at the Space Telescope Science Institute in Baltimore, Maryland. ... Alessandra Aloisi (Space Telescope Science Institute, chair) . Stefano Casertano (Space Telescope Science Institute, co-chair) . ... Alex Fullerton (Space Telescope Science Institute) . ... Claus Leitherer (Space Telescope Science Institute) . ...

The high-redshift radio-loud quasar PKS 2126-158 is found to have a large number of red galaxies in close apparent proximity.We use the Gemini Multi-Object Spectrograph (GMOS) on Gemini South to obtain optical spectra for a large fraction of these sources. We show that there is a group of galaxies at z 0.66, coincident with a metal-line absorption system seen in the quasar s optical spectrum. ... All confirmed members exhibit early-type galaxy spectra, a rare situation for a MgII absorbing system. ...

is split into spectral colours, corresponding to wavelength. Red light has long wavelengths, blue light has short wavelengths. from hot objects are continuous , like a rainbow . atoms only emit light of specific colours, revealing their fingerprints as a line spectrum . atoms in front of a hot object absorb light at these colours, giving an absorption spectrum . are predominantly absorption spectra . next

... The spectroscopic follow-up program of the X-ray sources detected in the 942 ksec exposure of the Chandra Deep Field South has been carried out with the ESO Very Large Telescope ( VLT ) in the time frame April 2000-December 2001 [ESO no. ... Table 5, finding charts, 1&2D spectra can be found at the following URLs: . Table 5 ASCII . Table 5 HTML . Finding charts (click on the ID number in the table) . 1 2D spectra (click on the ID number in the table) ...

... Laboratory for Spectroscopy of Molecular Structures . ... Optics and spectroscopy of molecular and liquid crystals, fullerenes, superthin molecular films. Optical studies of structure, phase transitions, pretransitional phenomena, structural modifications in external field and under high pressure. ... Methods developed in the laboratory enable to determine in free standing films of different types liquid crystals values of polarization, two-dimensional constants of orientational elasticity. ...

. Ivan Najdenov, Nicolai Somov, Tatjana Somova.

... MASTER COMPILATION of GOODS/CDF-S spectroscopy . CDF-S Master Spectroscopic Catalog - v1.2 ( 26/08/2004): . ... Vanzella et al., 2004, (astro-ph/0406591) . VLT/FORS2 spectroscopy . ... Le Fevre et al., 2004, (astro-ph/0403628) . ... Szokoly et al.,2004, (astro-ph/0312324) . ... 2004 ApJ 600 L99 . ... 2004, ApJ, 602, L5 . ... Strolger at al.,2004,(astro-ph/0406546) . ... ESO/WFI-R image with marked objects with existing public spectroscopic data in the GOODS/CDF-S area . ...

... A2267 Date Received: 2006-Oct-02 15:17:40 Technical Page Proposal Type: General Category : Sub- Category : Observation Category : Total Time Requested: Minimum Useful Time : Prop osal Title: ABSTRACT: Regular Astronomy Spectroscopy Extragalactic 10 Hours A search for 6 GHz OH lines at z 0.25 We propose to use the Arecibo 6-band receiver to obtain high resolution spectra of the redshifted OH J=5/2 excited-state transitions ...

... Registration of Attenuated Total Reflection (ATR) spectrum of a sample, contacting with the ATR-prism. ... studies of fine-grain material after landing: surface dust, precipitating atmospheric aerosols, samples taken by a robotic arm (or a drill); . studies of aerosols during descend (or flight aboard a balloon) in an atmosphere; . ... The ATR-technique was not used before in planetary exploration experiments and it’s development is aimed for future projects for Mars exploration. ...