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J/A+A/612/A6              RX J1713.7-3946 HESS spectrum            (HESS+, 2018)

H.E.S.S. observations of RX J1713.7-3946 with improved angular and spectral resolution: Evidence for gamma-ray emission extending beyond the X-ray emitting shell. H.E.S.S. Collaboration, Abdalla H., Abramowski A., Aharonian F., Ait Benkhali F., Akhperjanian A.G., Andersson T., Anguner E.O., Arrieta M., Aubert P., Backes M., Balzer A., Barnard M., Becherini Y., Becker Tjus J., Berge D., Bernhard S., Bernlohr K., Blackwell R., Bottcher M., Boisson C., Bolmont J., Bordas P., Bregeon J., Brun F., Brun P., Bryan M., Bulik T., Capasso M., Carr J., Casanova S., Cerruti M., Chakraborty N., Chalme-Calvet R., Chaves R.C.G., Chen A., Chevalier J., Chretien M., Colafrancesco S., Cologna G., Condon B., Conrad J., Cui Y., Davids I.D., Decock J., Degrange B., Deil C., Devin J., deWilt P., Dirson L., Djannati-Ata A., Domainko W., Donath A., Drury L.O'C., Dubus G., Dutson K., Dyks J., Edwards T., Egberts K., Eger P., Ernenwein J.-P., Eschbach S., Farnier C., Fegan S., Fernandes M.V., Fiasson A., Fontaine G., Forster A., Fukuyama T., Funk S., Fussling M., Gabici S., Gajdus M., Gallant Y.A., Garrigoux T., Giavitto G., Giebels B., Glicenstein J.F., Gottschall D., Goyal A., Grondin M.-H., Hadasch D., Hahn J., Haupt M., Hawkes J., Heinzelmann G., Henri G., Hermann G., Hervet O., Hinton J.A., Hofmann W., Hoischen C., Holler M., Horns D., Ivascenko A., Jacholkowska A., Jamrozy M., Janiak M., Jankowsky D., Jankowsky F., Jingo M., Jogler T., Jouvin L., Jung-Richardt I., Kastendieck M.A., Katarzynski K., Katz U., Kerszberg D., Khelifi B., Kieffer M., King J., Klepser S., Klochkov D., Kluzniak W., Kolitzus D., Komin Nu., Kosack K., Krakau S., Kraus M., Krayzel F., Kruger P.P., Laffon H., Lamanna G., Lau J., Lees J.-P., Lefaucheur J., Lefranc V., Lemiere A., Lemoine-Goumard M., Lenain J.-P., Leser E., Lohse T., Lorentz M., Liu R., Lopez-Coto R., Lypova I., Marandon V., Marcowith A., Mariaud C., Marx R., Maurin G., Maxted N., Mayer M., Meintjes P.J., Meyer M., Mitchell A.M.W., Moderski R., Mohamed M., Mohrmann L., Mora K., Moulin E., Murach T., de Naurois M., Niederwanger F., Niemiec J., Oakes L., O'Brien P., Odaka H., O ttl S., Ohm S., Ostrowski M., Oya I., Padovani M., Panter M., Parsons R.D., Pekeur N.W., Pelletier G., Perennes C., Petrucci P.-O., Peyaud B., Piel Q., Pita S., Poon H., Prokhorov D., Prokoph H., Puhlhofer G., Punch M., Quirrenbach A., Raab S., Reimer A., Reimer O., Renaud M., de los Reyes R., Rieger F., Romoli C., Rosier-Lees S., Rowell G., Rudak B., Rulten C.B., Sahakian V., Salek D., Sanchez D.A., Santangelo A., Sasaki M., Schlickeiser R., Schussler F., Schulz A., Schwanke U., Schwemmer S., Settimo M., Seyffert A.S., Shafi N., Shilon I., Simoni R., Sol H., Spanier F., Spengler G., Spies F., Stawarz L., Steenkamp R., Stegmann C., Stinzingy F., Stycz K., Sushch I., Takahashi T., Tavernet J.-P., Tavernier T., Taylor A.M., Terrier R., Tibaldo L., Tiziani D., Tluczykont M., Trichard C., Tu R., Uchiyama Y., van der Walt D.J., van Eldik C., van Rensburg C., van Soelen B., Vasileiadis G., Veh J., Venter C., Viana A., Vincent P., Vink J., Voisin F., Volk H.J., Volpe F., Vuillaume T., Wadiasingh Z., Wagner S.J., Wagner P., Wagner R.M., White R., Wierzcholska A., Willmann P., Wornlein A., Wouters D., Yang R., Zabalza V., Zaborov D., Zacharias M., Zdziarski A.A., Zech A., Zefi F., Ziegler A., Zywucka N. <Astron. Astrophys. 612, A6 (2018)> =2018A&A...612A...6H (SIMBAD/NED BibCode)
ADC_Keywords: Gamma rays - Supernova remnants Keywords: acceleration of particles - cosmic rays - ISM: supernova remnants - gamma rays: general - astroparticle physics Abstract: Supernova remnants exhibit shock fronts (shells) that can accelerate charged particles up to very high energies. In the past decade, measurements of a handful of shell-type supernova remnants in very high-energy gamma rays have provided unique insights into the acceleration process. Among those objects, RX J1713.7-3946 (also known as G347.3-0.5) has the largest surface brightness, allowing us in the past to perform the most comprehensive study of morphology and spatially resolved spectra of any such very high-energy gamma-ray source. Here we present extensive new H.E.S.S. measurements of RX J1713.7-3946, almost doubling the observation time compared to our previous publication. Combined with new improved analysis tools, the previous sensitivity is more than doubled. The H.E.S.S. angular resolution of 0.048° (0.036° above 2TeV) is unprecedented in gamma-ray astronomy and probes physical scales of 0.8 (0.6) parsec at the remnant's location. The new H.E.S.S. image of RX J1713.7-3946 allows us to reveal clear morphological differences between X-rays and gamma rays. In particular, for the outer edge of the brightest shell region, we find the first ever indication for particles in the process of leaving the acceleration shock region. By studying the broadband energy spectrum, we furthermore extract properties of the parent particle populations, providing new input to the discussion of the leptonic or hadronic nature of the gamma-ray emission mechanism. Description: FITS files with the very high-energy gamma-ray images, Fig.1, and the spectrum, Fig.3, as ascii text file. Objects: -------------------------------------------------------- RA (2000) DE Designation(s) -------------------------------------------------------- 17 12 27 -39 41.2 RX J1713.7-3946 = HESS J1713-397 -------------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file spectrum.dat 14 30 H.E.S.S. energy flux spectrum of RX J1713.7-3946 (Fig.3 of the paper) list.dat 109 2 List of fits images fits/* 0 2 Individual fits images
See also: J/A+A/612/A1 : H.E.S.S. Galactic Plane Survey (HESS+, 2018) J/A+A/612/A5 : W49B with H.E.S.S. and Fermi-LAT (HESS+, 2018) J/A+A/612/A7 : Vela Junior (RX J0852.0-4622) HESS image (HESS+, 2018) Byte-by-byte Description of file: spectrum.dat
Bytes Format Units Label Explanations
1- 5 F5.2 TeV E Energy 7- 14 E8.3 mW/m2 E2dN/dE Flux
Byte-by-byte Description of file: list.dat
Bytes Format Units Label Explanations
1- 9 F9.5 deg RAdeg Right Ascension of center (J2000) 10- 18 F9.5 deg DEdeg Declination of center (J2000) 20- 21 I2 arcsec/pix scale Scale of the image 23- 25 I3 --- Nx Number of pixels along X-axis 27- 29 I3 --- Ny Number of pixels along Y-axis 31- 33 I3 Kibyte size Size of FITS file 35- 49 A15 --- FileName Name of FITS file, in subdirectory fits 51-109 A59 --- Title Title of the FITS file
Acknowledgements: David Berge, d.berge(at)uva.nl References HESS collaboration, Paper I 2018A&A...612A...1H, Cat. J/A+A/612/A1 HESS collaboration, Paper II 2018A&A...612A...2H HESS collaboration, Paper III 2018A&A...612A...3H HESS collaboration, Paper IV 2018A&A...612A...4H HESS collaboration, Paper V 2018A&A...612A...5H, Cat. J/A+A/612/A5 HESS collaboration, Paper VI 2018A&A...612A...6H, Cat. J/A+A/612/A6 HESS collaboration, Paper VII 2018A&A...612A...7H, Cat. J/A+A/612/A7 HESS collaboration, Paper VIII 2018A&A...612A...8H HESS collaboration, Paper IX 2018A&A...612A...9H HESS collaboration, Paper X 2018A&A...612A..10H HESS collaboration, Paper XI 2018A&A...612A..11H HESS collaboration, Paper XII 2018A&A...612A..12H HESS collaboration, Paper XIII 2018A&A...612A..13H MAGIC collaboration, Paper XIV 2018A&A...612A..14M
(End) Patricia Vannier [CDS] 10-Feb-2017
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