2019ApJ...885..150A

Query : 2019ApJ...885..150A

2019ApJ...885..150A - Astrophys. J., 885, 150-150 (2019/November-2)

Measurement of the extragalactic background light spectral energy distribution with VERITAS.

ABEYSEKARA A.U., ARCHER A., BENBOW W., BIRD R., BRILL A., BROSE R., BUCHOVECKY M., CALDERON-MADERA D., CHRISTIANSEN J.L., CUI W., DANIEL M.K., FALCONE A., FENG Q., FERNANDEZ-ALONSO M., FINLEY J.P., FORTSON L., FURNISS A., GENT A., GIURI C., GUETA O., HANNA D., HASSAN T., HERVET O., HOLDER J., HUGHES G., HUMENSKY T.B., JOHNSON C.A., KAARET P., KERTZMAN M., KIEDA D., KRAUSE M., KRENNRICH F., KUMAR S., LANG M.J., MAIER G., MORIARTY P., MUKHERJEE R., NIEVAS-ROSILLO M., O'BRIEN S., ONG R.A., PFRANG K., POHL M., PRADO R.R., PUESCHEL E., QUINN J., RAGAN K., REYNOLDS P.T., RIBEIRO D., RICHARDS G.T., ROACHE E., ROVERO A.C., SADEH I., SANTANDER M., SEMBROSKI G.H., SHAHINYAN K., SUSHCH I., SVRAKA T., WEINSTEIN A., WELLS R.M., WILCOX P., WILHELM A., WILLIAMS D.A., WILLIAMSON T.J. and ZITZER B.

Abstract (from CDS):

The extragalactic background light (EBL), a diffuse photon field in the optical and infrared range, is a record of radiative processes over the universe's history. Spectral measurements of blazars at very high energies (>100 GeV) enable the reconstruction of the spectral energy distribution (SED) of the EBL, as the blazar spectra are modified by redshift- and energy-dependent interactions of the gamma-ray photons with the EBL. The spectra of 14 VERITAS-detected blazars are included in a new measurement of the EBL SED that is independent of EBL SED models. The resulting SED covers an EBL wavelength range of 0.56-56 µm, and is in good agreement with lower limits obtained by assuming that the EBL is entirely due to radiation from cataloged galaxies.

Abstract Copyright: © 2019. The American Astronomical Society. All rights reserved.

Journal keyword(s): Extragalactic astronomy - Active galactic nuclei - Diffuse radiation - Cosmology

Simbad objects: 15

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Number of rows : 15
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024 		#notes
1 3C 66A BLL 02 22 39.6114771888 +43 02 07.799534304   15.71 15.21 14.5   ~ 888 1
2 QSO B0229+200 BLL 02 32 48.6148874688 +20 17 17.486717388   18.0 18.00 13.96   ~ 340 1
3 QSO B0414+009 BLL 04 16 52.4945693352 +01 05 23.899102620   16.86 16.38 16   ~ 287 0
4 QSO B0502+675 BLL 05 07 56.1631660632 +67 37 24.225299292     17.0 17.2   ~ 181 1
5 M 1 SNR 05 34 30.9 +22 00 53           ~ 6203 1
6 6C 070609+591309 BLL 07 10 30.0683697888 +59 08 20.371772544   17.38 16.52 15.1   ~ 232 2
7 6C 101157+494057 BLL 10 15 04.1396533776 +49 26 00.706055496   16.56 16.15 14.58   ~ 370 3
8 6C 121520+302351 BLL 12 17 52.0819904040 +30 07 00.634936872   16.07 15.62 13.47   ~ 478 1
9 QSO B1218+304 BLL 12 21 21.9426947832 +30 10 37.158534012   16.50 15.85 15.7   ~ 469 1
10 QSO B1221+24 BLL 12 24 24.1862962656 +24 36 23.499792828   17.93 17.37     ~ 149 0
11 7C 1424+2401 BLL 14 27 00.3917926224 +23 48 00.037510776 14.52 14.34 14.95 14.5   ~ 367 1
12 QSO B1426+428 BLL 14 28 32.6090008440 +42 40 21.048123396   16.95 16.45 14.4   ~ 520 2
13 QSO B1553+113 BLL 15 55 43.0440048528 +11 11 24.365649948 14.91 14.72 14.57 13.99   ~ 572 1
14 QSO B1959+650 BLL 19 59 59.8520303688 +65 08 54.652536492     12.8 11.21   ~ 628 2
15 QSO B2344+514 BLL 23 47 04.8372110928 +51 42 17.877513168     15.50 10.7   ~ 464 0

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