DARTS/Astro Query System - SQL Search -

All the tables available for SQL Search and information on each table are listed in the Available Data page. Please see the User Guide for the usage of "SQL Search".

total 1

No.
object_name
center_ra
center_dec
center_ra_b1950
center_dec_b1950
center_ecliptic_lon
center_ecliptic_lat
center_galactic_lon
center_galactic_lat
roll_angle
observation_start_time_mjd
observation_start_time
observation_end_time_mjd
observation_end_time
observation_id
exposure
awarded_exposure
xis0_exposure
xis1_exposure
xis2_exposure
xis3_exposure
xis0_observation_mode
xis1_observation_mode
xis2_observation_mode
xis3_observation_mode
hxd_observation_mode
hxd_coarse_clock_rate_exposure
hxd_first_clock_rate_exposure
hxd_normal_clock_rate_exposure
hxd_all_clock_rate_exposure
hxd_wam_exposure
quantity_of_hxd_burst
processing_status
processing_date_mjd
processing_date
public_date_mjd
public_date
distribution_date_mjd
distribution_date
processing_version
processing_count
processing_software
proposal_id
proposal_abstract
proposal_category
proposal_category_code
proposal_priority
pi_name
co_pi_name
proposal_affiliated_country
proposal_cycle
observation_type
proposal_title
main_instrument
has_xis_injection
data_access_url
ql_access_url
ql_image_url
1 3C 111 64.5741 38.0889 63.737568 37.967565 69.370671 16.452489 161.62276278 -8.7838332 81.5451 54700.4141898148 2008-08-22 09:56:26 54703.1836111111 2008-08-25 04:24:24 703034010 122.378 120 122.386 122.378 0 122.378 2 2 0 2 1 0 0 109.7067 109.7067 239.2517 1 PROCESSED 57543.4018287037 2016-06-04 09:38:38 55084 2009-09-10 00:00:00 54713.6361226852 2008-09-04 15:16:01 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 031332 The origin of the high-energy emission from Broad-Line Radio Galaxies is still an open issue. A plausible scenario is reprocessed emission from a cold medium (disk) diluted by variable, non-thermal jet flux. To test this scenario we propose Suzaku observations of the BLRG 3C 111, which exhibits flux variability above 10 keV from available data, suggesting a jet contribution. Moreover, 3C 111 was previously detected with EGRET at GeV energies, and synergy with GLAST will thus be exploited in the proposed program. The coupled timing and spectral information provided by Suzaku are key to disentangle the disk and jet contributions, and determine their respective role for the source energy budget. EXTRAGALACTIC COMPACT SOURCES 7 A RITA SAMBRUNA USA 3 AO3 SUZAKU OBSERVATIONS OF 3C 111: UNCOVERING THE JET WITHIN HXD Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/703034010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '703034010'

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