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
|
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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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