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 98 | 59.723 | 10.4395 | 59.038566 | 10.297703 | 59.781896 | -9.882185 | 179.82925767 | -31.05249617 | 81.003 | 55812.5811342593 | 2011-09-08 13:56:50 | 55815.280787037 | 2011-09-11 06:44:20 | 706015010 | 101.144 | 100 | 101.144 | 101.144 | 0 | 101.144 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 89.8389 | 89.8389 | 233.214 | 3 | PROCESSED | 57603.1723611111 | 2016-08-03 04:08:12 | 56218 | 2012-10-18 00:00:00 | 55851.4528356482 | 2011-10-17 10:52:05 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 060055 | Whether radio-loud and radio-quiet AGN may be unified under one model is still open to debate. The most important limitation in such work is that jet beaming swamps nuclear emission, so we must study powerful radio sources which are not affected by this bias. These are the Narrow Line Radio Galaxies (NLRGs). Heavy obscuration means that their primary emission is visible only above 10 keV. 3C 98 is an important member of the NLRG class because its hard band power dominates the full radio to X-ray core luminosity. We propose a 100 ks observation of this source with Suzaku to detect the core continuum emission and reflection above 10 keV. 3C~98 is one of few NLRGs for which we can expect to model (rather than just detect) the hard X-ray flux, and hence use it for testing unification schemes. | EXTRAGALACTIC COMPACT SOURCES | 7 | B | POSHAK GANDHI | JAP | 6 | AO6 | HARD X-RAY EMISSION AND REFLECTION IN RADIO GALAXIES: 3C 98 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/706015010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '706015010'
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