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 B3 0309+411 48.2809 41.3324 47.459303 41.145685 57.252935 22.518841 149.59257755 -14.09014879 253.0016 55976.5100462963 2012-02-19 12:14:28 55979.0410532407 2012-02-22 00:59:07 706036010 104.6245 100 104.6245 104.6296 0 104.6245 2 2 0 2 1 0 0 95.453 95.453 218.6719 2 PROCESSED 57604.7018981482 2016-08-04 16:50:44 56360 2013-03-09 00:00:00 55992.2317824074 2012-03-06 05:33:46 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 062007 We propose to observe B3 0309+411, an X--ray bright FRII BLRG detected by INTEGRAL for 100 ks. BRLGs have been poorly studied in X-rays and usually show weak reprocessing spectral features with respect to their radio-quiet counterparts. B3 0309+411 has been already followed-up with XMM-Newton and, the XMM-Newton and INTEGRAL data suggests that the source could 1) be strongly reflection-dominated; 2) exhibit extreme flux/spectral variability; 3) be severely affected by absorption. The Suzaku observation will unveil the puzzling spectral shape of this peculiar BLRG, allowing to determine with accuracy the reflection properties which would have a large impact on our understanding of the disk/jet contribution in BLRG. EXTRAGALACTIC COMPACT SOURCES 7 B FRANCESCA PANESSA EUR 6 AO6 B3 0309+411: A REFLECTION--DOMINATED BROAD LINE RADIO GALAXY? XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/706036010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '706036010'

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