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 SDSSJ084234.9+362503 130.6534 36.3531 129.855939 36.532969 123.380084 17.503637 186.36195466 37.19411123 266.2333 53868.6856018518 2006-05-13 16:27:16 53871.41625 2006-05-16 09:59:24 701004010 109.9556 120 109.9716 109.9636 109.9556 109.9636 2 2 2 2 1 0 0 127.2306 127.2306 235.8948 1 PROCESSED 57534.3648032407 2016-05-26 08:45:19 54400 2007-10-27 00:00:00 53920.287650463 2006-07-04 06:54:13 3.0.22.43 5 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 010036 Type 2 QSOs are one of the key class to understand the structure and evolution of AGN, origin of the Cosmic X-ray background, and the history of black hole growth. We propose to measure a hard X-ray spectrum of the most luminous and brightest type 2 QSO candidate in the Sloan Digital Sky Survey. The selection by optical narrow line spectra is not biased toward Compton-thin AGNs and enables us to investigate the true nature of type 2 QSOs. The data will be used to measure the absorption column density, intrinsic luminosity, and to constrain the structure of the absorber. EXTRAGALACTIC COMPACT SOURCES 7 B YUICHI TERASHIMA JAP 1 AO1 THE MOST LUMINOUS TYPE 2 QSO IN SDSS HXD N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/701004010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '701004010'

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