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 RX J1633+4718 248.3342 47.2989 247.973952 47.402455 228.776709 67.659807 73.52584527 42.62417772 308.6809 55760.5047916667 2011-07-18 12:06:54 55761.4376388889 2011-07-19 10:30:12 706027020 37.51 40 37.51 37.51 0 37.51 2 2 0 2 0 0 0 0 0 0 0 PROCESSED 57602.5962847222 2016-08-02 14:18:39 56152 2012-08-13 00:00:00 55830.7262268518 2011-09-26 17:25:46 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 060089 RX J1633+4718 was detected in the ROSAT all sky survey, later identified as a radio loud narrow line Seyfert 1 (NLS1) galaxy. The soft X-ray spectrum of this source was fitted with a blackbody with temperature of 32eV plus a flat power law component. The blackbody temperature is much lower than 100-200eV, typical soft X-ray excess commonly observed in NLS1. Since radio to UV continuum spectrum of this souce resembles those of blazars, the flat power law X-ray component is likely to be a jet origin. The jet might supress accretion corona, and thus the emission from the accretion disk might visible in its bare form. Suzaku observation of this source will give us X-ray spectrum above 2keV and CCD resolution spectrum below 2keV for the 1st time. EXTRAGALACTIC COMPACT SOURCES 7 A KIYOSHI HAYASHIDA JAP 6 AO6 X-RAY EMISSION FROM DISK AND JET AROUND A SMBH IN RX J1633+4718 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/706027020/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '706027020'

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