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 NGC 4258 184.7518 47.3153 184.134648 47.592794 160.376562 44.164981 138.28789039 68.83430148 139.1798 55511.1601388889 2010-11-11 03:50:36 55512.7112615741 2010-11-12 17:04:13 705051010 103.8332 100 103.8332 103.8412 0 103.837 2 2 0 2 1 0 0 86.2257 86.2257 133.9688 1 PROCESSED 57554.0812384259 2016-06-15 01:56:59 55903 2011-12-08 00:00:00 55537.1754398148 2010-12-07 04:12:38 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 051451 We request a 100 ksec observation of the Low Luminosity AGN NGC 4258. This observation is meant to complement our existing 100 ksec Suzaku observation (Reynolds et al. 2009), and our 320 ksec Chandra-HETG observation (Murphy et al., in prep.). The goal is to further characterize the observed variability of the Fe Kalpha line and any associated changes in the continuum and/or absorption of NGC 4258. Given the unique constraints that we have on the mass, distance and accretion flow geometry in NGC 4258, as well as its role as a bridge between the most quiescent nuclei and powerful AGN, further Suzaku studies of NGC 4258 are clearly warranted. EXTRAGALACTIC COMPACT SOURCES 7 C MICHAEL NOWAK USA 5 AO5 HUNTING FOR THE VARIABLE IRON LINE IN NGC 4258 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/705051010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '705051010'

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