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 | 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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