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 APM 08279+5255 127.9265 52.7635 126.994318 52.932793 116.239859 32.72128 165.74397918 36.24189551 118.0523 54020.1580902778 2006-10-12 03:47:39 54022.3134143518 2006-10-14 07:31:19 701057010 102.3328 100 102.3408 102.3408 102.3328 102.3408 2 2 2 2 1 0 0 96.0187 96.0187 186.1858 3 PROCESSED 57535.8953125 2016-05-27 21:29:15 54702 2008-08-24 00:00:00 54053.9467013889 2006-11-14 22:43:15 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 011353 Motivated by the detection of a relativistic outflow of highly ionized gas in previous XMM-Newton and Chandra observations of the lensed quasar APM08279+5255 we propose to monitor this object with three 100ks observations with the aim of improving our understanding of the significance of such outflows in regulating black hole growth and in influencing structure formation. The main scientific goals are : (a) verify the present interpretations of Fe line features in this quasar, (b) monitor the time variability of the Fe absorption features and thus constrain the acceleration mechanism, (c) constrain the kinematic, ionization and absorbing properties of the outflow, and (d) show whether the low-energy ionized absorber is part of the relativistic outflow. EXTRAGALACTIC COMPACT SOURCES 7 A GEORGE CHARTAS USA 1 AO1 VIEWS OF RELATIVISTIC WINDS THROUGH NATURAL LENSES XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/701057010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '701057010'

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