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 4U 1344-60 206.8966 -60.619 206.036622 -60.369696 231.500761 -45.327278 309.76861534 1.50528265 97.6008 55572.7924189815 2011-01-11 19:01:05 55575.4751273148 2011-01-14 11:24:11 705058010 93.8773 100 93.9013 93.8933 0 93.8773 2 2 0 2 1 0 0 79.5617 79.5617 231.7537 3 PROCESSED 57600.6768865741 2016-07-31 16:14:43 55975 2012-02-18 00:00:00 55607.6933333333 2011-02-15 16:38:24 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 052018 We propose a 100 ks Suzaku observation of 4U 1344-60, a poorly studied (because at low Galactic latitude) but bright (about 2 millicrabs) AGN which showed, in an XMM-Newton observation, a strong relativistic disk iron line. The main aim of the proposal is to determine in detail the parameters of the disk, which is possible only with a high quality broad band observation which permits to control the continuum beneath the line. Presently, only Suzaku has the right combination of sensitivity, energy resolution and broad band coverage to achieve this objective. EXTRAGALACTIC COMPACT SOURCES 7 C JIRI SVOBODA EUR 5 AO5 4U 1344-60: A BRIGHT AGN WITH A STRONG RELATIVISTIC IRON LINE XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/705058010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '705058010'

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