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 0352+30 58.8427 31.0494 58.059686 30.903757 63.208913 10.461571 163.07655547 -17.13553633 77.7002 56166.360150463 2012-08-27 08:38:37 56170.0980208333 2012-08-31 02:21:09 407088010 153.4893 150 153.4893 153.4893 0 153.4893 2 2 0 2 1 0 0 140.9919 140.9919 322.9236 3 PROCESSED 57607.0637268518 2016-08-07 01:31:46 56582 2013-10-17 00:00:00 56212.7609722222 2012-10-12 18:15:48 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 072011 After 40 years of studies, surprisingly little is known about accreting pulsars at low-luminosities, yet these may be the most numerous class of neutron star binaries in the Galaxy. Upcoming large-scale surveys will likely reveal many such objects, but to identify them it is crucial to fully understand their properties. X Per, the archetypal source of this class, at 1 kpc from Earth is ideal target for detailed studies. In spite of that X Per is still puzzling. With the proposed program we aim to study X Per in detail, constrain its X-ray spectrum also as a function of the spin phase. Our study will be key to characterize the properties of low-luminosity X-ray pulsars population and will help to identify it in upcoming surveys. GALACTIC POINT SOURCES 4 B VICTOR DOROSHENKO EUR 7 AO7 CRACKING THE X PER XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/407088010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '407088010'

Your request has been accepted.
The download will start soon automatically.

Go to top of this page ⏏