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 H 1743+322 266.5667 -32.234 265.750828 -32.215343 267.051923 -8.827937 357.25546218 -1.83442728 271.9807 56924.2942476852 2014-09-24 07:03:43 56927.2779861111 2014-09-27 06:40:18 409059010 119.0885 100 119.0885 119.0965 0 119.5626 3 2 0 1 0 0 0 0 0 0 0 PROCESSED 57616.6267361111 2016-08-16 15:02:30 57310 2015-10-15 00:00:00 56940.6644560185 2014-10-10 15:56:49 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 092020 We propose a triggered Suzaku 100 ks observation of a high-inclination Galactic black hole binary in the hard intermediate state. This will be simultaneous with an already accepted XMM-Newton observation (PI: A. Ingram) to test the Lense-Thirring model for the low frequency quasi-periodic oscillations seen in black hole (and neutron star) binaries. The Suzaku PIN data will enable us to extend the energy range over which the QPO can be studied, allowing us to get much better constraints on the reflection component in the QPO spectrum, and hence to more tightly probe the geometry and emission processes in the regions closest to the black hole. GALACTIC POINT SOURCES 4 A MAGNUS AXELSSON EUR 9 AO9-TOO TESTING THE LENSE-THIRRING ORIGIN OF THE LOW FREQUENCY QPO IN BLACK HOLE BINARIES XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/409059010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '409059010'

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

Go to top of this page ⏏