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 24M2791 334.9577 63.2629 334.551329 63.011149 23.890285 63.530312 106.81877019 5.23758822 230.0008 55947.3704513889 2012-01-21 08:53:27 55948.0926388889 2012-01-22 02:13:24 406023010 34.6017 30 34.6177 34.6017 0 34.6097 2 2 0 2 1 0 0 35.0595 35.0595 62.3919 0 PROCESSED 57604.5087847222 2016-08-04 12:12:39 56340 2013-02-17 00:00:00 55973.1102893518 2012-02-16 02:38:49 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 060087 We propose to observe 5 Fermi unidentified gamma-ray sources which are selected by possible association with extremely bright infrared source. The infrared-selected Fermi unIDs in low-latitude plane are potentially very interesting because they could be a new class of gamma-ray emitter such as starburst galaxy, Seyfert, or X-ray binary. To investigate X-ray counterpart and identify what they are, we propose 30 ks observation for each object. GALACTIC POINT SOURCES 4 C MASANORI OHNO JAP 6 AO6 SEARCH FOR NEW CLASS OF GAMMA-RAY EMITTER BY X-RAY IDENTIFICATION OF BRIGHT INFRARED-SELECTED FERMI UNID SOURCES XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/406023010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '406023010'

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

Go to top of this page ⏏