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
|
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1 | 4C+74.26 | 310.7114 | 75.111 | 310.85824 | 74.929178 | 50.846162 | 74.615216 | 108.98584774 | 19.50187948 | 247.6342 | 55888.5409027778 | 2011-11-23 12:58:54 | 55890.613275463 | 2011-11-25 14:43:07 | 706028010 | 101.4125 | 100 | 101.4125 | 101.4125 | 0 | 101.4125 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 117.8827 | 117.8827 | 179.0297 | 2 | PROCESSED | 57603.9949074074 | 2016-08-03 23:52:40 | 56269 | 2012-12-08 00:00:00 | 55901.2441203704 | 2011-12-06 05:51:32 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 060101 | We propose the 120 ks observation of Broad Line Radio Galaxy 4C+74.26. The purpose is to estimate the angular momentum of the central super massive black hole from the broadness of Fe-K line. We study the spectral changes on spectra in details on the Fe-K lines and reflection hump in HXD-PIN band. We try to study the correlation between the radio intensity and black hole spins. | EXTRAGALACTIC COMPACT SOURCES | 7 | C | HIROFUMI NODA | JAP | 6 | AO6 | STUSY OF BROAD IRON LINE OF 4C+74.26 TO ESTIMATE THE SPIN OF CENTRAL SUPER MASSIVE BLACK HOLE | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/706028010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '706028010'
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