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 | 4U 1907+09 | 287.4001 | 9.8965 | 286.805564 | 9.814618 | 290.343315 | 32.116545 | 43.79892996 | 0.51344636 | 85.3836 | 54209.4191666667 | 2007-04-19 10:03:36 | 54211.2612731482 | 2007-04-21 06:16:14 | 402067010 | 80.6283 | 65 | 80.6283 | 80.6363 | 0 | 80.6363 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 73.2685 | 73.2685 | 159.1479 | 2 | PROCESSED | 57538.4515393518 | 2016-05-30 10:50:13 | 54702 | 2008-08-24 00:00:00 | 54216.2674189815 | 2007-04-26 06:25:05 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 021123 | The HMXB 4U 1907+09 shows a rich phenomenology: two cyclotron lines, an uncommonly weak iron line, intermittent X-ray fading, and a recent torque reversal. Compared to other persistent supergiant X-ray pulsars it has been less well observed, although it is a prime target to study the interaction of the neutron star's X-rays with the stellar wind and the accretion column. The latter has been confirmed by our 60ks AO1 observation which allowed for the first detection of a soft excess below 2keV as well as the determination of the paramters of the fundamental cyclotron line with unprecedented accuracy. Due to an unusually low source state during the AO1 exposure, however, an additional observation of 65ks is needed to perform the first phase resolved analysis of this interesting source. | GALACTIC POINT SOURCES | 4 | B | KATJA POTTSCHMIDT | USA | 2 | AO2 | THE BROAD BAND SPECTRUM OF 4U 1907+09 | HXD | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/402067010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '402067010'
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