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. |
observation_id
|
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
|
exposure
|
awarded_exposure
|
resolve_exposure
|
xtend_exposure
|
resolve_data_mode
|
resolve_with_filter_be
|
resolve_with_filter_fe55
|
resolve_with_filter_nd
|
resolve_with_filter_poly
|
resolve_with_filter_open
|
resolve_with_filter_undef
|
is_resolve_gatevalve_closed
|
is_resolve_mxs1
|
is_resolve_mxs2
|
is_resolve_mxs3
|
is_resolve_mxs4
|
xtend_number_modes
|
xtend_dataclass_file1
|
xtend_dataclass_file2
|
xtend_window1_exposure
|
xtend_window2_exposure
|
xtend_window1_burst_exposure
|
xtend_window2_burst_exposure
|
xtend_code
|
resolve_code
|
gen_code
|
processing_status
|
processing_date
|
public_date
|
distribution_date
|
processing_version
|
caldb_version
|
processing_software
|
proposal_id
|
proposal_abstract
|
proposal_category
|
proposal_category_code
|
proposal_priority
|
pi_name
|
co_pi_name
|
proposal_affiliated_country
|
proposal_cycle
|
proposal_type
|
proposal_title
|
observation_status
|
data_access_url
|
xtend_data_mode1
|
xtend_data_mode2
|
processing_count
|
remarks
|
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | 201004010 | GAMMA_CASSIOPEIAE | 14.1806 | 60.71741 | 13.42216 | 60.44712 | 43.93378 | 48.81447 | 123.57851 | -2.14771 | 223.95285 | 60721.16741 | 2025-02-15 04:01:04 | 60722.46185 | 2025-02-16 11:05:04 | 59.292 | 40.000 | 59.292 | 55.337 | PX_NORMAL | N | Y | N | N | Y | Y | Y | OFF | OFF | OFF | OFF | 2 | 31100010 | 320000A0 | 59.191 | 55.337 | 0.000 | 0.000 | 11110 | 313430 | 11310 | PROCESSED | 2025-03-20 15:58:57 | 2026-02-26 00:00:00 | 2025-02-23 12:27:17 | 03.00.013.010 | gen20241115_xtd20241115_rsl20241115 | Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 | 000013002 | Binary evolution is one of the most fundamental ingredients in astronomy. Binaries consisting of a high-mass star and a compact object constitute an important milestone in the evolution. Gamma Cas and its analogs could be the long-sought missing population of Be/WD binaries, though an alternative scenario exists. The two scenarios (a) Be/WD binary and (b) magnetic disk-star interaction on Be star surface differ most distinctively in the production site of the hard X-rays. We propose two straightforward and fully independent tests with Resolve to distinguish (a) and (b); the test 1 is the RV change of Fe lines as a function of the orbital phase. The test 2 is the line profile of the flurescent Fe Ka lines. Based on our PV experience, the two tests are only possible with Resolve. | ACCRETING WHITE DWARFS AND NOVAE | 2 | A | MASAHIRO TSUJIMOTO | SEAN GUNDERSON | JUS | 1 | NOR | SOLVING THE LONG-STANDING MYSTERY OF GAMMA CASSIOPEIAE WITH RESOLVE | processed | https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201004010/ | WINDOW2 | WINDOW1 | 2 | Observation Log: No remarks ; Pre-pipeline Log: No remarks |
Used SQL
SELECT * FROM xrism_master_data WHERE observation_id = '201004010'
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